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8 - How, and where, in the solar system …?

from PART II - ANSMET pays off: field results and their consequences

Published online by Cambridge University Press:  06 August 2009

William A. Cassidy
Affiliation:
University of Pittsburgh
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Summary

INTRODUCTION

Around 4.57 billion years ago, our part of the Galaxy was approaching a cusp in time and space that, once passed, would see the beginning of an irreversible process of star and planet formation. Our solar system would result. Just before it happened, our cloud of gas and dust had a past but no future – it wasn't quite dense enough on its own to begin gravitational contractions that would result in the birth of a star and associated planets. With no external stimulus it probably would just remain a cloud – formless, highly diffuse and without apparent purpose. But in a very intimate sense it was our cloud – we were all there, represented unknowingly by the atoms of which we are today composed.

A cusp is a point defined by the tangential convergence of two curves. The time line of our cloud was converging with the time line of a nearby giant star that had become unstable and was set to collapse inward with unimaginable intensity. This would initiate a supernova and splash part of itself out into space in an ejaculation of cosmic violence. Part of this giant splash was directed toward us (to be). The first signal of the nearby supernova was a flash of electromagnetic radiation, of which the part we call visible light is a tiny segment, washing into and through our cloud; perhaps for the first time illuminating its murky interior for no one to see.

Type
Chapter
Information
Meteorites, Ice, and Antarctica
A Personal Account
, pp. 186 - 224
Publisher: Cambridge University Press
Print publication year: 2003

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References

Brearley, A. J. and Jones, R. H. (1998) Chondritic meteorites, Ch 3. In Planetary Materials, ed. J. J. Papike, Reviews in Mineralogy vol. 36. Washington, D.C.: Mineralogical Society of America
Cameron, A. G. W., (2001) From interstellar gas to the earth-moon system. Meteoritics and Planetary Science 36, 9–22CrossRefGoogle Scholar
Chambers, J. E., and Wetherill, G. W., (2001) Planets in the asteroid belt. Meteoritics and Planetary Science 36, 381–399CrossRefGoogle Scholar
Mittlefehldt, D. W., McCoy, T. J. Goodrich, C. A. and Kracher, A. (1998) Non-chondritic meteorites from asteroidal bodies, Ch 4. In Planetary Materials, ed. J. J. Papike, Reviews in Mineralogy vol. 36. Washington, D.C.: Mineralogical Society of America
McSween, H. Y., Jr. (1999) Meteorites and Their Parent Planets, 2nd edn. Cambridge: Cambridge University Press
Scott, E. R. D., Haack, H., and Love, S. G., (2001) Formation of mesosiderites by fragmentation and reaccretion of a large differentiated asteroid. Meteoritics and Planetary Science 36 869–881CrossRefGoogle Scholar
Excellent color photos of antarctic meteorites can be found in the following publications: Yanai, K. (1981) Photographic Catalog of the Selected Antarctic Meteorites, Tokyo: National Institute of Polar Research
Yanai, K. and Hideyasu, K. (1987) Photographic Catalog of the Antarctic Meteorites, Tokyo: National Institute of Polar Research
Bernatowicz, T. J., and Walker, R. M. (1997) Ancient Stardust in the Laboratory. Physics Today 50, 26–32CrossRefGoogle Scholar

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