The name Aaqil is a baby boy name.

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Muslim Meaning:
The name Aaqil is a Muslim baby name. In Muslim the meaning of the name Aaqil is: Intellectual. Wise.

SoulUrge Number: 11

People with this name have a deep inner desire to inspire others in a higher cause, and to share their own strongly held views on spiritual matters.

Expression Number: 22

People with this name tend to be a powerful force to all whose lives they touch. They are capable, charismatic leaders who often undertake large endeavors with great success. They value truth, justice, and discipline, and may be quick-tempered with those who do not. If they fail to develop their potential, they may become impractical and rigid.


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But the Centaur would go on to perform two more burns and successfully deploy the MUOS 1 satellite three hours after liftoff.See a from the launch. Sunset from Centaur camera.Additional coverage for subscribers:VIDEO:ATLAS 5 ROCKET BLASTS OFF WITH MUOS 1 VIDEO:LAUNCH REPLAY: ATLAS 5 ROCKET SOARS DOWNRANGE VIDEO:LAUNCH REPLAY: BEACH MOUND CAMERA VIDEO:LAUNCH REPLAY: UP-CLOSE PAD VIEW VIDEO:LAUNCH REPLAY: VIF ROOF VIDEO:ATLAS ROLLED BACK TO ASSEMBLY BUILDING VIDEO:WEATHER SCRUBS SECOND LAUNCH ATTEMPT VIDEO:COUNTDOWN SCRUBBED AT T-75 SECONDS VIDEO:NARRATED PREVIEW OF ATLAS/MUOS LAUNCH VIDEO:ATLAS 5 ROCKET ROLLED OUT TO LAUNCH PAD STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. 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The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.New Navy satellite spreads wings, antennas in orbit SPACEFLIGHT NOWPosted: August 2, 2013 The massive U.S. Navy communications satellite launched from Cape Canaveral two weeks ago has completed prescribed maneuvers to reach geosynchronous orbit and successfully unfurled its umbrella-like antenna reflectors. An artist's concept of MUOS. Credit: Lockheed MartinCheckouts of the spacecraft that are expected to last several months are getting underway high above the Pacific Ocean testing location before the bird will be declared ready for service.The craft will be capable of covering nearly a third of the planet to provide mobile communications to U.S. warfighters on the move."Currently, all systems are working normally," said Steven A. Davis of the Space and Naval Warfare Systems Command.The Mobile User Objective System satellite No. 2 was lofted into space July 19 by the United Launch Alliance Atlas 5 rocket, achieving a highly elliptical preliminary orbit as planned.From there, the Lockheed Martin-built satellite performed a series of 7 engine firings to circularize the orbit and reduce its orbital tilt closer to the equator. The burns, which ranged from 23 to 52 minutes in length, put the spacecraft into the proper geosynchronous orbit 22,300 miles up. The orbit was reached on July 31, and the following 36 hours saw the spacecraft achieve its "flight configuration" by executing critical deployments of the power-generating solar wings that now stretch 94 feet tip-to-tip and two gold mesh, umbrella-like antenna reflectors.The antennas provide the same type of Ulta High Frequency communications like previous Navy spacecraft and the other offers modernized capabilities that the new MUOS system will create.Coverage to legacy users will transmit through a 17.7-foot-diameter reflector on the bottom of the craft and the advanced, multi-beam features of MUOS to significantly increase the transmission capacity over the Navy's previous satellites will use a large 46-foot reflector atop MUOS.All U.S. military forces rely upon Navy satellites for Ultra High Frequency narrowband communications. 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Credit: Lockheed MartinDestined for a classified position somewhere in orbit 22,300 miles above the planet, the Air Force's second Space Based Infrared System Geosynchronous satellite, known as SBIRS GEO 2 for short, will further upgrade the nation's surveillance network to detect and track missile launches around the globe."Our ability to provide strategic missile warning is critical to the nation's survival," says Gen. William Shelton, leader of Air Force Space Command.Devised in the Cold War to provide warning of intercontinental ballistic missiles launched at the U.S., this national security space project has broadened to cover short-range missiles and threats facing troops on the modern day battlefield."I would argue that the nation's missile warning system is critical now, or perhaps even more so, than it was even during Cold War," said Col. 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An artist's concept depicts a notional constellation of DSP, SBIRS GEO and SBIRS HEO platforms. Credit: Lockheed MartinThe first highly elliptical orbit hosted payload, known as HEO 1, finally went into space from Vandenberg Air Force Base, Calif., in 2006, a full decade into the development effort. HEO 2 followed from Vandenberg in 2008.Getting the first GEO off the ground from Cape Canaveral came in May 2011, bringing the modernized enhancements to the surveillance network.The second GEO awaits blastoff from the Cape on Tuesday at 5:21 p.m. EDT. ()GEO 1 has gone through rigorous testing and trial runs to prove its data can be trusted, and project officials say it should be fully accepted into the operational fleet later this year."Based on GEO 1's on-orbit performance to date, we expect GEO 2 to also provide exceptional improvements to global and theater mission capabilities to our warfighters and the nation," Planeaux said.Lockheed Martin is building four GEO satellites and four HEO payloads, and anticipates beginning production of GEOs 5 and 6 this year, to replenish the orbiting constellation as aging DSP spacecraft fade out. The military won't say exactly how many remain in service."SBIRS improved sensor technology and ground processing capabilities enable us to respond to growing needs, evolving threats, and will serve us as the foundation of the nation's overhead infrared constellation for many, many years to come," Planeaux said. The shrouded GEO 2 is hoisted atop the Atlas 5. Credit: United Launch AllianceThe GEO 2 satellite was mounted atop the Atlas rocket on March 7, allowing the integrated systems test between the duo to be performed successfully. This past week was spent installing ordnance, closing out the rocket's payload shroud and buttoning up the vehicle's other compartments.Mission managers conducted their launch readiness review at the Cape on Friday morning and granted approval for Monday's 10 a.m. EDT rollout of the Atlas 5 rocket from its assembly building to the pad at Complex 41.Tuesday's countdown will start ticking just after 10 a.m. EDT, followed by the loading of liquid oxygen and liquid hydrogen into the rocket a little after 3 p.m. EDT.The day's launch opportunity opens at 5:21 p.m. EDT (2121 GMT) and extends 40 minutes to 6:01 p.m. The window moves four minutes earlier if the liftoff is bumped back to Wednesday for some reason.Weather forecasters predict a 70 percent chance of acceptable conditions during Tuesday's window.It will mark the 37th launch of an Atlas 5 booster in the past decade, the 17th in the 401 configuration with a four-meter nose cone and no strap-on solid motors and the fourth Atlas flight in four months. It also represents United Launch Alliance's 69th mission in six years and the 29th using an Atlas 5.The previous SBIRS GEO 1 was entrusted to fly on Atlas and GEO 2 is the rocket's 12th launch for the Defense Department. Including NRO satellite deployments, this is the vehicle's 19th in service to U.S. national security payloads.The launch of GEO 2 will "take another big step in delivering the next generation of Air Force infrared surveillance capability," Planeaux said."While our current constellation of Defense Support Program satellites has served the nation and our allies well for over 40 years, SBIRS is bringing unprecedented new capabilities into service to support our mission areas, which are missile warning, missile defense, technical intelligence and battlespace awareness." An illustration shows the SBIRS GEO sensor systems. Credit: Lockheed MartinWeighing about 10,000 pounds at launch, the satellite will be injected by the Atlas 5 into a standard geosynchronous transfer orbit with a high point of 22,237 statute miles, low point of 115 miles and inclination of 22 degrees to the equator. Separation of the spacecraft from the rocket occurs about 43 minutes after liftoff.From there, ground controllers will spend about 9 days performing 6 firings of the craft's main engine to circularize the orbit before deploying the appendages and commencing the testing campaign."We are obviously very excited for the launch, we're also challenging our team and we're confident we can do this, to achieve the (satellite's) checkout and certification in a little over 6 months," Planeaux said.Built around Lockheed Martin's commercial A2100 satellite platform, with a 12-year design life, the craft is a clone of the GEO 1, having been built at the same time using the same parts. The birds are equipped with RH-32 radiation-hardened single board computers with reloadable flight software.After deploying its pair of power-producing solar arrays for 2,800 watts, GEO 2 will have a wing span of 49 feet. The craft also extends a light shade for the payload and unfolds gimbaled communications antennas for secure, spot beam transmissions.Its scanner and starer instruments, amounting to 1,000 pounds of hardware, have highly agile pointing mirrors and dual infrared sensors that feature short wave, mid wave and see-to-ground spectral band assemblies."At a time when this capability is more vital than ever, the addition of GEO 2 will further enhance our nation's capabilities for early warning detection of ballistic missile launches around the globe, support our nation's ballistic missile defense system, greatly expand our technical intelligence-gathering capability and provide enhanced situational awareness for warfighters on the battlefield," said Dave Sheridan, Lockheed Martin's SBIRS program director in Sunnyvale, Calif.Integration of the sensors and satellite for GEO 3 will be finished next year for launch in 2015, with GEO 4 following along about a year later in the sequence. 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Credit: Chris Miller/Spaceflight NowSky-watchers say the government has relay satellite networks flying the highly elliptical orbits as well as geosynchronous orbit around the planet's equator.Early versions of these relay craft were launched starting in the mid-1970s, followed by a second-generation of satellites that were carried aloft on space shuttle missions in 1989, 1990 and 1992 and a Titan 4 rocket in 1996.Atlas rockets deployed more-recent craft for the Satellite Data System program toward a Molniya-style orbit in January 1998 and August 2004, and toward a geosynchronous orbit in December 2000 and October 2001.Monday's ascent took a northeast trajectory off the launch pad similar to the earlier Atlas missions bound for a Molniya orbit, and experts say the liftoff appeared timed to intercept the orbit occupied by the aging satellite lofted by the Titan a dozen years ago.Launch photos can be seen .It was the 12th flight for an Atlas 5 rocket and the fourth this year. 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Credit: Pat Corkery/ULAThe 19-story booster blasted off at 5:35 p.m. EDT, the first moment of theday's launch opportunity that punctuated a trouble-free countdown.The rocket's nose cone, adorned with Lockheed Martin's corporate logo,shrouded the payload as it climbed through the atmosphere and out ofsight.The company acknowledged that it had built the communications satellite -- dubbed "PAN" -- under a commercial arrangement with the government. Yet few other details werereleased, such as what agency was behind the project or what it would do in orbit."Lockheed Martin is the prime contractor for the PAN mission, whichincludes a commercial-based satellite and launch system solution for theU.S. government," a Lockheed Martin statement released to Spaceflight Nowsaid.Within 18 minutes, the Centaur upper stage turned off its main engine andsettled into an initial parking orbit where it would coast away from theplanet for 98 minutes.A group of respected sky-watchers around the world who track satelliteswith remarkable precision and communicate their findings amongst eachother online eagerly awaited Tuesday's launch and a chance to test theirpre-flight guesses against reality.The leading theory suggested PAN was a quick-build satellite that wouldserve as a communications gap-filler between the aging constellation ofUltra-High Frequency Follow-On (UFO) spacecraft and the sophisticated next-generationMobile User Objective System that's still being developed.Some 34 minutes after the Atlas launched from Florida, observer Greg Roberts, aretired astronomer living in Cape Town, South Africa, detected "a strongbeacon signal" being emitted from the PAN satellite as it crossed his sky."The time, general location of the signal in the sky, and its Dopplershift were consistent with the expected parking orbit," said Ted Molczan,a noted member of the trackers.For 14 minutes, Roberts heard the passing satellite transmitting a frequency unique to the UFO spacecraft. He had to cut the session short due to bad weather, but the hobbyists immediately knew their speculation was proving well founded. "We know of no other U.S. satellites in geostationary orbit that use thatfrequency, so Greg's observation tends to support the UFO-MUOS gap-filler hypothesis," Molczan said.Roberts, like others in the small international group of hobbyists whofind and watch satellites in secret orbits, does his observing usingtelescopic still and video cameras, and radio receivers.The east-bound trajectory sent the Atlas into an elliptical geosynchronoustransfer orbit, though the power provided by the rocket coupled with thepayload's relatively slim weight, estimated by the observers to be approximately 7,700 pounds, enabled a higher perigee, or low point, than other such launches.A second firing of the Centaur propelled PAN into its targeted deploymentorbit with an apogee of 22,230 miles and a perigee of 4,550 miles. The payload's release an hour and 59 minutes after liftoff successfully completed the ascent."The secrecy surrounding PAN may be a clue to the identity of itssponsoring agency. It appears not to belong to the DoD, given that its UFOand MUOS are open programs, as was the U.S. Navy's 'UHF Hosted Payload'gap-filler solution, which it briefly considered in 2008," Molczan said."The most likely remaining possibility is that a civilian intelligenceagency, perhaps the CIA, decided much earlier, about 2005-06, that itcould not risk a coverage gap, and obtained approval to rapidly procureand launch a satellite compatible with the UFO satellites," Molczan added.An article in a Lockheed Martin newsletter, entitled "A small andpersistent team turns a great idea into an important new U.S. program" andpublished in the spring of 2007, said its Special Programs had started thePAN mission, also known as the P360 project."The team's innovative turnkey commercial-based satellite, ground andlaunch system solution established the foundation for a new governmentarchitecture. The team functions across time zones from Space SystemsCompany in Sunnyvale, Calif., to Commercial Space in Newtown, Pa.,Lockheed Martin Information Systems & Global Services in San Jose, Calif.,Integral Systems in Lanham, Md., as well as Lockheed Martin divisionsabroad. United Launch Alliance in Denver, Colo., rounds out thecontributors with the Atlas 5 launch vehicle," the article continued."Following several years of concept development, market analysis, andfinally proposal submittal, the contract was awarded to Lockheed Martin inOctober 2006. The team has had successful system and preliminary designreviews and is on schedule for launch in 30 months from contract start."The observers plan to continue monitoring the moves of the satellite inthe coming weeks as it maneuvers into a circular geostationary orbit. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: March 22, 2005NASA finally has test data indicating any foam debris falling from the space shuttle's redesigned external fuel tank almost certainly will be below the threshold expected to cause "entry critical" damage to wing leading edge panels, officials said today.But with less than two months to go before Discovery's launch on thefirst post-Columbia shuttle mission, engineers are still assessing whetherworst-case foam debris impacts could cause entry critical damage to theorbiter's heat-shield tiles. The STS-114 astronauts pose in front of Discovery's redesigned external fuel tank. Credit: Lockheed MartinIn some areas, like certain places around the landing gear doors or thearea where external tank propellant lines enter the belly of the shuttle,worst-case impact damage could be potentially catastrophic.The results of ongoing tests and analyses will be discussed during adebris verification review in early April and a broader shuttle-wide designcertification review before flights resume in mid May.But NASA managers are optimistic test data and the results ofsophisticated computer modeling will show the tank's insulation does notpose a significant safety threat to the wing leading edges."If you think back to what we knew before Columbia and what we thoughtour vulnerabilities were and where we are now, it is clear that before wewere guessing and now we know, within a few fractions of a percent, exactlyhow vulnerable we are," deputy shuttle program manager Wayne Hale said in aninterview late today. "We've come a long way."Columbia was destroyed during re-entry Feb. 1, 2003, because of a hole inthe leading edge of the ship's left wing that was caused by a major foamdebris impact during launch 16 days earlier.NASA's primary rationale for returning the shuttle to flight this May isthe elimination of the foam in question, along with other design changepected to minimize the amount - and size - of any foam debris that mightshake loose or pop off other areas during launch.The shuttle's redesigned fuel tank has been modified to ensure no piecesof foam heavier than 0.023 pounds - 0.37 ounces - can break away from theupper portions of the tank during launch.Debris from the upper part of the tank poses the greatest threat to theship's nose cap and reinforced carbon carbon leading edge panels, whichexperience the most intense heat during re-entry. The 0.023-pound limit isfor foam covering the liquid oxygen tank at the very top of the structure.Foam from the intertank area, where bipod struts attach the nose of theshuttle and where the foam originated that doomed Columbia, can be slightlymore massive: 0.03 pounds, or 0.48 ounces. Pieces of foam from the bottom ofthe tank pose less of a threat and thus can be larger still: up to 0.75pounds. These artist's concepts show the previous bipod foam design (top) and the new configuration for the post-Columbia era (below). Credit: Lockheed MartinA major question as the shuttle Discovery's May 15 launch targetapproaches has been whether foam in that range of sizes from the top of thetank could cause the kind of wing leading edge damage during ascent thatcould threaten a shuttle during re-entry.To the surprise of many, recent testing showed major cracks or holes inleading edge panels are not required to bring down a space shuttle. Coatingdamage alone could do it, if the damage was in a particularly bad spot andif the impact that marred the coating also caused internal delamination.Small cracks and holes, obviously, also pose serious threats.The problem was in the testing. Using a nitrogen gas-powered cannon and awing leading edge mockup at the Southwest Research Institute in San Antonio,Texas, engineers were able to create entry critical damage from pieces offoam as small as 0.044 pounds - 0.7 ounces - depending on impact velocityand angle of incidence.But they were not immediately able to test down to the range of sizepected to be liberated from a redesigned fuel tank because smaller foambullets tended to come apart before hitting the leading edge panels.Steve Poulos, manager of the shuttle project office at the Johnson SpaceCenter, said in an interview today that those issues appear to have beenresolved and test data show the sort of debris that could be expected tofall off the redesigned tank would be below the critical damage threshold."We have done testing that exceeded the parameters to help us in thevalidation of our models: higher speeds, higher angles, differentgeometries," he said. "And in some of those instances we did do damage tothe panels and quite honestly, we expected to do it because (the impactenergy was) greater than 1,500 foot pounds."I'm not one to live in the world of assumptions," he said. "I'm a testperson. I've got empirical data where we've impacted the panel and wehaven't damaged it once below 1,250 foot pounds of kinetic energy."That's a measure of the impact energies expected during an actual launch."Recently, they've done testing down to very small masses, I think thelast number I heard, and I could be wrong, was about .02 pounds, .025, atvelocities on the order of 2,500 feet per second. And zero damage (wasseen)." NASA has conducted extensive RCC impact testing. This file image was taken during the Columbia investigation in June 2003. Credit: NASAPoulos discussed the impact testing immediately after attending a meetingto review what level of damage a new laser sensor will be able to detect inorbit if, despite the test results, an impact causes a crack or mars thesurface coating of a wing leading edge panel.The sensor, or laser dynamic range imager - LDRI - and a televisioncamera, both mounted on the end of a 50-boot boom, will be used during thesecond day of Discovery's mission to inspect the shuttle's nose cap and wingleading edge panels."I saw the latest certification level test results from the LDRI and itshows clearly the ability to detect down to as low as a 15 thousandths (ofan inch) crack," Poulos said. "Coating loss is easily detectable with thesesensors as is a crack. So there's no concern from the sensor perspective tobeing able to detect coating loss or a crack."All in all, he said, "there is nothing today that I have seen from theexternal tank data that gives me any pause or any concern about having anydamage at all on our RCC panels."He said NASA now has "sufficient capability, based on all the testingthat's been done at Southwest Research and the Glenn Research Center and theKennedy Space Center, to verify in my mind that we have sufficientcapability for what the tank is expected to liberate."But Hale cautioned that impact testing alone is not enough. Sophisticatedcomputer modeling also is required to predict how debris might behave afterit comes off the tank and moves into the airflow around the shuttle. Assuch, there is still room for debate in the upcoming design reviews."The transport mechanism, which is a key element in this, is a model, acomputer model of aerodynamics," he said. "We've done a lot of wind tunnelwork to try to make sure it's right, but it's a model. So we do have anongoing discussion about the validity of models and usefulness of models."If you state it in absolutely black-and-white terms, I think you willget some discussion whether this is proven to within the last decimal place.... I'm almost hesitant to say anything in black and white until thatreview. But you've got a sense of where we're going."The debris verification review is planned for the first week in April,just a few days after the shuttle Discovery's planned April 4 rollout to thelaunch pad at the Kennedy Space Center. Launch is targeted for May 15. Discovery is scheduled to be moved into the Vehicle Assembly Building next Monday, as depicted in this file photo, for mating to its external tank and solid rocket boosters. Rollout to the pad is slated for April 4. Credit: NASARollout had been planned for late this month, but engineers andtechnicians needed more time to complete final processing, eating into the12 days or so of on-pad contingency time managers had built into theschedule. An April 4 roll out will leave the team with just a few days ofspare time to handle unexpected problems and still make the May 15 target.NASA insiders say the launch date likely will slip up to a week or sowhen all is said and done, but shuttle program manager Bill Parsons saidtoday no decisions will be made until after Discovery reaches the launchpad."We've slipped a few things (but) we feel very comfortable with wherewe're at in the processing and the milestones we still have in front of us,"he said at a news briefing. "We probably need about 30 more days ofprocessing before we can really say whether we should slip the May 15thlaunch date or not. But that is the opening of the window and currently, ifeverything was to go all our way, we feel we can make that."In the wake of the Columbia disaster, an independent accident reviewboard made 29 recommendations to improve safety. NASA tracks its progressmeeting those recommendations in a formal document known as the shuttlereturn to flight implementation plan.The latest version was released today and it included a new approach toshuttle re-entries based on the expected risk to the public below theorbiter's flight path if a shuttle has known damage or flight controlissues.When Columbia broke apart above Texas, debris rained down along itsflight path stretching from just west of Fort Worth all the way intosouthwestern Louisiana. In what still ranks as a remarkable stroke of luck,no one on the ground was injured and property damage was minimal.But new flight rules are being developed to minimize that risk. The crewof any shuttle with known damage that could affect structural integrity orany other problems that might affect flight control will be directed to landat White Sands, N.M., one of NASA's backup landing sites. Only one previous shuttle mission has landed at White Sands. Columbia used the alternate site in 1982 for landing of STS-3. Credit: NASA"If there is some kind of problem with the shuttle, a loss of its flightcontrol redundancy, for example, or a threat to the structural integrity ofthe vehicle ... these flight rules will call for us to go to (White Sands),"said Bryan O'Connor, NASA's director of safety.Descents to White Sands carry the shuttle over less densely populatedareas than those to the Kennedy Space Center in Florida or Edwards Air ForceBase in California's Mojave Desert."On average, entry opportunities into KSC are half the public risk levelof entries into EAFB," according to the implementation plan. "On average,entry opportunities into WSMR (White Sands Missile Range) are one-sevenththe public risk level of EAFB and one-third the public risk level of KSC."But because White Sands does not have the infrastructure needed tosupport routine shuttle landings, the preferred landing site for undamagedorbiters will remain the Kennedy Space Center with Edwards as backup."The bottom line is that the orbiter will normally land at KSC,"according to the implementation plan. "But if it is compromised in a waythat poses a threat to the public, it will land at WSMR."Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Demating Discovery After rolling back to the Vehicle Assembly Building from launch pad 39B, technicians demate space shuttle Discovery and its original external fuel tank. Discovery will be attached with another tank and set of solid rocket boosters for the return-to-flight mission. The new tank has additional ice-fighting heaters and instrumentation. The shuttle goes back to the pad in mid-June for its planned mid-July liftoff. Credit: NASA-KSCAdditional coverage for subscribers:VIDEO:TECHNICIANS PREPARE DISCOVERY FOR DEMATING VIDEO:SHUTTLE DISCOVERY IS REMOVED FROM TANK Return to Flight crew patchThe official mission STS-114 emblem for space shuttle Discovery's seven astronauts includes a tribute to Columbia.Choose your store: - - - Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle's last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Detectors help guard against flaws in shuttle's tank foam UNIVERSITY OF FLORIDAPosted: March 9, 2005The engineers who built the massive external fuel tank that will power the shuttle Discovery into orbit this spring used sophisticated X-ray detectors developed by University of Florida researchers to reduce the chance of a defect in the foam insulation covering the tank. The detectors, first invented as a new technology to find land mines, can identify tiny gaps, or air-filled voids, in the insulating foam without causing any damage. It is believed that such a gap - possibly located between the foam and the tank's surface - caused a suitcase-sized piece of foam to break off during Columbia's liftoff in January 2003. The chunk struck the edge of the shuttle's left wing, seriously damaging it and spurring the shuttle's destruction during re-entry on Feb. 1. "We can do the inspection of the foam as it exists already sprayed onto the tank. We don't have to cut into it," said Warren Ussery, team leader for the return to flight nondestructive evaluation team at Lockheed Martin's Michoud Assembly Facility in New Orleans, where the shuttle's external tanks are manufactured. "We're able to find critical voids with that (the UF detector)."UF nuclear engineering professor Ed Dugan and retired UF nuclear engineering professor Alan Jacobs began experimenting with the modified "backscatter" X-ray detector several years ago as part of research aimed at engineering a more effective landmine detector. Conventional X-ray machines propel radiation through a target object to radiographic film on the other side. Different objects absorb X-rays to differing extents, so some show up more prominently on film than others. Backscatter X-ray machines were developed for circumstances when it is impossible to place film behind the object, as is the case with the shuttle tank. Contrasting conventional machines, they obtain images by capturing the radiation scattered "back" from the target.Dugan said conventional backscatter detectors select only the radiation -- which takes the form of photons - that has had a single collision with the target object. The detectors ignore "multiple-collision" photons, which may have hit the target several times, because with conventional image processing, they tend to cloud the image. One of the unique advantages of the UF-built machine is that it draws useful images from these multiple-collision photons, he said."There's a lot of good information in multiple-collision photons, but learning how to use it was not trivial," Dugan said. Twin detectors pick up photons from both single- and multiple-collision photons, with a computer merging the two using complicated computer-processing algorithms. In U.S. Army-sponsored tests, the technology proved adept at locating landmines, but the images were equally striking because they showed tiny empty spaces in the mines themselves."The photons would zip across the voids and bounce back," Dugan said. "It allowed us to tell mines from tree stumps and stones, because we had high intensity areas where the voids were."Jacobs and Dugan realized this capability made the detectors ideal for identifying flaws and defects in materials such as the carbon fiber used in airplanes without having to rip the material itself apart. The first tests of the concept, done on airplane frame members and small components, proved promising. After the Columbia disaster, word of the positive results led to an inquiry from Lockheed Martin.For preliminary testing purposes, the aerospace giant provided the UF researchers with sample chunks of fuel-tank foam containing known flaws as well as samples with unknown flaws. Some of the foam pieces were melded to the aluminum skin of the fuel tanks, while others consisted solely of foam. The UF detectors identified all significant flaws both within the foam and lying between the foam and the fuel tank skin."The flaws we found ranged from a quarter inch to 2 inches, and they were both de-laminations and voids," Dugan said.The defense contractor then purchased four of the roughly $100,000 scanners, while NASA bought one.Ussery said Lockheed has used the detectors, in tandem with a private company's scanning technology called tetrahertz imaging, to scrutinize the foam on a roughly 100-square-foot section of Discovery's external fuel tank as well as a back-up tank.That's a tiny swath of the overall tank, which is 154 feet long, 27.6 feet around and has a total area of 12,620 feet -- so large it has to be transported from New Orleans to Kennedy Space Center by ocean-going barge. However, the section, located on a ramp that protects instrumentation during flight, is covered with relatively thick foam applied by workers rather than machines. With parts as thick as 7 inches, versus 1 or 2 inches elsewhere, that raises the risk of an air bubble void.The foam chunk that broke off Columbia was also hand-applied. But in the new tank, the area where the mishap occurred -- a bipod fitting that connected the tank to the orbiter -- is no longer covered with foam. Instead, heaters do the job the foam once performed.Ussery said Lockheed engineers scan about 1 square foot per hour using the backscatter X-ray machine. The machine can work about at about twice that speed, but the image resolution and ability to detect small gaps declines at high speeds, Dugan said. Lockheed engineers used the machine to seek out flaws near the surface of the foam, while they employed the tetrahertz imaging machines to probe deeper. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: September 4, 2006 Credit: NASA-KSCNASA managers today agreed to make three consecutive attempts to get the shuttle Atlantis off the ground if bad weather or technical problems prevent an on-time liftoff Wednesday.The forecast calls for an 80 percent chance of good weather Wednesday, decreasing to 70 percent "go" Thursday and Friday. If Atlantis isn't off the ground by Friday, the flight will be delayed to late October, barring a decision to relax NASA's current daylight launch requirement.The space agency normally gives the launch team a day off after two straight attempts but given the high stakes involved, and the impact of a major delay on NASA's plans to resume station assembly, the launch team agreed to make three attempts in a row if necessary.Liftoff Wednesday is targeted for 12:29 p.m., a week and a half behind schedule because of a launch pad lightning strike and delays caused by tropical storm/depression Ernesto."We certainly had our share of tropical weather, or at least the potential for tropical weather the last week or two, which put us a little behind in the schedule," said shuttle program manager Wayne Hale. "However, in the bigger scheme of things, a week or so waiting out the weather will not cause us any concern."We have a good shot at three consecutive launch dates coming up the middle of this week. We owe this to the really hard work from the launch team that spent not just today, the Labor Day holiday out here working, but the whole weekend and in fact every day since Ernesto passed as well. So we are looking forward to a really good mission."Launch director Mike Leinbach said NASA has only attempted three launches in a row once before. The normal practice is to make two attempts and then to stand down a day to give the launch team a break before making two more attempts."If you give us four attempts in five days, (our success rate is) something on the order of 90 to 95 percent," he said. "So three in a row is probably in the low 90s."The team is really excited to try to do this," he said. "This is what we're in the business for. To a man, to a woman, there were no disagreements at all about trying three in a row. We want to get this vehicle in orbit. I feel we have a pretty good shot at it, I really do. It's got to be in the 90-percentile range."While hoping for the best, NASA managers are continuing a review of the current daylight launch requirement, which permits photo documentation of the shuttle's heat shield and external tank insulation. Hale said if Atlantis doesn't get off this week, that review will play into discussions about when the shuttle could be readied for another attempt.The current launch window closes Friday because of conflict with launch of the space station's next full-time crew aboard a Russian spacecraft - Soyuz TMA-9 - and the Sept. 29 landing of the lab's outgoing crew aboard the Soyuz TMA-8 capsule. Based on lighting alone, the next shuttle launch window would open Oct. 26. Without that requirement, Atlantis could launch within days of the Soyuz TMA-8 landing.The goal of the 116th shuttle mission is to deliver and install a $372 million solar array truss, kicking off the resumption of space station assembly after a three-and-a-half-year hiatus.Atlantis' flight and the half dozen that follow will nearly complete the station's main solar array truss, which will stretch the length of a football field, and ready the outpost for attachment of European and Japanese research modules."Clearly, we are into the heart of the assembly sequence of the international space station," Hale said. "As we bring up the solar arrays, we are configuring the power system from its early assembly interim configuration to the final configuration and there is a huge rewiring on the station (required), both from the electrical power system, the generation and distribution of electrical power, as well as the cooling situation. Because all of that power, as it gets used, turns into heat and must be removed and the entire cooling system is being re-plumbed in the course of the next three or four shuttle assembly flights."And then following that, we bring up major modules, the international partners' modules that will be doing the bulk of the research, at least from their point of view, in addition to the U.S. lab that is just crucial to the success of the international space station. This is clearly a very complicated task. When you try to compare it to moonwalks or other things we have done in the past, then it's very difficult to compare. In terms of EVA tasks, spacewalk tasks, clearly these are the most complicated spacewalk and assembly tasks that have ever been done before."Hale said he was excited to be this close to launch "because this is the purpose for which we fly.""We're not flying the shuttle just as some kind of engineering experiment, although some folks would be happy to do that," he said. "We're flying the shuttle for a purpose, to carry a payload, to create this marvelous research outpost."It is really the purpose we are here for and I'm excited that after a substantial period of time of redesign and rethinking and retooling and preparation we are into the heart of the assembly. And we have certainly got our fingers crossed that it's going to go very well and we have made plans to cover every possible contingency we can think of."Additional coverage for subscribers:VIDEO:TODAY'S COUNTDOWN STATUS VIDEO:BIOGRAPHY MOVIE ON THE SIX ASTRONAUTS VIDEO:SHORT MOVIE PREVIEW OF ATLANTIS' MISSION VIDEO:OUTLOOK ON UPCOMING STATION ASSEMBLY FLIGHTS VIDEO:CREW ARRIVES IN T-38 TRAINING JETS VIDEO:COMMENTS FROM CREW AFTER ARRIVAL VIDEO:NEWS BRIEFING ON RETURN TO PAD VIDEO:ATLANTIS ROLLBACK BEGINS VIDEO:OFFICIALS EXPLAIN LIGHTNING SCRUB VIDEO:SEE THE LIGHTNING STRIKE AT PAD B VIDEO:ANOTHER VIEW OF LIGHTNING STRIKE VIDEO:COMPLETE PREVIEW OF ATLANTIS MISSION VIDEO:DETAILS OF THE THREE SPACEWALKS VIDEO:MEET THE SIX ASTRONAUTS MORE: STS-115 patchThe official crew patch for the STS-115 mission of space shuttle Atlantis to resume orbital construction of the International Space Station.Choose your store: - - - TelescopesLargest selection and the best prices anywhere in the world. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: August 27, 2006NASA managers met Sunday evening and agreed to wait until Monday morning to make a decision on whether to roll the shuttle Atlantis back to the Vehicle Assembly Building, preserving for now the option of launching the ship Tuesday on a space station assembly mission."We plan to get together early tomorrow morning and take a final look," said LeRoy Cain, chairman of NASA's Mission Management Team. "Based on the current timetable, we plan to make our decision one way or the other by 7 a.m. tomorrow morning."At issue is the progress of tropical storm/hurricane Ernesto and an updated forecast that calls for 40-knot winds at the Kennedy Space Center early Wednesday. A rollback would take 42 hours, so NASA could afford to wait until Monday morning before making a decision.If Ernesto weakens or its path changes, NASA could simply press ahead and make a run at launching Atlantis Tuesday at 3:42 p.m. Engineers have concluded there is no need to conduct time-consuming booster and self-destruct system tests in the wake of a launch pad lightning strike Friday. Forecasters say the forecast for Tuesday is favorable.But if Ernesto continues to threaten, however, NASA's Mission Management Team will order engineers to begin preparing for rollback early Monday."With the current storm predictions, it would take a relatively significant change from the current forecast we're seeing to prevent us from going into rollback preparations," Cain said. "If we see a change like that, then we'll press on. If we don't, then we'll be getting into our rollback preparations."Before Atlantis can be moved from the launch pad, engineers must first drain liquid oxygen and hydrogen from the ship's fuel cell system, a hazardous operation that requires the launch pad to be evacuated. After that, a variety of pyrotechnic charges would have to be disconnected and Atlantis would not be ready to roll until Tuesday afternoon.Draining the fuel cell system would preclude any chance of launching Tuesday. But if the forecast changes before rollback begins, NASA could keep Atlantis at the launch pad and avoid a long delay that would threaten to use up the available launch window. In that case, subsequent launch attempts could be made after Ernesto passes and after engineers reload the shuttle's fuel-cell system.If a rollback is ordered, Atlantis likely could not be returned to the launch pad until Saturday or Sunday. From that point, engineers would need at least eight days to ready the ship for launch. That would prevent any chance of launching Atlantis by Sept. 7, the current end of the launch window.NASA managers said earlier Sunday a rollback decision was needed by midnight based on earlier predictions that high winds could reach the Florida spaceport Tuesday night. While the shuttle can endure, in theory, 70-knot winds at the launch pad where wind and lightning protection is available, a shuttle cannot be rolled back to the VAB in winds higher than 40 knots."We're going to get some effects from the storm at the Kennedy Space Center," said launch director Mike Leinbach. "It remains to be seen how bad those effects are and that's the risk trade we make when these storms threaten us. Do we stay at the pad and accept some amount of wind? Or do we expect to have those levels of winds that would harm the orbiter and we have to roll back and protect her?"The goal of Atlantis' mission is to deliver a new set of solar arrays to the international space station. To reach the station, the shuttle must launch into the plane of its orbit during periods when the angle between that plane and the sun doesn't result in lower-than-allowable temperatures. Such temperature problems occur when the so-called beta angle drops below 50 to 60 degrees.In this case, the launch window also is affected by a self-imposed NASA requirement to launch in daylight for photo documentation of the shuttle's heat shield and external tank. Based on all three constraints, Atlantis' launch window extends through Sept. 13.The Russians plan to launch a fresh crew to the space station in mid September and to bring the lab's current crew home 11 days later. The Russians do not want to launch past Sept. 18 at the latest to avoid a dead-of-night landing for the returning station crew. This will be the first Soyuz recovery carried out under civilian management.As it now stands, Atlantis must launch by Sept. 7 to complete its docked mission and depart before arrival of the Soyuz.Mike Suffredini, space station program manager at the Johnson Space Center, said Sunday he planned to open discussions with the Russians early Monday about possible options."My opinion is, I think the system is fairly robust for night landings but again, you're weighing a risk to the crew with the schedule to go fly," he said. "We're responsible for shuttles. It's up to us to say we feel comfortable. They're responsible for Soyuz. So a really big part of this is not my opinion on risk trade, but whether they're willing, whether they want to take that risk because they're ultimately responsible for the crew. And just like how we feel about protecting our crews, they feel the same way."If Atlantis misses the September window, NASA would be faced with the prospect of just three lighted launch days between then and the end of the year - Oct. 26-27 and Dec. 23. The next lighted launch window after that opens Feb. 19, and that assumes NASA would launch with a beta angle of less than 50 to 60 degrees.Asked if NASA might be willing to relax the daylight launch constraint to open up more opportunities, Bill Gerstenmaier, NASA's senior space flight manager, said "we really want to keep the daylight launch" to ensure photo documentation of the shuttle's external tank, especially so-called ice-frost ramps that are still considered potentially dangerous."We really want to see how the ice-frost ramps perform, we really want to gather this data," said Bill Gerstenmaier, NASA's administrator for space flight. "So I think it's a pretty strong requirement. 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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 9, 2011 NASA's aging Voyager spacecraft, more than three decades outbound from Earth and approaching the outermost limits of the solar system, may be seeing signs of what scientists believe are huge magnetic bubbles churning at the interface between the sun's influence and interstellar space. The unexpected bubbles, shaped like sausages more than 100 million miles across, likely affect how high-energy cosmic rays pass into the inner solar system and may shed light on how stars interact with their galactic environments.Old and new views of the heliosheath. Red and blue spirals are the gracefully curving magnetic field lines of orthodox models. New data from Voyager add a magnetic froth (inset) to the mix. Credit: NASA"It's exciting. We're learning new things almost every day," Voyager project scientist Ed Stone said in a telephone interview.The outward flow of charged particles making up the solar wind, along with the sun's magnetic field, define a gigantic region in space known as the heliosphere. It is shaped somewhat like a teardrop because of the sun's motion, due to the rotation of the Milky Way, combined with the effects of the sun's passage through a cloud of interstellar debris produced by ancient supernova. The tail of the teardrop stretches away in the opposite direction of travel.The outward flow of the solar wind and the entwined magnetic field act as a shield of sorts for the inner solar system, affecting the passage of high-energy cosmic rays from deep space.NASA's twin Voyager 1 and 2 spacecraft were launched in 1977. Voyager 1 is roughly 11 billion miles from Earth while Voyager 2 is about nine billion miles out. Data from the spacecraft are transmitted to Earth with 20-watt transmitters."So it's 20 watts coming from 11 billion miles away," Stone said. "It's really a tiny amount of power. We have to use either the largest antennas, the 70-meter antennas, or we have to combine the signals from two 34 meter antennas in order to recover the data."The Voyagers are moving through a region known as the heliosheath and have reached a point where the outward velocity of the solar wind has dropped to near zero. Just in front of the heliosheath, which defines the outermost limit of the sun's influence, is the heliopause, the boundary between the heliosphere and the interstellar wind the sun is moving through. Just in front of the heliopause is a so-called bow shock where the interstellar wind crashes into the heliosphere."This heliospheric boundary is very important in shielding the heliosphere from galactic cosmic rays that come from outside our home," said Merav Opher, an astronomer at Boston University. "What shields us is the heliopause, this last region that separates us from the rest of the galaxy."Scientists believed the structure of the magnetic field at the interface between the heliosphere and interstellar space was relatively smooth. But based on data from the two Voyager spacecraft, it appears that huge magnetic bubbles may form in the heliosheath in the sun's direction of travel."A basic principle of magnetic fields in space is that they are tied to the ionized gas, because that gas is an excellent conductor of electricity, and where the gas goes, the field is stretched along with it and wherever the field goes, the gas has to go with it, too," said Eugene Parker, professor emeritus of physics at the University of Chicago. "So they're always together, stretched out through the solar system in this case."Field lines extend from the sun's north and south poles and are carried away by the solar wind. Because of the sun's rotation, the field lines become "twisted and wrinkled, a bit like a ballerina's skirt," Opher said in a statement. "Far, far away from the sun, where the Voyagers are, the folds of the skirt bunch up."Based on the Voyager data, scientists suspect magnetic field lines rapidly reconnect in the heliopause and form huge, disconnected bubbles that act like a permeable membrane to incoming cosmic rays. At least those coming from the sun's direction of travel."There had been recently some suggestions that the reconnections between the magnetic field in the heliosheath might be important," Stone told CBS News. "We hadn't really included that in any of the models because it's something that happens on a very small scale, it's hard to model."There are now models that suggest these bubbles will develop and that will change the nature of that region of the layer we're in, the heliosheath, and that might affect how cosmic rays from outside, can actually get inside the heliosphere. They have to sort of manage to get across all these bubbles."Stone is hopeful the Voyagers will cross the heliopause and move into interstellar space in the next few years."We must be getting very close because the outward motion of the (solar) wind in the heliosheath is basically zero, it's not moving outward any more, which means we're close," he said. "But how close? We don't know. It could happen any day, it could happen in the next several years. My own feeling is that it would be surprising if we don't cross the heliopause in the next four years or so."STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Water may be spurting on Mars NASA NEWS RELEASEPosted: December 6, 2006NASA photographs have revealed bright new deposits seen in two gullies on Mars that suggest water carried sediment through them sometime during the past seven years. "These observations give the strongest evidence to date that water still flows occasionally on the surface of Mars," said Michael Meyer, lead scientist for NASA's Mars Exploration Program, Washington. Liquid water, as opposed to the water ice and water vapor known to exist at Mars, is considered necessary for life. The new findings heighten intrigue about the potential for microbial life on Mars. The Mars Orbiter Camera on NASA's Mars Global Surveyor provided the new evidence of the deposits in images taken in 2004 and 2005. The images are available ."The shapes of these deposits are what you would expect to see if the material were carried by flowing water," said Michael Malin of Malin Space Science Systems, San Diego. "They have finger-like branches at the downhill end and easily diverted around small obstacles." Malin is principal investigator for the camera and lead author of a report about the findings published in the journal Science. Video coverage for subscribers only:VIDEO:MARS IMAGES PRESENTED BY THE SCIENTISTS VIDEO:QUESTION AND ANSWER SESSION The atmosphere of Mars is so thin and the temperature so cold that liquid water cannot persist at the surface. It would rapidly evaporate or freeze. Researchers propose that water could remain liquid long enough, after breaking out from an underground source, to carry debris downslope before totally freezing. The two fresh deposits are each several hundred meters or yards long. The light tone of the deposits could be from surface frost continuously replenished by ice within the body of the deposit. Another possibility is a salty crust, which would be a sign of water's effects in concentrating the salts. If the deposits had resulted from dry dust slipping down the slope, they would likely be dark, based on the dark tones of dust freshly disturbed by rover tracks, dust devils and fresh craters on Mars. Mars Global Surveyor has discovered tens of thousands of gullies on slopes inside craters and other depressions on Mars. Most gullies are at latitudes of 30 degrees or higher. Malin and his team first reported the discovery of the gullies in 2000. To look for changes that might indicate present-day flow of water, his camera team repeatedly imaged hundreds of the sites. One pair of images showed a gully that appeared after mid-2002. That site was on a sand dune, and the gully-cutting process was interpreted as a dry flow of sand. Today's announcement is the first to reveal newly deposited material apparently carried by fluids after earlier imaging of the same gullies. The two sites are inside craters in the Terra Sirenum and the Centauri Montes regions of southern Mars. "These fresh deposits suggest that at some places and times on present-day Mars, liquid water is emerging from beneath the ground and briefly flowing down the slopes. This possibility raises questions about how the water would stay melted below ground, how widespread it might be, and whether there's a below-ground wet habitat conducive to life. Future missions may provide the answers," said Malin. Besides looking for changes in gullies, the orbiter's camera team assessed the rate at which new impact craters appear. The camera photographed approximately 98 percent of Mars in 1999 and approximately 30 percent of the planet was photographed again in 2006. The newer images show 20 fresh impact craters, ranging in diameter from 7 feet (2 meters) to 486 feet (148 meters) that were not present approximately seven years earlier. These results have important implications for determining the ages of features on the surface of Mars. These results also approximately match predictions and imply that Martian terrain with few craters is truly young. Mars Global Surveyor began orbiting Mars in 1997. The spacecraft is responsible for many important discoveries. NASA has not heard from the spacecraft since early November. Attempts to contact it continue. Its unprecedented longevity has allowed monitoring Mars for over several years past its projected lifetime. NASA's Jet Propulsion Laboratory, Pasadena, manages the Mars Global Surveyor mission for the NASA Science Mission Directorate, Washington. For more information about NASA and agency programs, visit: STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. 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The first Heavy from Vandenberg flew in 2011 to successfully deploy a clandestine NRO satellite, becoming the largest rocket ever launched from the U.S. West Coast, and after another Medium went last year, rocket-maker ULA is getting ready to send up its next Heavy carrying a sizable payload for U.S. national security and the intelligence community."It is a very impressive rocket. It is the a largest, most powerful rocket in the U.S. inventory right now, produces approximately two million pounds of thrust at liftoff and is able to carry over 50,000 pounds to orbit. We only use this rocket, because of how large and complex it is, for our largest spacecraft, which tend to be the most strategically important national security payloads that we have. This is immensely critical," said Lt. Col. Dan Gillen, commander of the 4th Space Launch Squadron at Vandenberg and the Air Force launch director for the Heavy mission.The first Vandenberg Heavy launch in 2011 as seen from an off-shore oil platform. Credit: Air Force photo provided courtesy of the 30th Communications Squadron Optics sectionThe Delta 4-Heavy is created by taking three Common Booster Cores -- the liquid hydrogen-fueled motor that forms a Delta 4-Medium's first stage -- and strapping them together to form a triple-wide rocket, then adding a cryogenic upper stage.The rocket was constructed at ULA's factory in Decatur, Alabama, then shipped by sea to Vandenberg, completing the month-long, 4,000-mile voyage in December by docking at the base's harbor once envisioned for receiving the space shuttle fuel tank barge.The stages were unloaded and moved up the road to Horizontal Integration Facility at SLC-6, an unassuming garage-like hangar were the rocket core was fitted with the port and starboard boosters and the upper stage was attached.Then on Monday, riding horizontally on a motorized hauler, the 184,000-pound rocket was driven to the pad where hydraulic pistons on Tuesday pushed the 190-foot-tall vehicle upright to stand atop the pad."Over the last four-and-a-half months, we've been working multiple shifts a day in order to prepare for this milestone this week," Gillen said."All of that work has been in the horizontal where we've mated the three Common Booster Cores and also integrated the second stage with the first stage. All of that went extremely well and we were able to keep the milestone this week of rolling out to the pad and going to the vertical. On Monday we moved out from the Horizontal Integration Facility out to the pad and then Tuesday morning was when we went to the vertical, and everything went nominally," Gillen said.File photo of the first Delta 4-Heavy going vertical at Vandenberg. Credit: ULA videoWith the vehicle now standing on the pad, activities in May will focus on system testing and preparations for a realistic launch day simulation. That test, known as the Wet Dress Rehearsal, will occur in June and run through a full countdown and fueling of the rocket's eight liquid hydrogen and liquid oxygen tanks.The secretive payload will be mounted aboard the Heavy in July. The fully assembled rocket, with the shrouded cargo in its nose cone, will measure over 230 feet tall for launch."This is extremely exciting," Gillen said of getting the rocket rolled out. 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The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Delta 4-Heavy rocket panoramasThese panoramas of the Delta 4-Heavy rocket were shot in early January as the vehicle was undergoing pre-flight assembly inside the Horizontal Integration Facility hangar at Cape Canaveral's Complex 37.The rocket's cryogenic upper stage had not yet been attached when these pictures were taken.This vehicle will launch the NROL-26 mission for the National Reconnaissance Office.Photo credit: Chris Miller/Spaceflight Now Click for larger image. Credit: Chris Miller/Spaceflight Now Click for larger image. Credit: Chris Miller/Spaceflight Now Click for larger image. Credit: Chris Miller/Spaceflight Now | | | | 2014 Spaceflight Now Inc.Spaceflight Now +Subscribe to Spaceflight Now Plus for access to our extensive video collections!"Chandra's Universe"NASA's Chandra X-ray Observatory is providing new insights into the frontier of X-ray astronomy.Station's new toiletSpace station commander Mike Fincke shows the new U.S. toilet installed aboard the complex. 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The United Launch Alliance Delta 4-Heavy rocket, flying with upgraded main engines for even more power, blasted off Friday at 9:15 a.m. EDT on the NROL-15 satellite-deployment mission for the National Reconnaissance Office.See our coverage of the launch.Photo credit: Walter Scriptunas II/Spaceflight NowDelta 4-Heavy's demo flight critical to military missions SPACEFLIGHT NOWPosted: December 9, 2004America's new heavy-lifting rocket takes its much-anticipated test flight Saturday, if Mother Nature cooperates. The Boeing Delta 4-Heavy rocket was supposed to launch today, but the forecast for strong winds and stormy weather at Cape Canaveral postponed the liftoff by 24 hours. The Delta 4-Heavy rocket is ready for its inaugural flight. Credit: Boeing photo by Carleton BailieLaunch is scheduled for 2:31 p.m. EST (1931 GMT) at the opening of a two-hour, 56-minute window. Saturday's weather is iffy with a 60 percent chance of violating the launch rules.When the rocket does fly it will cap a six-year development effort that produced this massive vehicle designed to loft large payloads into space."It really has been a labor of love over the past six years to get to this point, which has taken the efforts of thousands and thousands of people from the U.S. Air Force, The Boeing Company and from all of our suppliers from far-flung reaches to make all of this happen. It's really the start of a great era in space launch with the Delta 4-Heavy," said Dan Collins, the Boeing vice president of expendable launch systems."I'm very proud to be able to lead this organization on the eve of this historic launch and look forward to watching the Delta 4-Heavy demo zoom over the horizon on its way to geosynchronous orbit -- as soon as the weather permits."The rocket, which takes three hydrogen-fueled booster stages and mounts them together, is a technical marvel. Each Common Booster Core has its own Rocketdyne RS-68 main engine generating over 650,000 pounds of thrust at liftoff."We've had a lot of independent folks look at this launch vehicle and the conclusion that's been come to, by all of the people, is we have a very robust launch system. In fact...it's much more robust than they had anticipated going in. But even that said, there is a recognition that this launch system is the most complex to come to the pad ...since the space shuttle," Collins said.The Heavy's main customer -- the U.S. government -- has purchased two missions, including next year's launch of a missile-warning satellite and a later classified reconnaissance cargo. This demonstration flight serves as a dress rehearsal for the rocket before the costly national security missions go forward."We're confident this mission is ready for flight, and will serve as the foundation for the first operational launch of Delta 4-Heavy next year," said Col. Mark Owen, the 45th Space Wing commander."It is tough to communicate to you the level of excitement that I feel and the 45th Space Wing team feels as we stand on the verge of history as the U.S. Air Force joins Boeing and its other mission partners preparing to launch the first Delta 4-Heavy from Cape Canaveral Air Force Station."The Delta 4-Heavy can loft payloads comparable in weight to the Titan 4 rocket that has been in service since 1989. But that Lockheed Martin-built booster is being retired after two more flights next year Florida and California. The Delta promises to provide launches far cheaper than Titan."This is somewhat similar to a baton pass in a race. With a sense of history, I note that the last heavy-lift Titan 4B from the Cape is stacked out at Launch Complex 40 at the same time we've got the first of the next-generation, we've got the Delta 4-Heavy out at SLC-37B," said Col. John Insprucker, the EELV system program director.The Air Force's Evolved Expendable Launch Program has backup capabilities between the rival Boeing Delta 4 and Lockheed Martin Atlas 5 families. But the two future operational Delta 4-Heavy missions have been awarded to Boeing and there are no plans to use Atlas 5."The Delta 4-Heavy is their ride to space," Col. Insprucker said, referring to the two cargos relying on the new rocket.The first operational Delta 4-Heavy, presently scheduled for next August, will carry the final Defense Support Program craft that detects enemy missile launches and nuclear weapon detonations from space. If things go seriously wrong Saturday and the U.S. military was in a pinch to find alternate launch options, that particular satellite could fly aboard a Lockheed Martin Atlas 5-551 configuration rocket, company officials said. That version of Atlas 5 uses five strap-on solid boosters. A two-booster configuration next week.The Air Force says the second operational Delta 4-Heavy launch currently booked, carrying a secret National Reconnaissance Office payload, could not fly on existing Atlas 5 configurations available today. The power of an Atlas 5-Heavy would be required to lift that cargo into space.Lockheed Martin's heavy-lift vehicle is proceeding through development and would be ready to fly its inaugural flight 30 months from the time it's ordered.The long-range military outlook for Heavy missions is sparse."The NRO still has another heavy satellite that will be ready to launch in about 2008," Col. Insprucker said. 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The arm moves like a backhoe,using four types of motion: up-and-down, side-to-side, back-and-forth and rotating.The arm can reach far enough to dig about half a meter (20 inches) deep. However, the subsurfaceice layer expected at the landing site may not lie that deep. Once the arm reaches theicy-soil layer, the powered rasp will be used to acquire samples.Because the arm will be making direct contact with icy soil that is conceivably a habitat wheremicrobes could survive, extra precaution has been taken with it to prevent introducing life fromEarth. Before the arm was given a sterilizing heat treatment in March 2007, it was enclosedin a biological barrier wrap. This barrier is keeping microbes off the arm during the subsequentmonths before launch. It will not open until after Phoenix has landed on Mars.The robotic arm uses design work for a similar arm flown on the 1999 Mars Polar Lander mission,with refinements including enhanced capability for collecting an icy sample.A team led by Robert Bonitz at NASA's Jet Propulsion Laboratory, Pasadena, Calif., engineeredand tested the Phoenix Robotic Arm. Alliance Spacesystems Inc., Pasadena, built it.Ray Arvidson of Washington University in St. Louis is the lead scientist for this instrument.The Robotic Arm Camera rides fastened to the arm just above the scoop. It will providecloseup color images of Martian soil at the landing site, of the floor and walls of trenches dugby the arm, and of soil and ice samples before and after they are in the scoop.Information the camera reveals about soil textures will aid in selecting what to pick up assamples for analysis. Observations of trench walls will determine whether they show fine-scalelayering, which could result from changes in the Martian climate.The camera has a double Gauss lens system, a design commonly used in 35-millimeter cameras.Images are recorded by a charge-coupled device (CCD) similar to those in consumer digitalcameras. The instrument includes sets of red, green and blue light-emitting diodes (LEDs)for illuminating the target area.The focus can be adjusted by a motor, which is a first for a camera on an interplanetary spacecraft. The focus can be set as close as about 11 millimeters (half an inch) and out to infinity.With a resolution of 23 microns per pixel at the closest focus, this camera can show detailsmuch finer than the width of a human hair.A team led by H. Uwe Keller at the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, and by Peter Smith at the University of Arizona originally built this camerafor the Mars Surveyor 2001 Lander mission, which was canceled in 2000. It is similar to acamera on the robotic arm of the unsuccessful Mars Polar Lander spacecraft, though with animproved illumination system. For the Phoenix Robotic Arm Camera, Keller is the lead scientistand Chris Shinohara of the University of Arizona is the lead engineer.The Surface Stereoscopic Imager will record panoramic views of the surroundings fromatop a mast on the lander. Its images from two cameras situated about as far apart as a pair ofhuman eyes will provide three-dimensional information that the Phoenix team will use in choosingwhere to dig and in operating the robotic arm.A choice of 12 different filters for each eye enables the instrument to produce images not onlyin full color, but in a several specific visual and infrared frequencies useful for interpreting geological and atmospheric properties. The multispectral and three-dimensional information willhelp scientists understand the geology of the landing area.The twin cameras will be able to look in all directions from a perch about 2 meters (7 feet)above Martian ground level. They will see with about the same resolution as human eyes,capturing each view onto 1-megapixel charge-coupled devices (a 1,024-by-1,024-pixel CCDfor each eye).The instrument will sometimes point upward to assess how much dust and water vapor is inthe atmosphere. When the robotic arm delivers soil and ice samples to deck-mounted instruments,the Surface Stereoscopic Imager will be able to look downward to inspect the samples.Views of the spacecraft's deck will also monitor dust accumulation, which is of scientific interestfor inferences about Martian winds and of engineering interest for effects of the dust buildupon solar panels.A University of Arizona team led by Chris Shinohara built the Phoenix Surface StereoscopicImager. Mark Lemmon of Texas A&M University, College Station, is lead scientist for this camera.The instrument closely resembles a stereo imager on Mars Polar Lander, which in turnused design features from the imager on Mars Pathfinder, which provided stereo views fromthe surface of Mars in July 1997.The Thermal and Evolved-Gas Analyzer will study substances that are converted to gasesby heating samples delivered to the instrument by the robotic arm. It provides two types of information.One of its tools, called a differential scanning calorimeter, monitors how much poweris required to increase the temperature of the sample at a constant rate. This reveals whichtemperatures are the transition points from solid to liquid to gas for ingredients in the sample.The gases that are released, or "evolved," by this heating then go to a mass spectrometer, atool that can identify the chemicals and measure their composition.The mass spectrometer will determine whether the samples of soil and ice contain any organiccompounds. It would be used to identify the types and amounts if any are present. Finding anywould be an important result for interpreting the habitability of the site.The instrument will also give information about water and carbon dioxide present as ices orbound to minerals. The amount of heat needed to drive off water or carbon dioxide that isbound to minerals is characteristically different for different minerals. The calorimeter's information from that process can help identify minerals in the soil, including carbonates if they are present.The mass spectrometer will measure the ratios of different isotopes of carbon, oxygen, hydrogen,argon and some other elements in the Martian samples. Isotopes are alternate forms ofthe same element with different atomic weights due to different numbers of neutrons. Ratioscan be changed by the effects of long-term processes that act preferentially on lighter or heavierisotopes of the same element. For example, some of Mars' original water was lost from theplanet by processes at the top of the atmosphere, favoring the removal of lighter isotopes ofhydrogen and oxygen and leaving modern Mars water with a raised ratio of heavier isotopes.The instrument has eight tiny ovens for samples, each to be used only once. The ovens areabout 1 centimeter (about half an inch) long and 2 millimeters (one-eighth inch) in diameter.At the start of an analysis, sample material is dropped into the oven through a screen. Theoven closes after a light-beam detector senses that it is full. The experiment gradually heatssamples to temperatures as high as 1,000 degrees Celsius (1,800 degrees Fahrenheit).Theheating process drives off water and any other volatile ingredients as a stream of gases. Thosegases are directed to the mass spectrometer.One of the samples that the instrument will analyze will be a special material that the landercarries from Earth, specially prepared to be as free of carbon as possible. This will serve asan experimental control as the instrument analyzes samples excavated at Mars. The controlmaterial is made of a machinable glass ceramic substance named Macor, from Corning Inc.The arm will scrape some of it up and deliver it to the analyzer to get a reading showing howwell the experiment can eliminate carbon carried from Earth. Carbon detected in assessmentsof Martian samples might be unavoidable traces of Earth carbon if the readings are no higherthan the amount in this control sample.The mass spectrometer part of the analyzer will examine samples of atmosphere at the landingsite, in addition to the evolved gases from scooped-up samples. The atmospheric measurementswill add information about humidity to the weather data monitored by the spacecraft'sMeteorological Station.The Thermal and Evolved-Gas Analyzer was built by teams at the University of Arizona, ledby William Boynton (science lead) and Heather Enos (project manager), and at the Universityof Texas, Dallas, led by John Hoffman. It is adapted from a similar instrument with the samename that flew on the Mars Polar Lander mission in 1999.The Microscopy, Electrochemistry and Conductivity Analyzer will use four tools to examinesoil. It will assess characteristics that a gardener or farmer would learn from a soil test,plus several more. Three of the tools will analyze samples of soil scooped and delivered bythe robotic arm -- a wet chemistry laboratory and two types of microscopes. The fourth tool ismounted near the end of the arm, and has a row of four small spikes that the arm will push intothe ground to examine electrical conductivity and other properties of the soil.The wet chemistry laboratory has four teacup-size beakers. Each will be used only once.Samples from Mars' surface and three lower depths may be analyzed and compared. Theinstrument will study soluble chemicals in the soil by mixing water with the sample to a soupyconsistency and keeping it warm enough to remain liquid during the analysis.On the inner surfaces of each beaker are 26 sensors, mostly electrodes behind selectively permeablemembranes or gels. Some sensors will give information about the pH of the soil -- thedegree to which it is acidic or alkaline. Soil pH is an important factor in what types of chemicalreactions, or perhaps what types of microbes, a soil habitat would favor, and it is has neverbeen measured on Mars. Other sensors will gauge concentrations of such ions as chlorides,bromides, magnesium, calcium and potassium, which form soluble salts in soil, and will recordthe level of the sample's oxidizing potential. One chemically important ion in soil, sulfate,cannot be directly sensed, so the analysis of each sample will end with a special process thatdetermines the amount of sulfate by observing its reaction with barium. Comparisons of theconcentrations of water-soluble ions in samples from different depths may provide clues to thehistory of water in the soil.The wet chemistry setup has a built-in robotic laboratory technician that adds potions to eachbeaker in a choreographed two-day sequence. Before each soil sample goes in, about 25cubic centimeters (nearly two tablespoons) of ice with dilute concentrations of several ionsis slowly melted in a special container, a process that takes one to two hours. After the wateris released into the beaker, the sensors make baseline measurements at this starting point.The first of five pill-size crucibles of prepared chemicals is then added to increase ion concentrationsby a known amount in order to calibrate the measurements. Next, a drawer abovethe beaker extends to receive the soil sample, and the scoop on the robotic arm drops up toone cubic centimeter (one-fifth of a teaspoon) of soil into the drawer, which then retracts anddumps the sample into the beaker. A paddle stirs the soup for hours while the sensors takemeasurements. The next day, the second crucible adds nitrobenzoic acid to the beaker to testhow ions from the soil react to increased acidity. The last three crucibles hold barium chloride.As they are added, one at a time, any sulfate from the soil reacts with the barium to make aninsoluble compound, taking both the barium and the sulfate out of solution. The amount of sulfatein the soil sample is determined by measuring the amount of unreacted barium left behind.The "microscopy" part of the Microscopy, Electrochemistry and Conductivity Analyzer will examinesoil particles and possibly ice particles with both an optical microscope and an atomicforce microscope. The robotic arm delivers soil samples to a wheel that rotates to presentthe samples to the microscopes. Along the perimeter of the wheel are substrates with differenttypes of surfaces, such as magnets and sticky silicone. This allows the experiment to getinformation from the particles' interaction with the various surfaces, as well as from the sizes,shapes and colors of the particles themselves.The biggest particles the optical microscope can view are about as long across as the thicknessof a dime, just over a millimeter. The smallest it can see are about 500 times smaller -- about 2 microns across. That would be the smallest scale ever seen on Mars, except thatthe atomic force microscope will image details down to another 20 times smaller than that -- assmall as about 100 nanometers, one one-hundredth the width of a human hair.The optical microscope obtains color information by illuminating the sample with any combinationof four different light sources. The illumination comes from 12 light-emitting diodes shiningin red, blue, green or ultraviolet parts of the spectrum. The atomic force microscope assemblesan image of the surface shape of a particle by sensing it with a sharp tip at the end of a spring,which has a strain gauge indicating how far the spring flexes to follow the contour of the surface.The process is like a much smaller version of a phonograph needle tracking the bumpinessinside the groove of a vinyl record.The shapes and the size distributions of soil particles may tell scientists about environmentalconditions the material has experienced. Tumbling rounds the edges. Repeated wetting andfreezing causes cracking. Clay minerals formed during long exposure to water have distinctive,plate-shaped particle shapes.The "conductivity" part of the Microscopy, Electrochemistry and Conductivity Analyzer will assesshow heat and electricity move through the soil from one spike to another of a four-spikeelectronic fork that will be pushed into the soil at different stages of digging by the arm. Forexample, a pulse of heat will be put onto one spike, and the rate at which the temperature riseson the nearby spike will be recorded, along with the rate at which the heated needle cools off.A little bit of ice in the soil can make a big difference in how well the soil conducts heat. Similarly, soil's electrical conductivity is a sensitive indicator of moisture in the soil. Soil moisture may have subtle stages intermediate between frozen solid and liquid, including warm ice andwater films, which may be biologically available. The device, called the thermal and electricalconductivity probe, adapts technology used in commercial soil-moisture gauges for irrigationcontrol systems.The conductivity probe has an additional role besides soil analysis. It will serve as a humiditysensor when held in the air. Also, slight temperature changes from one spike to the next canallow it to estimate wind speed.The Microscopy, Electrochemistry and Conductivity Analyzer is based on an instrument developedfor the Mars Surveyor 2001 Lander mission, which was canceled in 2000. The instrumentfor Phoenix inherited many of the original electronic and structural components. The conductivityprobe and other improvements have been added to the earlier design.A team led by Michael Hecht at NASA's Jet Propulsion Laboratory, Pasadena, Calif., designedand built the analyzer. A consortium led by Urs Staufer of the University of Neuchatel, Switzerland,provided the atomic force microscope. The University of Arizona provided the opticalmicroscope, equipped with an electronic detector (the same as in the Robotic Arm Camera)from the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany. JohnMarshall of the SETI Institute, Mountain View, Calif., is lead scientist for the optical microscope.Transfer Engineering and Manufacturing Inc., Fremont, Calif. (formerly Surface/Interface Inc.of Mountain View, Calif.) designed the sample wheel for the microscopes. Aaron Zent of NASAAmes Research Center, Moffett Field, Calif., is science lead for the thermal and electrical conductivity probe, built by Decagon Devices Inc., Pullman, Wash. For the wet chemistry experiment,Thermo Fisher Scientific (formerly the Water Analysis Division of Thermo Corp., Beverly,Mass.) provided the chemical beakers; Starsys Research Corp., Boulder, Colo. provided thechemistry actuator assemblies and Tufts University, Medford, Mass., prepared the crucibles ofreagents for mixing with the soil samples. Sam Kounaves of Tufts is lead scientist for the wetchemistry investigation.The Meteorological Station will track daily weather and seasonal changes using temperatureand pressure sensors plus a laser-reflection instrument. The information collected by thisfirst high-latitude weather station on Mars will aid understanding of how water is cycled seasonallybetween ice on the ground and vapor in the atmosphere.The laser tool, called a lidar for "light detection and ranging," uses powerful laser pulses ina way comparable to radio pulses emitted by a radar instrument. The laser beam is emittedvertically into the atmosphere. Atmospheric dust and ice particles in the beam's path reflect thelight, sending it in all directions, including straight downward. A telescope integrated into theinstrument detects the downward-reflected light. Analysis of the strength and time-delay of thereflections reveals information about the sizes and altitudes of the particles. Tracking changesin these atmospheric particles' abundances and locations over time will help researchers studyhow clouds and dust plumes form and move.The weather station includes a 1.2-meter (4-foot) mast bearing sensors at three heights tomonitor how temperature varies with height near the surface. The temperature sensors arethin-wire thermocouples; they measure temperature by its effect on the flow of an electricalcurrent through a closed circuit of two metals with different thermal properties. The thermocouplesuse the metals chromel (a nickel and chromium alloy) and constantan (a copper andnickel alloy). Also, hanging from the top of the mast is a wind telltale. This is a small tube thatwill be deflected by the wind. The science payload's stereo camera will record images of thetelltale that will be used to determine wind direction and speed. The top of the meteorologymast, at 1.14 meters (3.75 feet) above the deck, is the highest point on the lander.The Canadian Space Agency provided the Meteorological Station for Phoenix. Jim Whitewayof York University, Toronto, Ontario, leads the Canadian science team. The instrument constructionwas led by the Space Missions Group of MDA Ltd., Brampton, Ontario, with contributionsfrom Optech Inc., Toronto, for the lidar. The Finnish Meteorological Institute provided theinstrument for measuring atmospheric pressure. Aarhus University, Denmark, constructed thewind telltale.The Mars Descent Imager will take a downward-looking picture during the final momentsbefore the spacecraft lands on Mars. This image will provide a bridge between orbiter-scaleand lander-scale images. It is expected to show geological context helpful for planning thelander's activities and for interpreting other science instruments' observations and measurements.Conditions at the landing site have different implications if the site appears to be typicalof a much broader area than if the site happens to be an unusual patch of ground unlike itssurroundings.This camera is mounted on the outer edge of the payload deck of the lander. It was designedto take several images, but the plan was altered to just one image after testing showed that adata-handling component elsewhere on the lander had a small possibility of triggering loss ofsome vital engineering data if it receives imaging data during a critical phase of final descent.The timing of the image will be planned to yield higher resolution of the landing area than currentlypossible from orbit.The imager weighs just 480 grams (1 pound). The optics provide a field of view of 75.3 degrees.Exposure time is 4 milliseconds.. At that speed, some blurring may occur as the descentengines vibrate the spacecraft while the camera takes its image.Future spacecraft to the surface of Mars may need capability for steering themselves to avoidhazards or to reach specific landing sites. Descent imaging could be an important componentof the technology for accomplishing that.A tiny microphone is riding on the descent camera. It might catch sounds around the spacecraftwhile the camera is taking its image. There are no plans to power the camera to takepictures or to record sounds after the landing.The Mars Descent Imager that will fly on Phoenix was originally built for the Mars Surveyor2001 Lander mission, by a team led by Michael Malin at Malin Space Science Systems, SanDiego. A similar camera flew on Mars Polar Lander.Research StrategyThe planned operational life of the Phoenix Mars lander after it reaches Mars is 90 Martiandays. Each Martian day, often called a "sol," lasts about 40 minutes longer than an Earth day.That gives the Phoenix team three months to use the lander's instruments to address the waterand habitat questions of the mission's science objectives. Planning and practice simulationsbefore landing will prepare the team to make the best possible advantage of that time.Observations made by orbiter spacecraft during the evaluation of candidate landing sites forPhoenix provide a starting-point base of knowledge about the area. After Phoenix has landed,views from the Surface Stereoscopic Imager, with added context from the Mars Descent Cameraand closer looks with the Robotic Arm Camera, will be used for choosing where to collectthe first soil sample for analysis.The first samples fed into the lander's analyzers will come from the surface. Decisions abouthow much deeper to go before analyzing another sample will depend on results from thesurface material and on what the robotic arm camera and stereo imager see in the soil. TheThermal and Evolved-Gas Analyzer can check for organics and other volatiles in up to eightsamples. Researchers must be choosier with samples for the wet chemistry laboratory of theMicroscopy, Electrochemistry and Conductivity Analyzer, which can examine four differentsamples. The microscopes and conductivity probe can analyze soil more frequently during the90 sols. Meanwhile, the weather station and stereo imager will monitor changes in water anddust in the atmosphere throughout the mission. If the spacecraft remains functional longer thanthe 90-day prime mission, weather information might be collected during the approach of thenorthern hemisphere autumn on Mars, when dwindling sunlight will eventually make operationsimpossible, and buildup of carbon-dioxide frost will coat the spacecraft.What types of findings would help answer questions about the history of water? If the microscopesfind fine silty sediments or clay textures, that would be evidence supporting the hypothesisthat the northern highlands of Mars once held an ocean. The presence of carbonatesor other minerals that form in liquid water would be another. Rounded sand grains in the soilcould suggest a history of flowing water.The mass spectrometer will measure isotopic ratios. If there are differences between thoseratios in subsurface ice and in atmospheric water, that could suggest the subsurface ice is ancient.A gradient in the concentrations of salts at different depths in the soil would support thehypothesis that climate cycles periodically thaw some subsurface ice. The conductivity probe'sfindings about thermal properties of the soil, combined with determination of the depth to an icylayer, could strengthen estimates for how much change in climate would be needed to melt theice. The same ground-truth information will refine models of the ice's depth and of atmosphereiceinteractions in widespread areas of Mars that contain subsurface ice.Using the microscopes and arm camera to learn about how porous and layered the soil iswill help assess whether liquid water has come and gone. The conductivity probe will assesswhether, even today, the soil may have thin films of unfrozen water. Atmospheric measurementsas the season progresses through the Martian summer will aid the understanding ofhow water is seasonally cycled between solid and gas phases in the current Martian climate.What types of findings would help answer questions about whether this site could formerly orstill support microbial life? Three important factors in the suitability of a habitat for life are the availability of liquid water, the presence of carbon and access to energy. So evidence about thehistory of water will be one part of evaluating the habitat.The Thermal and Evolved-Gas Analyzer has the dramatic job of checking for organic carbonmolecules layer by layer as samples come from farther below the surface. Soluble sulfate mineralswould be a possible source of energy that could sustain life. The wet chemistry lab of theMicroscopy, Electrochemistry and Conductivity Analyzer can identify potential chemical-energysources if they are present in soil samples. While the science payload of Phoenix is not designedfor life detection, this mission is an important stepping stone in the search for whetherMars has life. Orbital observations indicate that areas with shallow subsurface ice make up atleast a quarter of the red globe. Phoenix will be the first mission to visit such a site. Its findings about habitability could guide where a future spacecraft searching for life is sent.Researchers have equipped Phoenix to look for answers to many questions posed in advanceabout water and habitat. However, if previous interplanetary missions are an indicator, some ofthe most important results from Phoenix may be surprises that raise new questions.John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA's Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Phoenix science investigationsFROM NASA PRESS KITThe Phoenix Mars Lander will investigate a site in the far north of Mars to answer questionsabout that part of Mars, and to help resolve broader questions about the planet. The mainquestions concern water and conditions that could support life.The landing region has water ice in soil close to the surface, which NASA's Mars Odysseyorbiter found to be the case for much of the high-latitude terrain in both the north and southhemispheres of Mars.Phoenix will dig down to the icy layer. It will examine soil in place at the surface, at the icy layer and in between, and it will scoop up samples for analysis by its onboard instruments. One keyinstrument will check for water and carbon-containing compounds by heating soil samples intiny ovens and examining the vapors that are given off. Another will test soil samples by addingwater and analyzing the dissolution products. Cameras and microscopes will provide informationon scales spanning 10 powers of 10, from features that could fit by the hundreds into theperiod at the end of this sentence to an aerial view taken during descent. A weather station willprovide information about atmospheric processes in an arctic region where a coating of carbon-dioxide ice comes and goes with the seasons.Mars is a vast desert where water is not found in liquid form on the surface, even in placeswhere mid-day temperatures exceed the melting point of ice. One exception may be fleetingoutbreaks that have been proposed to explain modern-day flows down some Martian gullies.Today's arid surface is not the whole story, though. Previous Mars missions have found thatliquid water has persisted at times in Mars' past and that water ice near the surface remainsplentiful today.Water is a key to four of the most critical questions about Mars: Has Mars ever had life? Howshould humans prepare for exploring Mars? What can Mars teach us about climate change?How do geological processes differ on Mars and on Earth? Water is a prerequisite for life, apotential resource for human explorers and a major agent of climate and geology. That's whyNASA has pursued a strategy of "follow the water" for investigating Mars. Orbiters and surfacemissions in recent years have provided many discoveries about the history and distribution ofwater on Mars -- such as minerals that formed in wet environments long ago and liquid flowsthat are still active today in hillside gullies.The landing site and onboard toolkit of Phoenix position this mission to follow the water further.The mission's three main science objectives are:1. Study the history of water in all its phases.On a time scale of billions of years, ice near the surface where Phoenix will land might be theremnant of an ancient northern sea. Several types of evidence point to plentiful liquid water onancient Mars, and the northern hemisphere is low and smooth compared to the southern hemisphere.Much of the water that could have remained liquid when ancient Mars had a thickeratmosphere may now be underground ice.On a time scale of tens of thousands to a few million years, ice near the surface where Phoenixlands might periodically thaw during warmer periods of climate cycles. The tilt of Mars' axis wobbles more than Earth's, and the shape of Mars' orbit also cycles over time, from rounderto more elongated. Currently, Mars is about 20 percent farther from the sun during northernsummer than during northern winter, so the summers are relatively cool in the north. As theorbit varies, the northern ice cap will enjoy warm winters on a 50,000-year cycle. The wobbleof Mars' axis may also cause the climate to change on a time scale of 100,000 to millions ofyears.On much shorter time scales, the arctic ground "breathes" every day and every season, convertingtiny amounts of ice into water vapor on summer days and condensing tiny amounts offrost from the atmosphere at night or in winter. In this way, the ice table slowly rises and recedesas the climate changes.Phoenix will collect information relevant for understanding processes affecting water at allthese time scales, from the planet's distant past to its daily weather.2. Determine if the Martian arctic soil could support life.Life as we know it requires liquid water, but not necessarily its continuous presence. Phoenixwill investigate a hypothesis that some ice in the soil of the landing site may become unfrozenand biologically available at times during the warmer parts of long-period climate cycles. Lifemight persist in some type of dormant microbial form for millions of years between thaws, ifother conditions were right.The spacecraft is not equipped to detect past or present life. However, in addition to studyingthe status and history of water at the site, Phoenix will look for other conditions favorable to life.One condition considered essential for life as we know it is the presence of molecules thatinclude carbon and hydrogen. These are known as organic compounds, whether they comefrom biological sources or not. They include the chemical building blocks of life, as well as substances that can serve as an energy source, or food, for life. Phoenix would be able to detecteven very small amounts and identify them. Two Viking spacecraft that NASA landed on Marsin 1976 made the only previous tests for organic compounds in Martian soil, and they foundnone. Conditions at the surface may be harsh enough to break organic molecules apart andoxidize any carbon into carbon dioxide. Phoenix will assess some factors in those oxidizingconditions, and it will check for organic chemicals below the surface, as well as in the top layeranic chemicals would persist better in icy material sheltered from sunshine than in surfacesoil exposed to harsh ultraviolet radiation from the sun.Phoenix will also be checking for other possible raw ingredients for life. It will examine howsalty and how acidic or alkaline the environment is in samples from different layers. It will assessother types of chemicals, such as sulfates, that could be an energy source for microbes.3. Study Martian weather from a polar perspective.In Mars' polar regions, the amount of water vapor in the thin atmosphere -- the humidity -- variessignificantly from season to season. Winds carrying water vapor can move water fromplace to place on the planet. The current understanding of these processes is based on observationsfrom orbit and limited meteorological observations from earlier Mars landers closer tothe equator. Phoenix will use an assortment of tools to directly monitor several weather variablesin the lower atmosphere at an arctic site.Phoenix will measure temperatures at ground level and three other heights to about 2 meters(7 feet) above ground. It will check the pressure, humidity and composition of the atmosphereat the surface. And it will identify the amounts, altitudes and movements of clouds and dust inthe sky above.Over the course of the mission, this unprecedented combination of Martian meteorologicalmeasurements will help researchers evaluate correlations such as whether southbound windscarry more humidity than northbound winds; whether drops in air pressure are associated withincreased dust; and how the amount of water vapor at the bottom of the atmosphere changesfrom late spring to mid-summer or later.STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Phoenix spacecraft headed to Mars to probe the water BY WILLIAM HARWOOD Cheap Gucci Womens Wedges Shoes

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Posted: December 7, 2009T-00:00LiftoffThe Delta 2 rocket's main engine and twin vernier steering thrusters are started moments before launch. All three strap-on solid rocket motors are ignited at T-0 to begin the mission.T+01:04.0SRB BurnoutThe six ground-start Alliant TechSystems-built solid rocket motors consume all their propellant and burn out.T+01:39.0Jettison SRBsThe solid rocket boosters are jettisoned to fall into the Pacific Ocean. The spent casings remained attached until the vehicle passed into preset drop zone, clear of offshore oil platforms.T+01:40.0Begin Dog-legAfter initially flying from Vandenberg along a 196-degree flight azimuth, the rocket begins steering itself to obtain the desired orbital inclination. This dog-leg maneuver continues for 40 seconds.T+04:24.2Main Engine CutoffAfter consuming its RP-1 fuel and liquid oxygen, the Pratt & Whitney Rocketdyne RS-27A first stage main engine is shut down. The vernier engines cut off moments later.T+04:32.2Stage SeparationThe Delta rocket's first stage is separated now, having completed its job. The spent stage will fall into the Pacific Ocean.T+04:37.7Second Stage IgnitionWith the stage jettisoned, the rocket's second stage takes over. The Aerojet AJ118-K liquid-fueled engine ignites for the first of two firings needed to place the WISE spacecraft into the proper orbit.T+04:56.0Jettison Payload FairingThe 10-foot diameter payload fairing that protected the WISE cargo atop the Delta 2 during the atmospheric ascent is jettisoned is two halves.T+10:22.5Second Stage Cutoff 1The second stage engine shuts down to complete its first firing of the launch. The rocket and attached spacecraft are now in a long coast period before the second stage reignites. The orbit achieved should be 299 nautical miles at apogee, 100 miles at perigee and inclined 97.5 degrees.T+51:40.0Second Stage RestartDelta's second stage engine reignites for a short firing to boost the elliptical orbit into a circular one.T+51:48.5Second Stage Cutoff 2The second stage shuts down after an 8.5-second burn. The orbit achieved should be 289.6 nautical miles at apogee, 282.1 miles at perigee and inclined 97.504 degrees.T+55:20.0Payload SeparationNASA's Wide-field Infrared Survey Explorer satellite is released from the Delta 2 rocket, completing the launch.Data source: ULA.STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Eavesdropping craft critical for monitoring terrorists BY CRAIG COVAULTSPACEFLIGHT NOWPosted: January 17, 2009 The Delta 4-Heavy rocket launches at 9:47 p.m. EST on January 17.Credit: Chris Miller/Spaceflight NowThe NRO payload on the Delta 4-Heavy is a 5-to-6 ton eavesdroppingspacecraft with a high tech deployable antenna as wide as 350 feet.The spacecraft is to enhance the capability for the U.S. tolisten in on communications in hostile governments like Iran andterrorist organizations like Al Qaeda.The NROL-26 mission has worried NRO officials and otherintelligence professionals because of concerns about flying thecritical satellite on the new Delta 4-Heavy.If the mission was to fail, it would spark another crisis in theU. S. intelligence community, already burdened with growing tasksfrom an increasingly dangerous world.The satellite is likely an "Advanced Mentor" design, accordingto GlobalSecurity, a military think tank. Earlier versions weredesignated Orion.Due to satellite development delays and a 1998 Titan launchfailure involving an earlier "Mercury" eavesdropper design, the U.S.has fallen as much as one or two spacecraft behind its original 10-yearschedule to launch such giant eavesdroppers. These spacecraft providethe kind of information the White House, State Dept. and Pentagonneed to make military and national foreign policy decisions.It is also likely a "broad spectrum" satellite that can update keyfrequency information on hostile radars and other detection systemsthat could threaten U.S. forces.The three earlier Mentor spacecraft introduced a very large'wrap-rib' deployable antenna design spanning up to 350 feet, saysGlobalSecurity. The Delta 4-Heavy rocket launches at 9:47 p.m. EST on January 17.Credit: Chris Miller/Spaceflight NowThe National Security Agency will be the prime distributor of thespacecraft's data, sending information from the satellite to theother 15 agencies and organizations that now make up theintelligence community.It has been five years since a large geosynchronous orbiteavesdropping satellite has been launched from Cape Canaveral. Thatearlier satellite, believed to have been a less capable version ofthe Mentor, was lofted on board a Titan-Centaur booster inSeptember 2003.Over the last two-and-a-half years, however, two different eavesdroppingsatellites have been launched on smaller Delta 4-Medium and Atlas 5rockets from Vandenberg Air Force Base, Calif. These spacecraft, withsmaller antennas, are in highly elliptical orbits of roughly 700 x 23,500miles.Instead of remaining parked over one location above the equator,these Vandenberg-launched satellites travel up and down over thenorthern hemisphere. They can listen into radio communications fromdifferent locations or radio waves monitored from different angles,compared with geosynchronous orbit satellites.The data from these different eavesdroppers is then combined andassessed with other sources of information including that obtained byaircraft such as advanced versions of the U-2.Additional coverage for subscribers:VIDEO:FULL LAUNCH EXPERIENCE VIDEO:LAUNCH PAD CAMERA NO. 1 VIDEO:LAUNCH PAD CAMERA NO. 2 VIDEO:THE DELTA 4-HEAVY ROCKET LIFTS OFF VIDEO:LAUNCH AS SEEN FROM PRESS VIEWING SITE VIDEO:TIME-LAPSE MOVIE OF THE GANTRY RETRACTING VIDEO:LAUNCH PAD'S MOBILE GANTRY ROLLED BACK MORE:STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Essential eavesdropping satellite launching Friday SPACEFLIGHT NOWPosted: November 17, 2010;Updated @ 7:52 p.m. with 24-hour launch delay to Friday night One cannot overstate the importance of Friday night's Delta 4-Heavy launch from Cape Canaveral to national security, a mission by the massive rocket that will deploy "the largest satellite in the world" to hear the whispers of evil. File image of a Delta 4-Heavy rocket. Credit: Pat Corkery/United Launch AllianceCountdown clocks are targeting a liftoff time of 6:06 p.m. EST (2306 GMT) from the Florida spaceport's Complex 37. The evening's available launch opportunity likely extends upwards of four hours.The original launch date of Thursday was delayed by 24 hours to fix an issue with ground pyrotechnics that release the big booster at liftoff. See our for live coverage.United Launch Alliance's Delta 4-Heavy is America's biggest unmanned rocket currently in service, capable of lofting the largest and heftiest cargos. The mammoth vehicle is created by taking three Common Booster Cores -- the liquid hydrogen-fueled motor that forms a Delta 4-Medium's first stage -- and strapping them together to form a triple-barrel rocket, and then adding an upper stage.The nighttime blastoff should be visually spectacular, lighting up the Space Coast with three distinct pillars of fire from the main engines trailing more than 200 feet long. Ideal viewing spots include off SR401 at Port Canaveral, along the 528 causeway or on the riverbanks in Titusville.Thundering eastward across the open Atlantic, the rocket will soar out of sight within a few minutes as it embarks on a multi-hour mission to serve the U.S. National Reconnaissance Office, the agency responsible for the country's fleet of intelligence-gathering satellites.The NRO's diverse spacecraft, including telescope-like observers and communications collectors, uncover looming dangers to the nation and provide surveillance over the world's hot spots."Always vigilant, the NRO's eyes and ears give America's policy markers, intelligence analysts, warfighters and homeland security specialists the critical information they need to keep America safe, secure and free," the agency says.The clandestine payload going up this time, known only by its launch identification number of NROL-32, is widely believed to be an essential eavesdropping spacecraft that requires the powerful lift provided by the Delta 4-Heavy to reach its listening post.In an address to the Air Force Association conference in September, NRO Director Bruce Carlson, a retired Air Force general, said this rocket launch would carry "the largest satellite in the world on it."The NRO has flown various types of communication-interceptors since the dawn of the space age, and analysts say it is virtually certain this Delta 4-Heavy is hauling another."I believe the payload is the fifth in the series of what we call Mentor spacecraft, a.k.a. Advanced Orion, which gather signals intelligence from inclined geosynchronous orbits. They are among the largest satellites ever deployed," said Ted Molczan, a respected sky-watcher who keeps tabs on orbiting spacecraft.Destined for geosynchronous orbit 22,300 miles above the planet, this new spacecraft supposedly will unfurl an extremely lightweight but gigantically huge umbrella-like antenna to overhear enemy communications and aid U.S. intelligence."The satellite likely consists of sensitive radio receivers and an antenna generally believed to span up to 100 meters (328 feet) to gather electronic intelligence for the National Security Agency," Molczan said.Observers think the mesh antenna's diameter is the size of a football field, comparable to the International Space Station's remarkable width. That explains why satellite-tracking hobbyists say these Mentor craft are "by far the brightest" in the high-flying geosynchronous orbital perch to see from the ground, outshining conventional television relay birds, weather sentinels and the like.Although NRO satellites are secretive by nature, the spacecraft are visible by just looking up. Molczan is member of a hobbyist group that routinely finds and watches the craft while monitoring the skies with precision.But despite the identity of this particular satellite being obvious, exactly where in the geosynchronous belt it will be positioned and what part of the globe it will cover are details that remain hush-hush."The upcoming launch may replace one of the older spacecraft in the series, or augment the fleet by occupying a new location in geosynchronous orbit," Molczan said. File image of a Delta 4-Heavy rocket launch. Credit: Pat Corkery/United Launch AlliancePrevious Mentor satellites were launched by Titan 4 rockets from Cape Canaveral in 1995, 1998 and 2003, plus the most recent Delta 4-Heavy in early 2009 carried one, according to the satellite-tracking hobbyists.The craft lineage can be traced to the two Magnum satellites trucked to orbit aboard the space shuttle Discovery during the STS-51C mission in 1985 and STS-33 in 1989, historians have indicated.An even earlier generation launched in the 1970s using Atlas rockets from the Cape, according to the authoritative website.Friday's rocket launch continues a surge of NRO spy satellite deployments after a lengthy 20-month lull. An Atlas 5 rocket began this ongoing campaign by dispatching a new-generation radar imaging satellite in September from Vandenberg Air Force Base, California.The upcoming schedule calls for several more significant launches in the next few months:A Delta 4-Heavy rocket for NROL-49 from Vandenberg on January 11A Delta 4 rocket for NROL-27 from Cape Canaveral on March 4An Atlas 5 for NROL-34 from Vandenberg on March 31Carlson said "this is the most aggressive launch campaign that the National Reconnaissance Office has had in 20 years, almost a quarter of a century.""The other thing I can tell you is these are very important, because they all go to update a constellation which is aging rapidly. We bought most of our satellites for three, five, or eight years, and we're keeping them on orbit for ten, twelve, and up to twenty years," Carlson said."Now, when I buy something people complain about how expensive it is, but nobody ever complains when it's time to die and it keeps right on ticking. Some of these guys are like the Energizer bunny and they have really done marvelous work."We're doing things that were designed to essentially operate during the era of the Soviet Union that are today doing tactical intelligence collection that leads us to actionable intelligence on bad guys every day. Every day. And we're doing it with equipment that's 15, 18, and 20 years old."STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.STS-133 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Discovery is symbolized in the official embroidered crew patch for STS-133. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia's historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard's historic Mercury mission with this collectors' item, the official commemorative embroidered patch. | | | | 2014 Spaceflight Now Inc.Experts using computer simulations in Delta 4 probe SPACEFLIGHT NOWPosted: January 30, 2005CAPE CANAVERAL, Fla. - While complex computer simulations are being run to understand what interrupted its main engines from finishing their firings, the entire six-hour maiden flight of the Boeing Delta 4-Heavy rocket was examined in deep detail last week as part of a planned post-mission review. Free hydrogen ignites as the three RS-68 main engines roar to life during the final seconds of the Delta 4-Heavy rocket's launch countdown. Credit: Gene Blevins/LA Daily News"The flight data review was extremely thorough, scrutinizing not only the extensive, standard flight telemetry data, but also the additional data from more than 500 channels of special instrumentation, specifically installed for this first Heavy mission," said Col. John Insprucker, Evolved Expendable Launch Vehicle Program Director at the Air Force's Space and Missile Systems Center.Officials sifted through mounds of data collected from liftoff through deployment of the mock satellite cargo during the Air Force-ordered test launch. The Defense Department awarded Boeing a $141 million contract to fly the first Delta 4-Heavy on a demonstration launch instead of carrying a real payload. "It's important to remember that the primary payload for this mission was really the instrumentation we carried onboard," Col. Insprucker said. "Our investment in telemetry and additional special instrumentation is helping us quickly zero in on the cause of the anomaly, and I'm confident the data will also enable us to fine-tune all aspects of our future Delta 4 heavy-lift missions."The December 21 flight was deemed a success despite a problem impacting the firing time of all three Common Booster Cores, which were strapped together to form the rocket's first stage. The Rocketdyne-made RS-68 main engine on each booster shut down several seconds early, causing a speed deficit that the rocket's upper stage could not overcome. The dummy satellite was delivered into an orbit much lower than planned and two nanosats were lost.The ongoing investigation to determine why the engines stopped firing 8 seconds prematurely on the port and starboard boosters and 9 seconds early on the center stage has narrowed the list of possible culprits. The leading theory continues to be a condition called cavitation where liquid oxygen flowing through the feedline from the tank to the engine turns to gaseous oxygen. This phenomenon is believed to have occurred around internal sensors that are designed to tell the engines when to shut down. The sensors reacted to the bubbles, thought the boosters had run out of liquid oxygen and commanded the RS-68s to cut off. But each motor had plenty of liquid oxygen remaining in their tanks to finish the normal firing time.Using the standard investigative tool known as a Fault Tree analysis, the team has cleared 42 of 49 potential causes, including the sensors themselves and the main engines. All 7 remaining branches in the Fault Tree involve various types of disturbances in the flow of liquid oxygen, the Air Force said. The Delta 4-Heavy rocket launches on its test flight. Credit: Gene Blevins/LA Daily News"The team is meeting daily across multiple locations to complete the investigation," said Dan Collins, vice president of Boeing Expendable Launch Systems. "Determining root cause from the remaining 7 open branches is the top priority."Computer models that simulate the liquid oxygen flow within the feedline on each booster are examining the cavitation scenario. The liquid oxygen tank is located at the top-end of each stage, above the liquid hydrogen fuel tank, with a feedline running down the length of the booster to the main engine. The Air Force says the engine cutoff sensors are positioned about five feet downstream of the liquid oxygen tank."Initial simulation runs have already given new insight into the flow dynamics in the feedline (velocity and pressure patterns). The team will progressively add details to the computer models to build up an accurate representation of the internal features of the tank and feedline, and to simulate the flight conditions at the time of the premature engine cutoff," the Space and Missile Systems Center said in a statement Friday."The simulation team will use these models, along with the flight sensor data, to identify where cavitation is most likely to have developed in the liquid oxygen flow for the Heavy demonstration flight conditions. The onset of cavitation is thought to be caused by a unique combination of vehicle acceleration,?liquid oxygen?level in the propellant tank,?tank pressures,?feedline internal features and flow rates in the feedline when the RS-68 engine is at full power."The team also plans to simulate liquid oxygen flow under flight conditions from previous Delta 4 missions, where the anomaly was not observed, to help verify the accuracy of the complex computer models."Three previous Delta 4 missions have flown -- all successfully and on target -- in the so-called Medium configuration that features just one Common Booster Core. The Heavy design uses three booster cores in order to launch much heftier payloads.Additional coverage for subscribers:VIDEO:FROM LIFTOFF TO BOOSTER SEPARATION VIDEO:THE DELTA 4-HEAVY LAUNCH (SHORT VERSION) VIDEO:ONBOARD CAMERA RECORDS LAUNCH VIDEO:ONBOARD CAMERA SEES BOOSTER SEPARATION VIDEO:ONBOARD CAMERA CAPTURES FAIRING JETTISON AUDIO:LISTEN TO THE 68-MINUTE PRE-LAUNCH NEWS CONFERENCE VIDEO:ANIMATION PROVIDES PREVIEW OF A DELTA 4-HEAVY LAUNCH VIDEO:RE-LIVE THE INAUGURAL DELTA 4 LAUNCH FROM 2002 VIDEO:ON-PAD FLIGHT READINESS ENGINE FIRING TEST VIDEO:TAKE TOUR OF LAUNCH PAD 37B Apollo 11 special patchSpecial collectors' patch marking the 35th anniversary of the historic Apollo 11 moon landing is now available.Choose your store: - - - Inside Apollo mission controlAn insider's view of how Apollo flight controllers operated and just what they faced when events were crucial. Choose your store: The ultimate Apollo 11 DVD This exceptional chronicle of the historic Apollo 11 lunar landing mission features new digital transfers of film and television coverage unmatched by any other.Choose your store: - - - Next ISS crewOwn a little piece of history with this official patch for the International Space Station's Expedition 11 crew. We'll ship yours today!Choose your store: New StationCrew PatchFree shipping to U.S. addresses!The Expedition 38 embroidered crew patch for the International Space Station is now available in our store!Apollo patchesThe Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.

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