Hostname: page-component-848d4c4894-tn8tq Total loading time: 0 Render date: 2024-06-30T22:11:33.331Z Has data issue: false hasContentIssue false
  • English
  • Français

Origin and Bulk Chemical Composition of Mercury

Published online by Cambridge University Press:  30 March 2016

Andrew J. R. Prentice  and
Daniel Jontof-Hutter
Andrew J. R. Prentice
Affiliation:
Mathematical Sciences, Monash University, Victoria 3800, Australia
Daniel Jontof-Hutter
Affiliation:
Mathematical Sciences, Monash University, Victoria 3800, Australia

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The origin of Mercury’s high metal content is examined within a gas ring model for the condensation of the planetary system. Mercury’s axial moment-of-inertia factor is predicted to be 0.325 ± 0.002.

Type
I. Joint Discussions
Information
Highlights of Astronomy , Volume 13 , 2005 , pp. 73 - 74
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Drake, M.J., & Righter, K. 2002, Nature, 416, 39 Google Scholar
Lewis, J.S. 1972, Earth Planet. Sci. Lett., 15, 286 Google Scholar
Prentice, A. J. R. 1978, Moon & Planets, 19, 341 Google Scholar
Prentice, A. J. R. 2001a, Earth Moon & Planets, 87, 11 CrossRefGoogle Scholar
Prentice, A. J. R. 2001b, www.lpi.usra.edu/meetings/mercury01/pdf/8061.pdf Google Scholar
Prentice, A. J. R., & Dyt, C.P. 2003, MNRAS, 341, 644 Google Scholar
Siegfried, R.W., & Solomon, S.C. 1974, Icarus, 23, 192 Google Scholar