Aabida

The name Aabida is a baby girl name.

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Muslim Meaning:
The name Aabida is a Muslim baby name. In Muslim the meaning of the name Aabida is: Worshippess. Adoress.

SoulUrge Number: 3

People with this name have a deep inner desire to create and express themselves, often in public speaking, acting, writing or singing. They also yearn to have beauty around them in their home and work environment.

Expression Number: 9

People with this name tend to be passionate, compassionate, intuitive, romantic, and to have magnetic personalities. They are usually humanitarian, broadminded and generous, and tend to follow professions where they can serve humanity. Because they are so affectionate and giving, they may be imposed on. They are romantic and easily fall in love, but may be easily hurt and are sometimes quick-tempered.

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: September 14, 2006Running behind schedule because of software problems, flight controllers early today began a slow, careful process to unfurl a new set of solar arrays aboard the international space station. The plan called for first deploying the huge panels just a few feet to let them warm up and decompress after years in storage. Later today, the Atlantis astronauts will send commands to fully extend the new arrays. The first section of solar wing was unfurled this morning. Credit: NASA TV/Spaceflight NowThe initial deployment had been planned for Wednesday night, but software problems held up checkout of a large rotary drive mechanism designed to rotate the new arrays 360 degrees to stay face on to the sun as the station circles the globe.One of two drive lock assembly - DLA - motors in the solar alpha rotary joint worked properly in an initial test, rotating the still-stowed arrays 180 degrees. But the drive gear in a redundant DLA appeared to be misaligned and testing was put on hold. Late last night, engineers traced the problem to a software commanding issue and after implementing a workaround, DLA-2 eventually moved the arrays through a 360-degree rotation as planned.Finally, at 5 a.m., the first set of arrays - 4A - began slowly unfurling on ground command as its self-assembling mast pulled the top few feet of folded solar cell blankets from its box. The other array, 2A, followed suit at 5:46 a.m.The Atlantis astronauts hope to complete solar array deployment later today in stages, sending commands to unfurl the panels first to 49 percent and then to a full 100 percent in what promises to be the most visually dramatic moment of the ongoing space station assembly mission.Here is an updated timeline of today's activities (NOTE: solar array deploy times are uncertain and not included; in EDT and mission elapsed time):12:15 AM041300STS/ISS crew wakeup03:35 AM041620EVA tool config05:40 AM041825ERCA troubleshooting06:10 AM041855Station robot arm reconfig06:45 AM041930Crew meals begin11:25 AM050010Canadian PAO event with Jett, MacLean11:45 AM050030Transfer tagup11:50 AM050035CNN, NPR interview Jett, Vinogradov, Williams11:50 AM050035Infrared camera setup12:10 PM050055EVA-3: Procedures review02:20 PM050305EVA-3: Campout mask pre-breathe (Tanner, Piper)03:05 PM050350EVA-3: Crew lock 10.2 depress03:45 PM050430ISS crew sleep begins04:15 PM050500STS crew sleep begins (Tanner, Piper in airlock)Each solar array wing is 15 feet wide and 115 feet long. Extending in opposite directions, the wings will stretch more than 240 feet from tip to tip when fully deployed. The so-called P4 array, or port 4 segment of the station's main power truss, is bolted to the SARJ mechanism on the outboard side of the P3 truss segment that also serves to route power and data to and from the solar panels.When completed, the space station's power truss will stretch more than a football field from end to end. Two huge solar arrays on each end of the truss will track the sun as the station circles the globe, rotating and changing pitch as required to maximize electrical generation.Finishing the main truss and wiring in the new arrays is a major element of near-term station assembly missions.One set of arrays, P6, is already attached to the station, providing power for the U.S. segment of the outpost. It is attached to the Z1 truss that extends upward from the Unity module at right angles to the main solar array truss. It will be moved next August to its final position next to the P4 arrays that were attached to the station Tuesday by Atlantis' crew.Two other sets of identical arrays will be mounted on the right side of the truss during shuttle assembly flights in February 2007 and June 2008.Designed by Boeing, the newly attached P4 truss features two motor-driven self-assesmbling masts designed to pull out a pair of solar blankets. For launch, the arrays are folded like venetian blinds in blanket boxes measuring 15 feet long but just 20 inches thick.The P3 truss was delivered to the Kennedy Space Center in November 1999. P4 followed suit in July 2000. The solar array blankets have not been unfolded since they were originally stowed for launch.Prior to Columbia's launch in January 2003, the arrays were certified to operate and deploy normally when stowed for up to 45 months. Because of the extended downtime after the Columbia accident, one of the blanket boxes on P4 was removed and shipped to California for deployment tests. A replacement blanket was installed aboard P4.As it turned out, the deployment tests went well and the blanket, which had been stowed 39 months at that point, worked normally. As a result, the certification age limit was boosted to 82 months. As of launch aboard Atlantis, the P4 blankets had been stowed for 67 and 73 months respectively.One other consequence of the Columbia recovery and subsequent launch delays was a decision to replace all 12 batteries in P4. The 372-pound batteries were swapped out in March and August of 2005.The solar array wings were designed by Lockheed Martin. They weigh more than 2,400 pounds and feature some 33,000 solar cells per blanket. They are designed to produce more power than the station actually needs to compensate for normal degradation as the outpost ages.The blankets must face the sun directly for maximum electrical generation and two mechanisms are in place to do just that. The wings can be rotated about their long axis by beta gimbal joints, much like the pitch of an airplane propeller can be adjusted. The SARJ, on the other hand, rotates the arrays through 360 degrees like a waterwheel around the axis of the main truss.The P4 integrated equipment assembly, or IEA, is a cube measuring 16 feet on a side and weighing nearly 17,000 pounds. It includes direct current converters, 12 batteries, battery chargers, control computers and an ammonia cooling system to keep the electronic gear at the proper temperature. A single set of folding radiator panels will extend 44 feet when fully deployed.Most of the work to ready the new P4 arrays for extension "is done by the flight control team," Jett said. "The EVA crew does the physical work, in terms of, positioning the arrays and releasing all the bolts and the launch restraints. But then the preparation to actually make the deployment happen, all the activation sequence and the activation of the rotary joint, is all performed by the ground team."The P4 arrays are identical to P6, which was attached to the space station during shuttle mission STS-97 in December 2000. When the first blanket was deployed, engineers were surprised to see several of the blanket panels had stuck together. When they jerked free, a tensioning cable jumped its guides and required repairs on a subsequent spacewalk. For the second array's deployment, the crew let the sun warm up the array and deployed it in a so-called high-tension mode. That technique worked, and the array unfurled without incident.For the P4 deploy, the arrays will first be extended the length of a single bay of each mast - a few feet worth - to relieve compression and to begin warming up the panels."The one-bay deploy is basically to start the relaxation of the blankets and to get ahead," station flight director John McCullough said Wednesday. "The time we're in an inertial attitude, the attitude where we continuously point the arrays at the sun, is limited because the rest of the space station doesn't really like that atitude."For this deploy, we want to have the sun in a certain cone to warm the back of the blankets and there's a limit to that. We can only be there for three revs around the Earth."Working in stages, the astronauts will extend the 4A mast to a distance of 49 percent early Thursday, wait a half hour or so for additional solar heating, and then the rest of the way to full extension. They will repeat that process for the 2A mast. It will take about 90 minutes for each panel to fully deploy."We're not too terribly concerned about stiction on the deploy," said Tanner, a veteran of the STS-97 mission. "We know it might happen in certain panels. The team went hard to work after STS-97 to figure out the mechanism of stiction and what we can do to reduce it. They came up with a good operational plan to nominally deploy."Now if for some reason one or two panels sticks after all that, then we can go out EVA, it would be on EVA 3, and actually manually peel the panels apart for the first 40 inches or so and doing a nominal deploy after that. All of our tests say they will peel open very easily. So we're not too terribly concerned about that."Space station Program Manager Mike Suffredini agreed that experience gained during the STS-97 mission in 2000 should result in a smooth deploy."The good news is we've done it twice before," Suffredini said. "The first time we deployed one of these arrays, we learned about a stiction issue that existed. After quite a bit of work during that mission, we deployed the second array in a little bit different technique, which allowed us to be successful. We learned a lot about techniques to get these arrays out without having the tension wire come loose, which is what happened when we tried to deploy the first one. It turns out after a lot of work ... we figured out a fix to go back in there to put it back in its original condition. And of course, the arrays have been fine ever since.Using an engineering model, "we did quite a bit of testing on this stiction issue and how these arrays can stick together based on the silicon bead that's on the arrays and then we compress them for long periods of time before they go fly. And that was basically the cause of the problem. Over a long period of time this silicon would tend to attach itself to the back part of the array. And so we've done a number of things, largely operational changes but also on how we dealt with the arrays."While the arrays were compressed for shipment to Florida, that pressure was relaxed until shortly before final preparations."Probably the largest changes were operational," Suffredini said. "We will partially deploy the array about one bay's worth and we'll let it warm up and sort of expand a little bit. Then the actual deploy process a little bit later will have us deploy the array halfway and then you'll see us sit for about 30 minutes as we warm it up and then we'll go the rest of the way."In addition to that, we're using what we call a high-tension mode. Instead of leaving the lower part of the array free to move up and down as the array gets deployed, we learned we need to hold it down against the bottom of the blanket box. So the new technique holds it down and then this particular deploy lets the heat warm things up, to allow the silicon to free itself, is the process we'll use to deploy. I have a lot of confidence in the deployment of the arrays."The new solar arrays will not be rotated on the SARJ because of interference with the port wing of the P6 array and they will not provide any power to the space station until reconfigurations during the next shuttle mission in December.For readers interested in a bit more detail, here is an overview provided by Boeing, the prime contractor.Source: BoeingElectrical power is the most critical resource for the ISS because it allows astronauts to live comfortably, safely operate the station, and perform complex scientific experiments. Since the only readily available source of energy for spacecraft is sunlight, technologies were developed to efficiently convert solar energy to electrical power. One way to do this is by using large numbers of solar cells assembled into arrays to produce high power levels. The cells are made from purified crystal ingots of silicon that directly convert light to electricity through a process called photovoltaics. Solar cells do the job, but a spacecraft orbiting the Earth is not always in direct sunlight so energy has to be stored. Storing power in rechargeable batteries provides a continuous source of electricity while the spacecraft is in the Earth's shadow.NASA and Lockheed Martin developed a method of mounting the solar arrays on a "blanket" that can be folded like an accordion for delivery to space. Once in orbit, astronauts deploy the blankets to their full size. Gimbals are used to rotate the arrays so that they face the Sun to provide maximum power to the Space Station. The solar arrays track the sun in two axes: beta and alpha.P4 is the second of four PVMs that will eventually be brought up to the International Space Station, converting sunlight to electricity. The first one, named P6, was brought on orbit by the STS-97 crew in November 2000. The primary functions of the P4 photovoltaic module are to collect, store, convert and distribute electrical power to loads within the segment and to other ISS segments. The P4 PVM consists of two beta gimbal/PV array assemblies, two beta gimbal transition structures, one integrated equipment assembly and associated cabling and tubing. The P4 PVM components were assembled by Boeing in Tulsa, Okla. and Lockheed Martin in Sunnyvale, Calif. prior to final assembly and testing by Boeing at Kennedy Space Center, Fla.There are two solar array wings (SAW) designed, built and tested by Lockheed Martin in Sunnyvale, Calif. on the P4 module, each deployed in the opposite direction from each other. Each SAW is made up of two solar blankets mounted to a common mast. Prior to deployment, each panel is folded accordion style into a solar array blanket box (SABB) measuring 20 inches high and 15 feet in length. Each blanket is only about two inches thick while in this stored position. The mast consists of interlocking battens which are stowed for launch inside a mast canister assembly (MCA) designed, built and tested by ATK-Able. When deployed by the astronauts, the SAW deploys like an erector set as it unfolds. It has two arms like a human torso when mounted on P4 which are rotated outwards by astronauts during a spacewalk so they can be fully deployed. Because these blankets were stored for such a long time, NASA, Boeing and Lockheed Martin conducted extensive testing to ensure they would unfold properly once on orbit to ensure there would be no problems with the blankets sticking together. This testing was completed in July 2003.When fully deployed, the SAW extends 115 feet and spans 38 feet across and extends out to each side of the integrated equipment assembly. Since the second SAW is deployed in the opposite direction, the total wing span is over 240 feet.Each solar array wing weighs over 2,400 pounds and use nearly 33,000 (32,800 per wing) solar array cells, each measuring 8-cm square with 4,100 diodes. The individual cells were made by Spectrolab and ASEC. There are 400 solar array cells to a string and there are 82 strings per wing. Each SAW is capable of generating nearly 32.8 kilowatts (kW) of direct current power. There are two SAWs on the P4 module yielding a total power generation capability approaching 66 kW, enough power to meet the needs of 30 average homes without air conditioning (based on an average 2kW of power).Additional coverage for subscribers:VIDEO:PORT 3/PORT 4 TRUSS KEEL PIN REMOVED AND STOWED VIDEO:HELMETCAM OF BURBANK REMOVING SARJ RESTRAINT VIDEO:SPACEWALKERS PAUSE FOR PICTURE TIME VIDEO:STEVE MACLEAN REPORTS LOST BOLT VIDEO:ROTARY JOINT LOCK REMOVED BY SPACEWALKER VIDEO:STEP-BY-STEP PREVIEW OF SPACEWALK NO. 2 VIDEO:POST-EVA 1 STATUS BRIEFING VIDEO:TANNER LOSES BOLT DURING ROTARY JOINT WORK VIDEO:PIPER UNFOLDS SOLAR BLANKET BOXES VIDEO:SECOND WING'S STRUCTURE DEPLOYED BY PIPER VIDEO:FIRST SOLAR WING'S STRUCTURE DEPLOYED BY TANNER VIDEO:STEP-BY-STEP PREVIEW OF SPACEWALK NO. 1 VIDEO:TRUSS HANDED FROM SHUTTLE ARM TO STATION ARM VIDEO:ARM MANEUVERS TRUSS OVER SHUTTLE WING VIDEO:TRUSS SLOWLY LIFTED OUT OF PAYLOAD BAY VIDEO:ATLANTIS' ARM GRAPPLES THE TRUSS VIDEO:MONDAY'S MISSION STATUS BRIEFING VIDEO:ATLANTIS WELCOMED ABOARD THE STATION VIDEO:DOCKING REPLAY FROM CAMERA ON SHUTTLE ARM VIDEO:SHUTTLE ATLANTIS DOCKS TO THE STATION VIDEO:ATLANTIS' BREATH-TAKING FLIP MANEUVER VIDEO:CREW'S CAMCORDER FOOTAGE OF EXTERNAL TANK VIDEO:NARRATED ANIMATION PREVIEWING TRUSS UNBERTHING VIDEO:NARRATED ANIMATION PREVIEWING THE DOCKING VIDEO:NARRATED ANIMATION OF PAYLOAD BAY CONFIGURATION MORE: VIDEO:BRIEFING ON TANK'S PERFORMANCE VIDEO:TANK'S ONBOARD CAMERA LIFTOFF TO SEPARATION VIDEO:FLIGHT DIRECTOR EXPLAINS INSPECTIONS VIDEO:SUNDAY'S MISSION STATUS BRIEFING VIDEO:LAUNCH OF ATLANTIS! 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Engineers are studying the test data to determine if there are any concerns about the joints in Discovery's boosters."With respect to the solid motor joint adhesive, I don't think I would even call it suspect because I don't know enough to be able to even put an adjective or a characterization of it," Cain said. "What we know is there is a test out there, or the results of a test, we need to look further at to determine whether or not we have any concerns. That's really and truly where we are. We don't even know enough to know if we have a concern."I wouldn't want to speculate, really, on either one of those problems as to where they might lead, but you can be certain we'll follow the data."The only other issue of any significance is the weather. 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Their complaint, like the amended LIBOR complaints also filed Monday night by a class of investors in exchange-traded, LIBOR-based securities and by Charles Schwab, is filled with charts and economic analysis purporting to show that the LIBOR panel banks deliberately reported lower borrowing rates than they were actually charged, with the apparent motive of making themselves look healthier than they were and of setting artificially low interest rates on LIBOR-based securities. (Here??s the by the exchange-traded securities class, which is represented by Kirby McInerney and Lovell Stewart Halebian Jacobson; here??s the , filed by Lieff Cabraser Heimann & Bernstein.) The complaints track LIBOR rates against other metrics, like the banks?? probability of default, Eurodollar deposit rates, and credit default swap spreads, to conclude that the rates banks reported every day to the unregulated LIBOR-setting body couldn??t be truthful. Wish List (0)

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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: November 20, 2007Floating in the Quest airlock module, space station commander Peggy Whitson and Dan Tani switched their spacesuits to internal battery power at 5:10 a.m. today to kick off a planned six-hour 40-minute spacewalk to route power and cooling to the new Harmony module. A second excursion will be needed Saturday to finish the job and help clear the way for launch of shuttle Atlantis Dec. 6 on a long-awaited mission to deliver a European laboratory module."A nice day at the office here," Tani said as he floated out of the airlock high above the north Atlantic Ocean. "Oh, it's just an awesome view!"This is the 98th spacewalk devoted to station assembly and maintenance since construction began in 1998, the 21st so far this year and the second for the Expedition 16 crew. Whitson and flight engineer Yuri Malenchenko carried out the crew's first EVA on Nov. 9, preparing the station's shuttle docking port for attachment to Harmony.With that work complete, the docking port was robotically removed from the front of the Destiny lab module on Nov. 12 and bolted to Harmony, which was initially mounted on the left-side of the central Unity module. The assembled Harmony/docking port "stack" then was moved to its permanent home on the front end of Destiny two days later.The goal of today's spacewalk by Whitson and Tani is to make a variety of electrical connections between Harmony and Destiny to route solar array power to the new module. They also will unstow and mount ammonia cooling lines that will run in a long tray from the complex's main power truss, across the Destiny module to the interface with Harmony.A second spacewalk Saturday will mirror today's work, giving Harmony the power and cooling necessary to support European and Japanese research modules that will be attached to the module's forward ports."We think we've got a good plan together, the teams on the ground have really helped us out and we feel ready," Whitson, the station's first female commander, said Monday."Peggy's always cool. I'm just trying to do the collected part," Tani joked. "We are excited and these EVAs I expect to be tough. When we practice them in the water, I always come out thinking, boy those are really some pretty challenging tasks that we're being asked to do. So we're looking forward to it."Plus, we know that we are in the critical path to getting the node (Harmony) fully activated so the next shuttle can launch. So there's a little bit of pressure there, but we like the pressure and we're really looking forward to getting outside and getting the work done."After leaving the station's airlock, the spacewalkers will meet on the lower side of the central S0 segment of the solar power truss to remove an ammonia shunt jumper from coolant loop A, permitting attachment of the loop A cooling line tray later in the EVA.After reconfiguring electrical connectors in the P1 solar array truss segment and removing caps from ammonia lines leading into Harmony, Whitson and Tani will unstow the hinged 18.5-foot-long 300-pound loop A tray from its storage location on the central solar array truss.The loop A tray will be mounted on top of the starboard avionics tray on the right side of the Destiny module. With the tray in place, the spacewalkers will make six ammonia fluid line connections to complete the loop A supply and return lines: Two connections between the S0 truss and the tray; two at a hinge in the tray; and two more between the end of the tray and Harmony.With coolant loop A in place, Whitson and Tani plan to turn their attention to making electrical connections. Tani will connect 11 cables on the other side of the lab module and Whitson will connect four cables between the shuttle docking port and Harmony.Saturday's spacewalk is virtually identical, with work to connect the loop B cooling lines, make additional electrical connections and to prepare Harmony's right-side port for the upcoming attachment of Columbus."Once we get through these EVAs, we still have some logistics-type tasks, nothing I would consider very y or noteworthy, but still things we need to get done between now and 1E (the Columbus flight)," said Kenny Todd, space station integration and operations manager."We've been on a tight schedule trying to get to this launch Dec. 6, so we are reviewing daily our tasking to ensure we're only doing those things we need to do to be able to support this flight in early December. We're all very, very excited about getting the Columbus module on orbit."The first of the Expedition 16 crew's three spacewalks had been scheduled to be carried out during the shuttle Discovery's recent visit. But unplanned work to fix a mangled solar array forced mission planners to defer the station crew's spacewalk to Nov. 9, after the shuttle's departure.Whitson, Tani and Malenchenko have been working pretty much non stop to get Harmony moved, hooked up and prepared for Columbus in time to permit the Atlantis flight during a short eight-day launch window that opens Dec. 6."They are not going to have Thanksgiving off," said station flight director Holly Ridings. "The crew knew that this month of November was going to be very, very challenging. And so they said right up front, if it works out that we need to work on Thanksgiving, we are more than happy to do that. And it did work out that way. So they will be working on Thanksgiving with a lot of us here working as well to support them."That doesn't mean they won't take time off for a traditional Thanksgiving Day meal in space. During a TV downlink Monday, Whitson and Tani took time to beam down a holiday greeting."We wanted to say happy Thanksgiving to all our NASA (television) viewers," Whitson said. "We feel particularly privileged and thankful to be up here on board the international space station this Thanksgiving and we're looking forward to our activities this week - we have a busy week with EVAs - and we hope that you also are having a great Thanksgiving."Said Tani: "My family, we gather for Thanksgiving and we spend a minute just thinking about the things we're thankful for and of course, I'm thankful for the continued health of my family and my loved ones. Also this year, I'm thankful that I'm safely on the space station, conducting our mission successfully and having a great time doing it. I'm thankful for all the people on the ground who support us and who are tireless in their devotion to the space station program, to the space program in general and to the crew. And I'm thankful for Peggy, my crewmate ... and Yuri."When we think about Thanksgiving, we think about the Pilgrims coming to the New World and expanding their knowledge of their universe, making new discoveries and making a better life for themselves. And Thanksgiving was an opportunity to be thankful for their survival of a very difficult time. And I think maybe where we are in the space program, of human space adventures, and thinking that well, here we are safely on the space station, we have setbacks but we solve them and hopefully this is the start of our generation, or our world, expanding our knowledge and learning how to live in space and expand our knowledge outside of low-Earth orbit."Whitson then took the microphone and said, "So we would like to wish everyone on Earth a happy Thanksgiving, and especially our NASA family. We're thankful to be part of that family."The two astronauts then showed off some of the food they enjoy in space, including Thanksgiving Day fare, including freeze-dried shrimp cocktail - "it's a favorite of almost everybody on board the station" - and Russian canned lamb and vegetables.Along with sliced oranges, Tani showed off a package of Italian ham sent up by his family and miniature, bite-size loaves of Russian bread that "are delicious complements to our food.""Finally, we don't go anywhere in the universe without chocolate," Tani said as Whitson let M&M candies float free. "These are the popular candy-coated chocolates and they're popular because of the color and the fun. I think they say they melt in the mouth and not on the lab."Holding up an empty bottle of hot sauce, Whitson said: "Our motto on board the station is, it's all about the sauce. The best part of eating here is you have to have the right sauce to put on it and typically, the hotter the sauce, the better. This one obviously is our favorite!"So happy Thanksgiving to all of you on the ground, we're thrilled to be here and have the opportunity to continue our assembly and we wish all the best for our friends and family and the NASA family as well. Thanks so much." 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. 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Credit: SpaceXSpaceX founder and chief executive Elon Musk debuted the space capsule from the company's headquarters here before a crowd of employees, VIPs and media.The white gumdrop-shaped space capsule, dubbed Dragon Version 2, is about halfway through development in a public-private cost-sharing arrangement between SpaceX and NASA, Musk said.The current iteration of the Dragon capsule has flown five times, all successfully, including three operational cargo deliveries to the space station under a $1.6 billion commercial resupply contract with NASA."Going from Dragon Version 1, we wanted to take a big step in technology," Musk said. "Some important characteristics of that is the ability to land anywhere on land propulsively. You'll be able to land anywhere on Earth with the accuracy of a helicopter, which is something I think a modern spaceship should be able to do."The spaceship can host up to seven astronauts for several days on its own after launching on SpaceX's Falcon 9 rocket. It can withstand a half-year in orbit when docked to the International Space Station.The capsule showcased Thursday featured touchscreen displays and seven leather seats emblazoned with a SpaceX logo. Musk described the interior during a webcast of the announcement."We've aimed for something with Dragon Version 2 for the interfaces and the overall aesthetic of something that's very clean -- very simple. As the pilot, you're able to interact with the screens overhead and control the spacecraft, and then we've got all the critical functions that are needed in an emergency situation as manual buttons."Speaking with reporters after the event, Musk said the touchscreen technology was borrowed brom Tesla, his electric car company. SpaceX CEO Elon Musk presents Dragon Version 2 at the company's headquarters in Hawthorne, Calif. Credit: Gene Blevins/LA Daily News"The biggest difference [between the two Dragon versions] is the SuperDracos," said Garrett Reisman, a former NASA astronaut and manager of SpaceX's commercial crew transportation program. "We can do launch abort and also return to land. There's a lot of other more subtle differences, but that's the big one."The crew-capable Dragon will still feature a trunk section to carry unpressurized cargo, but the extendable power-producing solar panels on the resupply version of the capsule are replaced by fixed panels attached to the craft's body. It is also designed to be reused up to 10 times without major refurbishment.Reisman said SpaceX is aiming to launch crews on Dragon spacecraft and complete an autopilot docking with the International Space Station on the same day."Another [difference] is this one gets to the space station all by itself. You don't have to grab it with the space station's robot arm."After training on the venerable Russian Soyuz spacecraft before a three-month expedition on the space station, Reisman said SpaceX's Dragon offers a roomier ride for astronauts."There's so much more elbow room in there compared to the Soyuz," he said. "Instead of just bringing two of your buddies, you can bring six ... It's got modern electronics, it's got modern materials in the heat shield. So technologically, it's a giant leap beyond the Soyuz." NASA is in the middle of a months-long process to select one or two companies to finish developing privately-owned, government-funded spacecraft to ferry astronauts to and from the space station. Officials say NASA plans to announce its decision in August or September.SpaceX, Boeing Co., and Sierra Nevada Corp. currently receive funding from NASA. Boeing and SpaceX won agreements in August 2012 worth $460 million and $440 million, respectively, to work on their CST-100 and Dragon capsules. Sierra Nevada was selected at the same time to continue development of the Dream Chaser lifting body spacecraft at a slower pace, receiving an award worth up to $212.5 million.NASA pays the companies upon the completion of certain milestones, such as tests and design reviews.NASA to date has committed $525 million to SpaceX, pending payments at the completion of several more milestones later this year. Once Boeing finishes work under its agreement with NASA, the aerospace giant will have received $580 million. Payments to Sierra Nevada will total $323 million at the end its agreement later this year. A look inside the seven-seat Dragon spacecraft. Credit: Gene Blevins/LA Daily NewsMusk said development of the upgraded human-rated version of Dragon will cost between $800 million and $1 billion. About half of they money has already been spent."For the spacecraft itself, it's going to be something on the order of 70 to 90 percent NASA-funded," Musk said. "The rocket is not NASA-funded at all."NASA faces a decision late this summer whether to pour its money into one spacecraft team, or spread its funding among two companies to maintain competition, which officials say would keep costs down."If we don't win the NASA contract, we'll do our best to continue the development and still make it happen," Musk said Thursday.The House of Representatives committee charged with NASA oversight wants to force NASA to pick one company, saying it will ensure U.S. crew flights begin as soon as possible, ending NASA's reliance on Russian Soyuz vehicles to transport astronauts to the space station.According to Musk, the Dragon Version 2 could be ready for an unmanned orbital test flight by the end of 2015. A piloted demonstration mission to the space station would follow in 2016 before NASA gives its blessing for operational crews to climb aboard the capsule."From a SpaceX standpoint, we actually expect to be ready to transport crew in 2016, about a year sooner than NASA needs it," Musk said. "NASA wants to be a little cautious in the timing of things, so they don't want to count on us being there in 2016, but we feel fairly confident that the vehicle will be ready in two years."NASA officials say a commercial crew spacecraft can be operational by the end of 2017 under the program's current budget.Musk unveiled the new version of Dragon in a presentation at the company's headquarters, highlighting the capsule's futuristic appearance and innovative technologies in a pep rally-like atmosphere.A curtain dropped to reveal the capsule on SpaceX's factory floor as a fog machine and multi-colored lights cast a dramatic glow on the spacecraft.Musk described the capsule as "flight hardware" in response to questions from reporters but officials did not say if or when any of the vehicle presented Thursday would fly. Artist's concept of a Dragon spacecraft with crew approaching the International Space Station. Credit: SpaceXEight SuperDraco rocket engines mounted around the circumference of the spacecraft will slow down the capsule during descent, guiding it to a gentle touchdown on a landing pad. The cargo version of the Dragon spacecraft parachutes into the Pacific Ocean."The biggest technology change for Dragon Version 2 was the SuperDraco engine," Musk said. "That has to produce a tremendous amount of thrust and yet be very light. It's also got to throttle over a wide range, so it's got to be able to go from a very low throttle range to a very high throttle range and react very quickly. It was quite a tricky thing to develop."SpaceX announced Tuesday it has finished qualification testing of the SuperDraco engine ahead of a planned pad abort test of the Dragon spacecraft later this year.The SuperDraco thrusters also function as a launch abort system, capable of whisking an astronaut crew to safety if a rocket exploded after liftoff.Each SuperDraco engine can generate up to 16,000 pounds of thrust, but their power can be adjusted during descent to control the capsule's trajectory and velocity. Musk said the engine's thrust chamber is made by 3D printers in what SpaceX claims is an unprecedented use of the simplified, low-cost manufacturing technology in spaceflight."If you can 3D print something with sufficiently good material properties, then that's the easiest way to do it, certainly in a rocket company," Musk said. "In the case of the SuperDraco engine, we didn't in the very beginning anticipate being able to 3D print it," Musk said. "We tried all sorts of normal methods of developing the engine, and to be honest, those did not have great success. We said, let's give 3D printing a try and see if it works. Initially, we thought of it as sort of a Hail Mary, and it actually turned out to work super well."Musk said the human-rated Dragon will still carry parachutes in case of a propulsion system failure during re-entry.Follow Stephen Clark on Twitter: .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!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. 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This artist's concept illustrates a Falcon 1 rocket. Credit: SpaceXThe South African amassed a fortune as co-founder of PayPal, the online payment system, and earlier the Zip2 software company. He's spending his cash to bring the Falcon rockets to the launch pad."The past few decades have been a dark age for development of a new human space transportation system. One multi-billion dollar government program after another has failed. In fact, they have failed even to reach the launch pad, let alone get to space," Musk said in testimony before a U.S. Senate committee last spring."The reaction of the public has been to care less and less about space, an apathy not intrinsic to a nation of explorers, but born of poor progress, of being disappointed time and again. When America landed on the Moon, I believe we made a promise and gave people a dream. It seemed then that, given the normal course of technological evolution, someone who was not a billionaire, not an astronaut made of 'The Right Stuff,' but just a normal person, might one day see Earth from space. That dream is nothing but broken disappointment today. If we do not now take action different from the past, it will remain that way."SpaceX has been selling its small Falcon 1 rocket for $5.9 million and the beefed up Falcon 5 for $15.8 million, plus launch site Range fees, which is significantly cheaper than other American rockets available today with comparable lifting capacity."In fact, it was precisely to improve the cost and reliability of access to space, initially for satellites and later for humans, that I established SpaceX (although some of my friends still think the real goal was to turn a large fortune into a small one)," Musk said in his Senate testimony."Our first offering, called Falcon 1, will be the world's only semi-reusable orbital rocket apart from the space shuttle. Although Falcon 1 is a light class launch vehicle, we have already announced and sold the first flight of Falcon 5, our medium class rocket."Long term plans call for development of a heavy lift product and even a super-heavy, if there is customer demand. We expect that each size increase would result in a meaningful decrease in cost per pound to orbit. For example, dollar cost per pound to orbit dropped from $4,000 to $1,300 between Falcon 1 and Falcon 5. Ultimately, I believe $500 per pound or less is very achievable." The first Falcon rocket is lifted upright on its Vandenberg launch pad. Photo: SpaceXThe relatively small coterie of engineers working for SpaceX, based in El Segundo, California, has developed the Falcon 1 vehicle and its two engine systems. Both stages of the rocket will consume a highly refined kerosene propellant and super-cold liquid oxygen.The first stage main engine, called Merlin, generates about 71,500 pounds of thrust at sea-level to boost the 70-foot tall, 5.5-foot diameter rocket off the ground. The motor fires for nearly three minutes before separating and parachuting into the ocean where an awaiting ship recovers the stage for reuse, a feature designed to hold down per-launch costs for Falcon's government and commercial customers.The upper stage's Kestrel engine, with its 7,500 pounds of thrust in vacuum, is capable of several re-ignitions during ascent. The Falcon booster stands vertical on its pad. Photo: SpaceXFalcon 1's lifting capacity puts the vehicle in a match-up with Orbital Sciences' rockets. Falcon 1 is designed to carry 950 pounds of payload into polar orbits, 1,280 pounds into the International Space Station's orbit and 1,480 pounds into a low-Earth orbit due east of Cape Canaveral.To substantially increase the amount of cargo SpaceX can launch, the company is developing the Falcon 5 that resembles a big brother of Falcon 1.Standing 100 feet tall and 12 feet in diameter, the Falcon 5 is a gradual evolution from the Falcon 1 design. But what distinguishes the booster is the cluster of five Merlin first stage engines. The powerplants will be feeding from the same kerosene and liquid oxygen tanks, which SpaceX says provides an "engine-out" capability. That means the first stage could suffer an engine failure -- and depending on when during ascent, as many of three lost engines -- and still complete the launch. Kevlar shielding wrapped around each engine is supposed to protect the good engines from one that is malfunctioning."In the case of SpaceX, we believe that our second generation vehicle in particular, the Falcon 5, will provide a factor of ten improvement in propulsion reliability. Falcon 5 will be the first U.S. launch vehicle since the Saturn 5 moon rocket that can complete its mission even if an engine fails in flight - like almost all commercial aircraft. In fact, Saturn 5, which had a flawless flight record, was able to complete its mission on two occasions only because it had engine-out redundancy," Musk told the Presidential Commission on the Moon-Mars Initiative last year. The Falcon rockets are built at the SpaceX factory in California. Photo: SpaceXOn the drawing board is the Merlin 2 engine that'll rev up to 100,000 pounds of thrust. But the initial version of Falcon 5 relies on the original Merlin of the Falcon 1 design.With the upgraded engine cluster producing a half-million pounds of thrust at launch, Falcon 5 will loft 10,530 pounds into polar orbit, 12,010 pounds to the station's altitude and 13,260 pounds to the low-Earth orbit from the Cape inclined 28 degrees north and south of the equator. What's more, the bigger booster will be capable of carrying 4,240 pounds into a geosynchronous transfer orbit, inclined 9 degrees, that is used by communications satellites destined for geostationary orbit 22,300 miles above the planet, and it can accelerate 2,650 pounds to escape velocity for planetary and deep space probes.The Falcon 5 upper stage will use another kerosene-fueled Merlin engine, a departure from earlier plans to fly two Kestrel engines on the rocket.Falcon missions begin with rocket construction in El Segundo. The completed rockets are strapped onto a special trailer and driven to the launch site. The payload is mated to the vehicle in the final days before liftoff while the rocket is still resting on the mobile transporter. As the countdown begins, the fully assembled booster is erected on the pad, fueled and readied for liftoff.The SpaceX design requires little infrastructure, with a large, portable tent covering the horizontal rocket at the launch site. The first Falcon rocket will be launched from Vandenberg Air Force Base, Calif., in March. Photo: SpaceXThree Falcon 1 rockets have been sold for launches this year. The first carries a U.S. military communications satellite from California's Vandenberg Air Force Base in March. That will be followed with another Defense Department mission from a Marshall Islands launch site being built in the Pacific. The later mission, also from the Marshall Islands, will loft a spacecraft for Malaysia. The first Falcon 5 on the manifest goes from Vandenberg in the second quarter of 2006 with a one-third scale test craft for Bigelow Aerospace's Earth-orbiting inflatable ."I think something has to be done about the cost of long-term access to space. My long term interest is actually in human transportation but I think it makes sense from sound business standpoint to start off with something small and where there is a clear market, which is satellite delivery, and down the road scale up the vehicle," Musk said in an earlier interview with Spaceflight Now.Musk acknowledged that developing the Falcon rocket from scratch has been difficult."I like challenging engineering problems and this is certainly quite challenging...Financially speaking, I'm a volunteer in this situation. I made enough money with PayPal and Zip2 that I don't really need to work. I guess it would have to be more interesting than living on a tropical island or something like that."For more on SpaceX and its plans at Cape Canaveral, see our separate .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.SpaceX to balance business realities, rocket innovation SPACEFLIGHT NOWPosted: June 6, 2014 Striving to be ready for an onslaught of launches under contract over the next few years, SpaceX plans to double the launcher production rate in its Southern California factory before the end of the year without compromising its commitments to develop a human-rated commercial spaceship, demonstrate rocket reusability, and further cut the cost of space transportation. A view of the Falcon 9 first stage's nine Merlin 1D engines. Credit: SpaceX"We need to meet our cadence of launch," said Gwynne Shotwell, president of SpaceX, at a discussion Wednesday at the Atlantic Council in Washington. "It's about one a month this year, and it's almost two a month next year."While SpaceX tries to manage a manifest packed with launches for NASA, commercial satellite operators, and perhaps soon the U.S. military, Shotwell said SpaceX chief executive Elon Musk is committed to keeping the company at the forefront of space transportation innovation."Elements in SpaceX clearly are focusing on operability and production," Shotwell said. "It's a transition that we're meeting the challenges of as we speak, but SpaceX will never be a company that is just operations and production focused. We'll always have a team of [research and development] engineers and technicians to ensure that we are constantly innovating. Elon's job is to make sure we are constantly innovating and pushing boundaries."In the next few years, SpaceX wants to develop a human-rated commercial spaceship and a reusable version of its Falcon 9 rocket. NASA is helping fund a crewed configuration of SpaceX's Dragon spacecraft, a project Musk estimates will cost about $1 billion, and SpaceX is using private capital to develop and demonstrate the Falcon 9 rocket's reusability.SpaceX has not disclosed how much the reusable rocket program will cost."We are focused on production and operability for part of the company, and the other part is the innovation piece, and we will continue that forever," Shotwell said.SpaceX had planned 10 or more Falcon 9 rocket launches this year, but delays caused by both internal technical issues and external forces have conspired to keep the commercial launchers from meeting the company's manifest.After a quick start to the year with the successful launch of the Thaicom 6 telecommunications satellite Jan. 6, SpaceX had to wait until April 18 for its second mission of the year, which faced delays as engineers completed upgrades to the company's Dragon cargo resupply capsule for the International Space Station.Engineers also discovered contamination in the Dragon's cargo bay, and then an electrical fire knocked a U.S. Air Force tracking radar offline at Cape Canaveral, triggering more delays.Throw in the difficulties of scheduling a mission to the International Space Station -- a process likened to air traffic control at an airport amid the comings and goings of international crew and cargo ships -- and SpaceX's resupply flights can only launch when the space station is ready to receive them.A helium leak in the Falcon 9 rocket's first stage liquid oxygen pressurization system was the culprit for SpaceX's most recent delay. Engineers discovered the anomaly on the launch pad on the eve of a planned liftoff with six Orbcomm data relay satellites, triggering a month-long launch slip."We had a helium leak," Musk said. "Helium is a pernicious little molecule, I've got to say."The Orbcomm mission is set for liftoff June 12 from Cape Canaveral in a 54-minute launch window opening at 9:07 p.m. EDT (0107 GMT on June 13). A view inside the SpaceX rocket factory in Hawthorne, Calif. Credit: SpaceXTwo communications satellites owned by AsiaSat of Hong Kong are next in SpaceX's launch queue. AsiaSat officials have said the spacecraft are complete and being stored at their Space Systems/Loral manufacturing plant in Palo Alto, Calif.The satellite processing clean room inside SpaceX's launch pad hangar at Cape Canaveral can only accommodate one payload at a time, so the shipment of the AsiaSat 8 satellite -- the next payload on SpaceX's manifest for launch this summer -- is on hold until the Orbcomm mission is launched."We have to execute on our manifest," Shotwell said. "I think the most recent criticism of SpaceX is can't we fly the missions that we say we're going to fly. I think we'll prove that [we can] over the coming months."SpaceX will not consider a public stock offering before achieving a predictable launch rate, Shotwell said."We have had delays as any development program does, but now we're starting to see where we're going to be waiting on our customers, which frankly is a relief to me," Shotwell said. "We're going to have to be good about predicting when we'll launch and what we'll launch before we change our [capitalization] strategy."Speaking to reporters via a conference call in April, Musk identified one manufacturing glitch, saying a primary constraint driving SpaceX's schedule "all boils down to this one particular part -- an injector casting.""We think we've resolved that particular issue, which should unlock quite a high rate of increased production," Musk said.SpaceX has 42 missions on its manifest at a value of $4.2 billion, according to Shotwell, who claimed the company captured "100 percent" of commercial Falcon 9-class launch business in 2011 and 2012. Many of the missions contracted in 2011 and 2012 are on SpaceX's launch schedule over the next 12 months.Shotwell said SpaceX will not hesitate to add new capabilities, upgraded components or other systems to its Falcon 9 rockets, as long as their customers are comfortable with it.SpaceX officials have said they will not use a Falcon 9 rocket as a reusability testbed unless the customer gives permission. Engineers are now trying to guide a Falcon 9 first stage to a precision ocean splashdown a few hundred miles downrange from the launch site, then recover the rocket for inspections.Some time soon -- Musk says as soon as next year -- SpaceX could be ready to fly a Falcon 9 rocket with a first stage with a flight already in its logbook."I believe we have to get out of this mindset that the best rocket and the best technology is the one that has stayed the same for decades," Shotwell said. "In no other industry is that the case. You can imagine the chip industry, Intel and Qualcomm, if their chips remained the same year after year. It would be a disaster. I do want to push the concept of innovating to make better, and we'll have to work through processes to make that OK."Just to be clear, customers can fly the certified configuration if that's what they want. I think we'll demonstrate that we can innovate and spin our design successfully. We've done it successfully to date ... We need to get our customers comfortable with the design process." SpaceX president Gwynne Shotwell. Credit: NASA/Jay WestcottBy the end of 2014, SpaceX will producing two rockets every month, Shotwell said. That is up from one per month at the current rate inside SpaceX's factory in Hawthorne, Calif."We're really screaming on production," Shotwell said.Each Falcon 9 rocket has 10 Merlin 1D engines, so building two rockets per month will demand SpaceX's engine shop produce at least 240 engines per year. The introduction of SpaceX's Falcon Heavy rocket, made of three Falcon 9 first stage cores with nine engines each, will make the propulsion team churn out even more engines.Each Falcon Heavy rocket flies with 28 Merlin engines on the first stage, strap-on boosters and the upper stage.The assembly line could get a reprieve if SpaceX can demonstrate the technical and economic feasibility of recovering and reusing the first stages of Falcon rockets."We anticipate probably 50 percent market capture as we build out the Falcon family of launch vehicles, if not more," Shotwell said.Follow Stephen Clark on Twitter: .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.SpaceX's mega-rocket to debut next year at pad 39A SPACEFLIGHT NOWPosted: April 15, 2014 SpaceX signed a 20-year lease Monday to operate and maintain one of Kennedy Space Center's historic launch pads, and the California-based company plans to debut the world's most powerful rocket at the facility next year. NASA Administrator Charlie Bolden, SpaceX president Gwynne Shotwell and Kennedy Space Center director Bob Cabana speak to reporters at launch pad 39A. Photo credit: NASA/Dan CasperThe agreement turns over control of Launch Complex 39A to the commercial space transportation firm, which plans to use the launch pad for the the initial flights of the Falcon Heavy, a mega-rocket featuring 27 first stage engines generating nearly 4 million pounds of thrust at liftoff.Pad 39A was the starting point for many historic Apollo and space shuttle missions, including the Apollo 11 moon landing in 1969 and the first and last shuttle launches in 1981 and 2011."We'll make great use of this pad, I promise," said Gwynne Shotwell, president of SpaceX, in remarks to the media moments after signing the lease. "We've had architects and our launch site engineering [team] working for many months on the sidelines. We will launch the Falcon Heavy from here first -- from this pad -- early next year."Shotwell said pad 39A would also host launches of astronauts aboard the crewed version of SpaceX's Dragon capsule, which is under development in a public-private partnership between the company and NASA.SpaceX is competing with Boeing Co. and Sierra Nevada Corp. to win another round of government funding to continue development of their human-rated spacecraft, culminating in crewed missions by 2017.Launch pad 39A becomes SpaceX's third launching base after an existing complex on Cape Canaveral Air Force Station a few miles to the south and a West Coast facility for flights into polar orbit at Vandenberg Air Force Base, Calif.SpaceX's Falcon 9 rockets have flown eight times -- seven launches from Cape Canaveral and one flight from Vandenberg.Without going into detail, Shotwell said SpaceX would make some modifications to pad 39A but leave historic elements of the complex, which has sat mostly untouched since the space shuttle Atlantis rocketed into orbit on July 8, 2011, to begin its last mission.The turnover of pad 39A marks another milestone in the space center's transformation following the retirement of the space shuttle. Lockheed Martin Corp. set up a factory for the Orion crew exploration vehicle inside KSC's Operations and Checkout Building, and Boeing plans to concentrate construction and processing of its CST-100 commercial crew capsule and the U.S. Air Force's unmanned X-37B space plane in two former space shuttle hangars. A view of the flame trench at launch pad 39A. Photo credit: NASA/Dan CasperSpaceX will operate and maintain pad 39A at its own expense, according to a NASA press release. NASA was spending about $1 million annually on upkeep for the launch pad.NASA officials see no need for pad 39A in its space exploration plans. Nearby Launch Complex 39B received a facelift over the last four years, which saw the demolition of its shuttle-era servicing towers, refurbishment of plumbing and propellant tanks, and modernization of its electrical and communications network.Pad 39B will be home to NASA's Space Launch System, a government-owned heavy-lift rocket that will launch astronaut crews on deep space expeditions. NASA plans its first destination to be an asteroid repositioned by a robotic spacecraft in a stable orbit near the moon.The first unmanned test launch of the SLS is scheduled before the end of 2017.Shotwell said SpaceX plans to build a new hangar near launch pad 39A to assemble rockets horizontally before transferring the launchers to the pad and lifting them atop a launch platform for liftoff.The Falcon Heavy is SpaceX's biggest booster. It is powered by three kerosene-fueled first stages and an upper stage derived from the Falcon 9 rocket.Each Falcon 9 first stage is powered by nine Merlin 1D engines. The Falcon Heavy, which uses a combined 28 engines, will be the most powerful space launcher in the world when it first flies in 2015.SpaceX says the Falcon Heavy can lift nearly 117,000 pounds, or 53 metric tons, into low Earth orbit and shoot 29,000 pounds of payload on a trajectory to Mars. When fueled for launch, the rocket will weigh more than 1,600 tons.The Falcon Heavy's inaugural flight was scheduled from Vandenberg Air Force Base, but the acquisition of launch pad 39A allows SpaceX to move the mission from California to Florida. Artist's concept of the Falcon Heavy. Photo credit: SpaceX"Until yesterday, we didn't actually have pad 39A," said Emily Shanklin, a SpaceX spokesperson, in an email response to questions. "Once the lease was signed, it became the option that made the most sense. Our first heavy missions are out of the Cape, and 39A will feature vertical integration as well, which is required by the military."The U.S. Air Force requires its most precious payloads to be attached to their rockets in a vertical orientation. SpaceX's current processing paradigm uses horizontal integration, where satellites are bolted to the launch vehicle inside a hangar, then the rocket rolls to the launch pad and is hoisted upright within hours of liftoff.SpaceX is seeking to break into the market to launch pricey Defense Department and intelligence missions. United Launch Alliance, a joint venture between Boeing and Lockheed Martin, currently launches all of the military's large satellites on Delta 4 and Atlas 5 rockets.The Air Force set aside 14 missions for competition between ULA and SpaceX -- and any other company wishing to bid -- over the next few years, but budget cuts and delays threaten to cut that number to fewer launches open for bidding.The military's insistence that its payloads be integrated with rockets vertically, an overlooked point in recent congressional hearings and debates on the future of the U.S. launch market, has forced SpaceX to rethink its concept of operations.Vertical integration requires the presence of a fixed or mobile tower at the launch pad, giving cranes and workers access to lift and attach satellites to the rocket.Launch pad 39A's fixed service structure, a holdover from the space shuttle era, would fit the requirement.NASA selected SpaceX to enter negotiations to use pad 39A in December after a protest from Blue Origin, a private rocket company owned by Amazon founder Jeff Bezos, challenging the fairness of the space agency's search for a tenant to assume control of the launch complex.Blue Origin claimed NASA expressed a preference for the future tenant of pad 39A to support a multi-user concept, in which several different rockets could utilize the facility. File photo of the launch of space shuttle Atlantis from pad 39A on the final shuttle mission. Photo credit: NASA/Tony Gray and Tom FarrarThe Government Accountability Office in December decided NASA had expressed no preference for either a multiple-user or an exclusive agreement for the launch pad. NASA announced its selection of SpaceX the day after the GAO rendered its decision.NASA officials say they will make launch pad 39B available to commercial users when it is not needed by the Space Launch System.The first two SLS flights are scheduled for 2017 and 2021 -- the first crewed launch -- so NASA officials say such a long gap will create an opportunity for other rockets to use launch pad 39B.The SLS will only stay at the launch pad for three-to-five days after rollout from KSC's massive Vehicle Assembly Building before liftoff, ensuring a minimal footprint and few scheduling conflicts for potential commercial users, officials said.Follow Stephen Clark on Twitter: .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.Spirit's last dispatches from Mars SPACEFLIGHT NOWPosted: June 5, 2011 Although NASA didn't give up on the Spirit rover until last month, scientists last heard from the robot explorer in March 2010, when it went silent at the onset of the cold and dark Martian winter.Assembled by and Marco Di Lorenzo from publicly-available NASA imagery, these mosaics show Spirit's final resting place in vivid color. A final single frame image from Spirit's panoramic camera was one of the final snapshots the rover sent back to Earth in March 2010.After blasting off from Earth in 2003, Spirit reached the Red Planet seven months later. Greatly surpassing its three-month mission goal, Spirit operated for more than six years before going into hibernation last year.Scientists hoped the rover would survive another Martian winter and continue returning data as a stationary research station. Officials blame its death on the rover being stuck in a stubborn sand trap, and the situation was exacerbated by two broken wheels.In the end, Spirit wasn't able to limp out of its predicament and spent the winter with its dusty solar panels pointed away from the sun as temperatures plummeted lower than the craft had ever experienced before.The images below are some of Spirit's final photographic contributions to the Martian science record. But researchers say the rover's data will continue being analyzed and will yield important insights for years to come.Spirit collected this mosaic in April 2009 as it approached a steep mound named "Von Braun" atop a modest plateau known as "Home Plate" on Sol 1869. Photo credit: Ken Kremer/Marco Di Lorenzo/NASA/JPL/CornellThis mosaic was assembled from imagery taken on Sol 2174 in February 2010. It shows Spirit's robot arm hovering over bits of light-colored Martian soil excavated as the rover spun its wheels in a fruitless attempt to pull itself out of a sand trap. Photo credit: Ken Kremer/Marco Di Lorenzo/NASA/JPL/CornellThis was Spirit's last panorama taken before the rover succumbed to its fourth winter on Mars. It shows the Columbia Hills as viewed from the rover's final resting place, a location dubbed "Troy" by scientists. Photo credit: Ken Kremer/Marco Di Lorenzo/NASA/JPL/CornellThis false color mosaic was assembled from frames taken by Spirit's microscopic imager under the rover's belly in June 2009. Photo credit: Ken Kremer/Marco Di Lorenzo/NASA/JPL/CornellIn one of its last images, Spirit's panoramic camera looked down to snap a black-and-white picture of the clumpy Martian soil and one of the rover's stuck wheels. Photo credit: NASA/JPL/CornellJohn 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.Spitzer in the crosshairs of budget-constrained NASA SPACEFLIGHT NOWPosted: May 19, 2014 Challenged by a lean budget withered by the development of the multibillion-dollar James Webb Space Telescope, NASA will likely have to shut down the infrared Spitzer telescope, one of the agency's famed Great Observatories, after an independent panel of scientists concluded there was not enough money to extend the mission. Artist's concept of the Spitzer Space Telescope. Credit: NASA/JPL-CaltechNASA's planet-hunting Kepler telescope, along with eight other operating missions, got better news. NASA approved funding for those projects, plus another two years of data analysis on observations by Europe's Planck cosmological probe, for at least two more years.The space agency's senior review, a biennial panel which recommends whether NASA should continue funding operating science missions, said Spitzer continues to produce quality science results but could not justify its relatively costly yearly budget."It is, of course, very disappointing when you are the one mission that is called out for termination, but we very much hope, on the other hand, that the positive science review that we got from the panel can be used by NASA to solve this problem," said George Helou, director of the Spitzer Science Center at the California Institute of Technology.The senior review board, which consisted of 10 scientists, called Spitzer's capabilities "unique and important," ranging from the characterization of planets around other stars to brown dwarfs, or failed stars, and galaxies in the early universe.But the mission's operating costs were higher than most of NASA's other astrophysics missions."The cost is particularly difficult in the context of an observatory with greatly reduced capabilities with respect to its prime mission," the panel wrote in its report to NASA. "The mission also did not present substantial plans to reduce operations costs with such reduced capabilities. Given the budget climate, the [senior review panel] cannot recommend funding of Spitzer at the levels requested."Should Spitzer be unable to produce valuable science results for less money, the board recommended NASA shut down the mission. NASA agreed with the recommendation.Paul Hertz, director of NASA's astrophysics division, said Friday that the Spitzer team can submit an amended proposal to NASA Headquarters with a further cut to the mission's operating budget, giving the space agency one more chance to see if it can afford to pay for curtailed observations with Spitzer.According to Helou, mission officials hope to send the updated proposal to NASA as soon as this week. But Helou cautioned any arbitrary budget cut to Spitzer would harm the science return which received high marks from the senior review."We understand that the situation is very tight, so we'll try and make it as responsive to the fiscal reality as possible," Helou said in an interview Friday. "But because it's an observatory that was designed as a Great Observatory and has capabilities matching that design, we cannot, say, operate at half the cost or a quarter of the cost. We have already reduced from the original cost of operations. We are down to a third of that cost and what we are proposing now was even less, but we'll work to see how much more we can trim."Without a budget boost from Congress or cost savings within the Spitzer project, money for the mission will run out Sept. 30 and NASA will decommission the telescope beginning this fall.Spitzer received $16.5 million to operate in fiscal year 2014, which ends Sept. 30. Helou said the initial proposal considered by NASA's senior review called for a reduced operating budget of $15.35 million in fiscal year 2015.Helou said the funding would have continued Spitzer's research into the atmospheres of exoplanets -- planets around other stars -- including measuring their temperatures, an aptitude not foreseen before Spitzer's launch in 2003.The Kepler mission, which won NASA's support in the senior review, detects planets around other stars. Spitzer's job is to follow up exoplanet discoveries, providing confirmation and finding details about their environment. Artist's concept of an exoplanet. Credit: NASA/JPL-Caltech"We are making great progress both in exoplanets and in the study of the very early universe, especially in the latter, where we're studying the galaxies formed in the first half billion years of the universe," Helou said.Spitzer's total cost, including its development, construction, launch and operations, comes to more than $1 billion.Spitzer's annual funding line is less than the 2014 operating budgets for the Hubble Space Telescope and the Chandra X-ray Observatory, NASA's other Great Observatories, which received $98 million and $55.3 million this year, according to Hertz.Other missions proposed to the senior review have annual operating budgets less than Spitzer's.Hubble and Chandra received four-year extensions, and seven other astrophysics funding lines were approved for two more years of operations. NASA is a junior partner on three of the missions with the European Space Agency and the Japan Aerospace Exploration Agency, but the senior review recommended continuing U.S. support for those projects.Projects getting extensions are the:Hubble Space TelescopeFermi Gamma-ray Space TelescopeChandra X-ray ObservatoryKepler Space TelescopeNuclear Spectroscopic Telescope Array, or NuSTARSwift Gamma-ray Burst ExplorerX-ray Multi-Mirror Mission-Newton, or XMM-Newton, an ESA missionPlanck, an ESA missionSuzaku/Astro E2, a Japanese missionThe Spitzer Space Telescope launched in August 2003 as the last of NASA's Great Observatories, a quartet of missions including the Hubble Space Telescope, the Chandra X-ray Observatory, and the Compton Gamma Ray Observatory, which was retired in 2000."Spitzer has given us a decade of excellent service," Hertz said.Spitzer launched with a supply of super-cold liquid helium to cool its most sensitive infrared detectors, which were designed to image some of the coldest reaches of the universe.Since 2009, Spitzer has only been able to use two of its shorter wavelength imaging bands after running out of cryogenic helium. Detectors in the near-infrared bands do not need to be chilled to do their work. This striking star formation region, mapped in infrared light by NASA's Spitzer Space Telescope, was recently spotted by one of Spitzer's Twitter followers searching through the GLIMPSE360 panorama of our Milky Way galaxy. Credit: NASA/JPL-CaltechHelou said the spacecraft is healthy despite its age. Spitzer was launched into an Earth-trailing orbit around the sun, and it is now located about 100 million miles from Earth, a distance that is gradually increasing. At some point in the next few years, even if the spacecraft is functioning fine, Spitzer would have to be shut down anyway because communications would become a problem when its orbit reaches the opposite side of the sun from Earth, officials said."The sensitivity in the channels that are still working is essentially the same that it was at launch, and in addition to that, because we now understand the spacecraft much better, we are able to make small improvements in the performance that translate directly into improved scientific capabilities -- that is the ability to measure the very faint signals which you need to do exoplanet research," Helou said.The senior review noted the high demand by astronomers for observing time on Spitzer."Researchers are asking for six times more hours of observing than we have to allocate," Helou said. "That's been the case for the last two years. There are 700 papers published every year that leverage Spitzer data."There's always disappointment when it's one's own kid that gets kicked to the curb," Helou said. "I sort of understand that the constraints were such that something had to be canceled, and it had to be something big ... I'm not saying they should have canceled something else. The real disappointment is this structural issue with the budget in astrophysics. At a time when there aren't a lot of new launches, they don't have the budget to continue operating a productive mission."Scientists participating in the senior review seemed to agree."American pre-eminence in the study of the Universe from space is threatened to the point of irreparable damage if additional funds cannot be found to fill the projected funding gaps," the review members wrote in their report."It's not only Spitzer, but you can look at several other mission that are getting insufficient support, or are not able to be supported at all, in the current condition," Helou said.NASA officials have acknowledged for several years the growth in the budget for the James Webb Space Telescope, the successor to Hubble set for launch in 2018, would likely force NASA to turn off astronomy missions prematurely.JWST received $658 million in the 2014 budget passed by Congress and signed by President Barack Obama. The rest of NASA's astrophysics mission, which covers all operating missions, data analysis, and development of smaller Explorer-class satellites, got $668 million.The White House and Congress have agreed JWST should be one of the top priorities for NASA, alongside the International Space Station and the construction of the heavy-lift Space Launch System mega-rocket for human expeditions beyond low Earth orbit.Helou said the termination of Spitzer this year will have a ripple effect on science with JWST once it comes online. Spitzer and JWST both observe the universe in infrared wavelengths largely invisible to telescopes on the ground."In terms of a true production capability, where you have an observatory that is very prolific in data, in particular for a pointing observatory like Spitzer, there is nothing else until we get JWST up there," Helou said. "One of the arguments we make scientifically for continuing Spitzer is to prepare for JWST, but also to make sure we have some capability that allows that part of the spectrum available for study, so when JWST comes around we have the best knowledge possible for that spectral range."NASA plans to release the results of a senior review looking at the agency's planetary missions in late June or early July, according to a NASA spokesperson.The budget situation in NASA's planetary division has raised fears some missions may be turned off.Follow Stephen Clark on Twitter: .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.Sporty sendoff planned for NASA's LADEE moon mission SPACEFLIGHT NOWPosted: April 8, 2014 NASA's LADEE space probe is in the final weeks of its $280 million lunar research mission as engineers put the diminutive spacecraft through a series of tricky maneuvers to test its limits and maximize its scientific return. Artist's concept of LADEE at the moon. Credit: NASA Ames/Dana Berry The Lunar Atmosphere and Dust Environment Explorer is now flying just a few miles above the moon's highest mountain ranges, collecting data and challenging ground controllers charged with keeping the spacecraft alive as long as possible.Running low on fuel, the mission is expected to end around April 21, when LADEE crashes into the far side of the moon. The violent ending will come less than 33 weeks since the probe launched in September, but it keeps with the mission's script.The mission was designed for a short lifetime, and its primary data-gathering phase lasted just 100 days and ended in March.Since arriving at the moon in early October, LADEE has "overachieved" its objectives, said Joan Salute, LADEE program executive at NASA Headquarters in Washington.LADEE's three science instruments scooped up dust particles, identified the chemical make-up of the moon's atmosphere, and looked for signs of hydrated compounds, such as water and hydroxyl (OH), migrating from the moon's middle latitudes toward polar cold traps in permanent shadow, where scientists say ice can sit undisturbed for billions of years.The unique spacecraft also hosts a laser communications terminal, which successfully accomplished the first laser linkup between the moon and Earth, demonstrating a new optical relay paradigm that could drastically boost data return from future deep space missions."It's always bittersweet," said Butler Hine, LADEE's project manager at NASA's Ames Research Center in California. "The mission was such a resounding success that everybody on the team is incredibly proud of the performance of the spacecraft and the team members."Officials will not know exactly when the end will come. The probe's trajectory is designed to impact somewhere on the far side of the moon around April 21."This represented six years of very hard work by a lot of people, so you're both very proud of the success and you're also a little melancholy that you won't be talking to the spacecraft again," Hine told reporters Thursday. "I think folks will actually miss talking to the spacecraft."Controllers last week fired LADEE's main engine to lower the spacecraft's altitude, putting it on a trajectory to skim as low as 1 or 2 miles over the moon's mountaintops.On Friday, engineers plan the mission's final engine burn to put LADEE on course to impact somewhere on the far side of the moon around April 21."That drops us to this relatively low spot that we can continue flying in for the rest of the mission until the planned impact," Hine said.A major test for LADEE will come April 15, when the Earth will move between the moon and the sun. The occurrence will create a spectacular lunar eclipse visible from Earth, but it will stress LADEE near its technological limits.LADEE was never designed to survive such an eclipse, when its solar panels will be starved of sunlight and the spacecraft must survive on stored battery power alone. LADEE will also get very cold during the four-hour eclipse, ac

By Women's Skirts and Dresses Sep 11, 2014

STORY WRITTEN FOR & USED WITH PERMISSIONPosted: July 1, 2004; Updated at 2:10 a.m. EDTNASA's $3.3 billion Cassini probe completed a seven-year, 2.2-billion mile voyage tonight, firing its main engine for a nerve-wracking 96 minutes to successfully brake into orbit around the ringed planet Saturn. Credit: ESAThroughout the all-or-nothing rocket firing, flight controllers at NASA's Jet Propulsion Laboratory in Pasadena, Calif., could only sit and wait, monitoring events that had already taken place 934 million miles away. At that distance, radio signals, moving at 186,000 miles per second, needed an hour and 24 minutes to complete a one-way trip between Saturn and Earth. As a result, Cassini's on-board computer was responsible for carrying out the most critical maneuver since launch Oct. 15, 1997, a maneuver that simply had to work or the mission would end in failure. To everyone's relief, Cassini's main engine fired up on time at 10:36 p.m. EDT and shut down at 12:12 a.m., putting the craft in its planned initial orbit around Saturn. "Flight, telecom," the Cassini communications officer called out. "The Doppler has flattened out." Translation: Cassini's engine had shut down and Cassini was in orbit. Flight controllers burst into cheers, sharing hugs and high fives as Cassini lived up to its reputation for near flawless operation. "It feels awfully good to be in orbit around the lord of the rings," said Charles Elachi, director of the Jet Propulsion Laboratory. "It's going to be a huge leap in our understanding of the Saturnian system." Ed Weiler, NASA's associate administrator for space science, described the rocket firing as 96 minutes of purgatory during a news briefing Wednesday. Halfway through the burn, "I started to think gee, here we are sitting on this little pale blue dot, third rock from the sun. We just landed on Mars twice. We flew by a comet and picked up some comet dust (with the Stardust mission) and all within six months, we're about to go into orbit around a planet a billion miles away. How do we get away with having so much fun? "This has just been an incredible ride," he said. "This wasn't NASA going into orbit around Saturn, it's the Earth going into orbit around Saturn because 17 countries made this happen. This is the way exploration should be done: by the Earth." David Southwood, director of science for the European Space Agency agreed Cassini is a "world mission." "But this evening I have to say, it's been the Americans' evening," he said. "This was America doing it right. ... There are Europeans involved in just about everything in the instrumentation, the science on Cassini and Huygens. It really is a mission where everybody is working together. "But this evening, you guys did it right," he said. "Thank you JPL, thank you USA, thank you NASA." Referring to ESA's Huygens probe, which will make a parachute descent into the atmosphere of Saturn's moon Titan in January, Southwood said the Saturn Orbit Insertion rocket firing would be a tough act to follow and "we have now to get it right, too." "You really showed us how it's done. It was a very professional show and frighteningly on the nail. We've got a lot to live up to. Thank you everybody. It's been a great eveing." The most sophisticated - and expensive - robotic spacecraft ever built, Cassini approached Saturn from below the plane of its rings. Using its high-gain antenna as a shield, the spacecraft sailed through the ring plane at 10:11 p.m., passing through a broad gap between Saturn's F and G rings. The region was thought to be empty of any debris larger than dust grains, but at Cassini's enormous approach velocity - more than 53,000 mph at that point - impacts posed a major concern. But right on schedule, after Cassini re-oriented itself for the Saturn Orbit Insertion rocket firing, ground stations in Australia and California picked up Cassini's radio carrier signal at 10:27 p.m. EDT, confirming the spacecraft had survived the ascending ring plane crossing. "One hurdle down, one to go," said Todd Barber, lead propulsion officer. "We're approaching two minutes before the SOI burn. The hopes and dreams of thousands of scientists and engineers are resting on the next few moments. So Godspeed, Cassini-Huygens. May we see you in orbit." And with that, the moment of truth was finally at hand. As timers counted down to the start of the Saturn Orbit Insertion rocket firing, engineers at JPL monitored computer screens showing a graphical representation of the carrier signal from Cassini. They were looking for a very precise, predicted change in the frequency of the signal due to the effects of the rocket firing, much like a siren changes pitch as a police car races past. And right on schedule, at 10:36 p.m., the signal changed exactly as predicted. On computer screens, a horizontal line representing the carrier frequency suddenly bent sharply downward, matching the slope predicted for a normal rocket firing. Flight controllers burst into applause, relieved to know Rocket Engine Assembly A had fired on time to begin slowing Cassini's ever-increasing velocity. Producing just 100 pounds of push against the enormous 54,000-mph velocity of the 9,970-pound Cassini, the main engine had to fire 96.4 minutes to produce the required deceleration and to ensure Saturn's gravity could capture the spacecraft and warp its trajectory into the planned orbit. Thirty minutes into the burn, at 11:06 p.m., Cassini moved behind Saturn's A ring as viewed from Earth, dimming the carrier signal for about 25 minutes. After fading in and out as it was blocked by ring debris, relatively clear reception was established at 10:31 p.m. when Cassini had a brief, clear view of Earth again through a gap in the rings known as the Cassini division. Six minutes later, exactly as predicted, communications dropped out again for 28 minutes or so as the spacecraft moved behind the thicker B ring. Still picking up speed from Saturn's gravitational attraction, Cassini reached periapsis, the closest it will ever be to Saturn - 12,400 miles from the cloud tops - at 12:03 a.m., just nine minutes before the end of the SOI burn. By that point, Saturn's gravity had boosted Cassini's velocity to a blistering 69,350 mph, four times faster than a space shuttle in Earth orbit and 32 times faster than the bullet from an assault rifle. Waiting for the carrier signal to reappear from behind the B ring, Barber provided an impromptu Saturn weather report, predicting temperatures of "minus 226 degrees Fahrenheit, winds of 1,100 miles per hour or so, pressure highly variable depending on where you are in the atmosphere. At the top of the atmosphere, better than the best vacuum on Earth. Down in the depths, millions of atmospheres of pressure. Chance of helium rain inside the interior: 100 percent. Hurricanes the size of the Earth." By the end of the SOI burn at 12:12 a.m., the velocity had dropped to around 68,000 mph as Cassini streaked away from the planet after close approach. While most reporters (including this writer) were not aware of it, navigators changed their prediction for the burn duration Wednesday, expecting 97 minutes instead of 96. Analysis of the carrier signal's frequency showed the rocket engine actually generated about 1 percent more thrust than expected. Cassini's flight computer compensated by shutting the engine down one minute early to achieve the planned deceleration of 1,400 mph. That translated into a 96-minute burn as originally expected. With the conclusion of the SOI rocket firing, Cassini was finally in its planned initial orbit around Saturn. Over the next four years, the spacecraft will study Saturn's windy atmosphere, its complex ring system, several of its icy moons and how the planet's magnetic field interacts with the space environment. In what promises to be one of the most exciting phases of the mission, a European-built probe called Huygens will be released from Cassini on Christmas Eve for a parachute descent into the thick nitrogen atmosphere of Saturn's moon, Titan, on Jan. 14. In all, Cassini is expected to complete 77 orbits of Saturn over the next four years, requiring 157 trajectory-nudging rocket firings. The gravity of Titan will be used for major course changes, with 45 planned flybys. Seven close flybys of smaller, icy moons also are planned. Safely in orbit, Cassini turned so that its high-gain antenna was aimed back toward Earth for a brief, 20-second burst of carrier signal at 12:30 a.m. That switch from the low-gain to the high-gain antenna confirmed the spacecraft was operating normally and had not suffered any "safing" events during the burn that could have shut down science operations during Saturn close approach. "We've got it!" Barber reported as yet another round of cheers and applause burst out. After sending the brief call home, Cassini turned away to begin a 75-minute sequence of ring observations. "I feel great!" said program manager Bob Mitchell. "It was kind of a nail biter throughout." One hour and 46 minutes after the end of the SOI burn, Cassini was expected to turn once again, orienting itself so the high-gain antenna could act as a shield during a descending ring plane crossing. Once safely through the ring plane, Cassini was expected to begin transmitting science and engineering data back to Earth. The first pictures were expected around 8:40 a.m. Thursday. On July 2, Cassini will make its first official flyby of Titan, passing the cloud-shrouded world at a distance of 205,000 miles. Larger than Pluto and Mercury, Titan's thick nitrogen atmosphere is thought to mirror Earth's shortly after the planet's formation. Based on approach photos, Cassini's cameras should be able to "see" the surface through specific spectral "windows." But just how well the cameras will be able to image the surface won't be known until after the Friday flyby. Data playback from the Titan flyby is expected to begin around 6:15 p.m. Friday. If all goes well, a minor trajectory correction maneuver is scheduled Saturday at 8:30 p.m. to fine tune the orbit with a predicted velocity change of just 11 mph. Starting July 6, Cassini will be out of contact while Saturn passes behind the sun as viewed from Earth, completing the initial phase of Cassini's orbital mission. In late August, a major rocket firing is planned to raise the low point of Cassini's orbit well beyond the rings and to set up the second Titan flyby Oct. 26. After another Titan flyby Dec. 13, the European Space Agency's Huygens probe will be released from Cassini on Christmas Eve for the three-week trip to Titan. Huygens will slam into Titan's atmosphere on Jan. 14 for a two-and-a-half-hour parachute descent to the surface. Data from Huygens, including panoramic pictures of its enigmatic surface, will be beamed back to Earth through Cassini's radio system. After that, Cassini will continue on its own, flying through a ballet of ever-changing orbits and beaming down up to four gigabytes of data per day.Additional coverage for subscribers:VIDEO:CASSINI BEGINS ENGINE FIRING TO ENTER ORBIT VIDEO:BURN ENDS SUCCESSFULLY TO PUT CASSINI IN ORBIT VIDEO:POST-ARRIVAL NEWS CONFERENCE VIDEO:WEDNESDAY'S 12 P.M. EDT CASSINI STATUS BRIEFING VIDEO:A LOOK AT INTERNATIONAL COOPERATION VIDEO:'RING-SIDE CHAT' ABOUT SPACE EXPLORATION VIDEO:AN OVERVIEW OF CASSINI'S RADIO SCIENCE VIDEO:TUESDAY'S CASSINI MISSION OVERVIEW BRIEFING VIDEO:CASSINI'S ARRIVAL AT SATURN EXPLAINED VIDEO:SCIENCE OBJECTIVES FOR CASSINI ORBITER VIDEO:HUYGENS LANDER SCIENCE OBJECTIVES Stargaze II DVDThe Stargaze II DVD has arrived! It features over 65 minutes of all new videos of the universe with newly-composed dolby digital and DTS 5.1 Channel surround sound music. Choose your store: - - - Solar system poster This new poster is popular for classrooms and children's bedrooms. It includes interesting facts and figures about the planets and their moons. Choose your store: - - - Apollo 15 DVD Relive on DVD the journey of Apollo 15, one of the great explorations of our time. This unique six-disc DVD set contains all the available television and 16mm film footage from the mission.Choose your store: - - - Shuttle patchesCollect the official mission patches for the first ten space shuttle flights and save off the regular price. Introducing the Space Shuttle Patch Collection.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Cassini to examine Saturn's mysterious 'black' moon NASA-AMES NEWS RELEASEPosted: June 9, 2004A NASA Ames planetary scientist is part of the science team that will study the data and images returned this week from the closest-ever flyby of Saturn's moon Phoebe.The spectral data and images obtained from the June 11 flyby will help scientists determine the icy moon's surface composition and properties. The Cassini spacecraft is closing in fast on its first target of observation in the Saturn system: the small, mysterious moon Phoebe, only 220 kilometers (137 miles) across. Left to right, the three views were captured between June 4 and June 7, from distances ranging from 2.6 million miles to 1.5 million miles. Credit: NASA/JPL/Space Science InstituteDownload larger image version "This is a unique opportunity," said Dr. Dale Cruikshank, co-investigator for the Cassini Visual and Infrared Mapping Spectrometer (VIMS), an instrument that will measure the chemical signatures of Phoebe's surface. "We've never had a close-up look at an irregular, low-reflective moon of any planet before, so we are prepared to be surprised," he said.Cruikshank will study the VIMS high-resolution spectral data to determine the distribution of recently observed water ice on Phoebe's surface. He also will use the data to determine the ability of Phoebe's surface to reflect light (known as its 'albedo') and the source of Phoebe's mysterious dark color. "This odd moon of Saturn has a little ice and a lot of black material on its surface, but beyond that, we know very little," Cruikshank noted.Phoebe's surface color appears almost black when observed by powerful telescopes, scientists say. The moon, which is about 130 miles in diameter, reflects only 6 percent of the sunlight it receives.Because of its dark color, and because Phoebe's orbit is irregular (elliptical, outside the plane of Saturn's equator and retrograde), scientists think the moon is probably a captured object, possibly a comet, asteroid or Kuiper Belt Object (KBO).KBOs are lumps of ice, rock and black material in the outer solar system that were never drawn together by gravity to form a planet. They are of great interest to scientists because they are believed to be primordial, which means they probably date back to the formation of the solar system some 4.6 billion years ago. About half of the comets that occasionally come near the Earth and sun are KBOs.One theory of Phoebe's mysterious dark color, which also is shared by the forward face of Iapatus, another nearby Saturn moon, is that it is due to the abundance of an organic material called tholin. Tholin is a sticky, waxy, dark red residue whose tiny particles cause the brownish haze of Saturn's largest moon, Titan.The tholin that may cover Phoebe is thought by Cruikshank and others to be abiotic, which means it is not made from living organisms. Scientists hypothesize the tholin is a natural by-product of the organic chemistry of the carbonaceous materials that make up Phoebe. Comet dust is an example of abiotic organic material.Since its discovery in 1898, Phoebe has been of interest to astronomers because it is so different from Saturn's other large moons. If Cassini finds that its surface is really made of carbonaceous organic material, scientists can use that information to learn about our solar system's formation and earlyhistory. Phoebe's surface material may even include amino acids, the building blocks of life.On June 11, the Cassini orbiter will fly within about 1,200 miles of Phoebe. Data and images will be returned on June 12.Cruikshank specializes in icy bodies in the outer solar system and the composition of small satellites, including all the satellites of Saturn.The principal investigator of the VIMS team is Dr. Robert H. Brown of the University of Arizona, Tucson, Ariz.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington. JPL designed, developed and assembled the Cassini orbiter. 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.Cassini's radar shows Titan's young active surface CASSINI MISSION RELEASEPosted: October 29, 2004The first radar images of Saturn's moon Titan show a very complex geological surface that may be relatively young. Previously, Titan's surface was hidden behind a veil of thick haze."Unveiling Titan is like reading a mystery novel," said Dr. Charles Elachi, director of NASA's Jet Propulsion Laboratory, Pasadena, Calif., and team leader for the radar instrument on Cassini. "Each time you flip the page you learn something new, but you don't know the whole story until you've read the whole book. The story of Titan is unfolding right before our eyes, and what we are seeing is intriguing." The Oct. 26 flyby marked the first time Cassini's imaging radar was used to observe Titan. The radar instrument works by bouncing radio signals off Titan's surface and timing their return. This is similar to timing the returning echo of your voice across a canyon to tell how wide the canyon is. Radio waves can penetrate the thick veil of haze surrounding Titan.Approximately 1 percent of Titan's surface was mapped during the Oct. 26 flyby. Radar images from Titan's northern hemisphere, a region that has not yet been imaged optically, show great detail and features down to 300 meters (984 feet) across. A wide variety of geologic terrain types can be seen. There are bright areas that correspond to rougher terrains and darker areas that are thought to be smoother."In the two days since this flyby, our understanding of Titan has grown tremendously," said Dr. Jonathan Lunine, Cassini interdisciplinary scientist, University of Arizona, Tucson. "Titan is a dynamic place with complex geologic processes that may be shaping its surface. Its surface may well be covered with organic materials, but we still don't know how much of the surface is liquid or solid. The fact that we have seen few craters tells us that Titan?s surface is young."The radar images show a world brimming with features that are dark and white, indicating sharp contrast. One area dubbed "Si-Si" or the "Halloween cat" because it is shaped like a cat's head is very dark and relatively smooth. That leads scientists to speculate that it might be a lake of some sort, but they caution that it is too soon to know for sure. "With the radar in its active mode, it is like shouting at Titan and listening for the echoes," said Dr. Ralph Lorenz, Cassini radar team member, University of Arizona, Tucson. "But we can also just listen with the sensitive radar receiver, the radiometry. The radiometry data shows early indications of the composition of the surface materials. One interpretation of what it is telling us is that Titan is a place covered with organics."The optical imaging cameras on Cassini show streaks on the surface. The streaking may be caused by movement of a material over the surface by wind, flowing hydrocarbon liquids, or a moving ice sheet like a glacier. Imaging scientists are also seeing multiple haze layers in Titan's atmosphere that extend some 500 kilometers (310 miles) above the surface. At the surface Titan's atmosphere is about four times denser than Earth's. With a remarkable flyby and complicated set of spacecraft gymnastics, Cassini will try its luck with Titan again on Dec. 13, 2004. The European Space Agency's Huygens probe will detach from Cassini on Christmas Eve and descend through Titan's dense atmosphere on Jan. 14, 2005."It's as if we were building a puzzle without the top of the box," said Lunine. "It will be necessary to piece together the clues provided by Cassini and Huygens over the next few years. Sometimes we'll be wrong and we'll need to take the pieces apart and reassemble them again until finally, a complete picture of the nature and evolution of Titan pops into view," said Lunine. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.Gemini 12Gemini 12: The NASA Mission Reports covers the voyage of James Lovell and Buzz Aldrin that capped the Gemini program's efforts to prove the technologies and techniques that would be needed for the Apollo Moon landings. Includes CD-ROM.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Cassini's rear-view image of Saturn's moon Titan released CASSINI PHOTO RELEASEPosted: July 27, 2004A day after entering orbit around Saturn, Cassini sped silently past Titan, imaging the moon's south polar region. This natural color image represents Cassini's view only about two hours after closest approach to the moon. Credit: NASA/JPL/Space Science InstituteDownload a larger version of image The superimposed coordinate system grid in the accompanying image at right illustrates the geographical regions of the moon that are illuminated and visible, as well as the orientation of Titan -- lines of longitude converge on the South Pole above the center of the image. The yellow curve marks the position of the boundary between day and night on Titan. Images taken through blue, green and red filters were combined to create this natural color view. The images were obtained using the Cassini spacecraft wide angle camera on July 2, 2004, from a distance of about 347,000 kilometers (216,000 miles) from Titan and at a Sun-Titan-spacecraft, or phase angle of 62 degrees. This view is an improvement in resolution of nearly a factor of four over the previously released natural color view of Titan (see PIA06081). The image scale is 21 kilometers (13 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Close-up views of Phoebe show moon's battered past NASA/JPL ANNOUNCEMENTPosted: June 12, 2004First images from the Cassini flyby of Phoebe reveal it to be a scarred, cratered outpost with a very old surface and a mysterious past, and a great deal of variation in surface brightness across its surface. Credit: NASA/JPL/Space Science InstituteDownload larger image version "What spectacular images," said Dr. Carolyn Porco, Cassini Imaging Team leader at the Space Science Institute in Boulder, Colo. "So sharp and clear and showing a great many geological features, large and small. It's obvious a lot of new insights into the origin of this strange body will come as a result of all this." "What we are seeing is very neat. Phoebe is a heavily cratered body. We might be seeing one of the chunks from the formation of the solar system, 4.5 billion years ago. It's too soon to say," said Dr. Torrence Johnson, Cassini imaging team member at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "It's important to see the big picture from all of the other instruments to get the global view on this tiny moon." Dr. Gerhard Neukum, an imaging team member from Freie University in Berlin, said, "It is very interesting and quite clear that a lot of craters smaller than a kilometer are visible. This means, besides the big-ones, lots of projectiles smaller than 100 meters (328 feet) have hit Phoebe." Whether these projectiles came from outside or within the Saturn system is debatable. There is a suspicion that Phoebe, the largest of Saturn's outer moons, might be parent to the other, much smaller retrograde outer moons that orbit Saturn. To see a movie of Phoebe's rotation, click .Dr. Joseph Burns, an imaging team member and professor at Cornell University, Ithaca, N.Y. said, "Looking at those big 50 kilometers (31 mile) craters, one has to wonder whether their impact ejecta might be the other tiny moons that orbit Saturn on paths much like Phoebe's." All planned 11 instruments operated as expected and all data was acquired. Scientists plan to use the data to create global maps of the cratered moon, and to determine Phoebe's composition, mass and density. It will take scientists several days to pour over the data to make more concrete conclusions. Cassini came within approximately 2,068 kilometers (about 1,285 miles) of the dark moon on Friday, June 11. The spacecraft was pointing its instruments at the moon during the flyby. Several hours later it turned to point its antenna to Earth. The signal was received through the Deep Space Network antennas in Madrid, Spain and Goldstone, in California's Mojave Desert, at 7:52 a.m. PDT today. Cassini was traveling at a relative speed of 20,900 kilometers per hour (13,000 miles per hour) relative to Saturn. It's been 23 years since a spacecraft last visited Phoebe. The Voyager 2 flyby in 1981 was at a distance from 2.2 million kilometers, (about 1.4 million miles), 1,000 times farther away. With the Phoebe accomplished, Cassini is on course for Saturn. A trajectory correction maneuver is scheduled for June 16. Cassini will conduct a critical 96-minute burn before going into orbit around Saturn on June 30 (July 1 Universal Time). During Cassini's planned four-year tour it will conduct 76 orbits around the Saturn system and execute 52 close encounters with seven of Saturn's 31 known moons. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo.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.Colorful threads and shadows of Saturn CASSINI NEWS RELEASEPosted: September 16, 2004 Saturn's faintly banded atmosphere is delicately colored and its threadbare rings cross their own shadows in this marvelous natural color view from Cassini. Credit: NASA/JPL/Space Science InstituteDownload larger image version The planet and its rings would nearly fill the space between Earth and the Moon. Yet, despite their great breadth, the rings are a few meters thick and in some places, very translucent. In this image, we can see through the C ring, which is closest to Saturn, and through the Cassini division, the 4,800-kilometer- (2,980-mile-) wide gap that arcs across the top of the image and separates the optically thick B ring from the A ring. The part of the atmosphere seen through the gap appears darker and more bluish due to scattering at blue wavelengths by the cloud-free upper atmosphere. The different colors in Saturn's atmosphere are due to particles whose composition is yet to be determined. The image was obtained with the Cassini spacecraft narrow angle camera at a distance of 7.6 million kilometers (4.7 million miles) from Saturn. Images taken with red, green and blue filters were combined to create this color view. The image scale is 46 kilometers (28 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Countdown to Phoebe PHOTO RELEASEPosted: June 11, 2004 Credit: NASA/JPL/Space Science InstituteDownload larger image version As Cassini sails toward its rendezvous with Phoebe, details on the small, dark moon are coming into view at a dizzying pace. The images shown here were taken 13 hours apart on Thursday, just one day prior to closest approach. There is a dramatic increase in detail between these two views. Phoebe completes one rotation about its spin axis in nine hours and 16 minutes. We are looking at opposite hemispheres in these two views. A large crater, roughly 50 kilometers (31 miles) across, is visible in the image on the left. The image on the right shows a body heavily pitted with craters of varying sizes, including very large ones, and displaying a substantial amount of variation in surface brightness. Features that appear to be cliffs may be the boundaries between large craters. Despite its exaggerated topography, Phoebe is more round than irregular in shape. Left to right, the two views were obtained at a phase, or Sun-Phoebe spacecraft angle, of 87 degrees, and from distances of 956,000 kilometers (594,000 miles) and 658,000 kilometers (409,000 miles), respectively. The image resolutions are 5.7 and 3.9 kilometers (3.5 to 2.4 miles) per pixel, respectively. To aid visibility, the images were magnified three times via linear interpolation; no contrast enhancement was performed. Phoebe is approximately 220 kilometers (137 miles) wide. On Phoebe, the spin axis points up and approximately 13 degrees to the left of the boundary between day and night. Cassini draws closer to its only flyby of this mysterious outer moon of Saturn. Closest approach to Phoebe will be at 4:56 p.m. EDT (2056 GMT) on June 11. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Crunch, squelch or splash on Saturn's moon Titan? PARTICLE PHYSICS AND ASTRONOMY RESEARCH COUNCIL RELEASEPosted: November 6, 2004The prospect of the Huygens probe landing on a hard, soft or liquid surface when it lands on Titan next January still remain following further analysis of data taken during the Cassini mother ship's closest encounter with Saturn's largest moon during its fly-by on October 26menting on the latest data results and implications for theHuygens probe Mark Leese of the Open University, Programme Manager forScience Surface Package [SSP] instruments that will unravel the mysteriesof Titan said: "It's interesting that all of the possible landingscenarios that we envisaged - a hard crunch onto ice, a softer squelchinto solid organics or a splash-down on a liquid hydrocarbon lake - stillseem to exist on Titan."Leese added, "A first look at the measurements of Titan's atmosphereduring the fly-by suggest that the "Atmosphere Model" we developed andused to design the Huygens probe is valid and all looks good for theprobe release on Christmas day and descent to the surface on 14thJanuary 2005."Further analysis of Titan's upper atmosphere, the thermosphere, hasrevealed a strange brew as Dr Ingo Mueller-Wodarg of Imperial CollegeLondon explained," Our instrument, the Ion Neutral Mass Spectrometer(INMS), made in-situ measurements of atmospheric gases in Titan's upperatmosphere and found a potent cocktail of nitrogen and methane, stirredup with signatures of hydrogen and other hydrocarbons. We are nowworking on a 'Weather Report' for the Huygens landing in January"menting on the surface characteristics of Titan Professor JohnZarnecki of the Open University, lead scientist for the Huygens SSPsaid: "The recent results from the fly-by have started to show us a verydiverse and complicated surface. Titan is geologically active but hasn'tyet given up all of its secrets. Combining the visible images withinfrared and RADAR data from this and future fly-bys should help toclarify the picture - but the arrival of the Huygens probe in Januarywill perhaps be the key to unlock these mysteries."Professor Carl Murray, of the Imaging Science System [ISS] team fromQueen Mary, University of London also commented on the surfacefeatures: "The images of the Huygens' landing site returned by the camerasshow a diverse range of features. We see bright and dark areas roughlyaligned in an east-west direction. These are similar to wind streaks seenon Mars and may indicate that material on Titan has been deposited bythe effects of wind blowing across the landscape. All indications suggestthat we are in for a real treat in January when the Huygens probe reachesTitan's surface and returns the first in situ data from this alien world."UK scientists and technologists are amongst an international teamcontinuing to analyse the latest data received from the NASA/ESA/ASICassini Huygens mission after the spacecraft made its close fly-by ofTitan last week. The data has provided a wealth of information aboutSaturn's largest moon, which will not only assist the European SpaceAgency's Huygens team in advance of the probe landing on Titan inJanuary 2005 but will also increase our understanding of the relationshipbetween Titan and its parent planet Saturn.Professor Michele Dougherty from Imperial College is lead scientist onthe Cassini Magnetometer, which is studying the interaction betweenthe plasma in Saturn's magnetosphere and the atmosphere and ionosphereof Titan. "We have been able to model the Magnetometer data very wellfrom the Titan flyby. There does not seem to be an internal magnetic fieldat Titan from the observations we obtained during this flyby, but we willhave a much better idea about this when we have a further flyby inDecember which is on a very similar trajectory. All we can say at thispoint is that if there is a magnetic field generated in the interior ofTitan, then it is very small."Dr Andrew Coates from University College London's Mullard SpaceScience Laboratory, a Co-Investigator on the Cassini ElectronSpectrometer team, said: "We received some remarkable new informationabout Titan's plasma environment within the context of Saturn'sfascinating magnetosphere. Unexpectedly, it looks like we can directly usefeatures of the electron results to understand what Titan's upperatmosphere is made of, supplementing the ion measurements from companionsensors on other instruments. Our electron results contain tell-talefingerprints of photoelectrons and Auger electrons which we will use forthis. Also, the total picture shows how important electrons, raining downon Titan's upper atmosphere, are in helping the feeble sunlight drive thecomplex chemistry in Titan's upper atmosphere."Nick Shave, Space Business Manager at UK IT company LogicaCMG said "Theamazing imagery and radar results recently received from Cassini ofTitan's surface is providing important early information and creatingreal excitement in the industrial community. UK industry's criticalcontributions to Cassini-Huygens via the LogicaCMG Huygens flightsoftware and other systems, such as the parachutes by Martin Baker, willenable even more spectacular science that could help unlock some of thesecrets of life on Earth."UK scientists are playing significant roles in the Cassini Huygensmission with involvement in 6 of the 12 instruments onboard the Cassiniorbiter and 2 of the 6 instruments on the Huygens probe. The UK has thelead role in the magnetometer instrument on Cassini (Imperial College)and the Surface Science Package on Huygens (Open University).UK industry had developed many of the key systems for the Huygensprobe, including the flight software (LogicaCMG) and parachutes (MartinBaker). These mission critical systems need to perform reliably in someof the most challenging and remote environments ever attempted by a manmade object.Titan BackgroundTitan is a highly complex world and is closer to a terrestrial planetthan a moon typical of the outer planetary systems. Titan was first seenby Dutch astronomer Christiaan Huygens (after which the ESA probe isnamed) in 1655.Not only is Titan the largest of Saturn's satellites, it is alsolarger than the planets Mercury and Pluto, and is the second largestsatellite in the solar system (Jupiter's Ganymede being larger). It isthe only satellite in the solar system with appreciable atmosphere,composed mostly of Nitrogen, but also contains aerosols and hydrocarbons,including methane and ethane. Titan's atmosphere was first confirmed in1944 when Gerard Kuiper confirmed the presence of gaseous methane withspectroscopy.Titan's peak surface temperature is about 95 K (-178 degrees C) andsurface pressure is 1.6 Earth atmospheres. At this temperature andpressure, many simple chemicals that are present in abundance (methane,ethane, water, ammonia) provide materials in solid, liquid and gaseousform which may interact to create exotic features on the surface.Precipitation, flowing liquids, lakes and eruptions are all possible.Titan orbits Saturn at a distance of just over 20 Saturn radii(1,222,000 km/759,000 miles) which is far enough to carry the moon inand out of Saturn's magnetosphere. Very little is known about Titan'sinterior structure, including whether it has its own magnetic field.Titan's surface has been difficult to study, as it is veiled by adense hydrocarbon haze that forms in the dense stratosphere as methaneis destroyed by sunlight. From the data collected so far, dark featurescan be seen crossing the equatorial region of Titan, with a large brightregion near longitude 90 degrees now named Xanadu, and possibly a largecrater in the northern hemisphere.The Cassini-Huygens mission is a cooperative project of NASA, theEuropean Space Agency and the Italian Space Agency. The Jet PropulsionLaboratory, a division of the California Institute of Technology inPasadena, manages the Cassini-Huygens mission for NASA's Science MissionDirectorate, Washington, D.C. The Cassini orbiter and its two onboardcameras were designed, developed and assembled at JPL.The Particle Physics and Astronomy Research Council (PPARC) is theUK's strategic science investment agency. It funds research,education and public understanding in four broad areas of science -particle physics, astronomy, cosmology and space science.PPARC is government funded and provides research grants andstudentships to scientists in British universities, gives researchersaccess to world-class facilities and funds the UK membership ofinternational bodies such as the European Organisation for NuclearResearch, CERN, the European Space Agency and the European SouthernObservatory. It also contributes money for the UK telescopes overseas onLa Palma, Hawaii, Australia and in Chile, the UK Astronomy TechnologyCentre at the Royal Observatory, Edinburgh and the MERLIN/VLBI NationalFacility.Cassini posterJust in time for the Cassini spacecraft's arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12x12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA's Mars Exploration Rover is now available from the Astronomy Now Store.An insider's view of how Apollo flight controllers operated and just what they faced when events were crucial. Choose your store: | | | | 2014 Spaceflight Now Inc.Encountering Iapetus CASSINI PHOTO RELEASEPosted: January 9, 2004On New Year's Eve 2004, Cassini flew past Saturn's intriguing moon Iapetus, capturing the four visible light images that were put together to form this global view. The scene is dominated by a dark, heavily-cratered region, called Cassini Regio, that covers nearly an entire hemisphere of Iapetus. Iapetus is 1,436 kilometers (892 miles) across. The view is centered on the moon's equator and on roughly 90 degrees west longitude -- a location that always faces the direction of Iapetus's orbital motion around Saturn. Credit: NASA/JPL/Space Science InstituteDownload larger image version Within Cassini Regio, and especially near the equator, dark deposits with a visual reflectivity of only about 4 percent coat nearly everything with remarkable uniformity. However, at latitudes of about 40 degrees, the surface transitions to a much brighter, icy terrain near the pole where the brightest icy materials have reflectivity over 60 percent. However, this region is not uniform: Close inspection reveals that the surface is stained by crudely north-south trending wispy streaks of darker material, typically a few kilometers wide and sometimes tens of kilometers long. An ancient, 400-kilometer wide (250 miles) impact basin appears just above the center of the disc. The basin is heavily overprinted by more recent, smaller impact craters. The basin rim is delineated by steep scarps that descend to the basin floor. Many of these scarps, as well as walls of nearby craters, appear bright, probably due to exposed outcrops of relatively clean ice. Particularly at mid-latitudes, the brightest scarp exposures appear to face away from the equator (i.e. toward the pole). Often, the opposite south-facing scarps are stained with the lower-brightness material. The most unique, and perhaps most remarkable feature discovered on Iapetus in Cassini images is a topographic ridge that coincides almost exactly with the geographic equator. The ridge is conspicuous in the picture as an approximately 20-kilometer wide (12 miles) band that extends from the western (left) side of the disc almost to the day/night boundary on the right. On the left horizon, the peak of the ridge reaches at least 13 kilometers (8 miles) above the surrounding terrain. Along the roughly 1,300 kilometer (800 mile) length over which it can be traced in this picture, it remains almost exactly parallel to the equator within a couple of degrees. The physical origin of the ridge has yet to be explained. It is not yet clear whether the ridge is a mountain belt that has folded upward, or an extensional crack in the surface through which material from inside Iapetus erupted onto the surface and accumulated locally, forming the ridge. The origin of Cassini Regio is a long-standing debate among scientists. One theory proposes that its dark material may have erupted onto Iapetus's icy surface from the interior. Another theory holds that the dark material represented accumulated debris ejected by impact events on dark, outer satellites of Saturn. Details of this Cassini image mosaic do not definitively rule out either of the theories. However, they do provide important new insights and constraints. The uniform appearance of the dark materials at the equator, the apparent thinning and spottiness of the dark materials at progressively higher latitudes and dark wispy streaks near the distal margin of Cassini Regio strongly suggest that dark material was emplaced as a coating. One of the important new results is that no clear evidence can be found that erupted fluids have resurfaced Cassini Regio. The high density of impact craters argues that the terrain underlying the dark coating is relatively ancient and has not been eradicated by its emplacement. Thus, Cassini Regio may have had its origin in plume-style eruptions in which dark particulate materials accumulated on the surface as fallout, perhaps in conjunction with the creation of the equatorial ridge. On the other hand, the dark deposits in Cassini Regio may be a surface coating consistent with, and perhaps more simply explained by, the fall of dark materials from outside. The view has been oriented so that the north pole is toward the top of the picture. Cassini acquired the images in this mosaic with its narrow angle camera on Dec. 31, 2004, at a distance of about 172,400 kilometers (107,124 miles) from Iapetus and at a Sun-Iapetus-spacecraft, or phase, angle of 50 degrees. The image scale is 1 kilometer (0.6 miles) per pixel. The image has been contrast enhanced to aid visibility of surface features. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.Eyes on Xanadu CASSINI PHOTO RELEASEPosted: October 25, 2004This image taken on Oct. 24, 2004, reveals Titan's bright "continent-sized" terrain known as Xanadu. It was acquired with the narrow angle camera on Cassini's imaging science subsystem through a spectral filter centered at 938 nanometers, a wavelength region at which Titan's surface can be most easily detected. The surface is seen at a higher contrast than in previously released imaging science subsystem images due to a lower phase angle (Sun-Titan-Cassini angle), which minimizes scattering by the haze. Credit: NASA/JPL/Space Science InstituteThe image shows details about 10 times smaller than those seen from Earth. Surface materials with different brightness properties (or albedos) rather than topographic shading are highlighted. The image has been calibrated and slightly enhanced for contrast. It will be further processed to reduce atmospheric blurring and to optimize mapping of surface features. The origin and geography of Xanadu remain mysteries at this range. Bright features near the south pole (bottom) are clouds. On Oct. 26, Cassini will acquire images of features in the central-left portion of this image from a position about 100 times closer. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. 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.First Huygens images show strange new world BY WILLIAM HARWOOD Women's Skirts and Dresses

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