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Evidence for a Solar Companion Star

Published online by Cambridge University Press:  04 August 2017

Richard A. Muller*
Affiliation:
Department of Physics and Lawrence Berkeley Laboratory, University of California, Berkeley, California 94720

Abstract

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Periodicity seen in both the mass extinctions and large impact cratering on earth can be explained if one postulates that the sun has a companion star, orbiting in a moderately eccentric orbit with a major axis of 2.8 light-years. No other explanations that have been suggested are compatible with known facts of physics and astronomy. If the companion is a red dwarf star, the most common kind in the galaxy, then no previous astronomical observations would have found it. A search for red objects with large parallax is now underway at Berkeley, and has a good chance of identifying the star in the near future.

Type
Section IV. Universal Aspects of Biological Evolution
Copyright
Copyright © Reidel 1985 

References

1. Alvarez, L. W., Alvarez, W., Asaro, F., Michel, H., Science 208, 10951108 (1980).Google Scholar
2. Alvarez, L.W., Proc. Natl. Acad. Sci. USA, 80, pp.627642 (January 1983).Google Scholar
3. Orth, C.J., Gilmore, J. S., Knight, J.D., Pillmore, C.L., Tschudy, R.H., Fassett, J.E., Science 214, 13411343 (1981).CrossRefGoogle Scholar
4. Bohor, B. F., Foord, E. E., Modreski, P. J., Triplehorn, D. M., Science 224, 867869 (1984).Google Scholar
5. Stanley, S. M., “Mass Extinctions in the Oceans”, Scientific American 250, p. 6472 (June 1984).Google Scholar
6. Raup, D. and Sepkoski, J. J., Proc. Nat. Acad. Sci. 81, 801805 (1984).Google Scholar
7. Harland, W. B., et al., A Geologic Time Scale, (Cambridge University Press, 1982).Google Scholar
8. Davis, M., Hut, P., and Muller, R. A., Nature 308, 715717 (1984).Google Scholar
9. Whitmire, D., Jackson, A., Nature 308, 713715 (1984).Google Scholar
10. Rampino, M. R. and Stothers, R. B., Nature 308, 709712 (1984).Google Scholar
11. Schwartz, R. D. and James, P. B., Nature 308, 712713 (1984).CrossRefGoogle Scholar
12. Grieve, R. A. F., Geol. Soc. Am. Spec. Pap. 190, 2537 (1982).Google Scholar
13. Alvarez, W. and Muller, R. A., Nature 308, 718720 (1984).Google Scholar
14. Dao-Yi, X., Shu-Lan, M., Zhi-Fang, C., Xuo-Ying, M., Yi-Ying, S., Qin-Wen, Z., Zheng-Zhong, Y., “Abundance Variation of Iridium and Trace Elements at the Permian-Triassic Boundary at Shangsi, Guangyuan, Sichuan, China”, to be published; also, yi-Ying, S. et al., “The Discovery of Iridium Anomaly in the Permian-Triassic Boundary Clay in Changxing, Zhejiang, China and its significance”, to be published.Google Scholar
15. Kare, J. T., Pennypacker, C. R., Muller, R. A., Mast, T. S., Crawford, F. S., and Burns, M. S., Lawrence Berkeley Laboratory report LBL-13317, also in “Supernovae: A Survey of Current Research”, Rees, M. J. and Stoneham, R. J., eds, p. 325339 (D. Reidel, Dordrect 1981).Google Scholar