Computer Science – Learning
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003trgeo...1...63b&link_type=abstract
Treatise on Geochemistry, Volume 1. Editor: Andrew M. Davis. Executive Editors: Heinrich D. Holland and Karl K. Turekian. pp. 71
Computer Science
Learning
Scientific paper
The solar nebula was the rotating, flattened disk of gas and dust from which the solar system originated ˜4.6 Gyr ago. Much of the motivation for cosmochemical studies of meteorites, comets, and other primitive bodies stems from the desire to use the results to constrain or otherwise illuminate the physical and chemical conditions in the solar nebula, in the hope of learning more about the processes that led to the formation of the planets. In addition to cosmochemical studies, there are important lessons to be learned about the planet formation process from astrophysical observations of young stellar objects and their accompanying protoplanetary disks, from the discovery of other planetary systems, and from theoretical models. A key resource for learning more about these subjects is the compendium volume (Mannings et al., 2000).
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