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Solar System - Interstellar Medium: A Chemical Memory of the Origins

Published online by Cambridge University Press:  07 August 2017

D. Despois
D. Despois*
Affiliation:
Observatoire de Bordeaux, B.P. 89, 33210 Floirac, France

Abstract

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The growing body of data on solar system objects and interstellar space provides us with new tests of the connection between the two. We emphasize here the role played by the study of comets through the properties of the dust, the chemical composition of volatiles and the elemental abundances. These data inform us on cometary matter formation, and hence on conditions in the protosolar nebula. Under the adopted scenario of formation in a cold environment, with little further processing, cometary abundances are even new constraints to interstellar (gas and solid phase) abundances. Several points specific to the chemical modelling of the collapsing cloud and of the protosolar nebula are listed.

Type
Solar System
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 451 - 458
Copyright
Copyright © Kluwer 1992 

References

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