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|    sci.space.science    |    Space and planetary science and related    |    1,217 messages    |
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|    Message 28 of 1,217    |
|    Ron Baalke to All    |
|    Sixth International Mars Conference will    |
|    14 Jul 03 18:06:25    |
      From: baalke@zagami.jpl.nasa.gov              Caltech News Release       For Immediate Release       July 14, 2003              Contact: Mark Wheeler        (626) 395-8733        wheel@caltech.edu              Sixth International Mars Conference will Include Public Event              PASADENA, Calif. - Next year, if all goes well, NASA's two Mars       rovers, Spirit and Opportunity, along with the British rover Beagle       2, will begin streaming back reams of data about the Red Planet, much       to the delight of Mars researchers everywhere.              That data won't be available in time for scientists attending the       Sixth International Conference on Mars at the California Institute of       Technology, July 20-25, but small matter. Data from two earlier       orbiter missions, the Mars Global Surveyor (MGS), launched in 1996,       and the Odyssey, launched in 2001, will give those attending the       conference an opportunity to review and debate some of the key       questions and controversies that have matured as a result of this       flood of information. "It's time for another review," says Arden       Albee, a professor of geology and planetary science, emeritus, at       Caltech. "Never before have scientists had such a comprehensive       record of the processes that operated on the surface of Mars and in       its atmosphere."              The conference will also include a free public event. On Wednesday       evening, July 23, the conference will sponsor "A Mars Picture       Gallery--Every Picture Tells a Story," from 8 to 10 p.m. in Caltech's       Beckman Auditorium. Featured will be Michael Malin, principal       investigator of MGS's Mars Orbiter Camera, and Philip Christensen,       principal investigator of Odyssey's THEMIS camera.              Malin, a 1976 Caltech graduate and an experienced planetary       geologist, is currently president and chief scientist of Malin Space       Science Systems, which operates the MGS camera. The camera has       returned more than 20,000 new images from Mars, showing the planet's       enigmatic features in great detail and tracking changes in its       atmosphere. Recently Malin has been able to obtain images at an       unprecedented resolution of 1.5 meters per pixel. This past spring,       Malin received a Caltech Distinguished Alumni Award for his work.              Christensen, a planetary geologist at Arizona State University, will       display recent images and results from the THEMIS (thermal emission       imaging system) camera, on the newest mission to Mars. "THEMIS       provides a unique new view of Mars in thermal infrared images that is       providing details on the physical properties of its surface, and the       processes that have acted over time," says Christensen. "These views       provide a broad perspective of Martian processes, and a context from       which to understand the history and evolution of the planet."              Both cameras, for example, have observed sites where water--and       therefore life--may have existed in ancient times.              The role of water and the possibility of life on Mars will attract       much attention at the sixth conference, says Albee, just as it did at       the earlier conferences. "Now we can focus questions in three       specific areas. The role of water in the climate of early Mars; the       current extent and location of water ice; and the tantalizing       evidence for the existence of very recent liquid water on its       surface."              Investigators using the new data argue that precipitation, either       rain or snow, and flowing water eroded the surface of Mars in its       first billion years despite the planet's frigid climate, says Albee.       Precise digital topography from MGS's laser altimeter now also makes       it possible to analytically compare valley networks on Earth and       Mars. "Unlike Earth," he says, "Mars has preserved much of its       ancient landscape, which may yield clues to the climatic conditions       under which it formed."              Instruments on Odyssey have mapped the presence of water ice in the       immediate subsurface of Mars and have shown that it is less abundant       toward the equator. Images show the presence of soil flowage and       other features found in permafrost regions on Earth.              The discovery of young gullies in photos of Mars has changed the       conception that it has been a dry and frigid planet in the recent       past, says Albee, noting that new theories abound. One suggests these       recent gullies were formed by debris flows that involved liquid water       of subsurface origin. Others have proposed flows driven by carbon       dioxide, while still others have proposed localized surface heating       under certain conditions.              The arguments over water are simply a sample of the many viewpoints       that will be argued during the conference, says Albee, including a       session on Tuesday afternoon entitled "Future Missions." In all, some       400 scientists from a number of countries are expected to attend.              --- SoupGate-Win32 v1.05        * Origin: you cannot sedate... all the things you hate (1:229/2)    |
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