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|    BAMA    |    Science Research Echo    |    1,586 messages    |
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|    Message 217 of 1,586    |
|    Roger Nelson to All    |
|    Curiosity and the Solar Storm    |
|    14 Dec 11 16:17:11    |
      Curiosity and the Solar Storm               Dec. 14, 2011: On Nov. 26th, Curiosity blasted off from Cape Canaveral atop an       Atlas 5 rocket. Riding a plume of fire through the blue Florida sky, the       car-sized rover began a nine month journey to search for signs of life Mars.               Meanwhile, 93 million miles away, a second lesser-noticed Mars launch was       underway. Around the time that Curiosity's rocket was breaking the bonds of       Earth, a filament of magnetism erupted from the sun, hurling a billion-ton       cloud of plasma (a "CME") toward the Red Planet.               http://science.nasa.gov/media/medialibrary/2011/12/14/twolaunches_strip.jpg               The two Mars launches of Nov. 26, 2011. On the left, a solar explosion hurls a       CME toward the Red Planet (Credit: SOHO). On the right, the Mars Science Lab       or "Curiosity" lifts off from Cape Canaveral. (Credit: Howard Eskildsen of       Titusville, FL)       There was no danger of a collision-Mars rover vs. solar storm. Racing forward       at 2 million mph, the plasma cloud outpaced Curiosity's rocket by a wide       margin.               Next time could be different, however. With solar activity on the upswing       (Solar Max is expected in 2012-2013) it's only a matter of time before a CME       engulfs the Mars-bound rover.               That suits some researchers just fine. As Don Hassler of the Southwest       Research Institute (SWRI) in Boulder, Colorado, explains, "We look forward to       such encounters because Curiosity is equipped to study solar storms."               Hassler is the principal investigator for Curiosity's Radiation Assessment       Detector--"RAD" for short. The instrument, developed at SWRI and Christian       Albrechts University in Kiel, Germany, counts cosmic rays, neutrons, protons       and other particles over a wide range of energies. Tucked into the left front       corner of the rover, RAD is about the size of a coffee can and weighs only       three pounds, but has capabilities of Earth-bound instruments nearly 10 times       its size.               Encounters with CMEs pose little danger to Curiosity. By the time a CME       reaches the Earth-Mars expanse, it is spread so thin that it cannot truly       buffet the spacecraft. Nevertheless, RAD can sense what happens as the CME       passes by.               "RAD will be able to detect energetic particles accelerated by shock waves in       some CMEs1," says Arik Posner of NASA's Heliophysics Division in Washington       DC. "This could give us new insights into the inner physics of these giant       clouds."               There's more to this, however, than pure heliophysics. Future human       astronauts will directly benefit from RAD's measurements during the cruise       phase.               http://msl-scicorner.jpl.nasa.gov/Instruments/RAD/               A photo of the Radiation Assessment Detector (RAD) in the laboratory. [more]       "Curiosity is nestled inside its spacecraft, just like a real astronaut would       be," notes Frank Cucinotta, Chief Scientist for NASA's Space Radiation Program       at the Johnson Space Center. "RAD will give us an idea of the kind of       radiation a human can expect to absorb during a similar trip to Mars."               Of particular interest are secondary particles. Galactic cosmic rays and       solar energetic particles hit the walls of the spacecraft, creating an inward       spray of even more biologically dangerous neutrons and atomic nuclei. RAD       will analyze the spray from the only realistic place to make such       measurements-inside the spaceship.               In this way, "RAD is a bridge between the science and exploration sides of       NASA," says Hassler. "The two objectives are equally exciting."               RAD was activated on Dec. 6th. Of the rover's ten science instruments, it will       be the only one active during the cruise to Mars. Daily transmissions to       Earth will let Hassler and colleagues monitor what's going on "out there."        "We're very excited about the possibility of more solar storms," he adds.               As important as RAD's cruise phase measurements are, the instrument's primary       mission doesn't really begin until it lands on the Red Planet.               Mars has a very thin atmosphere and no global magnetic field to protect it       from space radiation. Energetic particles reaching ground level might be       dangerous to life--both future human astronauts and extant Martian microbes.       RAD will find out how much shielding human explorers need on the surface of       Mars. RAD will also help researchers estimate how far below ground a microbe       might have to go to reach a radiation "safe zone."               Solar storms are just for starters. Stay tuned to Science@NASA for the second       installment of this story: Curiosity and the Habitability Mars.                       Author:Dr. Tony Phillips| Production editor: Dr. Tony Phillips | Credit:       Science@NASA               More Information       Footnote:1Posner notes that only the most powerful CMEs will still be       accelerating particles when they are as far from sun as Curiosity will be. For       a typical CME, the main thing RAD will detect is the modulation of galactic       cosmic rays passing through the CME. Cosmic ray modulation could reveal new       information about the interior structure of these storm clouds.               Mars-Bound Rover Begins Research in Space -- NASA press release               Mars Science Lab (a.k.a. "Curiosity") -- home page               The Strange Attraction of Gale Crater -- Science@NASA               A Mars Rover Named Curiosity -- Science@NASA               Curiosity Takes Off -- Science@NASA               Credits: The Mars Science Lab mission is managed by JPL, a division of the       California Institute of Technology in Pasadena, for NASA's Science Mission       Directorate in Washington. The rover was designed, developed and assembled at       JPL. NASA's Launch Services Program at the Kennedy Space Center in Florida       managed the launch. NASA's Space Network provided space communication services       for the launch vehicle. NASA's Deep Space Network will provide spacecraft       acquisition and mission communication.                       Regards,               Roger              --- D'Bridge 3.64        * Origin: NCS BBS (1:3828/7)    |
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