ETCS Pump Module changeout success following epic ISS EVA

Posted on 18th August 2010 by admin in Space Flight

International Space Station (ISS) astronauts Doug Wheelock and Tracy Caldwell-Dyson have completed their third specialized spacewalk to kick off a week that will hopefully result in the return of Loop A cooling on the External Thermal Control System (ETCS) for the first time since its failure at the end of last month. ISS EVA-17′s prime aim of installing the replacement Pump Module (PM) was a huge success.

Previous EVAs:

The NASA duo already have two epic EVAs under their belts, as they put into work a complex set of plans created by ground engineers – aided by simulation runs in the NBL (Neutral Buoyancy Laboratory) at the Johnson Space Center (JSC) – with an aim of returning the ETCS Loop A.

The ETCS provides cooling to the entire United States On-Orbit Segment (USOS). The ETCS consists of two independent loops, designated Loop A and Loop B – the latter of which is currently working without issue. With Loop A down, ISS crewmembers were forced to deactive various station systems and experiments to prevent overheating.

The system is designed to collect heat from the Internal Thermal Control Systems in the US Lab, Node-2, COL, JEM, and Node-3, via IFHXs (Interface Heat Exchanger). The PM provides the motive force to transport the ammonia around the loop.

The main task of EVA-1 was to remove the current PM – which suffered from a power spike which tripped a circuit breaker on July 31 – and replace it with a spare during the second EVA next week. However, issues with one of the Quick Disconnect (QD) lines resulted in a re-arranged timeline, and the potential for four EVAs to complete the entire task.

EVA-2 was highly successful, with the troublesome M3 QD literally forced off the faulty PM via the brute force of Wheelock – after ground controllers gave him permission to “violently” shake the QD – allowing for its removal from the S1 truss.

Caldwell-Dyson also played her part, aiding the next EVA tasks by releasing the non-functional PM electrical and data cables as well preparing similar tasks for the translation of the new PM on ESP-2 (External Stowage Platform) into its new home on the S1 Truss.

ISS EVA-17/EVA-3 for ETCS Troubleshooting:

On what was the 150th EVA devoted to space station assembly and maintenance since ISS construction began, the main aim was to install the new PM, bolting into place, with electrical and fluid connections attached – eventually allowing the process to bring back ETCS Loop A back to life.

“Install spare PM (Pump Module) mechanically. Mate & open spare PM fluid QDs (Quick Disconnects). Perform electrical & data continuity checks plus bump-start test (by MCC-H, to check pump functionality). Re-couple stbd & port CETA carts,” NASA noted the tasks for the EVA.

“Clean up spare PM/S1/CETA (Crew & Equipment Translation Aid) cart. Clean up SSRMS (remove APRF for walkoff). Install J612 extension cable for ULF5/PMM (Pressurized Multipurpose Module). Clean up tethers at S1 truss segment. Configure CETA cart to allow for WS8 (Worksite 8 ) ops. Move old PM to ESP-2/mate min electrical connectors (if time allows). Cleanup/Ingress.”

Should all go to plan, the ISS may be back into its nominal cooling configuration by Thursday.

Detailed EVA Events:

Eager to get out of the door, the spacewalkers were over 30 minutes ahead of the timeline for Quest Airlock, for what is expected to be a six hour, 30 minute EVA that officially began at 5:20am Central Time.

Both spacewalkers egressed from the Quest Airlock and began to set up tethers and tools, as the Space Station Remote Manipulator System (SSRMS) was placed into position to assist with the EVA.

“Setting up shop” at handrail 8024, Wheelock arranged his tethers and prepared to set up a Portable Foot Restraint on the SSRMS for his role in removing the replacement PM from ESP-2.

With both spacewalkers in position, Wheelock used the Pistol Grip Tool – with torque multiplier installed – to break the torque on the bolts holding the replacement PM into its home on ESP-2.

Meanwhile, Caldwell-Dyson removed insulation and worked electrical and fluid line connection caps in preparation for the PM’s removal for the platform.

Next, Wheelock started to fully release the bolts on the PM, starting with Bolt 1 – which proved to be troublesome. While Bolt 2 released without issue, use of the torque multiplier was required on the sticky bolt.

“Come on now, Bolt,” Wheelock exclaimed, as the bolt finally started to release. With the Scoop installed on to Bolt 2, Wheelock then moved to work on Bolt 4, which released without issue. Bolt 3 – the final bolt holding the PM into position on ESP-2 - also released.

With the Pump Module physically released from ESP-2, ground controllers to gave Wheelock a “GO” for PM removal.

With 780lbs of mass in his hands, Wheelock was translated on the end of the SSRMS with the replacement PM, over to the S1 truss, where he waited for Caldwell-Dyson to aid in the careful placement of the hardware into the vacated slot.

With fine-tuned SSRMS operations, Wheelock eased the PM into position on S1, wasting no time in securing the replacement into place by using his PGT to start work on the four associated bolts, while Caldwell-Dyson worked on mating several electrical connections, “waking up” the PM.

With the Thermal Systems officer Shaun Robinson standing by in the ISS Flight Control Room in Houston,  the key moment arrived for the orbiting outpost, as preparations for a “bump test” were readied on the PM – which proved to be successful, confirming they have a good PM installed, following its four year stay on ESP-2.

Next up was the closing and demating of the M4 fluid line from the jumper box, allowing for nitrogen to be vented through the new PM ahead of the flow of ammonia. M2 followed, allowing the jumper box to be handed over to Caldwell-Dyson for her task to install it on the CETA cart.

Key events followed, with the go to fill the PM with ammonia for the first time, as the troublesome M3 QD was installed – following some difficulty.

Once completed, Wheelock moved on to the mating of M2 and M1, which provided no issues, while ground controllers noted that the ammonia fill – a three minute process – was completed without a hitch.

On completion of the QD tasks, Wheelock held up his checklist, attached to his left arm, which had a special message for Tim Bond, a fluids engineer on the ground – reading: “Tim Bond 1-0 M3 QD – Game Over!! Thanks Tim.”

Wheelock then closed the thermal cover over the newly installed PM, while Caldwell-Dyson moved the two nearby CETA carts into a position that would best assist the STS-133 mission.

Also related to the upcoming mission for Discovery, a get-ahead task of installing a 10 foot long J612 cable between the Quest and Destiny modules was being worked, taking the EVA well past 7 hours PET. Managers continued to evaluate if to complete the task, which would have taken another 45 minutes.

With Wheelock only having 50 minutes of consumables remaining, Caldwell-Dyson would have been left to complete the task, and potentially breach the record time for an ISS EVA – depending on completion time. The ultimate decision was to cancel the get-ahead, clean up and ingress the Quest airlock – completing a superb EVA – ending after 7 hours and 20 minutes.

“The Pump is looking good,” noted MCC-H. “Aww, sweet! We got our Station back”, responded Wheelock.

Praise for the ETCS troubleshooting on the ISS has been noted throughout NASA, with Space Shuttle Program (SSP) manager John Shannon taking time to note how impressed he has been with the efforts.

“Flight Crew has been supporting the EVA and robotics development for the spacewalk. EVA is learning a lot from this Increment EVA,” noted the latest Shuttle Standup/Integration report (L2).

“Congratulations to the team on the great EVA,” added Mr Shannon. “It was impressive to see how they worked around all the problems.”

pixelstats trackingpixel

No related posts.

Endeavour continues eventful flow – OPF and ET-138 investigations continue

Posted on 18th August 2010 by admin in Space Flight

The mystery washer that managed to find its way into the LO2/LOX feedline on External Tank ET-138 is being classed as an isolated incident, as the Shuttle fleet work through numerous investigations. Work on Endeavour is back into a full flow, as an investigation board check into how an Air Hoist managed to fall on to a platform in her Orbiter Processing Facility (OPF).

STS-134 Processing Latest:

Endeavour is in a relatively relaxed flow inside OPF-2, as the youngest orbiter in the fleet prepares for a February 24 launch date target for what is likely to be her final trip to the International Space Station (ISS).

No Interim Problem Reports (IPRs) have been charged against her flow for some time, although the installation of the heat shield – which mounts on to the aft of the vehicle to surround the Space Shuttle Main Engines (SSMEs) – was interrupted by an Air Hoist falling on to one of the OPF platforms.

“An Air Hoist fell approx. 8 feet down on to 19-level platform (last week). No personnel injury or flight hardware damage occurred. A Standing Accident Investigation Board (SAIB) has been formed. SSME heat shield installation has been rescheduled,” noted the NASA Test Director (NTD) processing report (L2), before the status was updated.

“The Air Hoist (SAIB) is completing its work. The area is still controlled. Controls are expected to be removed and the air hoist re-installed. SSME heat shield installation is now scheduled to pick up tomorrow (Wednesday).

Other processing, away from the controlled area, had been proceeding without delay, with engineers completed resupplying the Freon Coolant Loop – which runs through the orbiter’s radiators to provide vehicle cooling when the Payload Bay Doors (PLBDs) are opened on orbit.

STS-134 Specific Articles: http://www.nasaspaceflight.com/tag/sts-134/

“OV-105 (STS-134). Window 7 has been installed for flight. Completed engine leak check and securing,” added NTD processing information. “Freon Coolant Loop top-off was completed. Sampling and adjust are scheduled.”

Waterproofing Endeavour is also being worked, after the process was recently carried out on Atlantis, marking the final few times the associated contractor – Evonik Degussa – will be working on the fleet

“Waterproofing of the vertical and side hatch are planned for Friday. This operation will result in a Bay clear,” added the NTD, following the clearance of OPF-1 for the opening work that was conducted on Atlantis this month.

Having already shutdown their production last month, the Program Requirements Control Board (PRCB) overviewed their ability to support the waterproofing of the orbiters with their stock of Dimethylethoxysilane (DMES) – the waterproofing agent – through to the Launch On Need (LON) support role of Atlantis, and/or if Atlantis gains the currently notional STS-135 mission.

“Tiles and Blankets are re-waterproofed by injection post flight. Approximately 42 one gallon bottles are used per Orbiter per flow. Current manifest shows two flows to the end of the program (STS-134, STS-335/135),” noted the associated PRCB presentations (L2) back in June.

“DMES is used to re-waterproof the Orbiter tiles and blankets prior to every flight. DMES has been in use at KSC since 1988. Only effective waterproofing agent that does not cause RTV reversion. Only material that is qualified for use on the Orbiter thermal protection tiles and blankets. Evonik Degussa plans to shut down the DMES plant and remove equipment once the contract expires on July 21, 2010.

Documentation shows that over 100 bottles of DMES will remain in stock after the final waterproofing is conducted, which should be an ample contingency ratio, taking into account it would take up to three years to find another supplier.

Endeavour’s primary payload, the Alpha Magnetic Spectrometer (AMS) – which was the primary cause of the launch scheduled realignment in April – is expected at the Kennedy Space Center (KSC) in just over a week’s time. Preparations for its eventual installation into Endeavour’s Payload Bay are currently on track.

“The Delta AMS Compatibility Review for STS-134 was held August 6.  It was followed up with a Ground Operations Working Group for AMS last week at KSC,” noted Flight Operations and Integration (Johnson Space Center) on the latest Shuttle Standup/Integration report (L2). “AMS is on track to deliver on August 26.”

“Payload Critical Path testing update: Alpha Magnetic Spectrometer (AMS) Power Transfer Unit (PTU) load test and Remotely Operated Electrical Umbilical (ROEU) 1553 BUS Characterization were rescheduled to this week,” added the NTD report.

Meanwhile, an Engineering Review Board (ERB) is being updated on the ET-138 investigation this week, after engineers removed the LOX 17” cover plate to perform angle and tip load measurements and found a washer had somehow found its way inside.

The washer was sent back to the Michoud Assembly Facility (MAF) in New Orleans, in order to attempt to track down its history, while options remain open to perform X-Rays on both ET-138 and the already-stacked ET-137 – which is set to fly with Discovery on STS-133.

“PR (Problem Report) ET-138 Washer update: Possible course of action will be to take X-rays, including areas inside the intertank, to look for additional FOD (Foreign Object Debris). The decision may also be made to perform X-ray inspections of ET-137,” added the NTD updates.

“The washer investigation is in work. Currently, it appears to be an isolated incident. There is an Engineering Review Board (starting) Tuesday, August 17. They will discuss potential inspections. The team is still working possible scenarios of how the washer got into the pipe.”

Processing of the tank – taking place inside its Checkout Cell in High Bay 2E (HB-2E) inside the Vehicle Assembly Building (VAB) – is continuing to plan for the meantime.

“ET-138 (VAB HB-2E): -Y protuberance air load foaming preps are in work,” added NTD processing status. “J box foaming preps are in work. Aft hardpoint primer is in cure. All systems electrical test is complete.”

Stacking of STS-134′s Solid Rocket Boosters (SRBs) have also picked back up in High Bay 1 (HB-1), following a few days of standdown due to poor local weather.

“In the VAB on SRB stacking, started back up last week; were delayed by weather for a couple of days. Moved the left forward center segment over; it is in work,” noted KSC Ground Operations on the Standup report, which was elaborated on via the NTD status update.

“SRB BI-145 / RSRM 113 (VAB HB-1): Left and Right tunnel cover bond preps are complete. Right Aft Center clevis preps are complete. Right Forward Center tang preps are complete. Right Center Joint segment mate preps are in work. Segment was lifted to HB-1 at 2000 (Monday).

“Leak check panel validation, run 4, complete. Right Aft Joint closeouts are complete. Right Aft Joint splice plate installation is complete. Hold down post ordnance preps: Upper shock absorbers are installed in blast containers. Clip installation is complete.”

pixelstats trackingpixel

No related posts.

ULA Atlas V successfully launches with AEHF satellte

Posted on 16th August 2010 by admin in Space Flight

A United Launch Alliance Atlas V has launched the first Advanced Extremely High Frequency satellite from Space Launch Complex 41 at Cape Canaveral at 11:07 UTC on Saturday. The satellite was successfully deployed 51 minutes into the flight, beginning its mission to provide communications for the armed forces of the US and its allies.

Launch Preview:

The AEHF-1 satellite is the first of four Advanced Extremely High Frequency (AEHF) satellites, and was constructed by Lockheed Martin. It is based around the A2100 satellite bus, and has a mass at launch of about 6,170 kilograms. AEHF spacecraft are intended to provide secure and jamming-resistant communications to the militaries of the United States, United Kingdom, Canada and the Netherlands, and will be used to relay communications for forces on land, in the air, or at sea.

AEHF will replace the earlier Milstar system, which consisted of six satellites launched atop Titan IV rockets between 1994 and 2003. One of those satellites was lost in a launch failure, when several flight events were incorrectly programmed to occur during the first orbit rather than later in the flight. Due to this, the Centaur upper stage that was to have boosted it from low Earth orbit to geosynchronous orbit made its three burns at the wrong times, and placed the satellite into a useless medium Earth orbit instead.

Despite the failure, the other five Milstar satellites were launched successfully, and the constellation is still in service. Control over the Milstar system was transferred to AEHF mission control earlier this month.

Originally six AEHF satellites were planned, however with the development of the Transformational Satellite Communications System, or TSAT, this was reduced to three. TSAT was cancelled in 2009 due to issues with its cost and delays in its development. A fourth AEHF satellite will be produced instead of TSAT, however reports of a fifth being planned are yet to be confirmed. The US Air Force currently describes AEHF as being a four-satellite constellation.

Saturday’s launch will use an Atlas V rocket, flying in the 531 configuration. This will be the first launch of the 531 configuration, and the twenty second launch of the Atlas V overall. The rocket which will be used for this launch is AV-019.

The 531 configuration consists of a payload fairing with a diameter of 5.4 metres, three solid rocket motors augmenting the first stage at liftoff, and a single-engined Centaur upper stage. For this flight, a short payload fairing, which has a length of 20.7 metres, will be used.

The Atlas V is, along with the Delta IV, one two rockets developed as part of the United States Air Force’s Evolved Expendable Launch Vehicle (EELV) programme. It made its maiden flight in 2002, successfully orbiting the Hot Bird 6 spacecraft for Eutelsat. Of its twenty one launches to date twenty have been successful, and one resulted in a partial failure.

That partial failure occurred on AV-009, carrying the USA-194 spacecraft, and was caused by a valve failing to close and allowing liquid hydrogen to leak from the upper stage. The spacecraft were placed into an incorrect orbit, but were still operable.

The Atlas V’s first stage, the Common Core Booster (CCB), is propelled by an RD-180 engine which is produced by NPO Energomash of Russia. The RD-180, which is derived from the RD-170 engine originally developed for the Energia and Zenit rockets, burns RP-1 propellant and uses liquid oxygen as an oxidiser. It will ignite at T-2.7 seconds, and 1.9 seconds later it will reach its expected thrust level for launch.

The three Aerojet solid rocket motors will ignite once the engine reaches full thrust, and at T+1.1 seconds the AV-019 will lift off. Five seconds into the flight, it will begin a series of roll, pitch and yaw manoeuvres to attain the proper trajectory for its ascent to orbit. The pitch and yaw manoeuvres will last around fifteen seconds, with the roll manoeuvre lasting twenty seven seconds.

Thirty four seconds into the flight, AV-019 will throttle down to pass through one of two areas of maximum dynamic pressure, or max-Q. It will throttle back up to full thrust nine seconds later, and one second later dynamic pressure will peak again. Ninety one seconds into the mission, the solid rocket motors will burn out; two will separate twenty three seconds later, with the third separating two seconds after those.

At two hundred and seven seconds after launch, the payload fairing will be jettisoned. It will fall into the Atlantic and is not expected to be recovered, however on the previous flight, which carried the first X-37B spacecraft, part of the fairing washed ashore in South Carolina and has since been put on display in a local museum. Six seconds after the faring separates, the forward load reactor, a device used to dampen vibrations within the fairing, will follow suit.

Booster Engine Cutoff (BECO), the extinction of the first stage, will occur 257 seconds into the flight, and will be followed six seconds later by the separation of the first stage. The Centaur’s RL10A-4-2 engine, which is cryogenically fuelled – burning liquid hydrogen oxidised by liquid oxygen, will ignite ten seconds after separation beginning its first burn. This burn will last nine minutes and thirty five seconds, and will precede an eight minute, nine second coast phase.

Following the coast, the Centaur will restart for a second burn, which will last five minutes and twenty seconds. This second burn will end twenty seven minutes and thirty seven seconds after launch, and will conclude the powered phase of the flight.

Following the end of its powered flight, AV-019 will coast for twenty three minutes and twenty three seconds before the AEHF-1 spacecraft will separate. The orbit at separation is expected to be a geosynchronous transfer orbit, with a perigee of 191.5 kilometres, an apogee of 35,786 kilometres, and 27 degrees of inclination. The argument of orbit’s perigee will be 180 degrees.

From this orbit, AEHF will raise itself to its operational geosynchronous orbit using what is believed to be a LEROS-1C apogee motor. The spacecraft also carries Hall Effect thrusters, which are ion engines that will be used for stationkeeping.

The launch of AV-019 will occur from Space Launch Complex 41 at Cape Canaveral, a complex which was originally built in the 1960s for use by the Titan family of rockets. It was first used for a Titan IIIC launch in December 1965, and was subsequently used for Titan IIIE and Titan IV launches, the last of which was a failed attempt to launch a Defense Support Program satellite in April 1999.

Following this launch, the complex was demolished and rebuilt to support Atlas V launches, and today’s will be the twentieth Atlas launch from the pad.

The complex follows the “clean pad” concept, with the rocket being assembled off-pad, atop a Mobile Launch Platform in the Vertical Integration Facility. Rollout of AV-019 to the launch pad was completed on Friday. Following its arrival at the pad, connections such as fuel and electrical supplies were connected to the platform, which will supply them to the rocket.

This is the third Atlas V launch of 2010, following that of the Solar Dynamics Observatory in February, and the first X-37B mission in April. The next Atlas V launch is scheduled to occur in September, when an Atlas V 501 will conduct NRO Launch 41, orbiting a classified payload for the US National Reconnaissance Office.

Another launch is currently scheduled for November, and will carry the GPS IIF SV-2 navigation satellite. United Launch Alliance is also expected to carry out two more Delta launches before the end of the year, both of which are currently scheduled for October.

A Delta IV Heavy will be used to conduct NRO Launch 32, carrying another classified payload, and a Delta II 7420 will launch the COSMO-4 radar imaging satellite for the Italian space agency and ministry of defence. The next launch of an AEHF satellite is currently scheduled for February 2011, and will also use an Atlas V 531.

Lead photo by Alan Walters – used with permission.

pixelstats trackingpixel

Related posts:

  1. Atlas V launches classified PAN satellite for US Government A United Launch Alliance Atlas V rocket has launched with PAN,…
  2. LIVE: ULA Atlas V launches WGS-2 for USAF United Launch Alliance (ULA) has launched the WGS-2 satellite on…
  3. Atlas V/Solar Dynamics Observatory launches at second attempt An Atlas V rocket has launched with NASA’s Solar Dynamics Observatory…

STS-133: Several troubleshooting reviews highlight a busy flow for Discovery

Posted on 15th August 2010 by admin in Space Flight

As Discovery closes in on rollover to the Vehicle Assembly Building (VAB) in just over three week’s time, engineers are working through a number of minor issues on the veteran orbiter, ranging from an O2 system Valve Position Indicator (VPI), a troublesome KU-band system, and a dent in one of her Payload Bay Doors (PLBDs) – which also requires a new Power Drive Unit (PDU).

STS-133 Processing Latest:

Discovery is still tracking a November 1 launch date target, as the complex ballet of operations focus in on the orbiter’s departure from her Orbiter Processing Facility (OPF-3) on what is currently scheduled to be September 8.

Several issues have been at the center of processing evaluations on the orbiter of late, none of which hold any major impact to her milestones during what is very likely to be her final lap of OPF processing for flight, with STS-133 scheduled to be her final mission.

“OV-103 (STS-133): Continued processing in OPF HB-3 (VAB High Bay 3). All the troubleshooting is complete on IPR (Interim Processing Report) #35 on the O2 crossover valve on the MO10W panel. This is in for final engineering review,” summarized KSC Ground Operations on the latest Shuttle Standup/Integration report (L2).

“On IPR #37 on the Ku-Band, troubleshooting wrapped up and it is in review. Looks like an EA1 (Electronics Assembly) or EA2 issue. Closed the PLBDs on Monday to facilitate the TPS (Thermal Protection System) blanket R&R (Removal and Replacement) and to do the positive pressure testing for the midbody. Completed the positive pressure tests.

“On the structures PR (Problem Report) on the door, the blanket was removed last night to perform the R&R. Small damage on the door was seen. This is being evaluated by Engineering. During door closure, there was a deferred PR on the PDU (Power Drive Unit) centerline latch, right-hand side 1-4. This ran longer than expected, so the actuator (will) be R&R’d.”

With the closure of the IPRs in work, nominal processing has continued on Discovery, via the scheduled closeouts and leak checks.

“OV-103 (OPF Bay 3): Airlock closeout for rollover was completed. The Forward structural leakage test was successfully completed,” added the NASA Test Director (NTD) processing updates (L2). “Final OPF flight controls cycling, SSME (Space Shuttle Main Engine) TVC (Thrust Vector Control) and ET (External Tank) actuator checkouts and aero-surface positioning were completed.”

STS-133 Specific Articles: http://www.nasaspaceflight.com/tag/sts-133/

On the specifics of the IPRs, an Engineering Review Board (ERB) was in the process of discussing the O2 cross-over valve issue, thus the Orbiter hydraulic system was configured with the issue in mind to allow the aforementioned flight control final OPF cycling, SSME TVC and ET actuator checkouts and aero-surface positioning to take place.

At present, it appears the problem with the misbehaving Valve Position Indicator (VPI) on the O2 system may be closed, after it was noted it would not hold an impact to the functionality of the Atmospheric Revitalization & Pressure Control System (ARPCS).

“Valve Position Indicator (VPI) transitioned from Closed to Open when pressure was applied to the inlet of the valve and the DSC was power cycled. With no pressure on the valve, DSC cycles had no response. The valve was left pressurized and the VPI was monitored for a change in state to Open. The VPI remained Closed,” noted the NTD.

“Performed a delta pressure test and a GN2 qualitative flow test with nominal results. A deferral is being discussed since the failure would not affect the ARPCS form or function.”

Notably, it was only recently that the orbiter fleet was given the ability to sense the mechanical state of the two O2 crossover valves, via the output of the VPI. Although the valves have always had VPIs fitted, its is only since STS-128 that they have been wired into the orbiter systems – as noted in at least two expansive Program Requirements Control Board (PRCB) processing baseline presentations (L2)

Prior to this modification it was only known whether or not voltage was being applied to the solenoid actuation coils, rather than the actual mechanical position of valve internals. The resulting wiring modifications gave the ground engineers – as opposed to the crew – insight into the valve states. Changes were also made to the Launch Commit Criteria (LCC) as a result of the modifications.

Given the valve itself appears to be working properly, with only the VPI talkback no longer reliable, the situation is still slightly improved on the pre-STS-128 configuration, as the state of the other crossover valve can still be verified.

On IPR 37, Discovery’s Ku-Band troubleshooting – related to the system failing the angle rate/pitch rate portion of the self test – is coming to a close, following its constraint to final stowing of the Ku-Band antenna during PLBD closure for rollover.

“A self test was re-performed to determine if powering down the system might have reset the problem however the same error signature was seen,” noted the NTD’s summary reports. “A breakout-box was installed and another self-test was performed. Three more self tests with same results as previously. Initial data suggests failures isolated to self test mode.”

As noted by KSC Ground Operations, one of the system’s Electronics Assemblies is believed to be the root cause, with engineering reviews are in work – which includes powering Discovery up over the weekend to aid the review into the Ku-band system.

Discovery’s PLBDs were already closed – but not for rollover – earlier in the week, to allow for final TPS work and pressure checks to take place on the orbiter. Two issues arose during this operation, one of which related to a stalled PDU as the doors were being closed and latched.

“During the PLBD closure for TPS on, C/L (Centerline) latch 1-4 Power Drive Unit (PDU) stalled going latched. This was similar to the previous times this has occurred,” noted the NTD. “However, this time it occurred during a dual motor operation indicating recent degradation.

“(Program) was uncomfortable accepting this condition for another flight, and is requesting the PDU be replaced. A spare PDU is available that was recently refurbished at the NSLD (NASA Shuttle Logistics Depot). Replacement is expected to take 3 or 4 days. Deployment of the RH radiator is required for access.”

The other issue related to an observation of a dent on a Fibrous Insulation Blanket (FIB) on the Right Hand (RH) PLBD, which is undergoing replacement. Prior to the damaged blanket’s removal, engineers took mold impressions to try and find out the root cause.

“PR: A depression was discovered in the FIB of RH PLBD 1. A 4”x4” section of the FIB was removed. Mold impression indicated a graphite epoxy dent with dimensions (in inches) of: length = 1.004, width = 0.9891, and depth = 0.0406. PR is under evaluation,” added the NTD, prior to providing an update.

“Ultrasound Inspection performed on the dented area of the PLBD. A small (0.125”), localized area of delamination was noted in the bottom of the dent and is contained within the defect area. Planned repair involves face-sheet removal, probable potting, and bonding of a doubler. No thermography is required, and no constraint to PLBD opening for further processing.”

Over in the VAB, the long-running repair on a Fairing Support Plate has come to a close, following the use of a recently arrived “new” SLA (Super Lightweight Ablative) kit.

“SRB BI-144 / RSRM 112 / ET-137 (VAB HB-3): PR: Damaged SLA on EB-2 Fairing Support Plate: Will Hand Pack both inboard and outboard. New SLA kit has been ordered (and arrived),” noted a series of NTD reports. “SLA removed, found missing primer. Preps to apply primer in work.”

EB-2 is a reference to the ET/SRB upper attach point on the right-hand side of the stack, which contains a 62lb bolt that is separated when the boosters depart from the stack after just over two minutes of powered flight (Booster Separation).

“Primer application complete. SLA application next,” continues the NTD reports over the period of around a week. “SLA hand pack is in cure (midweek). SLA repair complete (Friday).”

The completion of work on the Fairing Support Plate will allow for the checks to take place on the Forward Firing Line, as the stack prepares to welcome the arrival of Discovery for mating next month.

“Aft strut and HDP (Hold Down Posts) Firing Line checks complete. Forward Firing Line checks holding for completion of PR SLA application. Left and Right GEI/Igniter heater snap hot ready to work. Left & right forward crossover installation complete. Forward firing line check complete.”

pixelstats trackingpixel

No related posts.

ULA Atlas V set to launch with AEHF GPS satellte

Posted on 14th August 2010 by admin in Space Flight

A United Launch Alliance Atlas V is scheduled to launch the first Advanced Extremely High Frequency satellite from Space Launch Complex 41 at Cape Canaveral, with a 119-minute window opening at 11:07 UTC on Saturday. The GPS IIF SV-1 satellite is scheduled to be deployed 51 minutes into the flight, beginning its mission to provide communications for the armed forces of the US and its allies.

Launch Preview:

The AEHF-1 satellite is the first of four Advanced Extremely High Frequency (AEHF) satellites, and was constructed by Lockheed Martin. It is based around the A2100 satellite bus, and has a mass at launch of about 6,170 kilograms. AEHF spacecraft are intended to provide secure and jamming-resistant communications to the militaries of the United States, United Kingdom, Canada and the Netherlands, and will be used to relay communications for forces on land, in the air, or at sea.

AEHF will replace the earlier Milstar system, which consisted of six satellites launched atop Titan IV rockets between 1994 and 2003. One of those satellites was lost in a launch failure, when several flight events were incorrectly programmed to occur during the first orbit rather than later in the flight. Due to this, the Centaur upper stage that was to have boosted it from low Earth orbit to geosynchronous orbit made its three burns at the wrong times, and placed the satellite into a useless medium Earth orbit instead.

Despite the failure, the other five Milstar satellites were launched successfully, and the constellation is still in service. Control over the Milstar system was transferred to AEHF mission control earlier this month.

Originally six AEHF satellites were planned, however with the development of the Transformational Satellite Communications System, or TSAT, this was reduced to three. TSAT was cancelled in 2009 due to issues with its cost and delays in its development. A fourth AEHF satellite will be produced instead of TSAT, however reports of a fifth being planned are yet to be confirmed. The US Air Force currently describes AEHF as being a four-satellite constellation.

Saturday’s launch will use an Atlas V rocket, flying in the 531 configuration. This will be the first launch of the 531 configuration, and the twenty second launch of the Atlas V overall. The rocket which will be used for this launch is AV-019.

The 531 configuration consists of a payload fairing with a diameter of 5.4 metres, three solid rocket motors augmenting the first stage at liftoff, and a single-engined Centaur upper stage. For this flight, a short payload fairing, which has a length of 20.7 metres, will be used.

The Atlas V is, along with the Delta IV, one two rockets developed as part of the United States Air Force’s Evolved Expendable Launch Vehicle (EELV) programme. It made its maiden flight in 2002, successfully orbiting the Hot Bird 6 spacecraft for Eutelsat. Of its twenty one launches to date twenty have been successful, and one resulted in a partial failure.

That partial failure occurred on AV-009, carrying the USA-194 spacecraft, and was caused by a valve failing to close and allowing liquid hydrogen to leak from the upper stage. The spacecraft were placed into an incorrect orbit, but were still operable.

The Atlas V’s first stage, the Common Core Booster (CCB), is propelled by an RD-180 engine which is produced by NPO Energomash of Russia. The RD-180, which is derived from the RD-170 engine originally developed for the Energia and Zenit rockets, burns RP-1 propellant and uses liquid oxygen as an oxidiser. It will ignite at T-2.7 seconds, and 1.9 seconds later it will reach its expected thrust level for launch.

The three Aerojet solid rocket motors will ignite once the engine reaches full thrust, and at T+1.1 seconds the AV-019 will lift off. Five seconds into the flight, it will begin a series of roll, pitch and yaw manoeuvres to attain the proper trajectory for its ascent to orbit. The pitch and yaw manoeuvres will last around fifteen seconds, with the roll manoeuvre lasting twenty seven seconds.

Thirty four seconds into the flight, AV-019 will throttle down to pass through one of two areas of maximum dynamic pressure, or max-Q. It will throttle back up to full thrust nine seconds later, and one second later dynamic pressure will peak again. Ninety one seconds into the mission, the solid rocket motors will burn out; two will separate twenty three seconds later, with the third separating two seconds after those.

At two hundred and seven seconds after launch, the payload fairing will be jettisoned. It will fall into the Atlantic and is not expected to be recovered, however on the previous flight, which carried the first X-37B spacecraft, part of the fairing washed ashore in South Carolina and has since been put on display in a local museum. Six seconds after the faring separates, the forward load reactor, a device used to dampen vibrations within the fairing, will follow suit.

Booster Engine Cutoff (BECO), the extinction of the first stage, will occur 257 seconds into the flight, and will be followed six seconds later by the separation of the first stage. The Centaur’s RL10A-4-2 engine, which is cryogenically fuelled – burning liquid hydrogen oxidised by liquid oxygen, will ignite ten seconds after separation beginning its first burn. This burn will last nine minutes and thirty five seconds, and will precede an eight minute, nine second coast phase.

Following the coast, the Centaur will restart for a second burn, which will last five minutes and twenty seconds. This second burn will end twenty seven minutes and thirty seven seconds after launch, and will conclude the powered phase of the flight.

Following the end of its powered flight, AV-019 will coast for twenty three minutes and twenty three seconds before the AEHF-1 spacecraft will separate. The orbit at separation is expected to be a geosynchronous transfer orbit, with a perigee of 191.5 kilometres, an apogee of 35,786 kilometres, and 27 degrees of inclination. The argument of orbit’s perigee will be 180 degrees.

From this orbit, AEHF will raise itself to its operational geosynchronous orbit using what is believed to be a LEROS-1C apogee motor. The spacecraft also carries Hall Effect thrusters, which are ion engines that will be used for stationkeeping.

The launch of AV-019 will occur from Space Launch Complex 41 at Cape Canaveral, a complex which was originally built in the 1960s for use by the Titan family of rockets. It was first used for a Titan IIIC launch in December 1965, and was subsequently used for Titan IIIE and Titan IV launches, the last of which was a failed attempt to launch a Defense Support Program satellite in April 1999.

Following this launch, the complex was demolished and rebuilt to support Atlas V launches, and today’s will be the twentieth Atlas launch from the pad.

The complex follows the “clean pad” concept, with the rocket being assembled off-pad, atop a Mobile Launch Platform in the Vertical Integration Facility. Rollout of AV-019 to the launch pad was completed on Friday. Following its arrival at the pad, connections such as fuel and electrical supplies were connected to the platform, which will supply them to the rocket.

This is the third Atlas V launch of 2010, following that of the Solar Dynamics Observatory in February, and the first X-37B mission in April. The next Atlas V launch is scheduled to occur in September, when an Atlas V 501 will conduct NRO Launch 41, orbiting a classified payload for the US National Reconnaissance Office.

Another launch is currently scheduled for November, and will carry the GPS IIF SV-2 navigation satellite. United Launch Alliance is also expected to carry out two more Delta launches before the end of the year, both of which are currently scheduled for October.

A Delta IV Heavy will be used to conduct NRO Launch 32, carrying another classified payload, and a Delta II 7420 will launch the COSMO-4 radar imaging satellite for the Italian space agency and ministry of defence. The next launch of an AEHF satellite is currently scheduled for February 2011, and will also use an Atlas V 531.

Lead photo by Alan Walters – used with permission.

pixelstats trackingpixel

Related posts:

  1. Atlas V launches classified PAN satellite for US Government A United Launch Alliance Atlas V rocket has launched with PAN,…
  2. LIVE: ULA Atlas V launches WGS-2 for USAF United Launch Alliance (ULA) has launched the WGS-2 satellite on…
  3. Atlas’ 600th Mission launches with DMSP F18 from Vandenberg After nearly 52 years of venerable service to the United…

Both Crawler Transporters grounded – Crawlerway testing for HLV capability

Posted on 13th August 2010 by admin in Space Flight

The two veteran Crawler Transporters (CT) are currently grounded, as evaluations continue into a what is believed to have been a lightning strike on CT-2 – which was being prepared for tasks associated with the Ares I Mobile Launcher (ML). Test results are also being evaluated into how the Crawlerway is expected to perform under the weight of a Heavy Lift Launch Vehicle (HLV).

CT2 Incident:

The two 3,000 ton tracked vehicles have a storied history, responsible for carrying the NASA fleet of vehicles from the Vehicle Assembly Building (VAB) to the launch pads, ever since the Saturn IB and right through to today’s Space Shuttles.

The CTs would live on past the end of the Shuttle era, by transporting Ares I – after successfully debuting with the Ares I-X test vehicle – or a proposed Shuttle Derived Heavy Lift Launch Vehicle (SD HLV).

With at least two more shuttle missions to go, the Constellation Program (CxP) added a task that was set to take place ahead of STS-133′s rollout – to weigh and relocate the newly constructed Ares I ML.

The Ares I ML test and relocate involves both CTs – with the ML being weighed by the Crawler Transporter (CT-1) at its current location at the Mobile Launcher Platform (MLP) refurbishment site, while CT-2 works in tandem by freeing up the new location by moving MLP-1 to the VAB.

CT-1 will then move the Ares I ML the relatively short distance to its new home at the east refurb site, where it will be lowered down on to mounts. The entire operation – which was scheduled for late August – would be spread out over five days.

However, CT-2 was recently struck by lightning – it is believed, though still under an official investigation as to an exact root cause – after the recently installed special electrical equipment was damaged. The issues with the CT were found after a recent checkout, with problems associated with the control boards for the servo valve on the gel system. The repair work will take around four to six weeks.

“Crawler Transporter-2: Engineering is evaluating an issue with all eight of the Jacking Equalization & Leveling (JEL) servo valves,” noted the NASA Test Director (NTD) in an opening report on the problem (L2). “The four electronic control boards for these valves were removed and sent to the Malfunction Lab for evaluation.

“The Servo valves (have been removed) and valves shipped to the Vendor for evaluation and rebuild. Turnaround estimate is 4-6 weeks. A timeline is being built of events/tasks that have taken place on CT-2 from 1 April through 31 July. Included are: PM’s, repairs, welding, lightning events, and anything else that may help explain the event. Investigation continues as to possible causes of the failure.”

“The investigation continues with further troubleshooting as to the possible cause of the failures,” added a later update. “The failure analysis lab has been asked to do some additional analysis on the circuit cards to look for any data that would support a lightning strike or power supply failure.”

With CT-2 under investigation, CT-1 has also been grounded for the interim. However, it is likely the results of the lab testing will allow for the release of CT-1 in time to support STS-133′s rollout from the VAB, currently scheduled for September 28.

“Once all parts are received back from the vendor and re-installed, testing will be performed to verify no other CT systems were affected,” added the latest NTD update. “The use of CT-1 is currently being constrained by the CT-2 investigation. CT-1 may be released back into service when the failure analysis of the control cards is completed.”

Crawlerway Testing for HLV:

The home track of the CTs is also undergoing a study, as the prospect of a HLV riding down the crawlerway sooner than outlined in the FY2011 budget proposal increasing as the political refinements move forward.

Under what is still the current Program of Record (POR), Ares I is/was to be joined by Ares V – Constellation’s HLV. The Ares V program was rumored to be considering a larger type of Super Crawler, with six tracks, to carry the Ares V to the pad. (Left: Notional image based on early L2 information).

However, the first references to the challenge of ensuring such a heavy vehicle – one with two full fuelled five segment Solid Rocket Boosters (SRBs), as opposed to solely liquid-fuelled vehicles, tanked after arriving at the pad – were provided in this week’s review of construction at the Kennedy Space Center (KSC).

“Study involves testing of various crawlerway rock surfaces to better understand the feasibility of operating a tracked transporter for a heavy-lift program,” noted KSC Construction’s August presentation (L2). “Similar testing was last conducted in the mid-1960s in support of the Apollo Program.”

Initial testing has already been completed on an area of crawlerway just outside of Constellation’s Pad 39B, via a strange looking contraption which aimed to test the impact of over 25 million pounds on the rock surface of the track.

“This compatibility testing was conducted on the crawlerway just outside of LC-39B and was performed at the equivalent anticipated Ares V rollout weight of 25,200,000 pounds versus the Shuttle/Apollo rollout weight of 18,000,000 pounds,” added the presentation.

“Testing results will provide degradation characteristics, rate of deterioration, expected lifecycle of various materials, coefficients of friction and reaction forces exerted upon a crawler-transporter shoe.

“Several surfaces were tested and included rock expected to be optimal for a tracked transporter, rock anticipated to be optimal for a dual-use crawlerway (supporting both a tracked and wheeled transporter), and resilient surfaces targeted to reduce excessive loading of a crawler shoe as it crosses roadways and VAB transitions.”

The findings of the testing, which was conducted by NASA, the United Space Alliance (USA), Architect and Engineering firm Jones Edmunds and Associates (JEA) and a couple of additional contractors, are expected sometime in September. Additional testing will take place, with STS-133′s rollout also aiding the results.

“Testing and site demobilization at LC-39B are now complete, with a report from JEA targeted for September 2010, although there are plans to conduct some additional testing and instrumentation of the crawlerway during the next shuttle rollout,” added the notes.

The iconic 100-foot wide double pathway is made up of a seven foot deep bed of stones, which lies beneath a layer of asphalt and a river rock surface. The surface requires constant maintenance to ensure the smooth passage of the Shuttle during its ride on the CT to the pad.

The latest construction news noted that a major project will be undertaken to repair areas of crawler that lead up to Pad 39A, requiring 32,000 tons of the specialised Alabama river rock to be used.

“This project involves removing and replacing the severely degraded river rock along the surface of the LC-39 crawlerway from Ordnance Road to the Pad A surface. The uniformly rounded river rock surface provides the necessary cushioning and low-friction coefficient characteristics that are critical to all crawler-transporter operations,” added the presentation.

“While the crawlerway foundation includes a minimum of 3 feet of compacted limestone, the minimum depth of the rock surface varies between just 4 inches on the crawlerway straight sections to 8 inches on the curves. The estimated total amount of new rock necessary to complete this project is 32,000 tons.

“All the excavated rock is being stockpiled at the Diverted Aggregate Reclamation and Collection Yard (DARCY) site within the landfill and will be screened into separate piles of fine and larger rock for future reuse throughout KSC as decorative borders, road base and crawlerway repairs.”

Other major work is also listed, including news that Pad 39B will undergo major demolition work, as planned via the Constellation Program. Sources note this work is likely to be placed on hold due to large costs. An article will be published when inquires into the project’s status are addressed.

pixelstats trackingpixel

No related posts.

Large success for second EVA as failed Pump Module is removed

Posted on 12th August 2010 by admin in Space Flight

Following the eventful first Station EVA to remove and replace a failed ETCS (External Thermal Control System) Loop A PM (Pump Module), ISS crewmembers Tracy Caldwell-Dyson and Doug Wheelock once again ventured outside the ISS for the second of now three planned EVAs to bring the Station’s cooling system back to full operating capacity following the failure of the Loop A ammonia PM on July 31. The EVA was a big success.

ETCS Loop A NH3 Pump Module Failure Background:

On July 31 at ~20:00 EDT (00:00 GMT) the ETCS Loop A NH3 PM experienced a failure, effectively disabling half of the International Space Station’s critical cooling system.

The ETCS, which operates on two separate loops (Loop A and Loop B), contains one PM each.  The pumps are responsible for moving NH3 (ammonia) through the radiators, electrical boxes, and heat exchangers to facilitate the “dumping” of heat generated by the Station’s numerous systems and experiment racks.

When the Loop A NH3 PM failed on July 31st, the entire cooling system on the Loop A portion of the ETCS shut down due to an inability to move ammonia through the cooling lines.

As a result, station crewmembers, led by Caldwell-Dyson and Doug Wheelock began deactivation various station systems and experiments to prevent overheating. The crew installed jumpers to regain some cooling and data redundancy.

However, several systems (specifically experiments) are still shut down and cannot be reactivated until the Loop A PM has been replaced and full operational capability has been restored to Loop A of the ETCS.

According to NASA, a loss of science and scientific data has been an unfortunate but unavoidable result.

EVA-1 Problems:

As is a natural part of all human endeavors, things don’t always go according to plan. Based on the original two EVA plan to R&R and the failed Loop A ammonia Pump Module, EVA-15 (the first EVA of the R&R effort) was supposed to remove the nonfunctional ETCA Loop A PM and begin work on the new pump currently stockpiled on the outside of the ISS.

According to NASA, “EVA-16, on 8/11 (Wednesday), is being extensively & thoroughly re-planned as a result of the disappointing outcome of EVA-15 which failed to get the nonfunctional ETCS Loop A PM out and start work on the new pump.”

Wheelock and Caldwell-Dyson were unable to complete all the planned procedures during the record breaking stage EVA (no shuttle at station) due to a “significant” leak at the M3 QD (Quick Disconnect) at the failed Loop A PM.

The leak was first noticed during the initial attempt to remove the M3 QD. Once the leak was noticed, a QD bail was cycled but failed to resolve the leak. Furthermore, after cycling the QD bail, the detent button was found to be jammed – the button would not depress despite several attempts to manually manipulate the button.

Wheelock and Caldwell-Dyson were then instructed to continue with the removal of the next two QDs – which were both removed without any issue or leakage.

Caldwell-Dyson and Wheelock then returned to the M3 QD and attempted to release the stuck detent with the use of a hammer. After a few taps, the detent was successfully depressed and “the crew proceeded with closing the QD,” NASA stated.

However, this procedure resulted in the leakage of approximately 3 lbs of ammonia to space from the QD. The leak was quickly isolated to the system side of the PM due to a decrease in system pressure.

Because the system configuration prevents the stoppage of a leak from the “female” side of the jumper, Caldwell-Dyson and Wheelock were instructed to reattach the QD and reopen the QD valve – a procedure which stopped the leak.

At 8 hours 3 minutes in duration, this was the longest Stage (without the Shuttle present) EVA in ISS history.

Nonetheless, the QD ammonia leak was not the only issue faced during Wednesday’s EVA (EVA-15). A malfunctioning CO2 (Carbon Dioxide) sensor in Doug Wheelock’s EMU (Extravehicular Mobility Unit) also cropped up during the spacewalk.

As of Monday, “The CO2 sensor which failed in Wheels’ suit [had] not yet been recovered.” Steps to recover the sensor were still being discussed/implemented. One of these procedures included airing out the spacesuit by leaving it exposed to the ISS atmosphere to facilitate the drying out of the sensor – though there was no guarantee that that procedure would work.

Another potential method for recovering the failed sensor involved R&Ring in the HUT to “get a clean sensor.” However, this procedure has never been performed in orbit and would have required the dedication of two ISS crewmembers for over 8 hours.

Moreover, “Even if this is done, there’s no reason to believe we would not also fail the new sensor during an EVA.  Therefore we do not plan to perform a HUT R&R for Wheels’ suit,” noted NASA.

As such, a plan was developed to go into the second EVA assuming Wheelock’s CO2 sensor is failed or would fail during the course of the EVA should the sensor be recovered.

Overall, the crew was reported to be in good spirits with good cooperation and help from all six ISS crewmembers.

“Crew spirits are good, Russians helping and available to help.  Ground folks are 24/7 and doing tremendous things.  All are watching for fatigue etc. but are conscious of the calendar timeline risks we have until the system is restored.”

EVA-16 (Second EVA) Preparations:

As part of the final preparations for EVA-16, Tracy Caldwell-Dyson and Doug Wheelock spent Tuesday configuring the tools they will use on today’s spacewalk as well as reviewed last minute timeline/procedure updates and tech manuals.

According to the Aug. 10 Status Report, “FE-2 Tracy Caldwell-Dyson & FE-4 Doug Wheelock completed final preparations for tomorrow’s EVA-16.

Activities included “configuring tools needed during the spacewalk such as equipment tethers, wire ties, etc., and making further preparations in the A/L EL (Equipment Lock), checking on PGTs #1001 w/battery 1009 for EV-1, PGT #1006 w/battery 1008 for EV-2, backup PGT #1004 w/battery 1006 in bag), filling DIDBs (Disposable In-suit Drink Bags) from PWD (Potable Water Dispenser), and verifying installation of HL (Helmet Light) batteries (1029, 1030, 1031 &1035).”

After these activities were complete, Caldwell-Dyson and Wheelock were joined by fellow NASA astronaut Shannon Walker (FE-6) for a three (3) hour review of the latest EVA procedures, included updates to the Robo/SSRMS (Space Station Remote Manipulator System) instructions.

Meanwhile, and in addition to a teleconference between the three NASA astronauts and EVA specialists in MCC-Houston, Doug Wheelock attempted to restore functionality the failed CO2 sensor in his EMU.

“In an attempt to restore the failed CO2 sensor in Doug’s EMU#3005, Doug set up the sensor to flow O2 through it for an hour to remove the suspected moisture, and then check the sensor’s functionality,” notes Tuesday’s On-Orbit Status report.

The procedure was successful and the CO2 sensor is working and deemed “OK” for EVA-16.

Further preparations included the installation of one Russian “Pille-MKS” radiation dosimeter into each of the two EMUs to be used for EVA-16.

“Working with Doug, FE-3 Mikhail Kornienko retrieved three Russian “Pille-MKS” radiation dosimeters, recorded their dosages in the Reader and equipped each of the two EMUs for tomorrow’s spacewalk with a sensor unit (A0306 & A0307),” states the status report.

Finally, Shannon Walker – Robo/SSMRS operator for EVA-16 – reviewed all uplinked materials regarding Ammonia decontamination procedures should they be needed at the end of the spacewalk.

Walker also verified the readiness of all hardware that will be required for today’s spacewalk as well as configured the Cupola Robotic Workstation as a backup for the necessary SSRMS ops, replaced the Dynamic Onboard Ubiquitous Graphics (DOUG) cable from the A31p laptop used for EVA-15 to Station Support Computer-8, and confirmed proper receipt of telemetry from the Robotics systems for “driving” the DOUG animation during EVA-16.

Walker also deactivated the amateur radio equipment in the Service Module in order to prevent any RF interference during the spacewalk and closed the protective shutters on the Cupola and Destiny and JEM PM labs.

Caldwell-Dyson and Wheelock then began their EVA campout procedures at around 3:55p.m. EDT Tuesday, August 10 when they began a ~1-hour 5-minute oxygen mask prebreathe. Around this time the Quest Airlock (A/L) hatch was closed and the A/L depressurized from the standard 14.7 psi to 10.2 psi.

 The spacewalking duo then went to bed around 5:30p.m. EDT. Tuesday before awaking around 2a.m. EDT to begin final spacewalk preparations. The Quest A/L was then temporarily repressurized to allow Caldwell-Dyson and Wheelock a masked hygiene break from ~2:35a.m. EDT to ~3:35a.m. EDT

Shannon Walker then provided suited support in the Airlock beginning at ~3:45a.m. EDT. Also at this time the A/L hatch was closed and the A/L once again depressurized to 10.2 psi (from ~3:45a.m. EDT to 5:15a.m. EDT).

EMU suit purge followed from ~5:15a.m. EDT to 5:30a.m. EDT with spacesuit prebreathe occurring between ~5:30a.m. to 6:20a.m. EDT.

Caldwell-Dyson and Wheelock then maneuvered in the C/L (Crew Lock) where the final depressurization sequence occurred – with Walker supporting C/L depressurization until Caldwell-Dyson and Wheelock egressed to begin the EVA.

EVA-16 Overview:

For EVA-16 Doug Wheelock (EV-1) and Tracy Caldwell-Dyson (EV-2).  officially began  the spacewalk at 7:27am Central time.

After egressing the A/L, Wheelock retrieved the Vent Tool Extender (VTE) while Caldwell-Dyson translated to the PM worksite (referred to as Step 1 in the EVA-16 timeline overview).

By this time, the pressure inside the Loop A NH3 system was already lowered from 370 psi to ~200 psi to prevent as rapid a leak as seen during EVA-15, should the leak reoccur – which it didn’t.

Once Caldwell-Dyson was joined by Wheelock, Wheelock performed Step 2 – closing the M3 QD. 

Once the QD was closed, one of two procedures/timelines were open to the spacewalkers. If no leakage (or ‘snowflakes’) are observed then Step 4 of the EVA-16 timeline will be skipped – an event that could save ~2 hrs of EVA time – and the M3 QD left closed for the remainder of the EVA.

If a leak is detected, Wheelock will re-open the M3 QD to 90% using the Spool Positioning Device (SPD).

Small amounts of “snowflakes” were observed, but nothing to the levels seen during the opening EVA. The main problem came when Wheelock tried to remove the QD – which refused to budge.

After being given permission to “violently” shake the QD, in order to remove potential ice from hindering its removal, Wheelock’s brute force resulted in success, as the QD came loose. 

Wheelock then closed Male 1/Female 105 QD at the S1-to-S0 interface, while Caldwell-Dyson’s closing of the M1/F105 QD at the S1 DC to DC Conversion Unit wasn’t required.

With venting requirements also not required, Caldwell-Dyson released the non-functional PM electrical and data cables as well as releasing three bolts.

Meanwhile, Wheelock retrieved an Adjustable Grapple Bar (AGB) from External Stowage Platform 2; before the spacewalking duo attached the AGB to the failed PM. This proved to be slightly problematic, although they were already way ahead in the timeline, thanks to the lack of leaking from the M3 QD.

Under Step 13 of the scheduled timeline, Wheelock and Caldwell-Dyson removed the failed PM from the S1 truss and stowed it to a Mobile Base System (MBS) Payload ORU Accommodation (POA) at Worksite 2 where it will remain for an indefinite period of time.

With those procedures complete, Wheelock and Caldwell-Dyson had the option to perform three get ahead tasks for EVA-17 (the third EVA in the Loop A NH3 PM R&R effort).

These get ahead tasks include (in the order listed by NASA): C/L bag transfer to External Stowage Platform 2, venting of GN2 (gaseous nitrogen), and the breaking of torque bolts on the spare PM to be used during EVA-17.

Both spacewalkers made their way to ESP-2 to work on the new Pump Module, where it was decided they would not break the torques, but instead remove insulation tape and remove three of the electrical connections.

Following clean up tasks, the duo ingressed Quest to end a highly successful EVA at a total duration of 7 hours and 23 minutes.

pixelstats trackingpixel

No related posts.

Payload planning pre-empts an imminent NASA decision on STS-135

Posted on 12th August 2010 by admin in Space Flight

A decision to change Atlantis’ upcoming mission call sign from STS-335 to STS-135 – at least at the full planning level – is expected “shortly”, as Shuttle mission-related departments pre-empt the official go-ahead by building up their plans to finalize the payloads that would fly on the notional June, 2011 mission.

STS-135 Planning Latest:

Still officially tagged as STS-335 – the Launch On Need (LON) support for Endeavour’s STS-134 mission – the change to STS-135 would be taken by NASA’s administration, in conjunction with Space Operations Mission Directorate (SOMD).

The Space Shuttle Program (SSP) in Houston would then take the mission forward in planning, by baseline the flight via the Flight Definition and Requirements Directive (FDRD) process at the Program Requirements Control Board (PRCB) level.

A large amount of preliminary planning has already been undertaken, such as aligning the best potential launch date – currently classed as June 24, 2011 – which would maximize the benefits of the orbiter’s unrivalled upmass and downmass ability in order to leave the International Space Station (ISS) in the best possible logistical condition ahead of the debut CRS (Commercial Resupply Services) vehicles arriving at the orbital outpost.

A mission outline has also undergone an initial development cycle, calling for a four person crew flying on a 11+1+2 mission, with the support of a Soyuz LON plan in the highly unlikely event Atlantis was damaged to a point she was unable to return to Earth.

STS-335/135 Specific Articles: http://www.nasaspaceflight.com/tag/sts-135/

A major boost for adding STS-135 was recently received at the political level, with the popular Senate refinements to the FY2011 NASA budget proposal including direct authorization for the additional mission, now mirrored in the House version’s amendments – providing NASA is comfortable with required safety assessments.

While the Senate version aids the full approval of STS-135 by tasking the NASA Engineering and Safety Center (NESC) with the safety assessment, the House version calls for the Aerospace Safety Advisory Panel (ASAP) to carry out the overview – a body that has previously gone on record to oppose any form of extension of the shuttle manifest.

Those comments were made by ASAP’s chief Admiral Joseph W. Dyer, who claimed shuttle was becoming “more riskier,” when discussing the initial findings of the Augustine Review to a related House hearing last September.

The Admiral’s comments were retorted by SSP manager John Shannon, who said the remarks were “disturbing”, before adding “we are flying safer now, and have a better safety culture and integrated team approach with many checks and balances to ensure that we are flying as safely as absolutely possible.”

Mr Shannon’s factual remarks may have hit home with the ASAP, who have since changed their position to give their approval for STS-135 to fly.

“(NASA) briefed the ASAP on flying STS-335 (LON) as a logistics mission to Station in June 2011. All feedback indicates that both informally and formally, they approve. Working with the NESC to do a review of the draft language,” noted comments made on a July Shuttle Standup/Integration report (L2).

“They are looking at three items: Whether ISS has the capability to support the crew on board should there be a contingency, and additional risks not thought through, and any recommendation they might have for the Agency accepting the risk for this additional flight.”

The contingency support is a key area that requires the cooperation of the Russians, with numerous factors under consideration for the inclusion of a solid Soyuz rescue plan.

Firstly, if Atlantis did suffer from a major event, resulting in her inability to return, the four person STS-135 crew would need to take up residency on the ISS until they could return – two at a time – with a Russian cosmonaut on a returning Soyuz.

Secondly, Expedition crewmembers would have to give up their seats on the returning Soyuz, likely extending their stay on the Station to one year.

At present, Soyuz TMA-22 is set to launch to the ISS in September, 2011 for an ISS crew rotation. Another Soyuz is set to launch in November, 2011 – which will be the first of a new series of the veteran vehicle, designated Soyuz TMA-03M.

It is also highly unlikely an additional Soyuz could be added into the mix to ease such timelines, with the next two Soyuz vehicles scheduled to launch after TMA-03M due to lift-off in April and June, 2012 - and no more Soyuz’s are in production to launch prior to 2013.

Technically, the Soyuz plan could work, but numerous elements of planning would requirement refinement, such as the Contingency Shuttle Crew Support (CSCS) levels on the ISS, in order to ensure a ‘stranded’ STS-135 crew wouldn’t cause a major strain on Station consumables, especially considering they’d represent the final shuttle mission to visit the ISS, and thus no major replenishment could be arranged via another orbiter – as much as STS-135′s own payload boost would “cover their backs”.

Providing contingency support can be secured and deemed acceptable, the benefits of taking advantage of the flight hardware already being prepared for STS-335 will provide the ISS with a very welcome boost.

The latest notes from the Johnson Space Center’s (JSC) Flight Operations and Integration department point towards the ISS becoming the major beneficiary from the additional mission, more so when taking into account the recent Pump Module (PM) failure on the External Thermal Control System (ETCS) “Loop A”.

Those latest notes point to a preference to launch and/or return two Orbital Replacement Units (ISS) being noted by ISS manager Kirk Shireman.

“If the STS-335 mission becomes STS-135, Kirk Shireman decided not to pursue putting on the Goddard Technology demos; these are already manifested on another vehicle,” noted a recent Standup report.

“His recommendation is to fly the LMC (Lightweight Multi-Purpose Carrier) with two empty FRAMs (Flight Releasable Attachment Mechanism) that would support an ‘as needed’ launch or return of two ORUs. Are investigating whether this could be done.”

With the failed PM currently unable to return on either STS-133 or STS-134, and no current ability to return such hardware on one of the unmanned resupply vehicles, STS-135 would provide an opportunity for engineers on the ground to get their hands on the equipment, allowing for a vital root cause investigation into its failure to take place.

It is not currently known which two ORUs are top of the ISS’s priority list for a ride on the notional STS-135, or which other ORU – assuming the PM is indeed a major return priority – is requiring a trip home, although Atlantis’ main payload would be via the huge upmass of the MPLM (Multi-Purpose Logistics Module) – which is already baselined into STS-335 as a CSCS replenish requirement, in the event of being called up to support STS-134.

Another sign of management continuing their planning ahead of a NASA HQ decision on STS-135 was seen just last week, when the Flight Operations and Integration department once again noted key mission-related organizations are working through the pre-emptive path towards the mission’s approval.

“JSC-MO (Mission Operations) will organize a meeting with SSP and ISS teams to get an understanding of what would be on STS-135 if it were to become a real mission in terms of both the elements and the objective,” added the recent Standup note.

An official decision on taking STS-135 forward is expected this month, due to crewmember training (crew loading) and mission planning timeline requirements.

pixelstats trackingpixel

No related posts.

China launches military satellite YaoGan Weixing-10

Posted on 12th August 2010 by admin in Space Flight

Continuing what is expected to be a launch surge for the second half of 2010, China has launched a new remote sensing satellite on Tuesday, the sixth Chinese launch this year. YaoGan Weixing-10 was launched via a CZ-4C Chang Zheng-4C (Long March) launch vehicle at 06:49 local time on August 10 from the Taiyuan Satellite Launch Center.

Chinese Launch:

According to the Chinese media, the new satellite is intended for “scientific experiments, land survey, crop yield assessment, and disaster monitoring.” As was the case for previous launches of the YaoGan Weixing series, Western analysts believe this class of satellites is being used for reconnaissance and military purposes.

The previous satellite in the series, YaoGan Weixing-9, was launched March 5th from the Jiuquan Satellite Launch Center by a CZ-4C Chang Zheng-4C launch vehicle, the same launch vehicle used to launch YG-10.

YaoGan Weixing-9 was made up of three such satellites in orbit, flying in formation to form what appears to akin to a type of Naval Ocean Surveillance System (NOSS).

The ‘YaoGan Weixing’ designation appears to be used in a similar fashion to that of the old Soviet ‘Cosmos’ designation, hiding the true mission of the vehicles launched into orbit.

The first YaoGan Weixing satellite (29092 2006-015A) was launched by a CZ-4C Chang Zheng-4C (CZ4C-1) from the Taiyuan Satellite Launch Center on April 27, 2006. At the time the details about that satellite were closely guarded, before claiming it was the first Jian Bing-5 satellite, equipped with the first space-based Synthetic Aperture Radar (SAR).

Next up was the YaoGan Weixing-2 (31490 2007-019A) was launched on 25 May, 2007, by a CZ-2D Chang Zheng-2D (CZ2D-8) from the Jiuquan Satellite Launch Center. Details were also restricted, though it is claimed that the spacecraft was an electro-optical military observation satellite, complementing the results of the YaoGan Weixing-1.

This was followed on November 12, 2007, the YaoGan Weixing-3 (32289 2007-055A) satellite was launched by a CZ-4C Chang Zheng-4C (CZ4C-2) launch vehicle from Taiyuan. This satellite was noted as the second Jian Bing-3 SAR satellite.

On December 1, 2008, YaoGan Weixing-4 (33446 2008-061A) – the second electro-optical satellite on the series – was launched by a CZ-2D Chang Zheng-2D from Jiuquan, and on December 15, 2008, YaoGan Weixing-5 (33456 2008-064A) was launched by a CZ-4B Chang Zheng-4B (CZ4B-12) from the Taiyuan Satellite Launch Center – believed to be the fourth SAR bird on the series.

Finally, YaoGan Weixing-6 (34839 2009-021A) was launched by a CZ-2C Chang Zheng-2C-III from Taiyuan on April 22 this year – the fifth SAR satellite.

YaoGan Weixing-10 was launched by a CZ-4C Chang Zheng-4C launch vehicle that is a optimized version of the CZ-4B Chang Zheng-4B using an upper stage with restart capability and a new interstage adapter between the first and second stages.

This launch was the 128th Chinese orbital launch, the 30th orbital launch from the Taiyuan Satellite Launch Center, and the first orbital launch from Taiyuan this year. This was the sixth use of a CZ-4C Chang Zheng-4C launch vehicle.

Situated in the Kelan County on the northwest part of the Shanxi Province, the Taiyuan Satellite Launch Center is also known by the Wuzhai designation. It is used mainly for polar launches (meteorological, Earth resources and scientific satellites).

The launch center is equipped with a Mission Command and Control Center, a Technical Center and telemetry, tracking and communications centers. There are two launch complex buildings in Taiyuan.

The first orbital launch from Taiyuan took place on September 6, 1988 when the CZ-4 Chang Zheng-4 (CZ4-1) rocket launched the first FY-1A Feng Yun-1A (19467 1988-080A) meteorological satellite.

China plans to launch its second lunar probe, Chang’e-2, next October. The probe will be launched by a CZ-3C Chang Zheng-3C launch vehicle from the Xi Chang space center and before the end of the year is planned the launch of the FY-3B Feng Yun-3B meteorological satellite.

The Chinese schedule for the rest of the year includes the launch of at least another remote sensing bird, the launch of Chinasat-6A communications satellite, the launch of the ST-1B Shen Tong-1B / ZX-20 (2) ZhongXing-20 (2) military communications satellite and the launch of two more BeiDou navigation satellites.

Next year will see the launch of the TG-1 TianGong-1 space module. TiangGong-1 is expected to accomplish the country’s first space docking and is regarded as an essential step toward building a space station.

Weighing about 8.500 kg, TianGong-1 will be able to perform long-term unattended operation, which will be an essential step toward building a space station.

The unmanned Shenzhou-8 spacecraft will achieve China’s first space docking. The docking maneuvers are going to be controlled from the ground. Shenzhou-9 and Shenzhou-10, the two other spaceships to dock with Tiangong-1, would carry a crew of two or three.

TG-1 TianGong-1 is going to be launched by a modified CZ-2F Chang Zheng-2F launch vehicle, sometimes referred to as CZ-2F/G Chang Zheng-2F/G, sporting 170 technological modifications, including 38 major refinements.

China is also advancing on the development of the CZ-5 Chang Zheng-5 series of launch vehicle with the building of a launch vehicle production base in the northern municipality of Tianjin. This development has a total investment of 10 billion yuan and covers an area of more than one million square meters.

The base will be capable of producing 12 launch vehicles a year, and after the first phase of construction is completed in 2011, the base will be able to produce two launch vehicles.

Earlier reports point to the first launch of the CZ-5, with a maximum payload capacity of up to 25,000 kg, in 2014.

pixelstats trackingpixel

Related posts:

  1. China launch remote sensing satellite Yaogan-4 – with potential military use China has launched a new remote sensing satellite from the…
  2. Chinese launch again with YaoGan Weixing-6 remote sensing satellite China has launched the YG-6 YaoGan Weixing-6 remote sensing satellite…
  3. China launch YaoGan Weixing-9, announce increase in vehicle production China has launched a new “remote sensing” spacecraft – actually…

Opening ISS spacewalk to replace coolant pump completed

Posted on 9th August 2010 by admin in Space Flight

NASA’s Doug Wheelock and Tracy Caldwell Dyson have completed their eventful opening EVA to changeout a failed ammonia coolant Pump Module (PM) on the International Space Station’s (ISS) External Thermal Control System (ETCS) “Loop A”. Lasting eight hours and three minutes, the spacewalk will be followed by a second EVA next Wednesday.

EVA-1:

The main task of EVA-1 was to remove the current PM – which suffered from a power spike which tripped a circuit breaker on July 31 – and replace it with a spare during the second EVA next week. However, issues with one of the Quick Disconnect (QD) lines resulted in the old PM remaining in place for the meantime.

The ETCS provides cooling to the entire United States On-Orbit Segment (USOS). The ETCS consists of two independent loops, designated Loop A and Loop B – the latter of which is currently working without issue.

The system is designed to collect heat from the Internal Thermal Control Systems in the US Lab, Node-2, COL, JEM, and Node-3, via IFHXs (Interface Heat Exchanger). The PM provides the motive force to transport the ammonia around the loop.

The opening EVA was delayed twice, as engineers on the ground worked through refining the EVA timeline, while training runs were carried out inside the NBL (Neutral Buoyancy Laboratory) at the Johnson Space Center (JSC).

The EVA-1 tasks will run in the following order: “Demate connections and QDs (quick disconnects) on the old PM (Pump Module); Install PM jumper to bypass PM and connect ATA (Ammonia Tank Assembly) at S1 to Loop-A; Install AGB (Adjustable Grapple Bar), currently on ESP-2 (External Stowage Platform 2), on old PM.

“Remove old PM from S1 (starboard) truss and stow on POA (Payload ORU Accommodation) on the MT (Mobile Transporter) at WS2 (Worksite 2); Prepare spare PM (on ESP-2) for installation, and; Install spare PM on S1 and make electrical & data connections.”

Several leaks of ammonia – seen as snowflakes – were observed during the demating of QDs on the PM, half way through the EVA’s duration. However, the main issue was with one of the QDs that refused to demate.

With two alternative QDs demated with no issues, Wheelock returned to M3, which eventually released as planned – much to the pleasure of ground controllers, who burst out into applause. However, time was running out, leading to the removal of the PM being moved to EVA-2.

A larger leak of ammonia was then observed during M3′s demating, as the spacewalkers appeared to be working in a snowstorm, as the fluid leaked as flakes. Although no serious contamination was found during suit inspections, a 30 minute bake out inside the airlock ensured none of the hazardous material could return inside of the Station with the suits.

Ahead of Saturday’s spacewalk, the last US Stage EVA on the ISS was conducted in January, 2008.

Refer to the live thread for further details, and a review of the live play-by-play text and image coverage.

A Week Of Planning:

A large part of the evaluations have related to the Failure Investigation Team (FIT) efforts to overview what is known as the Next Failure Response – part of a week of extensive evaluations into supporting both the ISS and the EVAs.

“FIT for failure response actions dealt mainly with items related to supporting EVA with the next worst case failures that take down the 2nd cooling loop,” noted one a several expansive memos and overviews on the evaluations (L2).

“Actions that were noted for the crew include completing the EVA battery charging as soon as possible, looking for the adapter for the US LiOH cartridges for use on the Russian side, and when approval is gained from ISS Program management to request the crew to begin assembling materials to build a second contingency jumper via pin kits with the OGS jumper.

“The crew will need to be timelined appropriately to allow the associated hardware to be located for this spare jumper preconfiguration effort. Most of the discussion dealt with how to get the USOS configured to best support comm during an EVA since the Internal Audio Controller (IAC) required for UHF comm to the EV crew has a very short time to overheat (less than 30 minutes) that would result in the termination of the EVA.

“A scenario was discussed to recover cooling for an MBSU (Main Bus Switching Unit) failure but installation of power jumpers by the crew and thermal cooling reintegration would take approximately 1.5 hours. Improving air cooling via ducts, removing closeouts, and rotating racks was discussed where applicable to gain more thermal clock time.”

A long list of actions included work to determine the best configuration for removing closeout panels and rotating racks to ensure the best cooling capability in the modules, and bringing the spacewalkers safely back into the airlock – in the event of another failure before, during and after the opening EVA – full list on L2.

Other planning was dedicated to the EVA task, such as a pump module ammonia vent plan.

“The team had originally developed a pump module ammonia vent plan that could be completed using ground commanding of various isolation and vent valves in the ETCS,” added another overview.

“Due to the length of the tasks the crew would be required to perform during a single eclipse pass, coupled with a highly detailed choreography between the EV crew and ground to support this task there is no way to fit the necessary QD manipulations and Pump Module venting within a single eclipse period. 

“The team decided to proceed with the manual vent option which has no eclipse constraints but does require the crew to position and use the EVA vent tool. In support of this the nominal EVA 1 timeline will, in accordance with the Flight Rules, protect for 2 hours and 20 minutes of consumables at the end of the EVA for EMU decontamination protocols.

“In addition, an action was opened to analyse the requirement to vent the failed pump module during EVA1 or whether it can remain with NH3 in it until EVA 2.

Pending the results of this analysis, it may not be required to vent the PM during EVA 1 as long as the NH3 in the pump will not freeze and potentially prevent post failure analysis from determining what caused the original pump failure.”

A third EVA was being discussed on some memos during the week (L2), relating to an issue on a Remote Power Control Module (RPCM), which – it was feared – may have suffered from wiring damaged. By late this week, a third EVA to changeout the RPCM had become “less likely”.

A full overview of the status of the RPCM will be provided in the EVA-2 article.

pixelstats trackingpixel

No related posts.

STS-133: Discovery enters her final month of OPF processing ahead of rollover

Posted on 9th August 2010 by admin in Space Flight

With over 128 million miles on her clock, Discovery is now into the final month of her flow inside the Orbiter Processing Facility (OPF) for her 39th and final mission, as she prepares for rollover to the Vehicle Assembly Building (VAB) on September 8. Meanwhile, investigations are ongoing into the Reaction Control System (RCS) Test Article failure in New Mexico.

STS-133 Processing Latest:

Discovery is processing in OPF-3 for her November 1 launch to the International Space Station (ISS). STS-133 was set to be the final mission of the Space Shuttle Program (SSP) until payload problems resulted in a realigned manifest that pushed Discovery’s flight ahead of Endeavour’s heavily-delayed STS-134 mission.

In what is highly likely to be the veteran orbiter’s final processing flow for flight, the milestones of rollover and rollout will likely be marked by ceremonies that will be even more poignant than Atlantis’ STS-132 events – considering many observers were aware Atlantis already had one eye on an additional flight via the proposed STS-135 mission.

With just one more month of her OPF flow remaining, her dedicated engineers are seeing their own final milestones for the old girl, with the final closure of the Payload Bay Doors (PLBDs) upcoming this week – only to be opened one final time at the launch pad when she receives her payload.

“OV-103 (STS-133) Working on preps for PLBD closure, will close the PLBDs next week. Have some TPS (Thermal Protection System) work to do, then will cycle to final closure,” noted Ground Operations on the latest Shuttle Standup/Integration report (L2).

“Working preps for crew module leak checks to be performed tonight. Installing BRI tile on the ET (External Tank) doors. Working the valve position indicator (VPI) indicator on the O2 crossover valve, IPR-35 (Interim Problem Report), and will do some more troubleshooting on that.”

IPR 35 – relating to observations made during data reviews on the O2 system 1 crossover valve – found that the VPI indicated “on” when it should be indicating “off”. This issue remains under review.

“IPR 35 update: O2 system 1 crossover valve cycles (5) were performed.  When (engineering teams working the issue) returned (the) VPI state at power up had changed from the indication prior to orbiter power down. Troubleshooting indicates the valve is physically closed and the issue may reside with the VPI. Engineering evaluation continues,” noted the NASA Test Director (NTD) report (L2).

The NTD also noted other processing work being carried out on Discovery, including TPS operations that have been ongoing through the weekend, along with the closure of one of the early issues in the flow – IPR 5, the problem which was recently highlighted by cable issues.

“OV-103 (OPF Bay 3): Crew Module leak checks were completed and results were nominal. Nose Landing Gear boot repair was completed and RTV is in cure. IPR 5: finished troubleshooting the in-flight anomaly on the S-Band Antenna system. Were not able to duplicate the problem seen on-orbit and expects to close the IPR as an Unexplained Anomaly (UA).”

As per usual, managers will review the status of Discovery’s flow one week ahead of her scheduled rollover to the Vehicle Assembly Building (VAB) – which is currently on track for September 8.

STS-133 Specific Articles: http://www.nasaspaceflight.com/tag/sts-133/

“The Orbiter Rollout Review for STS-133 is September 1,” confirmed the KSC Launch Integration Manager on the Standup report. “On track from rollover to the VAB on September 8.”

There she will link up with External Tank (ET-137) and the twin Solid Rocket Boosters (SRBs) in High Bay 3 (HB-3) for mating operations. Repair work continues to be carried out inside the VAB on a Fairing Support Plate, following problems with the initial TPS work that was conducted over the last few weeks.

“SRB BI-144 / RSRM 112 / ET-137 (VAB HB-3): PR (Problem Report) ET-137: Damaged SLA (foam) on EB-2 Fairing Support Plate; Will Hand Pack both inboard and outboard. New SLA kit has been ordered and will arrive next week,” added the NTD.

“Aft Strut and HDP (Hold Down Post) Firing Line checks are complete. Forward Firing Line checks will be worked after ET Fairing is installed after SLA repair is complete on PR.”

RCS Test Article Failure Update:

The failure suffered by the RCS test article – otherwise known as the “Fleet Leader” – at the White Sands Test Facility (WSTF) remains under investigation, with the latest results scheduled to be reviewed by the Orbiter Project Office (OPO) this coming Wednesday.

Since 1989, the Fleet Leader Program has played a vital role in NASA’s ability to detect, predict, and prevent Orbital Maneuvering Subsystem (OMS) and RCS life-dependent failures and anomalies before they affect the shuttle fleet.

The New Mexico facility’s test article functional tests simulate orbiter flight and maintenance downtime period activities, and special propulsion subsystem tests, using all of the Fleet Leader test articles.

Other special tests have been performed to support the Fleet Leader Program, such as the OMS/RCS Crossfeed Line Gas Sweep Test (Test Stand 301), the Forward Interconnect System Test using FRCS Test Article (Test Stand 328), and Chamber Chiplife.

A problem during testing on the hardware was reported a few weeks ago, relating to a firing of the RCS fleet leader unit experiencing an unplanned controlled shutdown – a result of a large crack in a weld that is between the closeout of a fuel manifold and the injector.

The related hardware is being investigated via both Non Destructive Evaluations (NTE) techniques and more intrusive inspections, in order to understand the root cause.

“On the WSTF RCS test article investigation, the team has completed sectioning of the injector part that has the crack. Half of the part is being used for NDE development, and the other half for detailed destructive evaluation. The crack has been opened, and fractography is beginning,” noted OPO on the Standup report.

“Continuing to inspect the valve sensors, transducers and perform radiography. Also doing a chemical evaluation of what was flushed out of the thruster prior to the cut. There will be an OPO Tech Tagup next Wednesday to discuss all the known data.”

This issue will not impact STS-133′s upcoming Flight Readiness Reviews (FRRs) unless commonality with the fleet’s flight hardware is found.

pixelstats trackingpixel

No related posts.

NASA and Commercial industry combine to outline FTD Propellant Depot plan

Posted on 7th August 2010 by admin in Space Flight

A collaboration between experts at numerous NASA centers and commercial companies have created a plan for an “in-space LO2/LH2 PTSD (Propellant Transfer and Storage Demonstration) mission, to affordably support a 2015 demonstration and follow-on missions”, highlighting an exploration architecture built around existing vehicles and Propellant Depots.

PTSD Flagship Technology Demonstration:

Answering a Request For Information (RFI) in June, a broad range of NASA, other US government, academic and industrial participation resulted in a roadmap to enable a flagship demonstration mission of propellant storage and transfer ability in 2015.

Such a mission would build on the United Launch Alliance (ULA) exploration master plan, which removes the need for a Heavy Lift Launch Vehicle (HLV), instead combining the use of current EELV (Evolved Expendable Launch Vehicle) vehicles – such as Atlas V or Delta IV – with an on orbit ability to refuel in space via fuel depots.

See also: ULA claim gap reducing solution via EELV exploration master plan

“We as a group strongly believe that the use of orbital propellant transfer and storage (Depots) provides a breakthrough in space transportation enabling truly affordable, sustainable and flexible exploration to destinations beyond low Earth orbit (LEO),” noted the executive summary of the presentation – acquired by L2.

“We also believe that the most successful approach to a 2015 propellant storage and transfer flagship demonstration will build upon the foundation of the decades of cryogenic propellant experience developed and currently being used in our nation’s EELV fleet.”

Outlining a “simple, robust propellant transfer and storage mission”, the authors claim the architecture supports near term robotic and crewed missions to geostationary orbit (GEO), the Earth-Moon (EM) and Sun-Earth (SE) Lagrange points and the Moon, prior to evolving as technology and demand require, “efficiently supporting every destination in the Flexible Path including crewed missions to Mars.”

Strategically placed at one or more Lagrange points, such depots would remove the need for vehicles to launch with all the propellant required to complete a mission – one of the primary reasons for very large launch vehicles, due to the mass of the propellant they have to launch with.

“Propellant depots offer near-term ability to support demanding space missions without the expense of developing very large rockets to support each new mission. They also enable reuse of in-space stages and provide a market large enough to encourage access to orbit innovation,” noted the presentation.

Although the political refinements to the FY2011 budget proposal are ongoing, supporters of a flexible path exploration architecture note that propellent depots can save up to 57 percent of the launch mass being reserved for fuel, when undertaking high energy missions.

“With the proposed FY2011 budget, NASA intends to pursue a flexible exploration path that will take America to Lagrange points, near Earth objects (NEO’s), lunar and Mars orbit and lunar and eventually the Martian surface. All of these are high energy missions that require an energetic, high performance stage to initiate the journey from LEO,” added the presentation. “Use of LO2/LH2, vs. LO2/Methane, can reduce the initial mass in LEO by up to 57 percent.”

Options remain open on which propellents could be used, although all large-scale robotic and crewed beyond LEO missions propose the use of high efficiency LO2/LH2 propulsion for the majority of their propellant needs in LEO – as noted by the executive summary, and large sections of the presentation.

“To enable propellant storage and transfer to support such missions this decade, it is critical that the 2015 mission include LH2. The proposed flagship mission design takes full advantage of America’s decades of orbital LO2/LH2 CFM (Cryogenic Fluid Management) flight experience.”

Commonality with NASA’s own “Flexible Path” approach to exploration – a large presentation created after the Augustine Committee’s review into Human Space Flight – can also be found as part of the foundation of the PTSD FTD conclusions, which utilizes Orion with an EELV Upper Stage, such as the Atlas Centaur or the Delta Cryogenic Second Stage (DCSS).

Also see NASASpaceflight.com’s Flexible Path Review:
Part 1: Battle of the Heavy Lift Launchers – Monster 200mt vehicle noted
Part 2: Manned mission to construct huge GEO and deep space telescopes proposed
Part 3: NASA Flexible Path Evaluation of 2025 human mission to visit an asteriod
Part 4: Taking Aim on Phobos – NASA outline Flexible Path precursor to Man on Mars

“The crewed missions that NASA might conduct this decade are GEO, Lagrange points, lunar and NEOs. NASA will likely rely on Orion’s propulsion module, with storable propellants, for the return propulsion. Our recommendation is that NASA’s depot flagship mission focus on the storage, transfer and handling of LO2/LH2.

“Following the 12 month demonstration mission, a forward looking depot demonstration design would allow an Orion mission to a Lagrange point as early as 2016 using an existing EELV upper stage as the Earth Departure Stage (EDS).”

Historical and current experience are also cited as a positive in enabling a low risk approach towards the propellant depot FTD, with numerous Cryostats already in use or under development for scientific satellites, demonstrating the ability to efficiently store cryogens for long durations.

“America’s existing CFM capability is based on decades of experience storing LH2/LO2 in launch vehicle upper stages. This historic flight experience suggests that with proper design, a propellant depot can efficiently store large quantities of cryogenic liquid, including LH2, for years.

“Settled operations significantly simplify all aspects of orbital CFM enabling maximum use of existing, mature CFM techniques. Beyond greater technical maturity, settled CFM has been flight proven to actually enhance the cryo system operation by reducing liquid heating (much of the heating is absorbed by the ullage), reducing ullage mass (warmer ullage), reducing liquid residuals and improves reliability (avoids the requirement for pump circulation systems).”

Keeping the Cost Low:

The presentation also claims a simple LO2/LH2 depot – derived from existing hardware and CFM experience – can demonstrate all of NASA’s PTSD objectives within a $500m budget in under five years.

“Several groups have independently determined that LO2 and LH2 can be stored efficiently in a compact, light weight, affordable depot design. The simplicity of these depot concepts could support NASA’s 2015 PTSD demonstration mission. The depot could be launched on an Atlas 551 and stay within the proposed budget and schedule. The key to such a depot design is segregating the LO2, LH2 and warm equipment module.

Transverse spinning of the entire depot at ~1 degree per second would also provides a settled fluid environment that simplifies the cryo-fluid storage and handling.

“With effective design, analysis indicates that total system boil-off can be held to 0.01 percent per day, which is below the station keeping requirement. The use of propellant boiloff for station keeping was successfully used on the Saturn S-IVB stage (ullage motor) and hydrogen boil-off is currently used by the Delta IV Cryogenic Second Stage (DCSS) for settling.”

The aforementioned simplicity of the design – along with current technology of the EELV upper stage – are noted as key drivers for keeping the cost and schedule risk low.

“The LH2 module includes a large tank with minimal penetrations. This tank is connected to the mission module by six low conductivity composite struts. These struts, fluid transfer plumbing and wiring are vapor cooled to minimize heat reaching the LH2,” the presentation continued. “The entire tank is encapsulated in a robust, IMLI (insulation) blanket incorporating broad area cooling and MMOD protection.

“The LH2 module is launched empty and filled on orbit with Centaur residual LH2. Launching the LH2 module empty allows the module and adapter to be designed for orbital requirements and not ground and ascent environments. The LH2 module requires no foam insulation and the payload adapter structure can be very light weight and thermally efficient. Based on Centaur mass properties this LH2 module should weigh ~1 mT and have a 4.5 mT LH2 storage capacity.

“To minimize cost and schedule, the LH2 module can be derived from a Centaur tank. This allows hardware to be procured and outfitted in 2010/11 with large scale thermal vacuum testing starting as early as 2011. Near term experience with the system provides risk mitigation that is critical to a successful 2015 demonstration mission.

“Between the Centaur and the LH2 module resides the mission module. This module includes the solar panels, fluid controls, avionics and if desired, an orbital transfer vehicle (OTV) interface and remote berthing arm. The mission module could be derived from NASA’s planned automated rendezvous and docking (AR&D) demonstration vehicle.

“Alternatively the mission module could consist of a standard Atlas payload adapter containing avionics derived from existing spacecraft such as LCROSS, Orbital Express or XSS-11. The LO2 is stored in Centaur’s large LH2 tank. Storage of the LO2 in Centaur’s LH2 tank simplifies long duration, minimum boil-off storage.

“The Centaur is shrouded with IMLI (Insulation) to minimize heating. Hydrogen vapor cooling tubes are routed along key points on the upper stage to eliminate LO2 boil-off. The high sensible and latent heat of hydrogen makes hydrogen the ideal fluid for vapor cooling.”

For the PTSD mission, the LH2 and LO2 are provided as residuals from Centaur. Launching the PTSD on as Atlas 551 provides ~12 mT of combined LH2/LO2 residual if the PTSD weight is optimized, the presentation noted.

“Once on orbit the 2 mT of residual LH2 is transferred from Centaur’s LH2 tank to the thermally efficient LH2 module. Centaur’s LH2 tank is then vented to vacuum, fully evacuating the residual hydrogen gas. Following the LH2 tank ‘safing’, the ~10 mT of residual LO2 is transferred from Centaur’s LO2 tank to Centaur’s LH2 tank for long duration storage. This transfer eases the LO2 storage because Centaur’s LH2 tank is already very thermally efficient.”

Efficient system design, fluid in-flow into a tank, vapor cooling, integrated multi-layer insulation (IMLI) (incorporating micro-meteoroid and orbital debris (MMOD) protection and broad area cooling), transfer tube connection, subcooling and combined system operation are the critical technologies that must be demonstrated.

The Integrated MLI that provides enhanced thermal and MMOD protection is an innovative new technology where polymer substructures are integrated with radiation barriers to provide improved high performance cryogenic thermal insulation systems. IMLI is noted as having a significantly enhanced structural integrity and performance compared to standard cryogenic MLI.

“Standard MLI blankets have a surprisingly high level of protection from the impact of MMOD. The incoming particle is broken apart by the initial impact, and the resulting debris cloud is further retarded and broken up as it progresses through each layer. IMLI enhances standard MLI MMOD tolerance by combining increased and controlled spacing between layers and slightly thicker layers than standard MLI blankets.

“The inclusion of a thicker broad area cooling (BAC) layer further increases MMOD protection of IMLI. Increased spacing enhances the protective capability of the IMLI by providing distance over which a debris cloud spreads, thereby dissipating the energy of the cloud before impact onto the next layer.”

Reducing Boil-Off:

As intimated in the executive summary, the technology required to reduce the amount of LH2 boil-off from the depot is one of the key elements in the forward planning of such an architecture.

Options such as Vapor Cooled Shields (VCS) – using tank boil off (passive) or cryocoolers (active) – can be used to provide cooling. VCS systems have been flown by Ball Aerospace – who were one of the commercial companies involved in the presentation – on LH2 PRSA tanks.

“To incorporate passive cooling technologies, a combination of VCS and in-line para-to-ortho conversion can minimize boil-off losses from LH2 storage tanks. As a passive technique, VCS using cold evaporated hydrogen gas significantly reduces the amount of heat leakage into the LH2 storage tank over long mission durations. Para-to-ortho hydrogen conversion is an endothermic process which adsorbs heat.

“The VCS with a para-to-ortho converter can generate additional cooling and create a refrigeration effect to reduce boil-off of LH2. An integrated VCS with a parato-ortho hydrogen converter will must be analyzed, designed and ground tested in order to demonstrate its advantage for the cryogenic flagship propellant depot.

“Transition metal catalyst studies with supported iron, nickel, copper, etc., will need to be conducted to optimize the converter performance in terms of percent para-H2 conversion at a given hydrogen feed rate or an equivalent gas hourly space velocity (GHSV). As the design GHSV of the reactor catalyst system increases, the overall size and mass of the para-to-ortho converter can be reduced.”

Broad Area Cooling (BAC) - investigated by NASA between 2004 and 2006 under the In-Space Cryogenic Propellant Depot (ISCPD) Project to substantially reduce or entirely eliminate boil-off losses with a minimal increase of total system mass – might also be integrated with cryogenic propellant storage tanks.

Also, other options, such as subcooling propellent below their boiling point at atmospheric pressure prior to launch, and enhanced analysis tools incorporated in cryogenic propellant utilization (PU) capability – which predicts the thermodynamic state of an on orbit cryogenic upper stage requires a high degree of fidelity – are also examined in the presentation.

Technology Development and Demonstration:

Ground testing would be a key element to a successful demonstration mission, while also reducing the risk involved. The importance of ground testing the new technologies received a large overview in the proposed path outlined in the presentation.

“Relying on numerous new technologies on a single flagship mission is a recipe for failure. A combination of ground component development and system tests in parallel with low cost rideshare demonstration should be pursued concurrently with the flagship depot development.

“Ground testing can demonstrate the technology/system functionality while also providing data to anchor analysis tools enabling better support of the flagship mission. The technology development plan should encompass a continuous process beyond the 2015 flagship mission encouraging continuous developing and allowing new technologies to be incorporated as they mature and offer mission benefits.”

Should NASA’s forward path include Propellent Depots, several existing facilities would be put to good use, such as the Cryo-Fluid testing of Centaur tanks at the ULA facility – which can provide invaluable data on the actual performance of proposed thermal protection schemes.

“Many features of the advanced thermal protection system required to allow long-term, large scale cryogenic storage can be demonstrated on the ground. IMLI, vapor cooling, BAC, light weight tank structures can be effectively demonstrated on the ground.

“This ground testing is directly applicable to orbital depots that rely on settling to handle the fluid-gas interface and is useful for zero-g cryogenic storage.

“While much has been learned from the multi-purpose hydrogen test bed testing conducted at MSFC (Marshall Space Flight Center), it is crucial that further ground testing utilize structures that are representative of flight systems, not 0.5 inch thick ‘boilplate’ aluminum tanks where substantial wall conduction influences the results.

While ULA are listed as offering NASA the loan of a Centaur tank, NASA’s Plum Brook B2 facility classed as “perfect” for large scale integrated testing.

“NASA (GRC, KSC, MSFC, JSC, Ames and GSFC) and ULA are collaborating to pursue such testing at in NASA’s B2 vacuum chamber. ULA has offered to loan NASA a Centaur tank – which would allows for ground based system testing to begin as early as 2011, whilst arriving with its long flight history to boot.

“Centaur’s 194 flights provide a vast database, both settled and zero-g, with which to anchor ground test data. Centaur’s low thermal structural mass and low conductivity are critical for long duration flight cryo-storage tanks. Equally important it is possible to duplicate thermal protection enhancements tested at Plum Brook on upcoming flights thanks to the Atlas’s ability to encapsulate Centaur in the payload fairing during assent,” the presentation continued.

“NASA’s Spacecraft Propulsion Research Facility (B2) is the world’s only facility capable of testing full-scale upper-stage launch vehicles and rocket engines under simulated high-altitude conditions. The engine or vehicle can be exposed for indefinite periods to low ambient pressures, low-background temperatures, and dynamic solar heating, simulating the environment the hardware will encounter during orbital or interplanetary travel.”

Near Term Demonstrations:

Orbital demonstrations are also noted, with a specific reference to the CRYogenic Orbital TEst (CRYOTE) – which offers a near term, low cost method to demonstrate in-space propellant depot CFM technologies.

Several NASA, DoD, and commercial missions with launch dates beginning in 2012 have been identified as candidates, and its compact geometry and minimally intrusive, light weight design make it compatible with numerous upcoming Atlas missions.

“The CRYogenic Orbital TEst (CRYOTE) concept utilizes a very creative rideshare implementation to allow demonstration of cryo-fluid transfer, long duration storage and a host of CFM technologies while minimizing the impact to the launch vehicle. CRYOTE rides inside the Atlas V payload adapter, similar to how LCROSS’s hydrazine tank was mounted.

“Following payload delivery, residual LH2 (or LO2) is transferred from Centaur into the CRYOTE tank. The act of transferring the LH2 from Centaur requires chilldown of the transfer lines and storage tank while demonstrating the ability to fill a receiving vessel.

“Inside of CRYOTE’s tank a multitude of CFM technologies can be demonstrated including propellant management, long term storage, mass gauging and liquid acquisition. CRYOTE offers an end to end, sub-scale demonstration of all propellant depot CFM technologies. Targeted missions are those with at least 1,000 lbs of mission performance margin.”

Playing to the current FY2011 budget proposal – and indeed several elements of the proposed changes via at least the Senate bill – the presentation notes the CRYOTE project includes the involvement of nearly every NASA center, academia and several companies.

“CRYOTE provides a successful example of how we all benefit from collaboration. In addition to orbital rideshare opportunities, some of the emerging reusable suborbital vehicles, such as those under development by Masten Space Systems, Armadillo Aerospace, XCOR, and others can provide platforms for short-duration (3-5min) microgravity CFM experiments.

“While microgravity durations are shorter, those technologies that can be tested in that brief of a window can benefit from much shorter design-build-test iteration cycles. Also, depending on the size of the suborbital vehicle, there can be significant commonality with the orbital CRYOTE system.”

The use of propellant depots in a future architecture do hold a good level of support throughout the future path proposals. One of the more recent mentions came via the expansive SD (Shuttle Derived) HLV (Heavy Lift Launch Vehicle) assessment presentation, when it referenced a joint role of working with commercial and international vehicles in a Beyond Earth Orbit (BEO) architecture.

By way of providing benefits to Lunar and Deep Space missions, the 726 page presentation (L2) - which was the final assessment of the SD HLV, prior to the very recent restart of assessments to note additional information on the In-line SD HLV – noted the addition of propellant deports would significantly improve the overall exploration architecture.

Their approach notably differs by way of the depot being launched by a single HLV to L1, for it then to be refuelled using commercial vehicles, reducing the mass required to launch from Earth’s surface on a Lunar or deep space mission via ‘dry’ – and potentially reusable – landers.

A HLV – of any kind – is not listed in any current ULA or commercial documentation, with experts claiming such a vehicle isn’t required under the EELV and propellant depot architecture.

pixelstats trackingpixel

No related posts.

External Tank ET-138 under investigation after washer is found in feedline

Posted on 6th August 2010 by admin in Space Flight

Currently set to fly with Endeavour, External Tank ET-138 is under investigation – after engineers found a washer inside the LO2 Feedline. The investigation will follow a similar route to that undertaken on ET-129 – when a noise was heard inside that tank during processing inside the Vehicle Assembly Building (VAB) – in order to be completely satisfied with tank’s configuration.

STS-134 Processing Latest:

Endeavour is in a smooth flow insider her Orbiter Processing Facility (OPF-2), with all three of her Space Shuttle Main Engines (SSMEs) installed and undergoing integrated testing with the Main Propulsion System (MPS).

The Orbiter Boom Sensor System (OBSS) has also undergone simulated thermistor testing, in preparation for being left on the International Space Station (ISS) at the conclusion of STS-134′s docked phase of the mission.

“OV-105 (STS-134): Engines were installed last week, continuing with engine securing. In the midbody, are routing the payload harnesses. Completed testing this week on Window 7, and are scheduled to install it on the vehicle next Monday,” noted KSC Integration on the latest Shuttle Standup/Integration report (L2).

With the Space-to-Space Orbiter Radio (SSOR) SCAN retest completed, along with Endeavour’s Nose Landing Gear (NLG) strut GN2 decay check showing positive results, processing on the youngest orbiter in the fleet will standdown over the weekend.

“OV-105 (OPF Bay 2): SSME/MPS integrated testing is scheduled for Monday and Tuesday pending resolution of a galled bolt hole on Engine #3 GOX interface documented in the PR (Problem Report),” added the NASA Test Director (NTD) processing report (L2) on Friday morning, noting the only issue (minor) reported in Endeavour’s OPF flow.

STS-134 Specific Articles: http://www.nasaspaceflight.com/tag/sts-134/

“Window #7 Installation is scheduled for Friday. The KU-Band pre-mate testing is scheduled to begin Monday. Weekend work: none currently scheduled.”

Endeavour is also closing in on the business end of payload operations, with the installation of the Detailed/Development Test Objective (DTO) known as STORRM (Sensor Test for Orion RelNav Risk Mitigation) due next week.

The primary payload of the Alpha Magnetic Spectrometer (AMS-02) is currently undergoing its latest review at the time of this article’s publication.

The AMS Capability Review (Delta CIR) is Friday,” added Flight Operations and Integration (NASA/JSC) on the Standup report. “On STS-134, the STORRM (DTO) hardware is supposed to be at KSC this week, with installation next week.”

SRB Milestone:

Although STS-135 is likely to be approved within weeks, STS-134 remains the final scheduled shuttle mission on the official manifest. As such, numerous milestones are being met as STS-134′s stack builds up inside the VAB – the latest of which relates to the Solid Rocket Boosters (SRBs).

Friday marked the final major piece of SRB hardware to depart the Kennedy Space Center’s Assembly and Refurbishment Facility. It joined with the other segments, which are currently being stacked in High Bay 1 (HB-1).

“SRB BI-145 / RSRM 113 (VAB HB-1): Right Aft Center segment stacking is complete and post ops are complete. Right Aft Joint leak check is in work. Left Forward Center segment stacking is scheduled for next Monday and Tuesday,” added the NTD.

“Friday morning, transferred the right forward assembly for STS-134 over to the VAB. That is the final for the February flight.”

The transfer of the final segment was marked by a ceremony for the related workforce, hosted by United Space Alliance (USA) Director of Manufacturing Operations Greg Henry and Astronaut Kay Hire.

ET-138 Investigation:

The last “new” tank to be shipped from the Michoud Assembly Facility (MAF) – ET-138 – has been located in High Bay 2E’s checkout cell since its arrival in Florida, where it has undergone numerous checks and preparations for its mating with the SRBs.

It was during the evaluations on the LO2/LOX 17 inch feedline – which involves the removal of a cover plate to allow for inspections of the inner workings of the lines – that a washer was found.

“On ET-138, removed the LOX 17” cover plate to perform angle and tip load measurements; a loose washer was found in the feedline. The washer was removed and sent to MAF for analysis,” noted the Standup report, and also noted by the NTD.

“ET-138 (VAB HB-2E): A washer was found in the LO2 feed line during inspections and was removed. The washer has been sent and received at MAF for further engineering evaluations. Wipe samples were completed and routed to Wiltech for analysis.”

ET contractor Lockheed Martin are also part of the investigation both at MAF and KSC, where they will use lessons learned from ET-129 – relating to when a handful of engineers heard a metallic noise coming from inside the tank during its transition into the checkout cell ahead of STS-126.

Even though most of the engineers present didn’t hear the noise, managers immediately called for a full investigation – one which would reach as far as the Flight Readiness Review (FRR) and the Space Shuttle Program (SSP) management. A similar Foreign Object Debris (FOD) investigation will be used to confirm the tank is in a good condition to continue processing.

“Are going back to the ET-129 noise investigation assessment and looking for what was done during that to form any possible forward work for ET-138 to assure are satisfied with tank configuration,” added ET/Lockheed Martin.

“ET-138 On the washer observed in the feedline, the washer was removed, bagged, and returned to MAF. MAF is kicking off an investigation. In the photographs, it appears to be a cad-plated fastener. Cad-plated fasteners are used for flight, not for tooling at MAF. Looking for possible sources.”

Had Endeavour launched with an undiscovered FOD in such a location, it wouldn’t of been ingested into a critical system, due to the prevalve screens in the MPS.

pixelstats trackingpixel

No related posts.

Shuttle Program updates MPS Inventory for STS-133 and beyond

Posted on 5th August 2010 by admin in Space Flight

For what is likely the last time during the execution of the Space Shuttle launch/mission manifest, engineers from around the agency have updated the Main Propulsion System (MPS) Inventory – an extensive database aimed at continuously adding to and improving knowledge of the operational characteristics of this highly critical vehicle component.

Purpose and Background:

As part of the routine evaluations and updates to the MPS Inventory, a SICB meeting on July 20, 2010 officially approved a new line of changes to the MPS Inventory, changes that garner an additional 200 lbm of Ascent Performance Margin from the MPS for the final flights of the Shuttle manifest.

As stated by the MPS Inventory change presentation – available for download on L2 – “This presentation is meant to be a discussion topic to notify SSP Management of changes to the MPS Inventory that were approved at the 07/20/10 SICB.”

The increase to the “approximate performance impact” comes in large part from an update to the SSME (Space Shuttle Main Engine) Power Balance Model (PBM) – a physics-based, steady state system model which reduces flight/test data and also predicts/simulates the flow of propellants and transfer of energy in the SSME – in the Level II modeling assumptions.

This update carries minor impacts to the nominal flight of the Shuttle stack and provides a “larger impact on the understanding of SSME performance and off-nominal performance cases (e.g. ARD – Abort Region Determinator).”

In fact, while the MPS Inventory is “routinely” updated every ~1.5 years as specific flight information is added to the MPS database, changes to the Inventory are in fact more numerous than the typical 1.5 year interval and are made as warranted by system performance and understanding.

The last update was completed after STS-129 (Nov. 2009) and before STS-130 (Feb. 2010).

STS-133 Specific Articles: http://www.nasaspaceflight.com/tag/sts-133/In the last six years alone, there have been “many updates to the Inventory” related to investigations into Low Fuel Bias, LO2 Purity, and OBMR (Over Board Mixture Ratio). As a result, knowledge and understanding of the MPS system is constantly maturing.

Specifically, the Low Fuel Bias, LO2 Purity, and OBMR investigations have “led to many changes in not only how we reconstruct flights but also how we predict them (Inventory updates, Flight based tags, CMR changes, etc.),” notes the Inventory Update presentation.

Updates Overview:

For the current update, approved two weeks ago, the SSME PBM and updates to the Flight Dispersions databases were the primary areas of focus, stemming in part from the previous OBMR and LO2 Purity investigations.

“Following the OBMR and LO2 Purity Investigations, SSME project went back and reviewed earlier testing that had been run at low power levels,” notes the presentation.

This review was coupled with further low power level testing with planned CMR (Controller Mixture Ratio) runs at SSC (Stennis Space Center).

These reviews resulted in increased knowledge of the MPS system – which in turn translated into changes to the SSME PBM maps that “relate parameters to each other (Mixture Ratio, flow rate, Isp, Thrust, etc).”

The mixture ratio here has a direct effect on the SSME Influence Coefficients which are used by the MOD (Mission Operations Directorate) and Level II to “adjust performance based on power level.”

Prior to the recent MPS Inventory update, the Influence Coefficients were based on a constant Inlet Mixture Ratio; the Influence Coefficients are now based on a varying Inlet Mixture Ratio.

Taking this change into account, the presentation notes that there will be little change in the propellant consumption during a nominal no-fail ascent trajectory.

However, while the total propellant usage during a no-fail ascent trajectory does not change from the previous MPS Inventory, the manner in which the SSME prop consumption is distributed throughout the duration of flight does change.

Under the updates, LO2 flow rates will increase at lower power levels (i.e. during the throttle bucket and 3-g throttle) and decrease during 104.5 percent (nominal max). This will enable consumption to remain unchanged from previous.

This new distribution of consumption will result in corresponding thrust, Isp, and mixture ratio variability as well as an increase in thrust during the throttle bucket and 3-g throttling phase of ascent and a decrease in thrust at the nominal max setting – 104.5 percent.

Additionally, updating the SSME Influence Coefficients and tag values required an updating of all flight reconstructions from STS-95 through STS-132 and the associated Flight Derived Dispersions (FDD) databases.

An update of the FDD database resulted in a 400 lbs reduction (a 35% reduction) of the performance collector mean and a 21 lbs (23 percent) reduction of the Thrust Shape mean. Furthermore, the “axial force collector is of a smaller magnitude during the throttle bucket, showing the models better match the flight,” notes the presentation.

Accordingly, all flight reconstructions are more accurate and more closely resemble their flights.

Nonetheless, as a result of the SSME PBM and FDD updates, the average degraded SSME tags also had to be updated.

The presentation notes that the new MPS Inventory was balanced at an average OBMR of 6.0382 based on a current CMR of 6.043. This results in an updated Fuel Bias of 954 lbs over the previous 1,059 lbs.

Additionally, the MECO (Main Engine Cutoff) timer was also evaluated but left unchanged.

Combined, these MPS inventory changes result in a net performance gain of 200 lbs APM (Ascent Performance Margin), PTA occurring 5-seconds earlier, PTM occurring 4-seconds earlier, and a 14 fps increase to the stack’s underspeed during a stuck throttle in the bottom of the bucket scenario.

pixelstats trackingpixel

No related posts.

Ariane 5 ECA launches with Nilesat-201 and RASCOM-QAF1R

Posted on 4th August 2010 by admin in Space Flight

Following a scrub-prone launch campaign in June, Arianespace have enjoyed first-time success with Wednesday’s launch of their Ariane 5 ECA vehicle – her third mission of the year. The workhorse has two telecommunication passengers – Nilesat-201 and RASCOM-QAF1R – and launched slightly after the start of the long launch window.

Ariane 5 ECA:

Flight 196 is the 52nd Ariane 5 launch and the third in 2010. An Ariane 5 ECA (Cryogenic Evolution type A), the most powerful version in the Ariane 5 range, will be used for this flight, launching from the European Spaceport in Kourou, French Guiana.

Launcher 554, the 48th production phase Ariane 5, is the twenty-sixth of the 30 PA contract launchers, for which Astrium is production prime contractor. 554 is consequently the twenty-sixth complete launcher to be delivered to Arianespace, integrated and checked out under Astrium’s responsibility in the Launcher Integration Building (BIL).

Arianespace is looking to recover from the numerous issues associated with their Arabsat 5A and COMS 1 launch attempt on the 23rd, which suffered from an issue relating to the launcher subsystem late in countdown operations, resulting in a scrub for the day.

The countdown appeared to be going to plan on the following day, prior to a hold being called at T-17 seconds. With the clock reset to T-7 minutes, another attempt was made, before another hold was called at almost the same time as the earlier issue.

Lacking available time in the launch window to resolve the problem – classed as an issue with the spaceport’s launch infrastructure, a scrub was called, with the third attempt set for 48 hours later – which enjoyed an issue-free countdown, resulting with a launch at the start of the window.

For the latest campaign, Ariane 5 ECA is again using the dual-payload configuration, with the debut use of the SYLDA 5 K – seven metres high, i.e. 60 cm more than the usual SYLDA 5 A – system with an extended nose-cone (total height: 17 m), to carry the Egyptian NILESAT 201 satellite in the upper position and the African RASCOM-QAF1R satellite in the lower position.

Nilesat-201 will enable the Egyptian satellite operator Nilesat to deliver digital Direct to Home (DTH) TV and radio broadcasting and high-speed data transmission services to North Africa and the Middle East starting in September 2010.

Built on a Spacebus 4000B2 platform, Nilesat-201 is fitted with 24 Ku-band and 4 Ka-band transponders. It will be positioned at 7 degrees West longitude  and offers a design life of 15 years. Weight at launch will be about 3,200 kg, and it will generate 5.9 kW of power at end-of-life.

RASCOM-QAF1R will ensure service continuity for the operator RascomStar-QAF and its customers, by giving Africa access to advanced communications and information technologies, in particular rural telephony.

Based on the Spacebus 4000B3 platform, the RASCOM-QAF1R satellite Is equipped with 24 equivalent 36 MHz transponders in both Ku-band and C-band. The bird will provide 6.4 kW of power at end-of-life. Positioned at 2.9 degrees East longitude, RASCOM-QAF1R will cover the African continent, as well as parts of Europe and the Middle East.

RASCOM-QAF1R – which has a liftoff mass of about 3,050 kg. – will be deployed from Ariane 5’s lower passenger position at approximately 33 minutes into the flight.

The August 4 mission also will be Ariane 5’s third flight of 2010, which follows two previous dual-payload launches: the June 26 mission that orbited the Arabsat-5A and COMS spacecraft, and the May 21 launch with ASTRA 3B and COMSATBw-2.

pixelstats trackingpixel

Related posts:

  1. Ariane 5 ECA launches with HOT BIRD 10 and NSS-9 satellites Arianespace’s Ariane 5 ECA launch vehicle has lifted off from…

Two EVAs set up for ETCS coolant Pump Module changeout on ISS

Posted on 2nd August 2010 by admin in Space Flight

Expedition 24 Flight Engineers Doug Wheelock and Tracy Caldwell Dyson will undertake two EVAs – on Friday and Monday - slipping 24 hours on Monday’s initial schedule - to changeout an ammonia coolant Pump Module on the S1 truss, which is at the center of the Loop A failure on the External Thermal Control System (ETCS) on Saturday, resulting in the shutdown of several systems.

ETCS Loop A failure:

Issues with the ETCS were heard over the loop on Saturday evening, when alarms sounded – waking up the ISS crew on the orbital outpost – due to a circuit breaker trip. Within half an hour, mission controllers updated managers by memo.

“Loop A Shut down: Around 213/00:00 we lost the Loop A of the ETCS system. Currently the team is working balancing the thermal loads and analyzing the cause of the shut down,” noted a running order of memos acquired by L2.

“It is not clear at this time if it is a hybrid FET failure, RPCM (Remote Power Control Module) trip or pump problem. Specialists are either in or on way, MER (Mission Evaluation Room) is here and staffing up.”

The External Thermal Control System (ETCS) provides cooling to the entire United States On-Orbit Segment (USOS). The ETCS consists of two independent loops, designated Loop A and Loop B.

The system is designed to collect heat from the Internal Thermal Control Systems in the US Lab, Node-2, COL, JEM, and Node-3, via IFHXs (Interface Heat Exchanger). The Pump Module (PM) provides the motive force to transport the ammonia around the loop.

Heat is rejected to the space environment as each loop flows through a separate set of rotating radiator assemblies mounted on the S1 (Loop A) and P1 (Loop B) truss segments. The heat rejection capability is 35 kW per loop (70 kW total for the USOS).

The majority of ETCS components are located on the S1 (Loop A) and P1 (Loop B) truss segments. ETCS fluid lines are routed from the various USOS modules through the S0 Truss to the S1/P1 truss segments.

As part of the contingency plan, controllers ensured Loop B was providing the required assistance, as they evaluated options.

“Team is pressing into Loss of Loop A Powerdown. We’re going to get on a stable config on Loop B and then reassess w/ MER if/when to attempt restart of Loop A,” added the next memo. “From 50 Hz dump, the RPC trip on Loop A ETC pump was real. O1 (Orbit 1) team now running the show.”

Tracy Caldwell Dyson provided on-site assistance as controllers ran through the procedures for shutting down numerous systems, in order to reduce the amount of electronics that would require the cooling from the ETCS.

“The team is continuing work Procedure 2.674 Loss of Thermal Loop A Powerdown. The major impacts are 2 CMG’s (Control Moment Gyros 1 and 4), S-Band String 1, GPS String 1, Prime EXT MDM (Multiplexer Demultiplexer), Node 2-1 MDM, P1-1 MDM, P3-1 MDM, SO-1 MDM,  S1-1 MDM, S3-1 MDM , STR MDM and several DDCU’s (DC to DC Converter Units) in Node 2.  Momentum is currently stable at 31 percent. 

“Tracy Caldwell is still awake assisting with the powerdown. The rest of the crew is back in bed.”

Caldwell’s clearly tired – but highly professional – assistance also located a jumper cable, after its original location proved to be a mystery. Her actions also protected the remaining string on the S-Band communication system, as she joked it felt like she was “in a sim” (simulation).

“The team has completed most of the critical actions in ‘2.674 Loss of Thermal Loop A Powerdown – Warn’, the crew was up for their entire sleep period and is just now being put to bed,” summarized a memo sent out in the early hours of Sunday.

“They installed two jumpers to maintain maximum available redundancy, 1 contingency truss jumper to bypass DDCU S01A and maintain significant redundancy to systems especially driven by Sband string 1 heater and ops power (to maintain dual Sband redundancy capability) – good job by PHALCON and OSO to recommend that jumper.”

The crew were allowed to get in a decent sleep period prior to Sunday efforts to ensure the ISS remained in a good configuration.  Attempts to restart the motor were unsuccessful, although the pump did show signs of physically working, leading to theories that the fault is a short in the power system.

“The forward plan is to let the crew sleep 6-8 hrs, and we told them that after careful review on the ground we may elect to attempt to repower the loop A pump to see if it can be recovered while they are sleeping (teams are off assessing options at this time given the signature and dump data),” memos continued.

“Systems are in a stable configuration after about 8 hrs of reconfig and safing commanding by the team, including powering down 7 DDCUs (and then repowering S01A), deactivating or reconfiguring downstream loads, reconfiguring ITCS (Internal Thermal Control System), SARJ (Solar Alpha Rotary Joint), and TRRJ (Thermal Radiator Rotary Joint). Necessary loads are being supported by the 2/3 power domains.

“Truly a great job by all, the entire team is doing an outstanding job. A big thank you to the folks called in to support this activity. This is why we sim as we do, and it paid dividends.”

Attention then focused on the need to carry out two EVAs to replace the cause of the problem, the primary ETCS heat transportation component known as the Pump Module (PM), which circulates liquid ammonia at a constant flowrate to a network of coldplates and heat exchangers located on the external trusses and USOS modules, respectively.

The PM contains an accumulator, instrumentation, isolation and relief valves, various heaters, and a Pump and Control Valve Package (PCVP) – which is responsible for regulating the flowrate, filtering impurities to protect loop components, and for controlling temperature.

Wheelock and Caldwell Dyson originally were scheduled to perform a spacewalk to outfit the Russian Zarya module for future robotics work and prepare the station for the installation of a new US permanent multipurpose module.

However, because of the importance of restoring redundancy to the station’s cooling and power systems, Friday’s spacewalk will be dedicated to the pump module replacement. Another spacewalk will be scheduled for Monday to complete the repairs.

This will be the first time a “Big 14″ – the term for a major system on the ISS - Stage EVA will be conducted.

“There will be a team 4 effort spun up to start looking at EVA options for R&R, given a US EVA was already planned next week. There is a spare pump package and it is baselined as a full 2 EVA ‘Big 14′ task which will take a significant amount of work to get everyone prepared to execute,” added another memo (L2).

“The US EVA scheduled for Thursday 8/5/2010 will now be dedicated to a pump module (PM) R&R due to the criticality of restoring redundancy to the ISS. The pump module R&R will be a two EVA task with the second EVA no earlier than 2 days after EVA 1.” This slipped on Monday to a schedule of Friday and Monday for the EVAs.

The EVA tasks will be complex, with numerous electrical and fluid lines associated with the 780-pound pump module, along with robotics being required to aid the translation of the old and new PMs.

“The SSRMS (Space Station Robotic Manipulator System) will be an integral part of the EVA to assist in pump module translation and details are being worked by the team. A development NBL (Neutral Buoyancy Laboratory) run will be scheduled for Monday to run through the procedures, determine what modifications need to be made, and the feasibility of egress on Thursday.

“A final NBL run will be scheduled for Tuesday (8/3). The EV Crew (Caldwell/Wheels) had NBL task training on a pump module R&R back in Sept 09 and the MCC team will be sending refresher material on the R&R later today. Clearly if the collective team is not ready to proceed on Thursday the EVA will be moved to the right accordingly (as was the case).”

An executive summary then followed, as the plans matured at a pace. Considerations included further robotic assistance, hazards and contingencies for issues during the planned EVAs.

“The crew timeline this week is being scrubbed and will contain the necessary preparation including crew study time for the EVA. The Mobile Transporter (MT) will be moved to work site 2 (WS2) to allow the SSRMS to assist in the PM replacement,” added the summary (L2).

“Two DDCU power up tests with no cooling will be performed to provide data regarding heat up rates and how long they can remain powered for nominal Plasma Contactor Unit (PCU) use to preclude EMU shock hazards and SSRMS contingency support if required.

“Much of the discussion from the meetings involved the EVA timeline details and how to operate during the EVA with next worse failure as well as system configuration details (i.e. SSRMS redundancy). Good news is that even though cooling is not being provided for external DDCU’s on power channels 1 and 4, they can be operated for some amount of time to provide critical redundancy if required.

“The MER is providing an assessment as to how long these will last but the initial thought is around 8 hours or more based on anticipated loads. The failed PM venting plan is being worked and details will be discussed at (further) meetings since this activity could have a major impact to ISS system configurations (i.e. solar arrays) and EV NH3 exposure risk depending on when performed.

“Details regarding solar array positioning for longeron shadowing, PCU redundancy, SSRMS redundancy, and combined EVA/SSRMS operations were also discussed and will be finalized over the next several days.”

Thanks to the speedy and professional work carried out by ground controllers, engineers and the crew on orbit, the ISS is in a good configuration – which earned additional praise on the executive summary.

“The ISS systems are all nominal with the exception of the PM. The on console team continues to work on impacts and actions for next worse failures as a result of the current ISS configuration. Excellent work by the teams today working through the complexities associated with the EVA’s required to remedy this failure.”

Further updates may be added to this article. Refer to live update pages on the ISS section. L2 members refer to the documentation and memo update threads.

pixelstats trackingpixel

No related posts.

MOD positioning for potential Flagship Technology Demonstrations role

Posted on 1st August 2010 by admin in Space Flight

The highly skilled and experienced NASA Mission Operations Directorate (MOD) are attempting to find their place in the post-Shuttle era, a future that continues to be uncertain due to the ongoing political battle. Focusing on their involvement in technology demonstrations and planning, the MOD produced an overview of how their “Plan, Train, Fly” approach could be utilized ensuring they have a “seat at the table”.

MOD:

Director Paul Hill has made a series of keynote “All Hands” addresses over the last 12 months (presentations and videos available on L2), including the painful task of informing many of his workforce that their departments will be suffering from large job losses.

One such speech came last July, centered around the issue of not knowing what the future holds for NASA or MOD, which ironically continues to be the situation a year later.

However, Mr Hill appears to have been rather savvy in his pre-emption of what the future may hold, guiding the MOD towards the potential of commercial launch vehicles rising to the forefront, along with his hope for a “follow-on program” for Shuttle (such as HLV) – both of which are currently gaining the majority of support via the Senate bill’s refinements to the FY2011 budget proposal.

Mr Hill’s latest All Hands pushes the MOD towards a role in the Flagship Technology Demonstrations (FTD), via their “Plan, Train, Fly” experience – a key MOD motto.

“MOD Involvement in Tech Demo and Dev: NASA’s new direction includes significant investment in new technology development and demonstrations. MOD intends to be a significant player in these areas using our Plan/Train/Fly expertise,” noted presentations associated with the July All Hands meeting (available on L2).

“There are currently six main technology areas: Flagship Demonstrations; Enabling Technology Development and Demonstrations; Exploration Precursor Robotic Missions; Heavy Lift Propulsion; ISS-based Technology Development; Project M.”

How much of the FTD element will survive the political realignment of the FY2011 proposal is yet to be confirmed, although MOD appear to believe it is prudent to showcase their ability to pick up the baton on numerous areas that have been proposed both by FY2011, and via the political negotiations.

“New Technology Projects: Flagship Demonstrations, In-space Propellant Storage and Transfer; Inflatables and Advanced ECLSS; Automated/Autonomous Rendezvous and Docking; Entry, Descent, and Landing; Solar Electric Propulsion,” listed the presentation on FTDs, appearing to match closely with the FY2011 outlines.

“Enabling Technology Development and Demonstrations, Five Demo Projects (in situ resources, autonomous precision landing, telerobotics, fission surface power, etc.); Ten Foundational Projects (autonomous systems, advanced materials, life support, EVA, etc.)”

An In-Space Propellant Transfer and Storage Demonstration, under the Flagship Technology Demonstration program, has already gained a large amount of interest and support. However, via a separate presentation (L2 – article next week), how much of a role MOD will have is questionable, with the aforementioned presentation written by a large mix of commercial companies in tandem with various NASA centers – all of whom are likely to want a slice of the pie.

Also listed in the MOD All Hands materials were International Space Station (ISS) related demonstrations, which are likely to be key targets for the MOD – given the Johnson Space Center (JSC) and MOD’s heavy involvement with the orbital outpost.

“ISS-based Technology Development, ~25 project proposals across Agency; ISS Free Flyer for Inspection, Science, etc. (JSC lead); Inflatable Module (JSC lead); Life Support Technologies (JSC lead); In-space Cryo Fluid Management (JSC lead); Biomedical Diagnostics (JSC lead); Telerobotic Ops from ISS (JSC as partner); Electron Beam Manufacturing (JSC as partner); Electric Propulsion (JSC as partner).

“Project M (Robonaut); JSC Engineering led project proposal for a robotic Lunar mission.”

Project M is a good horse for MOD to back, with STS-133 – a mission which obviously has heavy MOD involvement – launching a Robonaut to the International Space Station later this year, as a precursor to a fascinating mission that will result in a fully formed Robonaut setting foot on the lunar surface “in 1000 days”.

The MOD All Hands materials also provide an insight into draft roadmap for inflatables, with development from 2011 to 2017, resulting in an ultimate goal of providing the ability to support human exploration via inflatable transport modules and surface habitation.

“Ground Development: Integrated system fleet leader Ground testing. Integration of key technologies developed by partners to ensure performance in required environments. Sub-scale demonstration of key enabling technologies while providing ISS expanded capability,” opened the roadmap overview.

The draft overview also listed the first flagship role would involve the orbital outpost, with a date of around 2015 cited.

“Flagship inflatable Habitat Test Vehicle. Demonstrate integrated technologies required for self-sustaining habitation,” which may provide rationale for what is currently being planned as Node 4, which – while unconfirmed – could provide a home for inflatable modules.

Node 4 – otherwise known as the Docking Hub System (DHS) – is currently being baselined as launching on a medium EELV (Evolved Expendable Launch Vehicle) – likely to be a 5×1 variant of an Atlas V, but potentially a Delta IV – in tandem with a yet-to-be-decided “Tug”, possibly utilizing the ARDV (Autonomous Rendezvous & Docking Vehicle) concept, which could be launched on an Atlas V.

The roadmap continues through to an ultimate goal of providing a role with the future Mars missions, benefiting from parallel work under the Enabling Technology Development & Demonstration (ETDD) Program.

“Beyond Earth Orbit (BEO) Extreme Thermal / Radiation Environment. Cruise Environment, Remote Deploy, Long-term self-sustaining,” added the roadmap. “Provide long duration habitation for missions beyond LEO for interplanetary transit and surface habitation.”

Such plans remain notional until NASA’s future has been confirmed by lawmakers and the Agency’s administration, with the main item on MOD’s wish-list relating to ensuring they “have a seat at the table”, and being involved as much as they were with the Constellation Program (CxP)

“MOD Engagement: Agency wrestling with difficult challenges – multiple teams doing project formulation, budgets, Congress, OMB, OSTP, White House. JSC formed an Advanced Development Office to coordinate involvement in all technology projects/ MOD formed a team to engage in all the appropriate technology areas,” added the presentations.

“Our intent is to capture the P/T/F work for those missions that we can do best. We also want to be involved in the mission and vehicle design and development aspects much like we were for Cx (Constellation). 48 MODers are serving as POCs to all of the areas. Additional people are supporting from within MOD. Getting engaged with JSC and other Center teams. Getting a seat at the table and speaking for ourselves.”

Aiding MOD’s vision of the future will be aided by JSC’s central role with the Exploration Precursor Robotic Missions, and the building on ties with the Jet Propulsion Laboratory (JPL) in California for the proposed Near Earth Orbit (NEO) missions. The goal is to gear up towards an October start date – though this is at the mercy of decisions at the Agency and political levels.

“What Has MOD Accomplished So Far? The POCs have done an outstanding job of engaging and participating. Most interactions with project teams are very positive and productive. We participated in Request for Information (RFI) responses. We are collecting and publishing real-world examples of MOD’s value in project design and operations,” added the presentations.

“We assumed JSC leadership for Exploration Precursor Robotic Missions. We have a very strong partnership with JPL for NEO missions. We brought the ISS-based cryo fluid demo ops work to MCC/ Firm decisions won’t come until August/September as the RFPs are completed. Project work is planned to start on October 1, but there’s a lot that has to come together across the Agency to make that happen.

“Success will come in small steps.”

pixelstats trackingpixel

No related posts.

Long March launches fifth GPS satellite for China

Posted on 1st August 2010 by admin in Space Flight

China launched its fifth satellite as part of its GPS satellite navigation system, with BeiDou-2 IGSO-1 placed into orbit via the CZ-3A Chang Zheng-3A (CZ3A-17/Y16) launch vehicle. Launch from the Xi Chang Satellite Launch Center, in Sichuan Province occured at 5:30am local time on Sunday.

Chinese Launch:

The satellite that was launched is the first BeiDou-2 IGSO (Inclined GSO) satellite of the system. This constellation of satellites will eventually consist of 35 vehicles, including 27 MEO satellites, 5 GSO satellites and 3 IGSO.

The satellites will transmit signals on the following carrier frequencies: 1195.14-1219.14MHz, 1256.52-1280.52MHz, 1559.05-1563.15MHz and 1587.69-1591.79MHz, notably overlaying the Galileo PRS band and the GPS M-code.

According to International Telecommunications Union (ITU) regulations, the frequencies have to be used within a certain time period. The priority for using the frequencies is given in order of reception of the requests at ITU, made seven years in advance.

The BeiDou-2 was developed in the basis of the DFH-3 satellite platform and has a lifespan of 8 years.

The Compass Navigation Satellite System (CNSS) is China’s second-generation satellite navigation system capable of providing continuous, real-time passive 3D geo-spatial positioning and speed measurement.

The system will initially used to provide high-accuracy positioning services for users in China and its neighboring regions, covering an area of about 120 degrees longitude in the Northern Hemisphere. The long-term goal is to develop a global navigation satellite network similar to the GPS and GLONASS.

Like their American and Russian counterparts, CNSS will have two types of services; a civilian service that will provide an accuracy of 10 meters in the user position, 0.2 m/s on the user velocity and 50 nanoseconds in time accuracy; and the military and authorized users service, providing greater accuracy.

The first phase of the project will provide for the coverage of the Chinese territory, ahead of the future use of the Compass constellation for the entire globe.

Previous BeiDou satellites were launched on October 30, 2000 ‘BeiDou-1A’ (Catalogue Number: 26599 International Designation: 2000-069A); December 20, 2000 ‘BeiDou-1B’ (26643 2000-082A); May 24, 2003 ‘BeiDou-1C’ (27813 2003-021A); February 2, 2007 ‘BeiDou-1D’ (30323 2007-003A); April 13, 2007 ‘BeiDou-2 Compass-M1′ (31115 2007-011A); April 14, 2009 ‘BeiDou-2 Compass-G2′ (34779 2009-018A), January 16 ‘BeiDou-2 Compass-G1′ (36287 2010-001A) and June 2, 1010 ‘BeiDou-2 Compass-G3′ (36590 2010-024A).

China used their CZ-3A Chang Zheng-3A launch vehicle to loft BeiDou-2 IGSO-1 uphill. The CZ-3A is a large-scale three-stage liquid launch vehicle, which has inherited the matured technology of the CZ-3 Chang Zheng-3.

An upgraded liquid hydrogen and liquid oxygen cryogenic third stage has been developed to enable CZ-3A performing greater geostationary transfer orbit (GTO) capability. The CZ-3A is equipped with a more flexible and sophisticated control system which supports substantial attitude adjustments to orient the payloads before spacecraft separation and provides adjustable satellite spin-up rotation rate.

It has paved the way for the development of CZ-3B Chang Zheng-3B and CZ-3C Chang Zheng-3C, and become the workhorse of GTO launches for China.

The CZ-3A can also be used for LEO, SSO and polar orbit missions, as well as dual-launch and multiple-launch missions. The launch capacity of the CZ-3A to GTO is 2.650 kg, the lift-off mass is 241.000 kg, the overall length is 52.5 meters, the diameter of first stage and second stage is 3.35 meters, the diameter of third stage is 3.0 meters, and the maximum fairing diameter is 3.35 meters.

The first stage and second stage of CZ-3A employ storable propellants, i.e. unsymmetrical dimethy1 hydrazine (UDMH) and nitrogen tetroxide (N2O4), and the third stage uses cryogenic propellants, i.e. liquid hydrogen (LH2) and liquid oxygen (LOX).

On the first stage, the CZ-3A uses a DaFY6-2 engine with a 2961.6 kN thrust, while the second stage is equipped with a DaFY20-1 main engine (742 kN) and four DaFY21-1 vernier engines (11.8 kN each). The third stage is equipped with two YF-75 engines (78.5 kN each).

The fairing diameter of the CZ-3A is 3,35 meters and has a length of 8.89 meters.

CZ-3A consists of rocket structure, propulsion system, control system, telemetry system, tracking and safely system, coast phase propellant management and attitude control system, cryogenic propellant utilization system, separation system and auxiliary system, etc.

The CZ-3A has a 100 percent launch success rate since its maiden flight on February 8, 1994 when it successfully launched two experimental satellites. And it was awarded the ‘Gold Launch Vehicle’ title by China Aerospace Science and Technology Corporation in June 2007.

China used a CZ-3A to successfully launch the Chang’e-1 lunar satellite on October 24, 2007, which indicated that has taken a substantial step for lunar exploration.

This was the 125th successful Chinese orbital launch, the 124th launch of a Chang Zheng launch vehicle, the 54th successful orbital launch from the Xi Chang Satellite Launch Center, the third successful orbital launch from the Xi Chang in 2010 and the fifth successful orbital launch from China in 2010.

The Xi Chang Satellite Launch Centre is situated in the Sichuan Province, south-western China and is the country’s launch site for geosynchronous orbital launches.

Equipped with two launch pads (LC2 and LC3), the centre has a dedicated railway and highway lead directly to the launch site. The Command and Control Centre is located seven kilometers south-west of the launch pad, providing flight and safety control during launch rehearsal and launch.

Other facilities on the Xi Chang Satellite Launch Centre are the Launch Control Centre, propellant fuelling systems, communications systems for launch command, telephone and data communications for users, and support equipment for meteorological monitoring and forecasting.

The first launch from Xi Chang took place at 12:25UTC on January 29, 1984, when the CZ-3 Chang Zheng-3 (CZ3-1) launched the Shiyan Weixing (14670 1984-008A) communications satellite into orbit. The launch of the new BeiDou-2 satellite was the 52nd successful orbital launch from Xi Chang.

Launch image: Xinhua/Du Cai

pixelstats trackingpixel

Related posts:

  1. China opens 2010 with BeiDou-2 satellite launch The Chinese have opened their 2010 campaign by orbiting a…
  2. China launch meteorological satellite Fengyun-2-06 China has launched a new meteorological satellite from its Xi…
  3. China orbits YaoGan-5 satellite via Chang Zheng-4B launch vehicle China has launched a new remote sensing satellite from the…

Diligent to the end – Endeavour’s engineers spot 0.005 inch FCV defect

Posted on 1st August 2010 by admin in Space Flight

Space Shuttle Program (SSP) manager John Shannon has praised the team responsible for installing the Flow Control Valves (FCVs) on Endeavour, after they spotted a 0.005 inch shim was missing from one of the three valves. Endeavour – processing for next year’s STS-134 – wouldn’t of suffered from any ill effects, had she launched with the since-replaced FCV.

STS-134 Processing Latest:

Endeavour is being processed inside her OPF-2 (Orbiter Processing Facility), ahead of her February, 2011 mission to carry the Alpha Magnetic Spectrometer (AMS-2) and Express Logistics Carrier 3 (ELC-3) to the International Space Station (ISS).

The 15,300lbs AMS-02 unit will undergo a milestone review next week, based on the changes made since engineers decided to replace the cryogenic super-fluid helium superconducting magnet with a permanent alternative – the reason the launch date slipped down the manifest.

“There will be a Delta Compatibility Review on August 6 for the AMS payload to ensure that all the changes made are still consistent with our engineering and their mission profile,” noted Flight Operations and Integration on the latest Shuttle Standup/Integration report (L2).

All three of her Space Shuttle Main Engines (SSMEs) were installed by Thursday of last week, and are now being put through closeout and interface procedures. Endeavour is currently enjoying the weekend off.

“OV-105 (OPF Bay 2): OIU (Orbiter Interface Unit) verification was successfully completed. SSME #2 was installed; all three engines are now installed. Closeouts continue,” noted the NASA Test Director (NTD) processing report (L2), which mentioned ongoing testing on the Orbiter Boom Sensor System (OBSS), which will remain with the ISS after Endeavour undocks.

“OBSS keep alive test was completed. SPEE premate testing was started and will resume once adapter cables are routed from Bay 3. Weekend work: None scheduled.”

Over in the Vehicle Assembly Building (VAB), engineers are stacking the twin Solid Rocket Boosters (SRBs) in High Bay 1 (HB-1), while External Tank (ET-138) continues it’s “shakedown” operations in HB-2E’s checkout cell.

“SRB BI-145 / RSRM 113 (VAB HB-1): L/R (Left/Right) Stud Tensioning; Need RT-455 pull test results. ETAR foam repair; PDL repair complete less closure. LA Joint Closeout; Cork pull test complete, on hold for PR (Problem Report) on ‘D’ dimension tool,” added the NTD report.

“ET-138 (VAB HB-2E): Bond Adhesion test repairs PDL (foam) application, trim and sand and final acceptance are complete, to engineering pre scaffold removal walkdown.”

STS-134 Specific Articles: http://www.nasaspaceflight.com/tag/sts-134/

Flow Control Valve Spot:

Most Shuttle followers will be only too aware of how the Flow Control Valves (FCVs) became an item of great interest, following the liberation of part of a valve’s poppet during Endeavour’s STS-126 launch in November 2008.

The finding led to the immediate inspection of the FCVs throughout the fleet, highlighted by Special Program Requirements Control Board (SPRCB) meetings and Flight Readiness Review (FRR) debates ahead of Discovery’s STS-119 mission.

The GH2 FCVs – of which there is one per SSME – are designed to provide the proper amount of pressurized GH2, while maintaining the ET LH2 tank flight pressurization limits.

However, one of the main concerns related to the potential of a large enough piece of the poppet liberating from the valve and impacting the downstream 90 degree elbow in the Main Propulsion System (MPS), which may cause an undesirable GH2 leak into the aft compartment.

FCV Specific Articles (Extensive): http://www.nasaspaceflight.com/tag/FCV/

Subsequent reviews of all FCV flight history and risk information revealed that the overall likelihood of a FCV poppet failure in flight is low. All the FCVs that have flown since have also undergone Non Destructive Evaluation (NDE) eddy current inspections, in order to spot any potential cracks forming in the valves prior to installation.

With no notable issues recorded by the valves since STS-126, the SPRCB and FRR conclusions and mitigation plans have again been proved to be correct. However, they are backed by highly experienced hands-on engineering teams at the Kennedy Space Center (KSC), who need to keep their eye on the ball at all times, and not just on areas of recent interest.

An example of their diligence was noted when one FCV on Endeavour was rejected via a tolerance problem, a five thousands-of-an-inch deviation from nominal, about the width of a sheet of paper.

“During installation of FCVs on OV-105 (Endeavour), one of the units failed an installation dimension requirement check,” noted the Orbiter Project Office (OPO) on the latest Standup report, noting the valve was sent back to its fabricator in California, who found the valve was missing one of its numerous – yet tiny – shims.

“That unit was sent back to the vendor where it was discovered that a 0.005 inch shim was missing. Orbiter is in the process of evaluating all the remaining units coming out of the vendor that have the proper configuration, and are confident that the units on the vehicle are in the proper configuration because they all passed the same installation dimension requirement check.”

A replacement valve has since been installed into Endeavour over the past few days and passed “mass spec” checks, confirming the new valve isn’t suffering from the same issue.

The spot earned praise from Mr Shannon on the Standup report, showing the teams are remaining extremely focused during what is a difficult time for the Program, with continuing lay-offs and uncertainty about the future after the fleet retires.

“Mr. Shannon said it was a good catch by the team installing the FCVs finding the tolerance problem; that is the way we want to do business,” he was noted as saying at the Standup meeting, before adding a message about the recent notices that informed nearly 1,500 workers they would lose their jobs in October.

“Please be compassionate and understanding as people’s lives are going to change, and we must still concentrate on getting the mission ahead of us done. It is vitally important that we do that, but it is a tough time for a lot of our team members. Please be aware of that and be compassionate about that.”

pixelstats trackingpixel

No related posts.

Engineers find a flexible solution for Discovery’s S-Band antenna cable

Posted on 30th July 2010 by admin in Space Flight

After it was revealed that several replacement S-Band antenna cables were found to be  ”too short”, Discovery’s engineers have opted to install an alternative type of cable. The flexible alternative was used to mitigate the issues surrounding the routing of the long cable through the tight pathways of Discovery’s middeck, which proved to be problemative with the original semi-rigid cables.

STS-133 Processing Latest:

No time is being lost in Discovery’s STS-133 flow, as processing is continuing unhindered. The orbiter still has around a month and a half of time remaining in her Orbiter Processing Facility (OPF-3) until she’s due to rollover to the Vehicle Assembly Building (VAB) for mating.

Integrated hydraulic testing was completed by the end of last week, while midbody “p-frame” installation and TPS (Thermal Protection System) work was conducted over the weekend.

“OV-103 (OPF Bay 3): APU (Auxiliary Power Units) 1, 2, and 3 gearbox pressurization is complete. The Freon coolant loop top-off was successfully completed Tuesday. SSOR (Space to Space Radio) retest was completed Tuesday. SSME (Space Shuttle Main Engine) dome heat shield installations are complete,” added the NASA Test Director (NTD) processing update (L2).

An Interim Problem Report (IPR) was charged to the STS-133 flow during recent OMS (Orbital Maneuvering System) work, relating to a failed vacuum leak check. However, the procedure was completed due to a known effect in the system that can relate to the leak rates.

“New IPR 0032 to COOS (Call sign of Fuel Systems Engineers): During oxidizer cross feed line eduction, the vacuum leak check failed. COOS stated there is a known leakage in with the OMS cross-feed lines that can affect the vacuum leak rate,” added the NTD report. “A dev was written to delete the step, and the line eduction was completed.”

Two further IPRs – one related to Discovery’s brake pressure on her right outboard Main Landing Gear (MLG), and another on her KU-band system – require further troubleshooting.

STS-133 Specific Articles: http://www.nasaspaceflight.com/tag/sts-133/

“New IPR 0033: During data review, right outboard brake pressure No. 2 was found to be off-scale high (2000 PSIA). Troubleshooting plan is to inspect and de-pin terminal board on Right Outboard MLG, then inject signal and verify proper response.

“New IPR 0034: Picked up during Orbiter KU-band DTV testing. Comm and Tracking could not get a signal lock. This is a constraint to continuing. Engineering troubleshooting is in work.”

This issue is not believed to be related to the primary problem suffered Discovery during her STS-131 Ku-Band troubles, which resulted in the loss of the Ku-Band communications high speed uplink and downlink capability. That issue has already been resolved via troubleshooting upon her return to the OPF.

The root cause of the issue was tracked back to a fault with the Deployed Assembly (DA) unit, which has since been removed and replaced.

Although it was only classed as a minor issue, engineers have all-but resolved IPR-5 – related to S-band troubleshooting (May 7) – called for after erratic readings were observed during STS-131.

With the engineering resolution centering around the replacement of a coax cable in the middeck, several spares were found to be too short – likely based around the challenges of routing a semi-rigid cable in what is a complex routing pattern in the orbiter.

All the S-band RF units are located in Avionics bay 3A which is at the right-hand rear of the middeck. With the antenna located on the upper left side of the forward fuselage – close to the payload bay cabin bulkhead – the total length of the cable is relatively long.

“Determined that replacing the coax cable with a flexible coax was selected as the best option. There are three similar length flexible coax in existing stock.” noted the updated processing reports. “A fit check was performed on Friday and found the best fit would be a 30″ flexible coax cable.

“The installation will be very straight forward by using an existing coax clamp that has room for one more coax and is attached to the wire tray. Installation of the coax is planned for Tuesday, with retest on Wednesday.”

As of Wednesday, the NTD confirmed the new cable was in place, and was undergoing the associated WLAN retest – (Thursday UPDATE) – which was successfully completed.

Meanwhile, the repair work on a Fairing Support Plate on the mated External Tank (ET-137) and Solid Rocket Boosters (SRBs) is proceeding in High Bay 3 (HB-3) of the Vehicle Assembly Building (VAB).

“Damaged SLA On EB-2 Fairing Support Plate: Hand pack cure and trim, and final acceptance are complete. Issue 2, (outboard SLA ear application on EB-2 is cracked full width across the closeout s/b no cracks). Removal of discrepant SLA, measurements and photo’s are complete,” added the NTD – (Thursday UPDATE) with the forward plan to carry out the repair on the second area.

“L/R (Left/Right) Forward Crossover; RH ET Fairing cover will be worked when damaged SLA PR (Problem Report) repair is complete.”

pixelstats trackingpixel

No related posts.