Cometary Isotopic Measurements - Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse
Journal Articles Space Science Reviews Year : 2015

Cometary Isotopic Measurements

Myrtha Hässig
  • Function : Author
  • PersonId : 961649
Stefanie N Milam
Simon Sheridan

Abstract

Isotopic ratios in comets provide keys for the understanding of the origin of cometary material, and the physical and chemical conditions in the early Solar Nebula. We review here measurements acquired on the D/H, N-14/N-15, O-16/O-18, C-12/C-13, and S-32/S-34 ratios in cometary grains and gases, and discuss their cosmogonic implications. The review includes analyses of potential cometary material available in collections on Earth, recent measurements achieved with the Herschel Space Observatory, large optical telescopes, and Rosetta, as well as recent results obtained from models of chemical-dynamical deuterium fractionation in the early solar nebula. Prospects for future measurements are presented.
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Dates and versions

hal-03722557 , version 1 (17-11-2022)

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Dominique Bockelée-Morvan, Ursina Calmonte, Steven B Charnley, Jean Duprat, Cécile Engrand, et al.. Cometary Isotopic Measurements. Space Science Reviews, 2015, 197 (1-4), pp.47-83. ⟨10.1007/s11214-015-0156-9⟩. ⟨hal-03722557⟩
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