Mapex

This is a composite image of NGC 1068, one of the nearest and brightest galaxies containing a rapidly growing supermassive black hole. The X-ray images and spectra obtained using Chandra’s High Energy Transmission Grating Spectrometer show that a strong wind is being driven away from the center of NGC 1068 at a rate of about a million miles per hour. This wind is likely generated as surrounding gas is accelerated and heated as it swirls toward the black hole. A portion of the gas is pulled into the black hole, but some of it is blown away. High energy X-rays produced by the gas near the black hole heat the ouflowing gas, causing it to glow at lower X-ray energies. X-ray data from the Chandra X-ray Observatory are shown in red, optical data from the Hubble Space Telescope in green and radio data from the Very Large Array in blue. The spiral structure of NGC 1068 is shown by the X-ray and optical data, and a jet powered by the central supermassive black hole is shown by the radio data. This Chandra study is much deeper than previous X-ray observations. Using this data, researchers believe that each year several times the mass of our sun is being deposited out to large distances, about 3,000 light years from the black hole. The wind likely carries enough energy to heat the surrounding gas and suppress extra star formation. These results help explain how a supermassive black hole can alter the evolution of its host galaxy. It has long been suspected that material blown away from a black hole can affect its environment, but a key question has been whether such “black hole blowback” typically delivers enough power to have a significant impact. NGC 1068 is located about 50 million light years from Earth and contains a supermassive black hole about twice as massive as the one in the middle of the Milky Way Galaxy. Image Credit: X-ray (NASA/CXC/ MIT/C.Canizares, D.Evans et al), Optical (NASA/STScI), Radio (NSF/ NRAO/VLA)

The latest Geostationary Operational Environmental Satellite, or GOES-P, lifted off Thursday aboard a Delta IV rocket at 6:17 p.m. EST from Space Launch Complex 37 at the Cape Canaveral Air Force Station, Fla.

NASA will highlight the educational activities planned on the next space shuttle mission during a news briefing at 12 p.m. CDT, Tuesday, March 9.

For the past 12 years, ESA’s Eduspace website has been a window on the world for secondary students and teachers. Now the website has been completely redesigned and updated, so that it provides an even more valuable introduction to Earth observation and its applications.

An oblong iceberg roughly as big as Rhode Island called B-09B (center right in this image) collided with the edge of the Mertz Glacier in eastern Antarctica this month breaking away a new iceberg (top left) that is nearly as large at B-09B. This image from Feb. 20, 2010, is one of a series of images from NASA’s Aqua satellite that showed the progression and aftermath of the collision. The floating ice tongue of the glacier is created as ice flows down from Antarctica and onto the water. Glacier tongues grow longer year by year until they eventually break off, calving a new iceberg. Image Credit: NASA

NASA, in cooperation with local technology firms and sponsors, launches a nationwide series of high school robotics competitions that begin March 5 and 6 at the Walter E. Washington Convention Center, 801 Mount Vernon Place N.W., in Washington.

Mars Express encountered Phobos last night, smoothly skimming past at just 67 km, the closest any manmade object has ever approached Mars’ enigmatic moon. The data collected could help unlock the origin of not just Phobos but other ‘second generation’ moons.