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The Noble Gas Abundances in the Coma of Comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA

Abstract : The Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA), the mass spectrometer suite on board the European Space Agency’s Rosetta mission, was dedicated to the measurement of the volatiles in the coma of comet 67P/Churyumov-Gerasimenko (67P) [1]. Among many other species, ROSINA DFMS, the Double Focusing Mass Spectrometer, detected and quantified the three noble gases argon, krypton, and xenon including their major isotopes [2,3]. Noble gases provide important clues to the physical and chemical conditions during and possibly even before and after the comet’s formation in the early solar system. Furthermore, measurements of the isotope ratios provide constraints on the amount of cometary material brought to Earth and its early atmosphere. In this presentation, we will report on the measured coma densities and derived nucleus bulk abundances of these three noble gases and investigate correlations with other volatiles. Furthermore, we will discuss the measured isotope ratios and the implications of these results.
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Submitted on : Friday, January 5, 2018 - 6:58:42 PM
Last modification on : Thursday, February 25, 2021 - 9:46:09 AM


  • HAL Id : insu-01676642, version 1


Martin Rubin, Kathrin Altwegg, Hans R. Balsiger, Jean-Jacques Berthelier, Christelle Briois, et al.. The Noble Gas Abundances in the Coma of Comet 67P/Churyumov-Gerasimenko from Rosetta/ROSINA. AGU 2017 Fall Meeting, Dec 2017, New Orleans, United States. ⟨insu-01676642⟩



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