BLACK HOLE BLAZARS AND THE RELEASE OF NEARLY LIGHT SPEED JETS

FROM:  NASA
WASHINGTON -- Astronomers are actively hunting a class of supermassive
black holes throughout the universe called blazars thanks to data
collected by NASA's Wide-field Infrared Survey Explorer (WISE). The
mission has revealed more than 200 blazars and has the potential to
find thousands more.

Blazars are among the most energetic objects in the universe. They
consist of supermassive black holes actively "feeding," or pulling
matter onto them, at the cores of giant galaxies. As the matter is
dragged toward the supermassive hole, some of the energy is released
in the form of jets traveling at nearly the speed of light. Blazars
are unique because their jets are pointed directly at us.

"Blazars are extremely rare because it's not too often that a
supermassive black hole's jet happens to point towards Earth," said
Franceso Massaro of the Kavli Institute for Particle Astrophysics and
Cosmology near Palo Alto, Calif., and principal investigator of the
research, published in a series of papers in the Astrophysical
Journal. "We came up with a crazy idea to use WISE's infrared
observations, which are typically associated with lower-energy
phenomena, to spot high-energy blazars, and it worked better than we
hoped."

The findings ultimately will help researchers understand the extreme
physics behind super-fast jets and the evolution of supermassive
black holes in the early universe.

WISE surveyed the entire celestial sky in infrared light in 2010,
creating a catalog of hundreds of millions of objects of all types.
Its first batch of data was released to the larger astronomy
community in April 2011 and the full-sky data were released last
month.

Massaro and his team used the first batch of data, covering more than
one-half the sky, to test their idea that WISE could identify
blazars. Astronomers often use infrared data to look for the weak
heat signatures of cooler objects. Blazars are not cool; they are
scorching hot and glow with the highest-energy type of light, called
gamma rays. However, they also give off a specific infrared signature
when particles in their jets are accelerated to almost the speed of
light.

One of the reasons the team wants to find new blazars is to help
identify mysterious spots in the sky sizzling with high-energy gamma
rays, many of which are suspected to be blazars. NASA's Fermi mission
has identified hundreds of these spots, but other telescopes are
needed to narrow in on the source of the gamma rays.

Sifting through the early WISE catalog, the astronomers looked for the
infrared signatures of blazars at the locations of more than 300
gamma-ray sources that remain mysterious. The researchers were able
to show that a little more than half of the sources are most likely
blazars.

"This is a significant step toward unveiling the mystery of the many
bright gamma-ray sources that are still of unknown origin," said
Raffaele D'Abrusco, a co-author of the papers from Harvard
Smithsonian Center for Astrophysics in Cambridge, Mass. "WISE's
infrared vision is actually helping us understand what's happening in
the gamma-ray sky."

The team also used WISE images to identify more than 50 additional
blazar candidates and observed more than 1,000 previously discovered
blazars. According to Massaro, the new technique, when applied
directly to WISE's full-sky catalog, has the potential to uncover
thousands more.

"We had no idea when we were building WISE that it would turn out to
yield a blazar gold mine," said Peter Eisenhardt, WISE project
scientist at NASA's Jet Propulsion Laboratory (JPL) in Pasadena,
Calif., who is not associated with the new studies. "That's the
beauty of an all-sky survey. You can explore the nature of just about
any phenomenon in the universe."  
                                                

                                                 Image of a Black Hole. Credit NASA 

JPL manages and operates WISE for NASA's Science Mission Directorate
in Washington. The principal investigator for WISE, Edward Wright, is
at UCLA. The mission was competitively selected under NASA's
Explorers Program, managed by the Goddard Space Flight Center in
Greenbelt, Md. The science instrument was built by the Space Dynamics
Laboratory in Logan, Utah, and the spacecraft was built by Ball

Aerospace & Technologies Corp. in Boulder, Colo. Science operations
and data processing and archiving take place at the Infrared
Processing and Analysis Center at the California Institute of
Technology (Caltech) in Pasadena. Caltech manages JPL for NASA.

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

Internet auf Mond, Mars und ISS

Internet auf Mond, Mars und ISS

ESA Portal - Czech Republic - Nečekané přerušení činnosti družice Envisat

ESA Portal - Czech Republic - Nečekané přerušení činnosti družice Envisat

SPACE SHUTTLE IMAX CAMERA ON DISPLAY AT SMITHSONIAN

FROM NASA
An IMAX camera that flew aboard a space shuttle is seen at the Moving Beyond Earth Gallery at the Smithsonian National Air and Space Museum, Wednesday, April 4, 2012, in Washington. This and another IMAX camera that flew in space became a part of the museum's collection. From 1984 to 1998 the 70mm cameras accompanied astronauts on 17 space shuttle missions offering stunning views of Earth from space and offered an up-close look at what it is like to live and work in a weightless environment. Image Credit: NASA/Paul E. Alers

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

T-38 ASTRONAUT TRAINING AIRCRAFT FLIES OVER THE CAPITAL

A NASA T-38 training jet is seen as it flies over Washington, DC, Thursday, April 5, 2012. NASA, in cooperation with the Federal Aviation Administration, conducted training and photographic flights over the DC metropolitan area. T-38 aircraft have been used for astronaut training for more than 30 years as they allow pilots and mission specialists to think quickly in changing situations, mental experiences the astronauts say are critical to practicing for the rigors of spaceflight. Image Credit: NASA/Carla Cioffi 

SOUTH POLE TELESCOPE HELPS EXPLAIN MYSTERIOUS DARK MATTER

FROM NATIONAL SCIENCE FOUNDATION
Credit: Daniel Luong-Van, National Science Foundation

NSF-funded 10-meter South Pole Telescope in Antarctica provides new support for the most widely accepted explanation of dark energy, the source of the mysterious force that is responsible for the accelerating expansion of the universe.

April 2, 2012
Analysis of data from the National Science Foundation- (NSF) funded 10-meter South Pole Telescope (SPT) in Antarctica provides new support for the most widely accepted explanation of dark energy, the source of the mysterious force that is responsible for the accelerating expansion of the universe.

The results begin to hone in on the tiny mass of the neutrinos, the most abundant particles in the universe, which until recently were thought to be without mass.
The SPT data strongly support Albert Einstein's cosmological constant--the leading model for dark energy--even though researchers base the analysis on only a fraction of the SPT data collected and only 100 of the over 500 galaxy clusters detected so far.
"With the full SPT data set we will be able to place extremely tight constraints on dark energy and possibly determine the mass of the neutrinos," said Bradford Benson, an NSF-funded postdoctoral scientist at the University of Chicago's Kavli Institute for Cosmological Physics.

Benson presented the SPT collaboration's latest findings, Sunday, April 1, at the American Physical Society meeting in Atlanta.

These most recent SPT findings are only the latest scientifically significant results produced by NSF-funded researchers using the telescope in the five years since it became active, noted Vladimir Papitashvili, Antarctic Astrophysics and Geospace Sciences program director in NSF's Office of Polar Programs.

"The South Pole Telescope has proven to be a crown jewel of astrophysical research carried out by NSF in the Antarctic," he said. "It has produced about two dozen peer-reviewed science publications since the telescope received its 'first light' on Feb. 17, 2007. SPT is a very focused, well-managed and amazing project."

The 280-ton SPT stands 75 feet tall and is the largest astronomical telescope ever built in the clear and dry air of Antarctica. Sited at NSF's Amundsen-Scott South Pole station at the geographic South Pole, it stands at an elevation of 9,300 feet on the polar plateau. Because of its location at the Earth's axis, it can conduct long-term observations.

NSF manages the U.S. Antarctic Program through which it coordinates all U.S. scientific research on the southernmost continent and aboard ships in the Southern Ocean as well as providing the necessary related logistics support.

An international research collaboration led by the University of Chicago manages the South Pole Telescope. The collaboration includes research groups at Argonne National Laboratory; Cardiff University in Wales; Case Western Reserve University; Harvard University; Ludwig-Maximilians-Universität in Germany; the Smithsonian Astrophysical Observatory; McGill University in Canada; the University of California, Berkeley; the University of California, Davis; the University of Colorado Boulder; and the University of Michigan, as well as individual scientists at several other institutions.

SPT specifically was designed to tackle the dark-energy mystery. The 10-meter telescope operates at millimeter wavelengths to make high-resolution images of Cosmic Microwave Background (CMB) radiation, the light left over from the big bang.

Scientists use the CMB to search for distant, massive galaxy clusters that can be used to pinpoint the properties of dark energy and also help define the mass of the neutrino.
"The CMB is literally an image of the universe when it was only 400,000 years old, from a time before the first planets, stars and galaxies formed in the universe," Benson said. "The CMB has travelled across the entire observable universe, for almost 14 billion years, and during its journey is imprinted with information regarding both the content and evolution of the universe."

The new SPT results are based on a new method that combines measurements taken by the telescope and by NASA and European Space Agency X-ray satellites, and extends these measurements to larger distances than previously achieved.

The most widely accepted property of dark energy is that it leads to a pervasive force acting everywhere and at all times in the universe. This force could be the manifestation of Einstein's cosmological constant that assigns energy to space, even when it is free of matter and radiation.

Einstein considered the cosmological constant to be one of his greatest blunders after learning that the universe is not static, but expanding.

In the late 1990s, astronomers discovered the universe's expansion appears to be accelerating according to cosmic distance measurements based on the relatively uniform luminosity of exploding stars. The finding was a surprise because gravity should have been slowing the expansion, which followed the big bang.

Einstein introduced the cosmological constant into his theory of general relativity to accommodate a stationary universe, the dominant idea of his day. But his constant fits nicely into the context of an accelerating universe, now supported by countless astronomical observations.

Others hypothesize that gravity could operate differently on the largest scales of the universe. In either case, the astronomical measurements point to new physics that have yet to be understood.

As the CMB passes through galaxy clusters, the clusters effectively leave "shadows" that allow astronomers to identify the most massive clusters in the universe, nearly independent of their distance.

"Clusters of galaxies are the most massive, rare objects in the universe, and therefore they can be effective probes to study physics on the largest scales of the universe," said John Carlstrom, the S. Chandrasekhar Distinguished Service Professor in Astronomy & Astrophysics, who heads the SPT collaboration.

"The unsurpassed sensitivity and resolution of the CMB maps produced with the South Pole Telescope provides the most detailed view of the young universe and allows us to find all the massive clusters in the distant universe," said Christian Reichardt, a postdoctoral researcher at the University of California, Berkeley and lead author of the new SPT cluster catalog paper.

The number of clusters that formed over the history of the universe is sensitive to the mass of the neutrinos and the influence of dark energy on the growth of cosmic structures.
"Neutrinos are amongst the most abundant particles in the universe," Benson said. "About one trillion neutrinos pass through us each second, though you would hardly notice them because they rarely interact with 'normal' matter."

The existence of neutrinos was proposed in 1930. They were first detected 25 years later, but their exact mass remains unknown. If they are too massive they would significantly affect the formation of galaxies and galaxy clusters, Benson said.

The SPT team has been able to improve estimates of neutrino masses, yielding a value that approaches predictions stemming from particle physics measurements.

"It is astounding how SPT measurements of the largest structures in the universe lead to new insights on the evasive neutrinos," said Lloyd Knox, professor of physics at the University of California at Davis and member of the SPT collaboration. Knox will also highlight the neutrino results in his presentation on Neutrinos in Cosmology at a special session of the APS on Tuesday, April 3.

NSF's Office of Polar Programs primarily funds the SPT. The NSF-funded Physics Frontier Center of the Kavli Institute for Cosmological Physics, the Kavli Foundation and the Gordon and Betty Moore Foundation provide partial support.

NASA ROBOTS SHOWCASED AT STANFORD UNIVERSITY'S 'ROBOT BLOCK PARTY'

MOFFETT FIELD, Calif. – Two cutting-edge NASA prototype robots will be
featured during a "Robot Block Party" at Stanford University,
Stanford, Calif. from 1 – 6 p.m. PDT, Wednesday, April 11, 2012. The
Center for Internet and Society at Stanford Law School is hosting the
free public event as part of the third annual National Robotics Week.

Robotic technology from the Intelligent Robotics Group (IRG) at NASA's
Ames Research Center, Moffett Field, Calif., will be on display,
including a volleyball-sized free-flying satellite, known as "Smart
SPHERES." Also featured will be a prototype robot based on a
dynamically-controlled "tensegrity structure" – a collection of rods
connected and suspended by tensioned cables – called "TenseBot."

The International Space Station currently houses three Synchronized
Position Hold, Engage, Reorient, Experimental Satellites (SPHERES)
equipped with a Nexus™ S Smartphone made by Samsung Electronics and
using Google’s Android™ platform. Later this year, the IRG will
remotely control the Smart SPHERES from the Mission Control Center at
NASA's Johnson Space Center, Houston. The test will simulate a mobile
inspection of the space station to see how well the free-flying
robots can collect data using the smartphone's camera and sensors.

The TenseBot will be used to explore how tensegrity structures, which
are typically built as architectural art exhibits, can be controlled
by computers. Researchers in the IRG are interested in tension-based
structures because they have great potential to save space, weight
and energy and can be used for a variety of tasks on NASA's future
space missions, including deploying antennas, aligning large payloads
and pointing solar arrays.

Other robotic technology on display at the Robot Block Party includes
robots that drive cars, climb walls, assemble delicate parts, and
help perform medical procedures.

The Robot Block Party will be held in the Volkswagen Automotive
Innovation Lab at 473 Oak Rd, off Stock Farm Rd, Stanford. Park in
Parking Structure 5, or adjacent lots.

National Robotics Week is organized by the Robotics Caucus of the U.S.
Congress and leading robotics companies, schools, and organizations.

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

VIEW OF DUBAI FROM THE INTERNATIONAL SPACE STATION

FROM:  NASA
City lights of Dubai, United Arab Emirates, are featured in this image taken by the Expedition 30 crew aboard the International Space Station. The City of Dubai--the largest metropolitan area within the emirate of Dubai--is a favorite subject of astronaut photography largely due to the unique artificial archipelagos situated directly offshore in the Persian Gulf, which were built such that their full design is only visible from the vantage point of an airplane -- or an orbiting spacecraft. The city presents an eye-catching appearance at night that vividly displays the urban development pattern. In this detailed image, taken with a long focal length lens and digital camera optimized for fast response and high light sensitivity, several interesting patterns can be observed. The highways and major streets are sharply defined by yellow-orange lighting, while the commercial and residential areas are resolved into a speckle pattern of individual white, blue and yellow-orange lights. Several large and brilliantly lit areas are large hotel and mall complexes, including the Burj Khalifa Tower, the world's tallest building at 2,717 feet, or 828 meters. The brilliant lighting of the city contrasts sharply with both the dark Persian Gulf to the northwest, and largely undeveloped and unlit areas to the southeast. Likewise, the clusters of lighting in the Palm Jumeira complex at bottom right correspond to the relatively small part of the archipelago that has been developed. Isolated areas of blurred city lights are due to patchy clouds. Image Credit: NASA

SPACESHIP OF STARS?

The NASA/ESA Hubble Space Telescope has spotted the "UFO Galaxy." NGC 2683 is a spiral galaxy seen almost edge-on, giving it the shape of a classic science fiction spaceship. This is why the astronomers at the Astronaut Memorial Planetarium and Observatory, Cocoa, Fla., gave it this attention-grabbing nickname. While a bird's eye view lets us see the detailed structure of a galaxy (such as this Hubble image of a barred spiral), a side-on view has its own perks. In particular, it gives astronomers a great opportunity to see the delicate dusty lanes of the spiral arms silhouetted against the golden haze of the galaxy’s core. In addition, brilliant clusters of young blue stars shine scattered throughout the disc, mapping the galaxy’s star-forming regions. Perhaps surprisingly, side-on views of galaxies like this one do not prevent astronomers from deducing their structures. Studies of the properties of the light coming from NGC 2683 suggest that this is a barred spiral galaxy, even though the angle we see it at does not let us see this directly. This image is produced from two adjacent fields observed in visible and infrared light by Hubble’s Advanced Camera for Surveys. A narrow strip which appears slightly blurred and crosses most the image horizontally is a result of a gap between Hubble’s detectors. This strip has been patched using images from observations of the galaxy made by ground-based telescopes, which show significantly less detail. The field of view is approximately 6.5 by 3.3 arcminutes. Image Credit: ESA/Hubble & NASA
The Photo and excerpt are from the NASA website:

NASA LOOKING TO FIND WASTE SOLUTIONS FOR SPACE TRAVELERS

The following excerpt is from the NASA website:
NASA, the U.S. Agency for International Development (USAID), the State 
Department and Nike today announced a challenge to identify 10 
game-changing innovations that could transform waste-management 
systems and practices. Waste management is important for planning 
long-duration human spaceflight missions to an asteroid, Mars or 
beyond. 

Humans living off the planet require waste solutions that mirror 
issues facing people on Earth. In the hostile environment of space, 
waste must be eliminated or transformed in the most efficient and 
cost-effective manner possible. The innovations, which will be 
presented at the LAUNCH: Beyond Waste forum, may lead to practical 
applications for astronauts as we send humans deeper into our solar 
system. 

The challenge will be open April 1-May 15 and will seek creative 
solutions to minimize waste or transform it into new products in 
space and on Earth. Forum partners will select 10 innovators to 
present their technology solutions at the LAUNCH: Beyond Waste forum, 
hosted by NASA July 20-22, at the agency's Jet Propulsion Laboratory 
in Pasadena, Calif. 

NASA and the LAUNCH Council -- thought leaders representing a diverse 
and collaborative body of entrepreneurs, scientists, engineers, 
government, media and business -- will participate in the forum and 
help guide these innovations forward. The selected LAUNCH innovators 
will receive networking and mentoring opportunities from influential 
business and government leaders, as well as portfolio presentations. 

Previous LAUNCH forums have focused on water, health and energy. These 
forums resulted in innovations, including technology that enables 
irrigation using brackish, saline and polluted water; a biodegradable 
needle that can deliver vaccines or medicine under the skin using a 
pressure device; a tiny holographic microscope attached to a cell 
phone that can detect parasites and bacteria in blood and water in 
remote locations; a handheld lab-in-a-box that diagnoses a variety of 
diseases in a matter of minutes; a modular, flexible smart-grid 
distribution technology to provide access to power for those in need; 
and a simple, affordable fuel cell that converts biomass directly to 
electricity. 

LAUNCH was created to identify, showcase and support innovative 
approaches to global sustainability challenges. LAUNCH searches for 
visionaries whose ideas, technologies or programs show great promise 
for making tangible impacts on society in the developed and 
developing worlds. 

ENDEAVOR'S OMS POD GETS A CLEANING

In Orbiter Processing Facility-2 at NASA's Kennedy Space Center in Florida, space shuttle Endeavour’s left orbital maneuvering system OMS pod is in position on the aft of the shuttle and ready for installation. The OMS pod underwent complete deservicing and cleaning at White Sands Space Harbor in New Mexico, part of the transition and retirement processing of each shuttle. Endeavour is being prepared for public display at the California Science Center in Los Angeles. Over the course of its 19-year career, Endeavour spent 299 days in space during 25 missions. Image credit: NASA/Dimitri Gerondidakis
The above photo and excerpt are from the NASA website: