Earth, Moon, and Planets

, Volume 105, Issue 2–4, pp 167–180 | Cite as

Isotopic Ratios in Comets: Status and Perspectives

  • E. Jehin
  • J. Manfroid
  • D. Hutsemékers
  • C. Arpigny
  • J.-M. Zucconi
Article

Abstract

Isotopic abundance ratios are excellently suited to probe the origin of solar system matter. We review the recent measurements of the isotopic ratios of the light elements (D/H, 12C/13C, 16O/18O, 14N/15N, 32S/34S) in cometary dust and gas and discuss briefly their implications. Special emphasis will be put on the determinations and progress performed in the field over the past years thanks to high resolution spectroscopy of cometary comae obtained with the ESO Very Large Telescope. Future perspectives from space missions and ground-based observations with new large and extremely large telescopes operating in the optical, infrared and submillimeter wavelengths will be presented.

Keywords

Comets Abundances Isotopic ratios Light elements Large telescopes 

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Copyright information

© Springer Science+Business Media B.V. 2009

Authors and Affiliations

  • E. Jehin
    • 1
  • J. Manfroid
    • 1
  • D. Hutsemékers
    • 1
  • C. Arpigny
    • 1
  • J.-M. Zucconi
    • 2
  1. 1.Institut d’Astrophysique et de Géophysique de l’Université de LiègeLiègeBelgium
  2. 2.Observatoire de BesançonBesanconFrance

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