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Chemistry in the Outer Solar System

Published online by Cambridge University Press:  25 May 2016

Tobias C. Owen ,
Paul Mahaffy ,
H. B. Niemann ,
S. K. Atreya ,
T. M. Donahue ,
A. Bar-Nun  and
I. de Pater
Tobias C. Owen
Affiliation:
Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA
Paul Mahaffy
Affiliation:
Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
H. B. Niemann
Affiliation:
Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
S. K. Atreya
Affiliation:
Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan 48109, USA
T. M. Donahue
Affiliation:
Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, Michigan 48109, USA
A. Bar-Nun
Affiliation:
Dept of Geophysics and Planetary Sciences, Tel-Aviv University, Ramat-Aviv, Israel
I. de Pater
Affiliation:
Department of Astronomy, U. of California, Berkeley, California 94720-3411, USA

Abstract

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The discovery by the Galileo Probe Mass Spectrometer that argon is enriched to the same extent as carbon and sulfur on Jupiter requires a revision of models for the formation of this giant planet. Evidently the excess heavy elements were carried to Jupiter in icy planetesimals that formed at temperatures ≤ 30 K. This result indicates that there is no original significance in the present position of Jupiter's orbit.

Type
Part 9. Outer Solar Nebula and Planetary Atmospheres
Information
Symposium - International Astronomical Union , Volume 197: Astrochemistry: From Molecular Clouds to Planetary Systems , 2000 , pp. 483 - 490
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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