Sunday, September 25, 2011

Huge UARS Satellite's Fall From Space Captivates Skywatchers, Sparks Hoaxes


Skywatchers around the world were hoping for some unique views overnight Friday (Sept. 23), as a NASA satellite plunged to Earth on its final scorching journey through the atmosphere.

The 6.5-ton Upper Atmosphere Research Satellite, or UARS, most likely pierced through Earth's atmospheric shield within 20 minutes of 12:16 a.m. EDT Saturday (0416 GMT), according to NASA officials. The agency is unable to confirm the precise time and location of the satellite's re-entry, but orbital debris scientists said that the satellite would have been flying over the vast Pacific Ocean at the time, well away from the North American coastline.

Throughout the night, rumors circulated that the defunct satellite crashed over Alberta, Canada, raining debris on the small town of Okotoks, which lies south of Calgary. Local authorities who were called to investigate later called the claims a hoax. [6 Biggest Spacecraft to Fall Uncontrolled From Space]

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Thursday, September 22, 2011

Landing of Dead NASA Satellite 'Too Early to Predict': NASA


A dead 6.5 ton NASA UARS satellite would make its re-entry into Earth's atmosphere on Friday, Sept. 23, bringing along a chance to watch a spectacular sky show. But NASA is still not sure where on Earth the satellite would land.

"It is still too early to predict the time and location of re-entry with any more certainty, but predictions will become more refined in the next 24 to 48 hours," National Aeronautics and Space Administration (NASA) said in a statement.

NASA added that the debris from the defunct satellite would not cause harm to humans.

NASA conducted a detailed re-entry risk assessment for UARS in 2002 and it showed that the debris from UARS is not harmful to human beings. Following are the excerpts of the study:

* Number of potentially hazardous objects expected to survive: 26

* Total mass of objects expected to survive: 532 kg

* Estimated human casualty risk (updated to 2011): About 1 in 3200

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Tuesday, September 20, 2011

Tonnes of satellite space junk to pelt earth on weekend


Look out for a six-tonne satellite plummeting from the sky this weekend.

NASA scientists are doing their best to predict exactly when and where it will fall.

For now, they believe the earliest it will hit is Friday (NZ time), while the latest is Sunday.

Scientists put the odds of it hitting someone at 1-in-3200.

Over the years, space debris has fallen into the ocean or empty spaces.

If you do come across what you think may be a satellite piece, NASA doesn't want you to pick it up.

Or sell it on eBay.

As US government-owned property, it should be returned to its rightful owner – by being reported to police.

The 20-year-old research satellite is expected to break into more than 100 pieces as it enters the atmosphere, most of it burning up, the New Zealand Herald reports.

Twenty-six of the heaviest metal parts are expected to reach Earth, the biggest chunk weighing about 136 kilograms. The debris could be scattered over an area about 800 kilometres long.

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Origin of Dinosaur-Killing Asteroid Remains a Mystery


PASADENA, Calif. -- Observations from NASA's Wide-field Infrared Survey Explorer (WISE) mission indicate the family of asteroids some believed was responsible for the demise of the dinosaurs is not likely the culprit, keeping open the case on one of Earth's greatest mysteries.

While scientists are confident a large asteroid crashed into Earth approximately 65 million years ago, leading to the extinction of dinosaurs and some other life forms on our planet, they do not know exactly where the asteroid came from or how it made its way to Earth. A 2007 study using visible-light data from ground-based telescopes first suggested the remnant of a huge asteroid, known as Baptistina, as a possible suspect.

According to that theory, Baptistina crashed into another asteroid in the main belt between Mars and Jupiter about 160 million years ago. The collision sent shattered pieces as big as mountains flying. One of those pieces was believed to have impacted Earth, causing the dinosaurs' extinction.

Since this scenario was first proposed, evidence developed that the so-called Baptistina family of asteroids was not the responsible party. With the new infrared observations from WISE, astronomers say Baptistina may finally be ruled out.

"As a result of the WISE science team's investigation, the demise of the dinosaurs remains in the cold case files," said Lindley Johnson, program executive for the Near Earth Object (NEO) Observation Program at NASA Headquarters in Washington. "The original calculations with visible light estimated the size and reflectivity of the Baptistina family members, leading to estimates of their age, but we now know those estimates were off. With infrared light, WISE was able to get a more accurate estimate, which throws the timing of the Baptistina theory into question."

WISE surveyed the entire celestial sky twice in infrared light from January 2010 to February 2011. The asteroid-hunting portion of the mission, called NEOWISE, used the data to catalogue more than 157,000 asteroids in the main belt and discovered more than 33,000 new ones.

Visible light reflects off an asteroid. Without knowing how reflective the surface of the asteroid is, it's hard to accurately establish size. Infrared observations allow a more accurate size estimate. They detect infrared light coming from the asteroid itself, which is related to the body's temperature and size. Once the size is known, the object's reflectivity can be re-calculated by combining infrared with visible-light data.

The NEOWISE team measured the reflectivity and the size of about 120,000 asteroids in the main belt, including 1,056 members of the Baptistina family. The scientists calculated the original parent Baptistina asteroid actually broke up closer to 80 million years ago, half as long as originally proposed.

This calculation was possible because the size and reflectivity of the asteroid family members indicate how much time would have been required to reach their current locations -- larger asteroids would not disperse in their orbits as fast as smaller ones. The results revealed a chunk of the original Baptistina asteroid needed to hit Earth in less time than previously believed, in just about 15 million years, to cause the extinction of the dinosaurs.

"This doesn't give the remnants from the collision very much time to move into a resonance spot, and get flung down to Earth 65 million years ago," said Amy Mainzer, a co-author of a new study appearing in the Astrophysical Journal and the principal investigator of NEOWISE at NASA's Jet Propulsion Laboratory (JPL) in Pasadena. Calif. "This process is thought to normally take many tens of millions of years." Resonances are areas in the main belt where gravity nudges from Jupiter and Saturn can act like a pinball machine to fling asteroids out of the main belt and into the region near Earth.

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Monday, September 19, 2011

NASA satellite expected to crash to Earth in days


The sky is not falling. A 12,500-pound NASA satellite the size of a school bus is, though.

It's the Upper Atmosphere Research Satellite, and it's tumbling in orbit and succumbing to Earth's gravity. It will crash to the surface Friday.

Or maybe Thursday. Or Saturday.

Out-of-control crashing satellites don't lend themselves to exact estimates even for the precision-minded folks at NASA. The uncertainty about the "when" makes the "where" all the trickier, because a small change in the timing of the re-entry translates into thousands of miles of difference in the crash site.

As of the moment, NASA says the 35-foot-long satellite will crash somewhere between 57 degrees north latitude and 57 degrees south latitude - a projected crash zone that covers most of the planet, and particularly the inhabited parts. In this hemisphere, that includes everyone living between northern Newfoundland and the frigid ocean beyond the last point of land in South America.

Polar bears and Antarctic scientists are safe.

It's the biggest piece of NASA space junk to fall to Earth in more than 30 years. It should create a light show. The satellite will partially burn up during re-entry, and, by NASA's calculation, break into about 100 pieces, creating fireballs that should be visible even in daytime.

An estimated 26 of those pieces will survive the re-entry burn and will spray themselves in a linear debris field 500 miles long. The largest chunk should weigh about 300 pounds.

As the Friday-ish crash gets closer, NASA will refine its estimate of timing and location, but the fudge factor will remain high.

"There are too many variations on solar activity which affect the atmosphere, the drag on the vehicle," said Nicholas Johnson, chief scientist for orbital debris at NASA.

The good news is that the satellite will probably splatter into the open ocean, because Earth is a water planet. And humans, for all their sprawl, occupy a very limited portion of its surface.

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Thursday, September 15, 2011

Satellite falls faster than forecast


NASA's Upper Atmosphere Research Satellite is now expected to fall to Earth sometime between Sept. 23 and 25, orbital experts reported today.

That's toward the early end of the original projections for UARS' fiery descent: Last week, when NASA announced that the long-defunct, six-ton satellite would crash, the time frame was given as late September to early October. That wide window of possibilities was due to the uncertainties over atmospheric conditions. Now the picture is becoming clearer, said Nicholas Johnson, head of NASA's Orbital Debris Program Office at Johnson Space Center in Texas.

"The sun has become very active since the beginning of this week, and it's accelerating the prediction," he told me.

Higher solar activity heats and expands the upper atmosphere, creating more drag for satellites in decaying orbits. The increased drag pulls down those satellites more quickly — and that's what's behind the earlier prediction.

NASA's UARS status page said the bus-sized satellite's orbit was 143 by 158 miles (230 by 255 kilometers) as of today, compared with 155 by 174 miles (250 by 280 kilometers) a week ago. Johnson said the status page would be updated again on Friday.

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Tuesday, September 13, 2011

Behind the Scenes of NASA’s Upcoming MMORPG


These days, nearly every game company is trying to get their fingers in the MMORPG (Massively Multiplayer Online Role Playing Game) pie. Given the past successes of games like Ultima Online and Everquest and the current success of games like EVE Online and World of Warcraft, it’s no surprise that companies want try to create the next “killer app” of the MMORPG market.

One such game company that will be launching a new game is the company partnered with NASA to develop a space-based MMORPG for the space agency. Having raised nearly $40,000 in pledged funding via kickstarter, the company aims to start beta testing their offering some time next year.

So what does this new MMORPG do differently that will attract and retain paying customers? What makes Astronaut: Moon, Mars and Beyond different from say, EVE Online, Star Trek Online, or Star Wars Galaxies?

When a game developer becomes associated with a “big-name” property, expectations from both fans and developers can be quite high. Despite securing a license to create a game based on the Stargate franchise, a game development company never released the game and eventually ended up in bankruptcy. Star Trek Online, despite being one of the most anticipated MMORPG franchises went through two developers and when finally released had less than stellar sales. Of course, many fans of MMORPG’s are all too familiar with the myriad issues that plagued Star Wars Galaxies.

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Tuesday, July 19, 2011

Twisted Tale of our Galaxy's Ring

New observations from the Herschel Space Observatory show a bizarre, twisted ring of dense gas at the center of our Milky Way galaxy. Only a few portions of the ring, which stretches across more than 600 light-years, were known before. Herschel's view reveals the entire ring for the first time, and a strange kink that has astronomers scratching their heads.

"We have looked at this region at the center of the Milky Way many times before in the infrared," said Alberto Noriega-Crespo of NASA's Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena. "But when we looked at the high-resolution images using Herschel’s sub-millimeter wavelengths, the presence of a ring is quite clear." Noriega-Crespo is co-author of a new paper on the ring published in a recent issue of Astrophysical Journal Letters.

The Herschel Space Observatory is a European Space Agency-led mission with important NASA contributions. It sees infrared and sub-millimeter light, which can readily penetrate through the dust hovering between the bustling center of our galaxy and us. Herschel's detectors are also suited to see the coldest stuff in our galaxy.

When astronomers turned the giant telescope to look at the center of our galaxy, it captured unprecedented views of its inner ring -- a dense tube of cold gas mixed with dust, where new stars are forming.

Astronomers were shocked by what they saw -- the ring, which is in the plane of our galaxy, looked more like an infinity symbol with two lobes pointing to the side. In fact, they later determined the ring was torqued in the middle, so it only appears to have two lobes. To picture the structure, imagine holding a stiff, elliptical band and twisting the ends in opposite directions, so that one side comes up a bit.

"This is what is so exciting about launching a new space telescope like Herschel," said Sergio Molinari of the Institute of Space Physics in Rome, Italy, lead author of the new paper. "We have a new and exciting mystery on our hands, right at the center of our own galaxy."

Observations with the ground-based Nobeyama Radio Observatory in Japan complemented the Herschel results by determining the velocity of the denser gas in the ring. The radio results demonstrate that the ring is moving together as a unit, at the same speed relative to the rest of the galaxy.

The ring lies at the center of our Milky Way's bar -- a bar-shaped region of stars at the center of its spidery spiral arms. This bar is actually inside an even larger ring. Other galaxies have similar bars and rings. A classic example of a ring inside a bar is in the galaxy NGC 1097, imaged here by NASA's Spitzer Space Telescope. The ring glows brightly in the center of the galaxy's large bar structure. It is not known if that ring has a kink or not.

The details of how bars and rings form in spiral galaxies are not well understood, but computer simulations demonstrate how gravitational interactions can produce the structures. Some theories hold that bars arise out of gravitational interactions between galaxies. For example, the bar at the center of our Milky Way might have been influenced by our largest neighbor galaxy, Andromeda.

The twist in the ring is not the only mystery to come out of the new Herschel observations. Astronomers say that the center of the torqued portion of the ring is not where the center of the galaxy is thought to be, but slightly offset. The center of our galaxy is considered to be around "Sagittarius A*," where a massive black hole lies. According to Noriega-Crespo, it's not clear why the center of the ring doesn't match up with the assumed center of our galaxy. "There's still so much about our galaxy to discover," he said.

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Wednesday, July 13, 2011

Gas Giant Spacecraft All Gassed Up

Juno Mission Status Update

The Juno spacecraft completed hydrazine fuel loading, oxidizer loading and final tank pressurizations this week, and now the complete propulsion system is ready for the trip to Jupiter. The spacecraft is currently at the Astrotech processing facility in Titusville, Fla.

Hydrazine is the fuel of choice for most spacecraft because of its stored energy. When the fuel is mixed with the oxidizer, the liquid ignites in the propulsion system's main engine to perform the spacecraft's four large maneuvers. One of these maneuvers includes inserting the spacecraft into orbit around Jupiter in 2016.

With the fueling completion, the spacecraft is 99 percent ready for launch. Once the final thermal blanket closeouts and wet spin tests are complete, the spacecraft will be 100 percent ready for installation onto the Atlas 551 launch vehicle.

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Juno mission for the principal investigator, Scott Bolton, of Southwest Research Institute in San Antonio. The Juno mission is part of the New Frontiers Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems, Denver, built the spacecraft. Launch management for the mission is the responsibility of NASA's Launch Services Program at the Kennedy Space Center in Florida. JPL is a division of the California Institute of Technology in Pasadena.

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Monday, June 27, 2011

SpaceShipTwo a rocket plane designed to take tourists on suborbital flights

SpaceShipTwo, a privately built rocket plane designed to take tourists on suborbital flights, continues to chalk up more flight time as it glides through the skies over the Mojave Air and Space Port in California.

Another successful glide of the first SpaceShip Two craft, christened VSS Enterprise, took place June 23, marking the 14th glide flight test of the vessel — an 8-minute, 55-second free fall after midair release from its mothership. The test came a week after VSS Enterprise proved it could be flown on back-to-back days.

The two-pilot SpaceShipTwo is designed to rocket six paying passengers on a suborbital trajectory to space without making a full orbit around the Earth. The ride to the edge of space will come at a per-seat price of $200,000.

Friday, June 24, 2011

UrtheCast Announces New Space Venture


Joint Canadian, Russian and UK Space Venture to Install World's First Ever High Definition Streaming Video Cameras on the International Space Station





UrtheCast is building, launching, and operating the world's first and only high definition streaming video cameras being installed on the International Space Station (ISS).


UrtheCast will supply video data and imagery of Earth collected by two HD cameras on the Russian module of the Space Station. This data and imagery will be down-linked to ground stations around the planet and then displayed in real time on the Internet and distributed directly to UrtheCast's exclusive partners and customers.

The UrtheCast web platform will allow Users to constantly track the location of the Space Station, anticipating when it will pass over a particular geographic location. Users will be able to search for videos of a particular location, type, or theme and will have the ability to interact with the HD video feed from the UrtheCast servers. They will be able to zoom in and out, virtually steer the camera from side to side, rewind, and fast forward as they check out areas and things of interest on Earth. UK based Rutherford Appleton Labs is building two high definition cameras. A medium resolution camera will provide a three colour image with a swath of 45 kilometers and a resolution of 5.5 meters. The high-resolution camera will offer a video image with a frame rate of 3.25 frames per second with a resolution that is comparable to much of Google Earth. This will allow Users to see man-made objects and groups of people.

As a result of all this unique functionality, the UrtheCast web platform will spark a great deal of awareness, creativity, and unique user events from around the world. The UrtheCast website will feel like a blend of Google Earth with the video playback and search functionality of YouTube. The UrtheCast web platform will combine a consumer centric website, mobile application for smart phones, and an open Application Program Interface (API). The API enables third party developers to create their own applications and upload them to the UrtheCast web platform.

"Users will be able to view Earth from space. It will operate seamlessly with social media sites like Facebook and Twitter," explains Scott Larson, President of UrtheCast. ISS is a low orbit, human-inhabited satellite. The station travels at 26,000 km/h, orbiting Earth sixteen times per day, at an altitude of approximately 350 km. The ISS is a collaborative project between the Russian, Canadian European, Japanese, and US space agencies. UrtheCast has signed an exclusive agreement with RSC Energia, who maintains operational control of the Russian segment on the ISS. RSC Energia will take UrtheCast's cameras, install them on the outside of the ISS, and provide the necessary maintenance and transfer of the data. The cameras are being built by UK based Rutherford Appleton Laboratories (RAL), who is a world leader in building cameras for aerospace and satellite purposes.

"Being part of a project that not only taps into the recent renewed interest in space, but also provides a connection between people and the rest of the world is what is most intriguing about this project," Richard Holdaway Director, RAL Space.

UrtheCast will officially launch this project in Calgary on June 28th at 12:00pm. Dr. Dave Williams, one of NASA's most accomplished astronauts, will be speaking at the launch at the Calgary Chamber of Commerce.

"The UrtheCast camera will support the ISS and continue to inspire youth to pursue advanced studies in space sciences and spark interest in science, technology, engineering and the environment," says Dr.Williams.

Dr. Williams blasted into space aboard the Space Shuttle Columbia, and again on Shuttle Endeavour where he walked out into the great beyond. He has set records in space walking and has logged more than 687 hours in space. He will be speaking about space flight, space exploration, space science and technology, environmental stewardship and educational awareness as it relates to seeing the Earth from Space. "This unprecedented UrtheCast initiative is helping position Canada as a leading space-faring nation and driving science and innovation while actively inspiring young people across our country to take their place as members of Canada's next space generation," stated Dr. Williams.

Tuesday, June 07, 2011

Having a Solar Blast



The Sun unleashed an M-2 (medium-sized) solar flare, an S1-class (minor) radiation storm and a spectacular coronal mass ejection (CME) on June 7, 2011 from sunspot complex 1226-1227. The large cloud of particles mushroomed up and fell back down looking as if it covered an area of almost half the solar surface.

The Solar Dynamics Observatory (SDO) observed the flare's peak at 1:41a.m. ET (0641 UT). SDO recorded these images (above) in extreme ultraviolet light that show a very large eruption of cool gas. It is somewhat unique because at many places in the eruption there seems to be even cooler material -- at temperatures less than 80,000 K. All of the solar Heliophysics System Observatory missions captured the event.

When viewed in Solar and Heliospheric Observatory's (SOHO) coronagraphs (top right), the event shows bright plasma and high-energy particles roaring from the Sun.

Also to the right are links to the Solar Terrestrial Relations Observatory (STEREO) Ahead and Behind coronograph videos showing the CME expansion as viewed from each side of the sun. The STEREO Ahead satellite precedes the Earth as it circles the Sun. The STEREO Behind satellite follows behind the Earth in it's orbit of the Sun.

This not-squarely Earth-directed CME is moving at 1400 km/s according to NASA models. The CME should deliver a glancing blow to Earth's magnetic field during the late hours of June 8th or June 9th. High-latitude sky watchers should be alert for auroras when the CME arrives.

Sunday, June 05, 2011

NASA Satellite Data Reveals Joplin Tornado Track

joplin-tornado
The image shows the Advanced Spaceborne Thermal Emission and Reflection Radiometer, or ASTER, satellite data acquired on May 30, 2011, showing the damage track resulting from for the EF-5 tornado associated with the May 22, 2011, Joplin, Mo. storm. The complex pattern of ASTER data indicate variability in land use characterized by colors in this three-channel composite. Vegetated areas are shown in red and green, urban areas are aqua and the damage track from the tornado is also aqua. Clouds are white and cloud shadows are dark in color. The ASTER data here shows the tornado damage scar, aqua in color, left by the violent tornado as damage disrupts other, more typical land use patterns. The variation in width is likely correlated to tornado intensity. The tornado abruptly moved in a more southeasterly direction to the east of the city as is somewhat apparent through the clouds in the ASTER imagery.

This image was created by the NASA Short-term Prediction Research and Transition, or SPoRT, Center at Marshall Space Flight Center in Huntsville, Ala., using ASTER data provided courtesy of NASA's Goddard Space Flight Center in Greenbelt, Md.; the United States Geological Survey Land Processes Distributed Active Archive Center in Sioux Falls, S.D.; Japan’s Earth Remote Sensing Data Analysis Center in Tokyo, Japan; the Ministry of Economy, Trade and Industry, along with the Japan Research Observation System Organization. Final ASTER imagery was produced using resources of the Nebula Cloud Computing Platform, tiled, and displayed within Google Earth. Storm survey information was provided by the National Weather Service Forecast Office in Springfield, Mo.

Thursday, June 02, 2011

Last Female Shuttle Astronaut Available For Interviews

NASA astronaut Sandra Magnus, who will fly on the last space shuttle mission next month, is available for live satellite interviews from 7 to 9 a.m. CDT on Monday, June 6. Shuttle Atlantis is targeted to launch July 8 with Magnus, Commander Chris Ferguson, Pilot Doug Hurley and Mission Specialist Rex Walheim to deliver supplies and spare equipment to the International Space Station.After her first spaceflight in 2002, Magnus became the 34th out of 47 woman to fly aboard the shuttle, which launched the first American woman into space, Sally Ride, in 1983. With the upcoming STS-135 launch, Magnus will be the last female astronaut to fly on the storied vehicle.

Magnus is a native of Belleville, Ill. She earned a bachelor's and a master's from the University of Missouri-Rolla and a doctorate from the Georgia Institute of Technology.She is a veteran of two shuttle flights and a 4.5-month stay aboard the station as a member of the Expedition 18 crew. Her first spaceflight was aboard shuttle Atlantis on the STS-112 mission in October 2002. She later flew to the station aboard shuttle Endeavour on STS-126 in November 2008 and returned to Earth aboard shuttle Discovery on STS-119 in March 2009.

To arrange an interview, news media representatives must contact Karen Svetaka at 281-483-8684, no later than 4 p.m. on Friday, June 3. Participating media must tune into NASA Television's Live Interview Media Outlet channel. The channel is a digital satellite C-band downlink by uplink provider Americom.It is on satellite AMC 3, transponder 9C, located at 87 degrees west, downlink frequency 3865.5 MHz based on a standard C-band, horizontal downlink polarity. FEC is 3/4, data rate is 6.0 Mbps, symbol rate is 4.3404 Msps, transmission DVB-S, 4:2:0. NASA TV will air the Magnus interviews live. Video b-roll of STS-135 flight preparations will air June 6 at 6:30 a.m

Tuesday, May 31, 2011

Space Shuttle Endeavour Returns to Earth for Final Time Wednesday

Space shuttle Endeavour is scheduled to return to Earth for the final time on Wednesday, June 1, completing a 16-day mission to outfit the International Space Station. If Endeavour lands Wednesday, it will have spent 299 days in space and traveled more than 122.8 million miles during its 25 flights. It launched on its first mission on May 7, 1992.Wednesday's landing opportunities at NASA's Kennedy Space Center in Florida are at 2:35 a.m. and 4:11 a.m. EDT. Endeavour's entry flight control team led by Tony Ceccacci will evaluate weather conditions at Kennedy before permitting Endeavour to land.
If the shuttle is unable to return Wednesday, additional opportunities are available on Thursday at Kennedy and at backup landing site Edwards Air Force Base in California. For recorded updates about landing, call 321-867-2525.Approximately two hours after Endeavour lands, NASA officials will hold a briefing to discuss the mission. The participants will be:

Endeavour
  • Bill Gerstenmaier, associate administrator for Space Operations

  • Mike Moses, space shuttle launch integration manager

  • Mike Leinbach, space shuttle launch director

After touchdown, the astronauts will undergo routine physical examinations and meet with their families. The crew is expected to participate in a post-landing news conference about six hours after landing. Availability is subject to change due to real time circumstances. The news events will be broadcast live on NASA Television and the agency's website.

The Kennedy Press Site will be open for shuttle Atlantis’ rollout to Launch Pad 39A scheduled for 8 p.m. Tuesday and will remain open until 4:30 p.m. Wednesday.News media representatives who have been approved for STS-134 mission badges but have not picked them up yet may do so at NASA's Pass and Identification Building on State Road 3 on May 31 from 4 - 6 p.m. and 10:30 p.m. to 12:30 a.m. on June 1.The last bus will depart from the news center for the Shuttle Landing Facility one hour before landing.If the shuttle landing is diverted to Edwards after Wednesday, reporters should call the public affairs office at NASA's Dryden Flight Research Center at 661-276-3449. Dryden has limited facilities available for previously accredited journalists.

Friday, May 27, 2011

Spitzer Sees Crystal Rain in Infant Star Outer Clouds

olivine
Tiny crystals of a green mineral called olivine are falling down like rain on a burgeoning star, according to observations from NASA's Spitzer Space Telescope. This is the first time such crystals have been observed in the dusty clouds of gas that collapse around forming stars. Astronomers are still debating how the crystals got there, but the most likely culprits are jets of gas blasting away from the embryonic star.

You need temperatures as hot as lava to make these crystals, said Tom Megeath of the University of Toledo in Ohio. He is the principal investigator of the research and the second author of a new study appearing in Astrophysical Journal Letters. "We propose that the crystals were cooked up near the surface of the forming star, and then carried up into the surrounding cloud where temperatures are much colder, and ultimately fell down again like glitter."

Spitzer's infrared detectors spotted the crystal rain around a distant, sun-like embryonic star, or protostar, referred to as HOPS-68, in the constellation Orion. The Spitzer observations were made before it used up its liquid coolant in May 2009 and began its warm mission.

Wednesday, May 25, 2011

Endeavour's Late Inspection Complete

space shuttle
Space shuttle Endeavour's crew completed today's inspection of the shuttle's thermal protection system at 2:16 a.m. EDT. The crew began the inspection early. They used the 50-foot-long Orbiter Boom Sensor System to conduct a high fidelity, three-dimensional scan of areas of the shuttle that experience the highest heating during entry - the wing leading edges and nose cap. Managers and engineers in Mission Control will review the data to validate the heat shield's integrity and assure it has suffered no significant micrometeoroid and orbital debris damage.

The late inspection occurred earlier in the mission than normal, prior to undocking. As a consequence, the risk of re-entering with undetected micrometeoroid debris is increased but deemed acceptable.

During the mission's fourth and final spacewalk on Friday, the boom will be left at the space station to extend the robotic reach. Mike Fincke and Greg Chamitoff will prepare it for its stay by replacing its grapple fixture with a power data grapple fixture to enable its use as the new International Space Station Boom Assembly. Once on station without power and in the extended exposure to the vacuum of space, the boom's imagery sensors will cease functioning.

Monday, May 23, 2011

Asteroid Research Begins Under the Sea

view high resolution

NASA is using a capability-driven approach to new concepts of human exploration for multiple destinations in our solar system; one of those destinations are near-Earth asteroids. Across the agency, experts are being called into action to develop solutions to this new challenge. In particular, the NEEMO 15 analog field test, slated for mid-October this year, will test new tools, techniques, time lining approaches and communication technologies which could be useful when humans approach asteroids in space.

During the week of May 9-15, 2011, the NEEMO 15 support team is conducting engineering evaluations in the Aquarius undersea research laboratory in Key Largo, Fla. The purpose of these engineering tests is to understand the equipment, techniques and test concepts that will be implemented in the October NEEMO 15 mission, to make sure that all systems are ready for more rigorous testing when the crew will be living full-time in the Aquarius undersea habitat.

The specific operations for visiting an asteroid have not been considered in great detail before. Gravity on an asteroid is negligible, so walking around on one isn't really an option. Anchoring to the surface will probably be necessary, but asteroids are made up of different materials - some solid metal, some piles of rubble and some, a combination of rock, pebbles and dust. Weak gravity and diverse materials present problems whose solutions can be experimented with on the ocean floor, which is what the NEEMO 15 mission is trying to do.

NEEMO 15 will focus on three different aspects of a mission to an asteroid surface. The first is anchoring to the surface of the asteroid. Unlike the moon or Mars, an asteroid would have little, if any, gravity to hold astronauts or vehicles to its surface, so an anchor would be necessary. To move around on the surface of an asteroid will require a method of connecting multiple anchors to form pathways. The best way in which to connect these anchors will be the second aspect of a near-Earth asteroid mission addressed by NEEMO 15. Finally, since NASA's purpose in visiting an asteroid would be for scientific research, the third aspect of this mission investigated by NEEMO 15 would be different methods of sample collection.

Friday, May 20, 2011

NASA'S Mars Atmosphere Mission

maven

NASA's mission to investigate the mystery of how Mars lost much of its atmosphere passed a critical milestone on October 4, 2010. NASA has given approval for the development and 2013 launch of the Mars Atmosphere and Volatile Evolution (MAVEN) mission. Clues on the Martian surface, such as features resembling dry riverbeds and minerals that only form in the presence of liquid water, suggest that Mars once had a denser atmosphere, which supported the presence of liquid water on the surface. As part of a dramatic climate change, most of the Martian atmosphere was lost. MAVEN will make definitive scientific measurements of present-day atmospheric loss that will offer insight into the Red Planet's history. This project is a vital complement to past, present, and future Mars missions. MAVEN will take us a step closer in learning about the evolution of our intriguing celestial neighbor.”

NASA Goddard will manage the project, which will cost $438 million excluding the separately government-furnished launch vehicle and telecommunications relay package. Goddard will also build some of the instruments for the mission. In addition to the PI coming from CU-LASP, the university will provide science operations, build instruments, and lead Education/Public Outreach. Lockheed Martin of Littleton, Colo., will build the spacecraft based on designs from NASA's Mars Reconnaissance Orbiter and 2001 Mars Odyssey missions and perform mission operations. The University of California-Berkeley Space Sciences Laboratory will also build instruments for the mission. NASA’s Jet Propulsion Laboratory, Pasadena, Calif., will provide navigation support, the Deep Space Network, and the Electra telecommunications relay hardware and operations.

Thursday, May 19, 2011

NASA's Next Mars Rover Nears Completion

NASA's Mars Rover

Assembly and testing of NASA's Mars Science Laboratory spacecraft is far enough along that the mission's rover, Curiosity, looks very much as it will when it is investigating Mars.

Testing continues this month at NASA's Jet Propulsion Laboratory, Pasadena, Calif., on the rover and other components of the spacecraft that will deliver Curiosity to Mars. In May and June, the spacecraft will be shipped to NASA Kennedy Space Center, Fla., where preparations will continue for launch in the period between Nov. 25 and Dec. 18, 2011.

The mission will use Curiosity to study one of the most intriguing places on Mars -- still to be selected from among four finalist landing-site candidates. It will study whether a selected area of Mars has offered environmental conditions favorable for microbial life and for preserving evidence about whether Martian life has existed.

Wednesday, May 18, 2011

Nasa future mission Juno




Juno’s principal goal is to understand the origin and evolution of Jupiter. Underneath its dense cloud cover, Jupiter safeguards secrets to the fundamental processes and conditions that governed our solar system during its formation. As our primary example of a giant planet, Jupiter can also provide critical knowledge for understanding the planetary systems being discovered around other stars.

With its suite of science instruments, Juno will investigate the existence of a solid planetary core, map Jupiter's intense magnetic field, measure the amount of water and ammonia in the deep atmosphere, and observe the planet's auroras.

Juno will let us take a giant step forward in our understanding of how giant planets form and the role these titans played in putting together the rest of the solar system.

Key things to know about Juno
o Spacecraft launches in August 2011
o Five-year cruise to Jupiter, arriving July 2016
o One year at Jupiter will complete the mission (orbiting the planet 32 times)
Juno will improve our understanding of our solar system’s beginnings by revealing the origin and evolution of Jupiter.

Specifically, Juno will…
o Determine how much water is in Jupiter’s atmosphere, which helps determine which planet formation theory is correct (or if new theories are needed)
o Look deep into Jupiter’s atmosphere to measure composition, temperature, cloud motions and other properties
o Map Jupiter’s magnetic and gravity fields, revealing the planet’s deep structure
o Explore and study Jupiter’s magnetosphere near the planet’s poles, especially the auroras – Jupiter’s northern and southern lights – providing new insights about how the planet’s enormous magnetic force field affects its atmosphere.

Monday, May 09, 2011

Sunset from an Astronaut's Perspective


Astronauts onboard the International Space Station see the Earth from a unique perspective — for example, in one 24-hour period, they see not one sunrise and sunset, but 16 on average. Each changeover between day and night is marked by the terminator, a line on Earth's surface separating the sunlit side from the darkness.

While the terminator is often conceptualized as a hard boundary, in reality the edge of light and dark is diffuse due to the scattering of light by the Earth's atmosphere. This zone of diffuse lighting is experienced as dusk or twilight on the ground; while the Sun is no longer visible, some illumination is still present due to light scattering over the local horizon.

The terminator is visible in this panoramic view across central South America, looking towards the northeast. An astronaut shot the photo at approximately 7:37 p.m. local time. Layers of the Earth's atmosphere, colored bright white to deep blue, are visible on the horizon (or limb). The highest cloud tops have a reddish glow due to direct light from the setting sun, while lower clouds are in twilight.

Friday, May 06, 2011

China's First Space Station: A New Foothold in Earth Orbit


China's state-run news outlets report that preparations of the country's first space station module, called Tiangong-1, are in full swing for a launch in the second half of this year and will be followed by an unpiloted spacecraft.

The spacecraft twosome, the station module and China's Shenzhou 8 vehicle, will mark the country's first round of orbital rendezvous and docking tests – viewed as a springboard to larger space adventures. A Long March 2F rocket is the booster of choice for the individual launches, according to reports by China's Xinhua news agency.

According to state media reports, the Tiangong-1 space station module is outfitted with a docking port on its front and rear ends. It will tip the scales at roughly 8 1/2 tons and purportedly will have a two-year lifetime in Earth orbit. Next year, China's Shenzhou 9 and Shenzhou 10 missions, each carrying astronauts, are expected to link up with the station module, according to current plan.


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Thursday, May 05, 2011

Space Tourist Trips Around the Moon Get Roomier Spaceship


Fifty years after the first American astronaut rocketed into space, one commercial spaceflight company is hoping to push the envelope even further, with tourist trips around the moon. And now they plan to use a bigger spaceship.

The Virginia-based space tourism firm Space Adventures has brokered commercial rides to the International Space Station for the last 10 years under a partnership with Russia's Federal Space Agency, which provided the Soyuz spacecraft for the flights. The three-person Soyuz vehicle also forms the core of Space Adventures' trip for two around the moon at $150 million per passenger, but the U.S. company on may 5th announced a new twist: an extra module to give customers more room during the lunar visit.

Space Adventures already has one customer signed on for the circumlunar joyride and is in contract negotiations with a second, which means the first flight could occur as soon as the end of 2015, said the company's chairman Eric Anderson. "The mission, in my mind, will be another watershed event," Anderson said in a news briefing today. "It's remarkable that a private company will be able to work in the market and finance what is likely to be humanity's first return to the moon in what will, at that time, be 45 years."

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Wednesday, May 04, 2011

Virgin Galactic's Space Tourist Ship Passes Major Flight Test


A private spaceship built to carry space tourists on suborbital flights for the company Virgin Galactic passed a major glide test flight while flying over California's Mojave Desert on 4th may 2011: The spacecraft tested out the novel system it will use when re-entering Earth's atmosphere. Today's flight marked Virgin Galactic's seventh glide test for its first SpaceShipTwo spacecraft, called the VSS Enterprise, and took off from the Mojave Air and Space Port.

Today's flight marked Virgin Galactic's seventh glide test for its first SpaceShipTwo spacecraft, called the VSS Enterprise, and took off from the Mojave Air and Space Port. The WhiteKnightTwo/SpaceShipTwo combo serves as a launch system, the backbone of Virgin Galactic’s aspirations to create a spaceline -- one that would whisk tourists into space on a suborbital trajectory. SpaceShipTwo vehicles are designed to carry six passengers and two pilots to the edge of space and back.

The pay-per-view flights are billed as giving tourists a spectacular view of the Earth and several minutes of weightlessness. A per-seat price of $200,000 is being offered by Virgin Galactic. The space liner operations are backed by British billionaire, Sir Richard Branson, founder of the firm.

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Sunday, May 01, 2011

Largest 3-D Map Opens Window to the Ancient Universe


The largest-ever three-dimensional map of the distant universe has been created using the light of the brightest objects in the cosmos. Since this distant light took eons to reach Earth, the map is essentially a window back in time, providing an unprecedented view of what the universe looked like 11 billion years ago.Normally, researchers make maps of the universe by looking at galaxies.

"Here, we are looking at intergalactic hydrogen gas, which blocks light," said researcher Anže Slosar, a physicist at the U.S. Department of Energy's Brookhaven National Laboratory. "It's like looking at the moon through clouds -- you can see the shapes of the clouds by the moonlight that they block."

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Friday, April 29, 2011

NASA's Voyager Probes to Leave Solar System


It may be decades before humanity sets foot on Mars, but we're only five years away from sampling the vast stretches of interstellar space beyond our solar system for the first time, researchers say. NASA's twin unmanned Voyager spacecraft, which were launched in 1977, are streaking toward the edge of the solar system at around 37,000 mph (60,000 kph). At that rate, they'll probably pop out of our sun's sphere of influence and into interstellar space by 2016 or so, according to mission scientists.

"They are about to break free of the solar system," Ed Stone, Voyager project scientist at Caltech in Pasadena, Calif., said during a media teleconference yesterday (April 28). "We are trying to get outside of our bubble, into interstellar space, to directly measure what is there.

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Sunday, April 24, 2011

Asteroid or Planet?



Scientists still aren't sure what to make of Vesta, a small body that orbits the sun. Is it an asteroid or a planet? NASA's Dawn spacecraft could settle the matter. Vesta was spotted 200 years ago and is officially a "minor planet" — a body that orbits the sun but is not a proper planet or comet. Yet, many astronomers call Vesta an asteroid because it lies in the main asteroid belt between Mars and Jupiter.

But Vesta is not a typical member of that orbiting rubble patch. The vast majority of objects in the main belt are relative lightweights, 62 miles(100 kilometers) wide or smaller, compared with Vesta, which is 329 miles(530 km) wide. If Vesta is an asteroid, it would be the second-largest in the solar system. Some scientists, however, are skeptical about that designation. "I don't think Vesta should be called an asteroid," said Tom McCord, a Dawn team member at the Bear Fight Institute in Winthrop, Wash. "Not only is Vesta so much larger, but it's an evolved object, unlike most things we call asteroids."

The evolution of Vesta

The onion-like structure of Vesta (core, mantle and crust) is the key trait that makes Vesta more like planets such as Earth, Venus and Mars than the other asteroids, McCord said. Like the planets, Vesta had sufficient radioactive material inside when it formed, releasing heat that melted rock and enabled lighter layers to float to the outside. Signatures of a type of volcanic rock called basalt were detected in 1972, which meant that the body had to have melted at one time.

Thursday, April 21, 2011

Mars' Thick Dry Ice Sheet Points to Planet's Wetter Past


The south pole of Mars has a layer of dry ice that is 30 times thicker than previously thought, a find that suggests the Red Planet may have had more liquid water on its the surface in the distant past, scientists say. While most of the ice at the Martian south pole is frozen water, some of the ice pack is composed of dry ice — frozen carbon dioxide.

A team of scientists used a radar instrument on NASA's Mars Reconnaissance Orbiter to calculate the depth of dry ice deposits. By measuring how long it took for the radar waves to travel through the ice and bounce back to the MRO spacecraft, the researchers determined the dry ice cache was nearly 2,300 feet (700 meters) thick.

"The volume of the deposit is about the volume of Lake Superior," said study leader Roger Phillips of the Southwest Research Institute.

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A Galactic Rose Highlights Hubble's 21st Anniversary


In celebration of the 21st anniversary of the Hubble Space Telescope's deployment into space, astronomers pointed Hubble at an especially photogenic group of interacting galaxies called Arp 273.

This image, taken by the NASA/ESA Hubble Space Telescope, shows a group of interacting galaxies called Arp 273. The larger of the spiral galaxies, known as UGC 1810, has a disc that is tidally distorted into a rose-like shape by the gravitational pull of the companion galaxy below it, known as UGC 1813. The swathe of blue jewels across the top is the combined light from clusters of intensely bright and hot young blue stars. These massive stars glow fiercely in ultraviolet light.

The smaller, nearly edge-on companion shows distinct signs of intense star formation at its nucleus, perhaps triggered by the encounter with the companion galaxy.

Tuesday, April 19, 2011

Pluto's Atmosphere Found Poisonous and Surprisingly High


Poisonous carbon monoxide gas has been discovered in the atmosphere of the dwarf planet Pluto, after a worldwide search that lasted nearly two decades, according to a new study that also detected the planet's atmosphere extending much higher above the surface than previously thought. A British-based team of astronomers, led by Jane Greaves of the University of St. Andrews in Scotland, found a strong signal of carbon monoxide gas in Pluto's atmosphere using the 15-meter James Clerk Maxwell Telescope in Hawaii.

The atmosphere of Pluto was known to extend more than 60 miles (about 100 kilometers) above the surface, the researchers said, but the new findings raise that height to more than 1,860 miles equivalent to a quarter of the distance out to Pluto's largest moon, Charon.

Greaves will present the new discovery on Wednesday (April 20) at the Royal Astronomical Society's National Astronomy Meeting in Wales. Pluto was discovered in 1930 and was considered to be the smallest and most distant planet orbiting around the sun. In 2006, its status was demoted to dwarf planet, making it one of a handful of such bodies that orbit beyond Neptune in the outer reaches of the solar system.


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Monday, April 18, 2011

Why Is It So Hard to Travel to Mars?


The Challenger and Columbia space shuttle disasters were perhaps two of the most prominent reminders of how crucial it is that everything work just right for a spacecraft to travel to space and successfully return back to Earth. Whether it was the failure of the seal used to stop hot gases from seeping through, or a piece of foam insulation that damaged the thermal protection system, scientists and engineers must make thousands of predictions of all the things that could go wrong during flight.

NASA's human Mars mission presents even more challenges of sending humans safely to a farther distance and to a more dangerous environment. Designing an aircraft that can safely enter and exit Mars' unpredictable atmosphere is a big challenge. "Each time we fly to Mars, we learn a little more and get a little smarter," said Walter Engelund of NASA's Langley Research Center. "One thing we have learned is that the Mars atmosphere is certainly a big variable. It is much more dynamic than our own Earth's atmosphere." For missions that require entry and re-entry into an atmosphere, the design of the spacecraft is typically guided by its EDL system.

Engelund, along with several other NASA colleagues, published a review of the EDL systems currently being proposed for a future manned mission to Mars in a recent book titled "The Human Mission to Mars. Colonizing the Red Planet." The book is a compilation of studies written by a team of more than 70 scientists, including four astronauts (two who walked on the moon), offering a detailed guide of how to successfully accomplish a human mission to Mars. Engelund is the lead author of the EDL study.

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Friday, April 15, 2011

April's Full Moon Arrives Sunday With Easter Name


Sunday (April 17) brings us the first full moon of the new spring season in the Northern Hemisphere, bringing a lunar delight named – in part – for Easter. The official moment that the moon will turn full is 10:44 p.m. EDT. Traditional names for the full moons of the year are found in some publications such as The Farmers' Almanac. The origins of these names have been traced back to native America, though they may also have evolved from old England or, as Guy Ottewell, editor of the annual publication, "Astronomical Calendar" suggests, "writer's fancy."

Traditionally, the April full moon is known as the "Pink Moon,"supposedly because the grass pink or wild ground phlox is one of the earliest widespread flowers of the spring. Other monikers were the Full Sprouting Grass Moon, the Egg Moon, and – among coastal tribes – the Full Fish Moon, when the shad come upstream to spawn.

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Thursday, April 14, 2011

New U.S. Spy Satellite Launches on Clandestine Mission


A rocket carrying a new U.S. spy satellite lit up the California night sky Thursday on a secret mission for the National Reconnaissance Office. The spy satellite NROL-34 soared into orbit atop an unmanned Atlas 5 rocket after launching from a pad at the Vandenberg Air Force Base at 9:24 p.m. PDT (0424 GMT on April 15) to begin the latest classified flight for the NRO. The details of the satellite's purpose and final orbit are classified, but the new spacecraft will definitely serve a role for the U.S. military, officials said.

"This launch supports the military's national defense mission," officials with the United Launch Alliance, which orchestrated the satellite launch for the NRO, said in a mission description. Because of the satellite's secret purpose, a media blackout was put in place about 4 1/2 minutes after the Atlas 5 rocket launched toward orbit. The rocket lifted off with the help of a single solid rocket booster to propel it into space.


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Tuesday, April 12, 2011

Why There's No Replacement for the Space Shuttle


After the wheels of the space shuttle roll to a stop for the final time, NASA astronauts will have to rely on Russian spaceships for their rides into space until commercial American vehicles are ready to fly crews to orbit. A capsule-based spacecraft, called Orion, is also in development, but NASA's current plans are to use it primarily as an escape ship for the International Space Station.

Over the course of the shuttle program's 30-year career, NASA and its various partners explored a number of different vehicle options to succeed the space shuttles, but none were brought to fruition, said Roger Launius, space history curator at the Smithsonian's National Air and Space Museum, in Washington.One by one, each program ended after development plans bumped up against funding and politics – an experience familiar throughout NASA's history. "There's a whole series of factors – some of them were political, but a lot of the problems were technical," Launius said. "Could they have been solved if they had more money? Probably. So, was it a technical problem or a political problem? I could argue both sides."

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Is Space Tourism the New Space Race?


Fifty years after the Soviet Union beat the United States to send the first human to space, a new space race is heating up. This time, the players are not nations — rather, they're commercial companies that aim to send the first paying passengers to space on private spaceships. "It's an exciting time for the industry," said George Whitesides, president of suborbital spaceship company Virgin Galactic. "I really believe that we're at the edge of an extraordinary period of innovation which will radically change our world."

If Virgin and other companies succeed, space could soon become one more conquered frontier, with rocket rides to space becoming as accessible as plane rides across the Atlantic. "We're just about to the point where low-Earth orbit really ought to be considered part of our normal regime," said Roger Launius, a space history curator at the Smithsonian National Air and Space Museum. But while we may be nearing a tipping point where access to space expands widely beyond the select few who've left Earth to date, Launius and others caution that it's not a done deal yet.


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Sunday, April 10, 2011

NASA's Space Shuttles at 30

NASA's space shuttle program may be coming to an end later this year, but the agency's fleet of orbiters is preparing to celebrate an important milestone next week – the 30th anniversary of the very first space shuttle flight. On April 12, 1981, the shuttle Columbia blasted off from NASA's Kennedy Space Center in Cape Canaveral, Fla.,on the program's inaugural STS-1 mission. Thirty years later, the workhorse shuttles have played an instrumental role in constructing the International Space Station, launching critical satellites and observatories into orbit including the prolific Hubble Space Telescope and carrying numerous supplies and science experiments into space.

Over the course of his career, Wayne Hale, NASA's former space shuttle program manager, bore witness to many of these crowning achievements. Hale joined NASA in 1978 as a propulsion officer at the Johnson Space Center in Houston. He then worked as a flight director in Mission Control, presiding over 40 shuttle flights before becoming manager of the program in 2005. Hale played a critical role in the agency's recovery from the catastrophic loss in 2003 of the shuttle Columbia and its seven-astronaut crew. He now serves as Director of Human Spaceflight Programs at Special Aerospace Services, located in Boulder, Colo.


Wednesday, April 06, 2011

Russian Spaceship 'Gagarin' Arrives at Space Station

A Russian spaceship bearing the name of history's most famous cosmonaut docked at the International Space Station late Wednesday to deliver three new crew members to the orbiting lab. The Soyuz TMA-21 — nicknamed "Gagarin" after Yuri Gagarin, who became the first person in space on April 12, 1961 — successfully docked with the station's Poisk module at 7:09 p.m. EDT (2309 GMT). The spacecraft had launched from Baikonur Cosmodrome in Kazakhstan on April 4, blasting off from the same pad used for Gagarin's historic flight nearly 50 years ago. "Contact and capture — docking confirmed," a NASA official announced as the "Gagarin" sidled up to the orbiting lab. The "Gagarin" launched into space Monday (April 4 EDT) carrying two cosmonauts and one NASA astronaut to join three other crewmembers already aboard the station, rounding out the orbiting lab's Expedition 27.

The three spaceflyers — NASA's Ron Garan and Russians Alexander Samokutyaev and Andrey Borisenko — will also stay on as part of the next station mission, Expedition 28. "It was a great couple of days and we're ready to get to work," Garan said. Garan and Samokutyaev will be flight engineers on both expeditions. Borisenko will serve as a flight engineer on Expedition 27 and later serve as the commander of Expedition 28. [Vote Now! The Best Spaceships of All Time]. The crew received a flood of congratulatory calls from Russia's Mission Control center near Moscow after docking at the space station. Russian space official and the families of the astronaut and cosmonauts were on hand to wish the crew well. "We love you," Garan's wife Carmel told her husband and his crewmates after their arrival on the station. "We'll keep the fires burning at home, and we'll welcome you home with open arms at the end of your successful mission."

Tuesday, April 05, 2011

Company planning biggest rocket since man on moon


A high-tech entrepreneur unveiled plans Tuesday to launch the world's most powerful rocket since man went to the moon. Space Exploration Technology has already sent the first private rocket and capsule into Earth's orbit as a commercial venture. It is now planning a rocket that could lift twice as much cargo into orbit as the soon-to-be-retired space shuttle. The first launch is slotted for 2013 from California with follow-up launches from Cape Canaveral in Florida.

Space X's new rocket called Falcon Heavy is big enough to send cargo or even people out of Earth's orbit to the moon, an asteroid or Mars. Only the long retired Saturn V rocket that sent men to the moon was bigger. "This is a rocket of truly huge scale," said Space X president Elon Musk, who also founded PayPal and manufactures electric sports cars. The Falcon Heavy could put 117,000 pounds into the same orbit as the International Space Station. The space shuttle hauls about 54,000 pounds into orbit. The old Saturn V could carry more than 400,000 pounds of cargo.

Monday, April 04, 2011

NASA Delays Final Launch of Shuttle Endeavour to Avoid Space Traffic Jam

NASA has delayed the last launch of the shuttle Endeavour toward the International Space Station by at least 10 days, to April 29, in order to avoid a space traffic jam with an unmanned Russian cargo ship, also headed for the orbiting laboratory later this month. Endeavour is now targeted to blast off on its STS-134 flight on Friday, April 29 at 3:47 p.m. EDT, NASA officials said. The decision to postpone the launch removes a scheduling conflict with a Russian Progress cargo ship, which is currently scheduled to launch April 27. The robotic Progress vehicle will arrive at the station on April 29.

Discussions between NASA and its international partners have been ongoing for weeks, Beutel said, and the decision to delay Endeavour's flight was made after several other options, including moving the Progress' launch date, were deemed impractical. "Apparently there is a biological experiment onboard the Progress that has a very short shelf life onboard that spacecraft," Beutel said. "We even looked at the possibility of putting that experiment on Endeavour, but logistically that didn't work out as well." Balancing traffic at the space station and on the ground has proved challenging for the various space station partners, but is especially crucial for NASA, in order to capitalize on the unrivaled cargo-carrying capabilities of the space shuttles. The main objective of the remaining shuttle flights is to ferry supplies to the station so that the orbiting laboratory is in a good position for the years ahead, following the retirement of the agency's shuttle fleet later this year.

NASA preparing Mars rover for launch


NASA engineers are putting the finishing touches on a mega-rover to Mars before shipping it off to Florida for launch later this year. A small army of technicians dressed in protective bunny suits has been working around the clock inside a clean room at the Jet Propulsion Laboratory near Los Angeles assembling the craft, called Curiosity, and testing its science instruments. The $2.5 billion mission was supposed to launch in 2009, but problems during construction forced a two-year delay.

With launch scheduled for late November, engineers have been busy testing the spacecraft's various systems — all the while making sure that contamination from Earth doesn't accidentally hitch a ride to Mars. The nuclear-powered Curiosity — the size of a small SUV — will probe rocks and soil to determine whether the red planet ever had the right environment to support primitive life. It will carry the most high-tech instruments to the Martian surface including a laser that can zap boulders from afar. To the dismay of some space fans, Curiosity won't carry a high-resolution 3-D camera that "Avatar" director James Cameron was helping to build. NASA recently nixed it because there wasn't enough time to fully test the zoom lens before launch.

Scientists expect Curiosity to build on the discoveries of the twin rovers Spirit and Opportunity, which have uncovered geologic evidence of ancient water and the Phoenix lander, which found ice at its Martian north pole landing site. Curiosity's road to the launch pad has been bumpy. Engineers had to redesign the rover's heat shield and fix problems with the parachute. NASA also faced delivery delays from subcontractors that affected the launch timetable and raised the mission price tag.

Friday, April 01, 2011

NASA Test Stand Passes Review for Next-Generation Rocket Engine Testing


Forty-five years after its first Saturn V rocket stage test and 35 years after its first space shuttle main engine test, the A-2 Test Stand at NASA’s John C. Stennis Space Center achieved a milestone in preparation for its third major rocket engine test project. A facility readiness review in mid-March indicated all major modifications have been completed on the historic A-2 stand to begin testing the next-generation J-2X rocket engine this summer.

The new test project comes as Stennis celebrates its 50th anniversary year. On Oct. 26, 1961, NASA publicly announced plans to build the south Mississippi facility to test the massive Saturn V rocket stages for the Apollo Program. The first test of a Saturn V second stage at Stennis was performed at the A-2 stand on April 23, 1966. Stennis engineers tested 27 first and second Saturn V rocket stages for the Apollo Program, including those used to carry humans to the moon.