Differences between the impact regimes of the terrestrial planets: implications for isotopic abundances

Horner, J. and Mousis, O. and Jones, B. W. (2008) Differences between the impact regimes of the terrestrial planets: implications for isotopic abundances. In: 39th Lunar and Planetary Science Conference (LPSC 2008), 10-14 Mar 2008, League City, TX. United States.

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Abstract

We provide results on the relative impact flux experienced by the planets Venus, Earth and Mars from populations of asteroids and comets, in the context of a discussion of the relative deuteration of the water reservoirs on each world.


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Item Type: Conference or Workshop Item (Commonwealth Reporting Category E) (Paper)
Refereed: No
Item Status: Live Archive
Additional Information: © 2008 Lunar and Planetary Institute. This publication is copyright. It may be reproduced in whole or in part for the purposes of study, research, or review, but is subject to the inclusion of an acknowledgment of the source.
Faculty / Department / School: Historic - Faculty of Engineering and Surveying - No Department
Date Deposited: 23 Jul 2014 04:31
Last Modified: 04 Sep 2014 05:27
Fields of Research : 02 Physical Sciences > 0201 Astronomical and Space Sciences > 020110 Stellar Astronomy and Planetary Systems
02 Physical Sciences > 0201 Astronomical and Space Sciences > 020108 Planetary Science (excl. Extraterrestrial Geology)
02 Physical Sciences > 0201 Astronomical and Space Sciences > 020101 Astrobiology
Socio-Economic Objective: E Expanding Knowledge > 97 Expanding Knowledge > 970102 Expanding Knowledge in the Physical Sciences
URI: http://eprints.usq.edu.au/id/eprint/25539

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