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| | Genesis Web Science Document A: Isotopic Composition of the Solar System |
 | | In natural terrestrial and lunar matter, isotopic abundance variations arise from (a) radioactivity, (b) isotopic fractionation accompanying physical or chemical processes (evaporation, diffusion, precipitation, etc.), and (c) nuclear reactions (galactic cosmic rays, or to a lesser extent, solar flare ions for lunar samples). |
 | | Knowledge of the initial elemental and isotopic abundances of volatile species is imperative for identifying evolutionary mechanisms that might have acted, whether the modeling is forward, from presumed compositions in primordial atmospheres, or backward from known compositions in contemporary atmospheres. |
 | | Podosek F.A., Huneke J.C., Burnett D.S., and Wasserburg G.J. (1971) Isotopic composition of Xe and Kr in the lunar soil and solar wind. |
| www.gps.caltech.edu /genesis/DocumentA.html (9405 words) |
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