XXVII GENERAL ASSEMBLY

AUGUST 03 - 14, 2009 - Rio de Janeiro - Brazil



Water on Planets


James F. Bell III www.cornell.edu

Astronomy Department, Cornell University
Ithaca, NY, USA

August 6, 2009 - 18:00 hr


H2O is a ubiquitous molecule in the Cosmos, and of course is a critical ingredient in assessing the habitability of worlds and the biochemistry of any life forms on those worlds. As such, the origin, distribution, and evolution of water in our solar system, in other solar systems, and in other interstellar and galactic reservoirs is the topic of intense research and debate. Models of solar system formation can be used to predict the heliocentric distance beyond which primordial water could have condensed from the solar nebula as ice (the so-called "snow line") and thus have been available for accretion into planetesimals. However, such models do not factor in possible subsequent mixing of that water throughout the solar system via planetary migration or other complex interactions that can lead to impacts between icy and rocky bodies. Thus, simple explanations for the origin and inventory of water on particular planets compete for viability with chaotic, potentially ad hoc explanations. This talk will review the accumulated evidence, from telescopic and space mission observations, for the distribution of water on planets, satellites, asteroids, and comets in our solar system. While there is substantial data available on the distribution and abundance of water on planetary bodies from direct observations as well as laboratory and meteorite studies, significant mysteries remain unsolved. Where did Earth's water come from? How much water did/does Mars have? What happened to Venus' water? Is there ice in unlikely places like the poles of the Moon and Mercury and oceans in unlikely places like the interiors of outer solar system satellites? These kinds of mysteries continue to guide our search for water in our solar system, and beyond.



National Organizing Committee - NOC
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