SPACEX PREPARES FOR LAUNCH

FROM:  NASA
SpaceX and NASA Prepare for Launch
In a processing facility at Space Launch Complex-40 on Cape Canaveral Air Force Station in Florida, Space Exploration Technologies technicians attach the Dragon capsule to the second stage of the company’s Falcon 9 rocket. Known as SpaceX, the launch will be the company's second demonstration test flight for NASA's Commercial Orbital Transportation Services program, or COTS. During the flight, the capsule will conduct a series of check-out procedures to test and prove its systems, including rendezvous and berthing with the International Space Station. If the capsule performs as planned, the NanoRacks-CubeLabs Module-9 experiments and other cargo aboard Dragon will be transferred to the station. The cargo includes food, water and provisions for the station’s Expedition crews, such as clothing, batteries and computer equipment. Under COTS, NASA has partnered with two private companies to provide resupply missions to the station. The launch is TBD. For more information, visit http://www.nasa.gov/spacex. Photo credit: NASA/Jim Grossmann

JAPANESE PRIME MINISTER YOSHIHIKO NODA ACCEPTS MONTAGE FROM NASA ADMINISTRATOR CHARLES BOLDEN

FROM:  NASA
Japanese Prime Minister Yoshihiko Noda, fourth from left, accepts a montage from NASA Administrator Charles Bolden, third from left, during a meeting at the Blair House as Associate Administrator for Science and former astronaut John Grunsfled, left, Associate Administrator for Education and former astronaut Leland Melvin, second from left, and JAXA (Japan Aerospace Exploration Agency) astronauts Koichi Wakata and Satoshi Furukawa, right, look on, Monday, April 30, 2012, in Washington. Image Credit: NASA/Bill Ingalls

MAIDEN VOYAGE OF SPACE SHUTTLE COLUMBIA

FROM:  NASA
On April 12, 1981, astronauts John Young and Bob Crippen launched into space on space shuttle Columbia on the STS-1 mission--NASA's first mission aboard a reusable spacecraft. STS-1 was NASA's first manned mission since the Apollo-Soyuz Test Project in 1975. In this image, the two solid rocket boosters are aglow after being jettisoned. Image Credit: NASA

TEACHING A SPACESHIP HOW TO FLY

FROM:  NASA
A test model of the Orion spacecraft with its parachutes was tested the skies high above the U.S. Army’s Proving Grounds in Yuma, Ariz. on Feb. 29, 2012. This particular drop test examined the wake -- or the disturbance of the air flow behind Orion -- that is caused by the spacecraft. The U.S. Space Launch System, or SLS, will provide an entirely new capability for human exploration beyond Earth orbit and the Orion capsule is a major part of this program. The Orion spacecraft will replace the space shuttle as NASA's vehicle for human space exploration and is designed to accommodate four to six astronauts traveling into space. It also will supplement commercial and international partner transportation services to the International Space Station. Designed to be flexible for crew or cargo missions, SLS will continue America's journey of discovery from the unique vantage point of space. Image Credit: NASA

FIRST STAGE OF ANTARES ROCKET

FROM:  NASA
The first stage of Orbital Sciences Corporation’s Antares rocket stands in launch position during pathfinder operations at NASA’s Wallops Flight Facility and the Mid-Atlantic Regional Spaceport. Orbital’s Antares launch vehicle will be conducting missions for NASA under its Commercial Orbital Transportation Service Program and Cargo Resupply Services contract. Image Credit: NASA/P.Black

SPACE SHUTTLE DISCOVERY DISCOVERS ITS FINAL RESTING PLACE

FROM:  U.S. NAVY
The space shuttle Discovery attached to its 747 transport passes over the nation's capital. It will land in Washington D.C. to become an exhibit at the Smithsonian Air and Space Museum. Discovery, along with the rest of the shuttle fleet, has been retired from active service after 32 years of operations. U.S. Navy photo by Mass Communication Specialist 1st Class Jason M. Graham 

GALACTIC COLLISION

FROM:  NASA
Using a combination of powerful observatories in space and on the ground, astronomers have observed a violent collision between two galaxy clusters in which so-called normal matter has been wrenched apart from dark matter through a violent collision between two galaxy clusters.

Finding another system that is further along in its evolution than the Bullet Cluster gives scientists valuable insight into a different phase of how galaxy clusters -- the largest known objects held together by gravity -- grow and change after major collisions.

Researchers used observations from NASA's Chandra X-ray Observatory and Hubble Space Telescope as well as the Keck, Subaru and Kitt Peak Mayall telescopes to show that hot, X-ray bright gas in the Musket Ball Cluster has been clearly separated from dark matter and galaxies.

In this composite image, the hot gas observed with Chandra is colored red, and the galaxies in the optical image from Hubble appear as mostly white and yellow. The location of the majority of the matter in the cluster (dominated by dark matter) is colored blue. When the red and the blue regions overlap, the result is purple as seen in the image. The matter distribution is determined by using data from Subaru, Hubble and the Mayall telescope that reveal the effects of gravitational lensing, an effect predicted by Einstein where large masses can distort the light from distant objects.

In addition to the Bullet Cluster, five other similar examples of merging clusters with separation between normal and dark matter and varying levels of complexity, have previously been found. In these six systems, the collision is estimated to have occurred between 170 million and 250 million years earlier.

In the Musket Ball Cluster, the system is observed about 700 million years after the collision. Taking into account the uncertainties in the age estimate, the merger that has formed the Musket Ball Cluster is two to five times further along than in previously observed systems. Also, the relative speed of the two clusters that collided to form the Musket Ball cluster was lower than most of the other Bullet Cluster-like objects.

The special environment of galaxy clusters, including the effects of frequent collisions with other clusters or groups of galaxies and the presence of large amounts of hot, intergalactic gas, is likely to play an important role in the evolution of their member galaxies. However, it is still unclear whether cluster mergers trigger star formation, suppress it, or have little immediate effect. The Musket Ball Cluster holds promise for deciding between these alternatives.

The Musket Ball Cluster also allows an independent study of whether dark matter can interact with itself. This information is important for narrowing down the type of particle that may be responsible for dark matter. No evidence is reported for self-interaction in the Musket Ball Cluster, consistent with the results for the Bullet Cluster and the other similar clusters.

The Musket Ball Cluster is located about 5.2 billion light years away from Earth. A paper describing these results was led by Will Dawson from University of California, Davis and was published in the March 10, 2012 issue of The Astrophysical Journal Letters. The other co-authors were David Wittman, M. James Jee and Perry Gee from UC Davis, Jack Hughes from Rutgers University in NJ, J. Anthony Tyson, Samuel Schmidt, Paul Thorman and Marusa Bradac from UC Davis, Satoshi Miyazaki from the Graduate University for Advanced Studies (GUAS) in Tokyo, Japan, Brian Lemaux from UC Davis, Yousuke Utsumi from GUAS and Vera Margoniner from California State University, Sacramento.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra's science and flight operations from Cambridge, Mass.

NASA 905 WILL TAKE SHUTTLES TO FINAL RESTING PLACES

FROM:  NASA
The Shuttle Carrier Aircraft glides down the runway of the Shuttle Landing Facility at NASA’s Kennedy Space Center in Florida. The aircraft, known as an SCA, arrived at 5:35 p.m. EDT to prepare for shuttle Discovery’s ferry flight to the Washington Dulles International Airport in Sterling, Va., on April 17. This SCA, designated NASA 905, is a modified Boeing 747 jet airliner, originally manufactured for commercial use. One of two SCAs employed over the course of the Space Shuttle Program, NASA 905 is assigned to the remaining ferry missions, delivering the shuttles to their permanent public display sites. NASA 911 was decommissioned at the NASA Dryden Flight Research Center in California in February. Discovery will be placed on permanent public display in the Smithsonian's National Air and Space Museum Steven F. Udvar-Hazy Center in Chantilly, Va. Image Credit: NASA/Frankie Martin

ESA'S AUTOMATED TRANSFER VEHICLE APPROACHES INTERNATIONAL SPACE STATION

FROM:  NASA
In this photo taken from the International Space Station, the European Space Agency’s Automated Transfer Vehicle-3 (ATV-3) is seen on approach for docking. The unmanned cargo spacecraft docked to the space station at 6:31 p.m. EDT on March 28, 2012. The ATV-3 delivered 220 pounds of oxygen, 628 pounds of water, 4.5 tons of propellant and nearly 2.5 tons of dry cargo. Among other items, the station crew received experiment hardware, spare parts, food and clothing. The six-member Expedition 30 crew adjusted its sleep schedule to accommodate the ATV-3 docking. The crew stayed up late to monitor the approach and docking. Image Credit: NASA

ISF VIEWS NORTH WESTERN EUROPE BENEATH THE AURORA BOREALIS

Flying at an altitude of about 240 miles over the eastern North Atlantic, the Expedition 30 crew aboard the International Space Station photographed this nighttime scene. This view looks northeastward. Center point coordinates are 46.8 degrees north latitude and 14.3 degrees west longitude. The night lights of the cities of Ireland, in the foreground, and the United Kingdom, in the back and to the right, are contrasted by the bright sunrise in the background. The greens and purples of the Aurora Borealis are seen along the rest of the horizon. This image was taken on March 28, 2012. Image Credit: NASA

NASA OFFERS NEW VIEW OF ORION NEBULA

The photo and excerpt below are from the NASA website:
This new view of the Orion Nebula highlights fledgling stars hidden in the gas and clouds. It shows infrared observations taken by NASA's Spitzer Space Telescope and the European Space Agency's Herschel mission, in which NASA plays an important role. Stars form as clumps of this gas and dust collapses, creating warm globs of material fed by an encircling disk. These dusty envelopes glow brightest at longer wavelengths, appearing as red dots in this image. In several hundred thousand years, some of the forming stars will accrete enough material to trigger nuclear fusion at their cores and then blaze into stardom. Spitzer is designed to see shorter infrared wavelengths than Herschel. By combining their observations, astronomers get a more complete picture of star formation. The colors in this image relate to the different wavelengths of light, and to the temperature of material, mostly dust, in this region of Orion. Data from Spitzer show warmer objects in blue, with progressively cooler dust appearing green and red in the Herschel datasets. The more evolved, hotter embryonic stars thus appear in blue. Infrared data at wavelengths of 8.0 and 24 microns from Spitzer are rendered in blue. Herschel data with wavelengths of 70 and 160 microns are represented in green and red, respectively. This image was released on Feb. 29, 2012. Image Credit: NASA/ESA/JPL-Caltech/IRAM

SPITZER SPACE TELESCOPE SHOWS STAR WITH TWO GAS JETS

“NASA's Spitzer Space Telescope took this image of a baby star sprouting two identical jets (green lines emanating from fuzzy star). The jet on the right had been seen before in visible-light views, but the jet at left -- the identical twin to the first jet -- could only be seen in detail with Spitzer's infrared detectors. The left jet was hidden behind a dark cloud, which Spitzer can see through. The twin jets, in a system called Herbig-Haro 34, are made of identical knots of gas and dust, ejected one after another from the area around the star. By studying the spacing of these knots, and knowing the speed of the jets from previous studies, astronomers were able to determine that the jet to the right of the star punches its material out 4.5 years later than the counter-jet. The new data also reveal that the area from which the jets originate is contained within a sphere around the star, with a radius of 3 astronomical units. An astronomical unit is the distance between Earth and the sun. Previous studies estimated that the maximum size of this jet-making zone was 10 times larger. The wispy material is gas and dust. Arc-shaped bow shocks can be seen at the ends of the twin jets. The shocks consist of compressed material in front of the jets. The Herbig-Haro 34 jets are located at approximately 1,400 light-years away in the Orion constellation. Image Credit: NASA/JPL-Caltech “

The above picture and excerpt are from the NASA website: