The International Space Station. Credit: NASA

Sunday, September 30, 2012

VIEW OF A QUASAR


 
Quasar Drenched in Water Vapor
FROM: NASA/JPL

This artist's concept illustrates a quasar, or feeding black hole, similar to APM 08279+5255, where astronomers discovered huge amounts of water vapor. Gas and dust likely form a torus around the central black hole, with clouds of charged gas above and below. X-rays emerge from the very central region, while thermal infrared radiation is emitted by dust throughout most of the torus. While this figure shows the quasar's torus approximately edge-on, the torus around APM 08279+5255 is likely positioned face-on from our point of view.


Sunday, September 23, 2012

HYDRATED MINERALS ON VESTA


Capturing the Surface of Asteroid Vesta

This full view of the giant asteroid Vesta was taken by NASA's Dawn spacecraft, as part of a rotation characterization sequence on July 24, 2011, at a distance of 3,200 miles (5,200 kilometers). A rotation characterization sequence helps the scientists and engineers by giving an initial overview of the character of the surface as Vesta rotated underneath the spacecraft. This view of Vesta shows impact craters of various sizes and grooves parallel to the equator. The resolution of this image is about 500 meters per pixel.

Image credit: NASA/JPL-Caltech/UCLA/MPS/DLR/IDA


FROM: NASA

Dawn Spacecraft Sees Hydrated Minerals on Giant Asteroid

WASHINGTON -- NASA's Dawn spacecraft has revealed the giant asteroid Vesta has its own version of ring around the collar. Two new papers, based on observations from the low-altitude mapping orbit of the Dawn mission, show volatile, or easily evaporated, materials have colored Vesta's surface in a broad swath around its equator.

The volatiles were released from minerals likely containing water. Pothole-like features mark some of the asteroid's surface where the volatiles boiled off. Dawn did not find actual water ice at Vesta. However, it found evidence of hydrated minerals delivered by meteorites and dust in the giant asteroid's chemistry and geology. The findings appear Thursday in the journal Science.

One paper, led by Thomas Prettyman, the lead scientist for Dawn's gamma ray and neutron detector (GRaND) at the Planetary Science Institute in Tucson, Ariz., describes how the instrument found signatures of hydrogen, likely in the form of hydroxyl or water bound to minerals in Vesta's surface.

"The source of the hydrogen within Vesta's surface appears to be hydrated minerals delivered by carbon-rich space rocks that collided with Vesta at speeds slow enough to preserve their volatile content," said Prettyman.

A complementary paper, led by Brett Denevi, a Dawn participating scientist at the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., describes the presence of pitted terrain created by the release of the volatiles.

Vesta is the second most massive member of our solar system's main asteroid belt. Dawn was orbiting at an average altitude of about 130 miles (210 kilometers) above the surface when it obtained the data. Dawn left Vesta on Sept. 5 EDT (Sept. 4) and is on its way to a second target, the dwarf planet Ceres.

Scientists thought it might be possible for water ice to survive near the surface around the giant asteroid's poles. Unlike Earth's moon, however, Vesta has no permanently shadowed polar regions where ice might survive. The strongest signature for hydrogen in the latest data came from regions near the equator, where water ice is not stable.

In some cases, space rocks crashed into these deposits at high speed. The heat from the collisions converted the hydrogen bound to the minerals into water, which evaporated. Escaping water left holes as much as six-tenths of a mile (1 kilometer) wide and as deep as 700 feet (200 meters). Seen in images from Dawn's framing camera, this pitted terrain is best preserved in sections of Marcia crater.

"The pits look just like features seen on Mars, and while water was common on Mars, it was totally unexpected on Vesta in these high abundances," said Denevi. "These results provide evidence that not only were hydrated materials present, but they played an important role in shaping the asteroid's geology and the surface we see today."

GRaND's data are the first direct measurements describing the elemental composition of Vesta's surface. Dawn's elemental investigation by the instrument determined the ratios of iron to oxygen and iron to silicon in the surface materials. The new findings solidly confirm the connection between Vesta and a class of meteorites found on Earth called the Howardite, Eucrite and Diogenite meteorites, which have the same ratios for these elements. In addition, more volatile-rich fragments of other objects have been identified in these meteorites, which supports the idea the volatile-rich material was deposited on Vesta.

The Dawn mission is managed by NASA's Jet Propulsion Laboratory for the Science Mission Directorate in Washington. The spacecraft is as a project of the Discovery Program managed by NASA's Marshall Space Flight Center in Huntsville, Ala. The University of California, Los Angeles, is responsible for overall mission science. Orbital Sciences Corporation of Dulles, Va., designed and built the spacecraft.

The framing cameras that saw the pitted terrain were developed and built under the leadership of the Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, with contributions by the German Aerospace Center (DLR) Institute of Planetary Research, Berlin, and in coordination with the Institute of Computer and Communication Network Engineering, Braunschweig. The framing camera project is funded by NASA, the Max Planck Society and DLR. The gamma ray and neutron detector instrument was built by Los Alamos National Laboratory, N.M., and is operated by the Planetary Science Institute.

Sunday, September 16, 2012

THE DRY ICE OF MARS

Photo:  Mars South Pole.  Credit:  NASA.
FROM: NASA
NASA Orbiter Observations Point to 'Dry Ice' Snowfall on Mars

PASADENA, Calif. -- NASA's Mars Reconnaissance Orbiter (MRO) data have given scientists the clearest evidence yet of carbon dioxide snowfalls on Mars. This reveals the only known example of carbon dioxide snow falling anywhere in our solar system.

Frozen carbon dioxide, better known as "dry ice," requires temperatures of about minus 193 degrees Fahrenheit (minus 125 Celsius), which is much colder than needed for freezing water. Carbon dioxide snow reminds scientists that although some parts of Mars may look quite Earth-like, the Red Planet is very different. The report is being published in the Journal of Geophysical Research.

"These are the first definitive detections of carbon dioxide snow clouds," said the report's lead author Paul Hayne of NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif. "We firmly establish the clouds are composed of carbon dioxide -- flakes of Martian air -- and they are thick enough to result in snowfall accumulation at the surface."

The snow falls occurred from clouds around the Red Planet's south pole in winter. The presence of carbon dioxide ice in Mars' seasonal and residual southern polar caps has been known for decades. Also, NASA's Phoenix Lander mission in 2008 observed falling water-ice snow on northern Mars.

Hayne and six co-authors analyzed data gained by looking at clouds straight overhead and sideways with the Mars Climate Sounder, one of six instruments on MRO. This instrument records brightness in nine wavebands of visible and infrared light as a way to examine particles and gases in the Martian atmosphere.

The data provide information about temperatures, particle sizes and their concentrations. The new analysis is based on data from observations in the south polar region during southern Mars winter in 2006-2007, identifying a tall carbon dioxide cloud about 300 miles (500 kilometers) in diameter persisting over the pole and smaller, shorter-lived, lower-altitude carbon dioxide ice clouds at latitudes from 70 to 80 degrees south.

"One line of evidence for snow is that the carbon dioxide ice particles in the clouds are large enough to fall to the ground during the lifespan of the clouds," co-author David Kass of JPL said. "Another comes from observations when the instrument is pointed toward the horizon, instead of down at the surface. The infrared spectra signature of the clouds viewed from this angle is clearly carbon dioxide ice particles and they extend to the surface. By observing this way, the Mars Climate Sounder is able to distinguish the particles in the atmosphere from the dry ice on the surface."

Mars' south polar residual ice cap is the only place on Mars where frozen carbon dioxide persists on the surface year-round. Just how the carbon dioxide from Mars' atmosphere gets deposited has been in question. It is unclear whether it occurs as snow or by freezing out at ground level as frost. These results show snowfall is especially vigorous on top of the residual cap.

"The finding of snowfall could mean that the type of deposition -- snow or frost -- is somehow linked to the year-to-year preservation of the residual cap," Hayne said.

JPL provided the Mars Climate Sounder instrument and manages the MRO Project for NASA's Science Mission Directorate in Washington.

Thursday, September 13, 2012

ESA Portal - Spain - Oportunidad para colegios españoles: ampliado el plazo de inscripción para la competición europea de robótica

ESA Portal - Spain - Oportunidad para colegios españoles: ampliado el plazo de inscripción para la competición europea de robótica


RADIATION BELT STORM PROBES


Sunday, September 9, 2012

THE SONG OF MARS

PHOTO: GAIL CRATER ON MARS. CREDIT: NASA/ JPL/ CALTECH
 
FROM: NASA

Curiosity Rover Plays First Song Transmitted From Another Planet

PASADENA -- For the first time in history, a recorded song has been beamed back to Earth from another planet. Students, special guests and news media gathered at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., today to hear "Reach for the Stars" by musician will.i.am after it was transmitted from the surface of Mars by the Curiosity rover.

NASA Administrator Charles Bolden addressed the crowd in a video message encouraging students to study science, technology, engineering and math (STEM). "Mars has always fascinated us, and the things Curiosity tells us about it will help us learn about whether or not life was possible there," Bolden said. "And what future human explorers can expect. will.i.am has provided the first song on our playlist of Mars exploration."

In opening remarks, NASA Associate Administrator for Education and space shuttle astronaut Leland Melvin said, "I can think of no greater way to honor NASA pioneer Neil Armstrong's life and legacy than to inspire today's students to follow his path. That first footprint that Neil placed on the lunar surface left an indelible mark in history. Perhaps one of our students here today or watching on NASA Television will be the first to set foot on the surface of Mars and continue humanity's quest to explore."

Musician and entrepreneur will.i.am shared his thoughts about "Reach for the Stars" becoming the first interplanetary song and an anthem for NASA education. The entertainer is a well-known advocate of science and technology education. He said, "Today is about inspiring young people to lead a life without limits placed on their potential and to pursue collaboration between humanity and technology through STEAM education. I know my purpose is to inspire young people, because they will keep inspiring me back."

After completing a journey of more than 300 million miles from Earth to Mars and back, the opening orchestral strains of "Reach for the Stars" filled the auditorium. The event added to continuing worldwide interest in Curiosity's mission.

NASA engineers spoke to attendees about the Curiosity mission, and the systems engineering and orbital mechanics involved in getting the song file back from Mars. Students had the opportunity to ask questions of all program participants. Earlier in the day, students received a guided tour of JPL to view rover models and learn about STEM career options.

During the event, will.i.am's i.am angel Foundation and Discovery Education announced a $10 million classroom education initiative that will reach 25 million students annually, including many from underserved communities. Focused on STEAM (science, technology, engineering, arts and mathematics) educational themes, the Discovery Education initiative will incorporate NASA content and space exploration themes as part of the curriculum.

Sunday, September 2, 2012