2002-2003 Colloquium Series


NAU Physical Sciences (Bldg 19, Rm 321), Friday, 17 January 2003, 4:00 PM
(Refreshments at 3:45 PM)

ASTROBIOLOGY GOLLOQUIUM
Impact Craters as Indicators of Water on Mars

Nadine Barlow , Northern Arizona University

Abstract

Fresh Martian impact craters display a distinctive ejecta morphology, which is believed to result from heating and vaporization of subsurface volatiles during crater formation. Different types of ejecta morphologies may provide clues to target characteristics, such as layered materials and the physical state of the volatiles (ice versus liquid). Our team has recently completed an analysis of the regional variations in the different types of ejecta morphologies. Ejecta morphologies believed to result from impact into ice-rich target material are found globally on Mars. However, those morphologies believed to be due to impact into layered targets or to excavation into liquid-rich reservoirs are concentrated in specific regions of the planet which show interesting correlations with the recent detection of near-surface ice from the Mars Odyssey mission's Gamma Ray Spectrometer.
 

Biography

Dr. Nadine Barlow is an Assistant Professor in the Department of Physics and Astronomy at Northern Arizona University. She received her PhD in Planetary Sciences from the University of Arizona. Prior to coming to NAU, she worked at the Lunar and Planetary Institute and NASA Johnson Space Center (both in Houston, TX) and at the University of Central Florida in Orlando where she developed the astronomy program and served as director of the UCF Robinson Observatory. Her research interests include the evolution of the impact record over the age of the solar system, the geologic evolution of solid surfaced bodies, and the determination of surface properties on other worlds. Her current research focuses on the use of Martian impact craters to determine the distribution of subsurface volatile reservoirs. She also is a member of the team proposing the Gusev impact crater as a landing site for the 2003 Mars Exploration Rovers.
 


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