Mapex

Archive for August, 2010

ESA PR 2010-19 Media representatives are cordially invited to a briefing on the occasion of ten years of scientific discoveries by ESA’s Cluster mission.

This image from the Lunar Reconnaissance Orbiter shows the floor of the moon’s Anaxagoras crater, including a portion of the crater’s anorthositic central uplift. The boulders perched on ridges are eroding out of densely fractured bedrock. This image was taken by the Lunar Reconnaissance Orbiter Camera, or LROC, which consists of a pair of narrow-angle cameras and a single wide-angle camera. The mission is expected to return over 70 terabytes of image data. Image Credit: NASA/GSFC/Arizona State University

NASA and Alliant Techsystems Inc. (ATK) will conduct a full-scale test of a five-segment, first-stage solid rocket motor at 11:05 a.m. EDT, Tuesday, Aug. 31.

Two extremely bright stars illuminate a greenish mist in this image from the Spitzer Space Telescope’s “GLIMPSE360″ survey. This mist is comprised of hydrogen and carbon compounds called polycyclic aromatic hydrocarbons (PAHs), which also are found here on Earth in sooty vehicle exhaust and on charred grills. In space, PAHs form in the dark clouds that give rise to stars. These molecules provide astronomers a way to visualize the peripheries of gas clouds and study their structures in great detail. They are not actually green; but are color coded in these images to allow scientists see their glow in infrared. This image is a combination of data from Spitzer and the Two-Micron All-Sky Survey (2MASS). The Spitzer data was taken after Spitzer’s liquid coolant ran dry in May 2009, marking the beginning of its “warm” mission. Image Credit: NASA/JPL-Caltech/2MASS/SSI/University of Wisconsin

High school students from different ESA Member States were able to watch their own ‘satellites’ soar into the sky aboard suborbital rockets during the first European CanSat competition, held at the Andøya Rocket Range in Norway.

As part of their training, ESA’s new astronauts experience ‘parabolic flight’, creating weightless conditions to simulate working in space, featured on the cover and inside the ESA Bulletin. Read the Bulletin and other publications online, with our visualiser tool.

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This image shows the eruption of a galactic ?super-volcano? in the massive galaxy M87, as witnessed by NASA’s Chandra X-ray Observatory and NSF’s Very Large Array (VLA). At a distance of about 50 million light years, M87 is relatively close to Earth and lies at the center of the Virgo cluster, which contains thousands of galaxies. The cluster surrounding M87 is filled with hot gas glowing in X-ray light (and shown in blue) that is detected by Chandra. As this gas cools, it can fall toward the galaxy’s center where it should continue to cool even faster and form new stars. However, radio observations with the VLA (red) suggest that in M87 jets of very energetic particles produced by the black hole interrupt this process. These jets lift up the relatively cool gas near the center of the galaxy and produce shock waves in the galaxy’s atmosphere because of their supersonic speed. The interaction of this cosmic ?eruption? with the galaxy’s environment is very similar to that of the Eyjafjallajokull volcano in Iceland that occurred in 2010. With Eyjafjallajokull, pockets of hot gas blasted through the surface of the lava, generating shock waves that can be seen passing through the grey smoke of the volcano. This hot gas then rises up in the atmosphere, dragging the dark ash with it. This process can be seen in a movie of the Eyjafjallajokull volcano where the shock waves propagating in the smoke are followed by the rise of dark ash clouds into the atmosphere. In the analogy with Eyjafjallajokull, the energetic particles produced in the vicinity of the black hole rise through the X-ray emitting atmosphere of the cluster, lifting up the coolest gas near the center of M87 in their wake. This is similar to the hot volcanic gases drag up the clouds of dark ash. And just like the volcano here on Earth, shockwaves can be seen when the black hole pumps energetic particles into the cluster gas. Image Credits: X-ray: NASA/CXC/KIPAC/N. Werner et al Radio: NSF/NRAO/AUI/W. Cotton

If you like music, the space program and are a little nostalgic, NASA has the perfect opportunity for you.

Making the stuff of science fiction into reality, NASA engineers are testing solar sails–a unique propulsion technology that one day could enable deep space missions. Much like the wind pushing a sailboat through water, solar sails rely on sunlight to propel vehicles through space. The sail captures constantly streaming solar particles, called photons, with giant sails built from a lightweight material. Over time, the buildup of these particles provides enough thrust for a small spacecraft to travel in space. This image is of a four-quadrant solar sail system, measuring 66 feet on each side that is being tested in the world’s largest vacuum chamber at NASA’s Glenn Research Center at Plum Brook Station in Sandusky, Ohio. Image Credit: NASA

Global plant productivity that once was on the rise with warming temperatures and a lengthened growing season is now on the decline because of regional drought according to a new study of NASA satellite data.