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Off-Disk Implantation of Early Solar Wind Into A Planetesimal-Dust Cloud

Published online by Cambridge University Press:  12 April 2016

Sho Sasaki
Sho Sasaki*
Affiliation:
Institute of Geology and MineralogyFaculty of ScienceHiroshima UniversityHiroshima 730Japan

Abstract

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Off-disk implantation of ancient solar wind into a protoplanetary dust cloud can explain the present amounts of solar-type noble gases in gas-rich meteorites and Venus, even if the dust cloud is very opaque along its midplane.

Type
Origin of Interplanetary Dust: from Comets and Asteroids, Back to Interstellar Dust
Information
International Astronomical Union Colloquium , Volume 126: Origin and Evolution of Interplanetary Dust , 1991 , pp. 425 - 428
Copyright
Copyright © Kluwer 1991

References

Goswani, J.N., Lal, D. and Wilkening, L.L. (1984) ’Gas-rich meteorites: probes for particle environment and dynamical processes in the inner solar system’, Space Sci. Rev. 37, 111–159.Google Scholar
Hayashi, C., Nakazawa, K., and Nakagawa, Y. (1985) ’Formation of the solar system’, in Black, D. C. and Matthews, M. S. (eds.), Protostar and Planets II, the University of Arizona Press, Tucson, pp.1100–1153.Google Scholar
McElroy, M. B. and Prather, M.J. (1981) ’Noble gases in the terrestrial planets’, Nature 15, 535–539.CrossRefGoogle Scholar
Nakano, T. (1988) ’Formation of planets around stars of various masses - II. Stars of two and three solar masses and the origin and evolution of circumstellar dust cloud’, Mon. Not. R. astr. Soc. 230, 551–571.Google Scholar
Pollack, J.B. and Black, D.C. (1982) ‘Noble gases in planetary atmospheres: implications for the origin and evolution of atmospheres’, Icarus 51, 169–198.Google Scholar
Prinn, R.G. and Fegley, B. Jr. (1989) ’Solar nebula chemistry: origin of planetary, satellite and cometary volatiles’, in Atreya, S. K., Pollack, J.B., and Matthews, M. S. (eds.) Origin and Evolution of Planetary and Satellite Atmospheres., The University of Arizona Press, Tucson, pp.78–136.Google Scholar
Sasaki, S. (1989) ’Penetration of the solar wind after dissipation of the solar nebula: origin of Venusian Ar by off-disk implantation of the solar wind’, Proc. NIPR Symp. Antarct. Meteoites 2, 326–334.Google Scholar
Sasaki, S. (1991) ‘Off-disk penetration of ancient solar wind’, Icarus 90. in press.CrossRefGoogle Scholar
Wetherill, G.W. (1981) ‘Solar wind origin of36 Ar on Venus’, Icarus 46, 70–80.Google Scholar