This dazzling image shows the globular cluster Messier 69, or M 69 for short, as viewed through the NASA/ESA Hubble Space Telescope. Globular clusters are dense collections of old stars. In this picture, foreground stars look big and golden when set against the backdrop of the thousands of white, silvery stars that make up M 69.

Another aspect of M 69 lends itself to the bejeweled metaphor: As globular clusters go, M 69 is one of the most metal-rich on record. In astronomy, the term "metal" has a specialized meaning: it refers to any element heavier than the two most common elements in our Universe, hydrogen and helium. The nuclear fusion that powers stars created all of the metallic elements in nature, from the calcium in our bones to the carbon in diamonds. Successive generations of stars have built up the metallic abundances we see today.

Because the stars in globular clusters are ancient, their metallic abundances are much lower than more recently formed stars, such as the Sun. Studying the makeup of stars in globular clusters like M 69 has helped astronomers trace back the evolution of the cosmos.

M 69 is located 29 700 light-years away in the constellation Sagittarius (the Archer). The famed French comet hunter Charles Messier added M 69 to his catalogue in 1780. It is also known as NGC 6637.

The image is a combination of exposures taken in visible and near-infrared light by Hubble’s Advanced Camera for Surveys, and covers a field of view of approximately 3.4 by 3.4 arcminutes.

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Blanketing NASA's Webb Telescope's Science Instrument Electronics

These engineers from Genesis Engineering Solutions are doing what’s called "blanket closeout" and it took two days to complete.

The gold louvers are composite mirrors, made of gold-coated carbon fiber, designed to remove the heat from inside the IEC to deep space. 

The IEC holds computing hardware for each of the science instruments. This special part of the telescope allows the computer hardware to operate at room temperature on the cold side of the telescope by directing heat away so that the telescope can deliver infrared imagery.

"As heat radiates off the panel that they are attached to, the mirrors focus it in a particular direction (namely, away from the telescope)," says Lutter. 

After the engineers completed blanketing, the IEC was then placed in the thermal chamber to be tested against the chill of a space-simulated environment. This process is called the thermal vacuum and balance test. During this test, temperatures drop to about 90 degrees Kelvin (-297.67 degrees Fahrenheit or -183.15 degrees Celsius). 

"This is important because we need to know how effective the IEC is at keeping heat away from the cold side of Webb," says Lutter. "If even a little heat escapes the IEC in the direction of the telescope, the telescope's sensitivity could be ruined."

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Inside NASA’s Curiosity: It’s an Apple Airport Extreme… with wheels

Late last night, Mars Science Laboratory (MSL) Curiosity successfully navigated its way through Seven Minutes of Terror and touched down on the surface of the Red Planet, heralding a new age of extraterrestrial exploration that will eventually result in the human colonization of Mars.

Hardware
At the heart of Curiosity there is, of course, a computer. In this case the Mars rover is powered by a RAD750, a single-board computer (motherboard, RAM, ROM, and CPU) produced by BAE. The RAD750 has been on the market for more than 10 years, and it’s currently one of the most popular on-board computers for spacecraft. In Curiosity’s case, the CPU is a PowerPC 750 (PowerPC G3 in Mac nomenclature) clocked at around 200MHz — which might seem slow, but it’s still hundreds of times faster than, say, the Apollo Guidance Computer used in the first Moon landings. Also on the motherboard are 256MB of DRAM, and 2GB of flash storage — which will be used to store video and scientific data before transmission to Earth.

BAE RAD750 single-board, radiation-hardened computerThe RAD750 can withstand temperatures of between -55 and 70C, and radiation levels up to 1000 gray. Safely ensconced within Curiosity, the temperature and radiation should remain below these levels — but for the sake of redundancy, there’s a second RAD750 that automatically takes over if the first one fails.

Software
On the software side of things, NASA again stuck to tried-and-tested solutions, opting for the 27-year-old VxWorks operating system. VxWorks, developed by Wind River Systems (which was acquired by Intel), is a real-time operating system used in a huge number of embedded systems. The previous Mars rovers (Sojourner, Spirit, Opportunity), Mars Reconnaissance Orbiter, and the SpaceX Dragon spacecraft all use VxWorks. VxWorks also powers BMW iDrive, the Apache Longbow helicopter, and the Apple Airport Extreme and Linksys WRT54G routers (really).

I said that VxWorks is 27 years old, but that’s a bit unfair: The initial release was in 1985 (around the same time as MS-DOS 3.0), but it has been in constant development since then, reaching v6.9 last year. Why does Curiosity use VxWorks? It’s reliable, has a mature development toolchain, and presumably its low-level scheduling and interrupt systems are ideal for handling real-time tasks like EDL (entry, descent, and landing; aka, seven minutes of terror).

NASA's Space Launch System Passes Major Agency Review, Moves to Preliminary Design

The rocket that will launch humans farther into space than ever before passed a major NASA review Wednesday. The Space Launch System (SLS) Program completed a combined System Requirements Review and System Definition Review, which set requirements of the overall launch vehicle system. SLS now moves ahead to its preliminary design phase.

The SLS will launch NASA's Orion spacecraft and other payloads, and provide an entirely new capability for human exploration beyond low Earth orbit.

These NASA reviews set technical, performance, cost and schedule requirements to provide on-time development of the heavy-lift rocket. As part of the process, an independent review board comprised of technical experts from across NASA evaluated SLS Program documents describing vehicle specifications, budget and schedule. The board confirmed SLS is ready to move from concept development to preliminary design.

"This new heavy-lift launch vehicle will make it possible for explorers to reach beyond our current limits, to nearby asteroids, Mars and its moons, and to destinations even farther across our solar system," said William Gerstenmaier, associate administrator for the Human Exploration and Operations Mission Directorate at NASA Headquarters in Washington. "The in-depth assessment confirmed the basic vehicle concepts of the SLS, allowing the team to move forward and start more detailed engineering design."

The reviews also confirmed the SLS system architecture and integration with the Orion spacecraft, managed by NASA's Johnson Space Center in Houston, and the Ground Systems Development and Operations Program, which manage the operations and launch facilities at NASA's Kennedy Space Center in Florida.

"This is a pivotal moment for this program and for NASA," said SLS Program Manager Todd May. "This has been a whirlwind experience from a design standpoint. Reaching this key development point in such a short period of time, while following the strict protocol and design standards set by NASA for human spaceflight is a testament to the team's commitment to delivering the nation's next heavy-lift launch vehicle."

SLS reached this major milestone less than 10 months after the program's inception. The combination of the two assessments represents a fundamentally different way of conducting NASA program reviews. The SLS team is streamlining processes to provide the nation with a safe, affordable and sustainable heavy-lift launch vehicle capability. The next major program milestone is preliminary design review, targeted for late next year.

The first test flight of NASA's Space Launch System, which will feature a configuration for a 70-metric-ton (77-ton) lift capacity, is scheduled for 2017. As SLS evolves, a three-stage launch vehicle configuration will provide a lift capability of 130 metric tons (143 tons) to enable missions beyond low Earth orbit and support deep space exploration.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the SLS program. Across the country NASA and its industry partners continue to make progress on SLS hardware that will be integrated into the final design. The RS-25 core stage and J-2X upper-stage rocket engine in development by Pratt & Whitney Rocketdyne of Canoga Park, Calif., for the future two-stage SLS, will be tested at NASA's Stennis Space Center in Mississippi. The prime contractor for the five-segment solid rocket boosters, ATK of Brigham City, Utah, has begun processing its first SLS boosters in preparation for an initial qualification test next year, ahead of their use for the first two exploration missions. The Boeing Co. in Huntsville is designing the SLS core stage, to be built at NASA's Michoud Assembly Facility in New Orleans and tested at Stennis before being shipped to Kennedy. 

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Nasa hires SpaceX for science satellite launch

Nasa hired Space Exploration Technologies to launch an ocean monitoring satellite Nasa officials say.This is a key win for the start-up rocket company that also wants to break into the US military’s launch business.

The $82 million contract covers launch, payload processing and other services for the National Oceanic and Atmospheric Administration’s ocean-measuring Jason-3 satellite, which is slated to fly in December 2014.Launch would take place from SpaceX’s new complex at Vandenberg Air Force Base in California.

Nasa, which handles procurements for NOAA, also awarded three launch contracts, worth $412 million for Delta 2 rockets built by United Launch Alliance, a joint venture of Lockheed Martin Corp and Boeing Co.

One of the satellites earmarked for a Delta 2 flight is the replacement for a carbon dioxide tracking satellite lost in February 2009 after a failed launch on an Orbital Sciences Corp Taurus rocket.The launches, slated for July 2014, October 2014 and November 2016, also will take place at Vandenberg.

SpaceX, which is owned and operated by internet entrepreneur Elon Musk, already holds Nasa contracts worth $1,6 billion to fly cargo to the International Space Station, a $100 billion laboratory that orbits about 240 miles (386 kilometres) above Earth.

The company in May successfully flew a demonstration mission to the station, a key milestone in its efforts to win US military launch contracts as well.

ULA currently has a monopoly on US military launch business. But in an attempt to certify more launchers, the Air Force is expected to award a non-ULA launch services contract this year for the Deep Space Climate Observatory (DSCOVR), a former Nasa Earth-monitoring satellite being repurposed by NOAA into a solar observatory. A request for bids under the Air Force’s Orbital/Suborbital Program (OSP-3) was released May 11.

The criteria for new launchers was jointly developed by the Air Force, the National Reconnaissance Office and Nasa.The new Nasa contract is the first evidence that Falcon 9 meets the new launcher criteria.

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First Space-Bound Orion on Its Way to Kennedy

A major milestone has been achieved for NASA’s Orion program with the first Orion destined for space being shipped to the Kennedy Space Center. Construction on the spacecraft was finished at NASA’s Michoud Assembly Facility in Louisiana this week, and final outfitting and heat shield installation will take place at KSC.

This spacecraft will fly on Exploration Flight Test-1, an unmanned test that is scheduled two years from now. The EFT-1 flight will take Orion to an altitude of more than 3,600 miles, more than 15 times farther away from Earth than the International Space Station. Orion will return home at a speed of 25,000 miles per hour, almost 5,000 miles per hour faster than any human spacecraft. It will mimic the return conditions that astronauts experience as they come home from voyages beyond low Earth orbit. As Orion reenters the atmosphere, it will endure temperatures up to 4,000 degrees F., higher than any human spacecraft since astronauts returned from the moon.

This first Orion will fly atop a Delta IV Heavy, a rocket operated by United Launch Alliance. While this launch vehicle will provide sufficient lift for the EFT-1 flight plan, NASA’s SLS rocket will be needed for the vast distances of future exploration missions.

Following EFT-1, the first integrated flight test will launch an uncrewed Orion on the SLS in 2017. That test will put the entire integrated exploration system through its paces. The Orion spacecraft will have the capability to carry astronauts to the moon, asteroids, Mars and other deep space destinations. 

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NASA's Ocean Salinity Pathfinder Celebrates its First Year in Orbit

It's been a busy first year in space for Aquarius, NASA's pioneering instrument to measure ocean surface salinity from orbit.

Designed to advance our understanding of what changes in the saltiness of the ocean's top layer say about the water cycle and variations in climate, Aquarius took only two and a half months after its launch to start measuring global salinity patterns. Since then, it has also observed regional features such as the freshwater plume gushing from the Amazon River and localized changes in ocean saltiness following a tropical storm.

"It was a very remarkable achievement, that within such a short period of time after turning the instrument on we were producing very good-looking data," said Aquarius Principal Investigator Gary Lagerloef, of Earth & Space Research in Seattle. "It was beyond our expectations."

Lagerloef said that objectives for Aquarius' second year in orbit include correcting a few remaining calibration errors and validating the Aquarius dataset with thousands of direct in-water measurements of salinity.

The Aquarius/Satélite de Aplicaciones Científicas (SAC)-D mission is an international collaboration of NASA and Argentina's space agency. The satellite also carries instruments from partner institutions in Canada, Italy and France.

A Delta II rocket carrying the international observatory launched from Vandenberg Air Force Base in California, on June 10, 2011. Less than an hour later, the satellite separated from the rocket, started its deployment and established communications with ground stations.

"The first time the thing chirped, we got the data and posted it on the Web. It was just basic telemetry at that point, but it showed that all the systems we had put in place to share the data worked," said Gene Feldman, Aquarius project manager at NASA Goddard Space Flight Center in Greenbelt, Md. "We didn't get to pop champagne – we didn't have the time!"

Aquarius is the first NASA instrument specifically designed to study superficial ocean salinity from space, and it does it at a rate of about 300,000 measurements per month. It uses three passive microwave sensors, called radiometers, to record the thermal signal from the oceans' top 0.4 inches (10.1 millimeters). This signal varies depending on the concentration of salt and the temperature of the waters.

"An overarching question in climate research is to understand how changes in the Earth's water cycle – meaning rainfall and evaporation, river discharges and so forth – ocean circulation, and climate link together," Lagerloef said. Most global precipitation and evaporation events take place over the ocean and are very difficult to measure. But rainfall freshens the oceans' surface waters, and Aquarius can detect these changes in saltiness. "Salinity is the variable we can use to measure that coupling effect. It's a critical factor and it will eventually be used to improve climate forecast models."

Aquarius became operational on Aug. 25, 2011. The project's scientists soon created a map of global ocean saltiness using the first two and a half weeks of measurements, which had been compared against reference salinity data. The map showed variations in salinity patterns in much greater detail than Aquarius researchers had expected to see so early in the mission. Another welcome surprise was the observation of the effects on the ocean of Tropical Storm Lee (Sept. 2-3, 2011). Heavy rains produced a low-salinity feature that lasted more than a month in the Gulf of Mexico between the Mississippi River delta and the Florida panhandle.

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NASA Flight Tests New ADS-B Device on Ikhana UAS

NASA's Dryden Flight Research Center flew its Ikhana MQ-9 unmanned aircraft with an Automatic Dependent Surveillance-Broadcast, or ADS-B, device, for the first time on March 15.

It was the first time an unmanned aircraft as large as Ikhana – with a 66-foot wingspan, a takeoff weight of more than 10,000 pounds, and a cruising altitude of 40,000 feet -- has flown while equipped with ADS-B. ADS-B is an aircraft tracking technology that all planes operating in certain U.S. airspace must adopt by January 2020 to comply with Federal Aviation Administration (FAA) regulations.

It also was the first flight of hardware for the NASA Aeronautics research project known as UAS in the NAS, which is short for Unmanned Aircraft Systems Integration in the National Airspace System.The equipment performed well during a flight lasting nearly three hours in restricted air space over Dryden's Western Aeronautical Test Range, which is part of Edwards Air Force Base and the China Lake Naval Air Warfare Center.

Being equipped with ADS-B enables NASA's Ikhana to provide much more detailed position, velocity, and altitude information about itself to air traffic controllers, airborne pilots of other ADS-B equipped aircraft flying in its vicinity, and to its pilots on the ground. Currently, only air traffic controllers can see all the aircraft in any given section of the sky.

The ADS-B checkout flight aboard Ikhana kicked off a series in which researchers will collect ADS-B data while performing representative air traffic control-directed maneuvers.

As part of a collaborative effort, FAA's William J. Hughes Technical Center in Atlantic City, N.J., recorded ADS-B data from the flight and will help analyze the performance of the system installed in the aircraft. Researchers also evaluated new ADS-B laptop software for displaying surrounding air traffic information to the UAS pilots on the ground.

"ADS-B is a cornerstone capability required in the NextGen, and understanding its performance and suitability for integrating unmanned aircraft into the national airspace system is critical to the overall goals of the project," said Sam Kim, deputy manager of integrated test and evaluation for NASA's UAS in the NAS Project.

Developing technologies that will enable unmanned aircraft to fly safely among other planes in the nation's skies is the job of Kim's team.

ADS-B is a key component of the largest transformation of air traffic control ever attempted in the United States. Known as the Next Generation Air Transportation System, or NextGen, it is a multi-billion-dollar technology modernization effort that will make air travel safer, more flexible and more efficient. As the system gets better, its capacity will grow and the demand for different types of air transportation – even unmanned aircraft – will increase.

Current tracking devices aboard aircraft are called transponders, but the ADS-B isn't just a new-fangled transponder. It provides much more detailed and accurate information to air traffic controllers, and will enable navigation by satellite in addition to the current system of ground radars.

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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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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.

NASA Satellite Data Reveals Joplin Tornado Track

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.

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

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:

• 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.

Spitzer Sees Crystal Rain in Infant Star Outer Clouds

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.

Endeavour's Late Inspection Complete

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.

Asteroid Research Begins Under the Sea

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.

NASA'S Mars Atmosphere Mission

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.

NASA's Next Mars Rover Nears Completion

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.

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.