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Terrestrial planet orbits in the habitable zones of exoplanetary system

Published online by Cambridge University Press:  26 May 2016

B. W. Jones
Affiliation:
Astronomy Group, The Open University, Milton Keynes MK7 6AA, UK
P. N. Sleep
Affiliation:
Astronomy Group, The Open University, Milton Keynes MK7 6AA, UK

Abstract

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We have investigated whether terrestrial planets can exist in orbits in known exoplanetary systems such that life could have emerged on those planets. We have shown that Rho CrB and 47 UMa could have terrestrial planets in orbits that remain confined to their habitable zones for biologically significant lengths of time. We have also shown that the Gliese 876 and Ups And systems are very unlikely to have such orbits.

Type
Part II: Progress in the theory of planet formation
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Chambers, J.E. 1999, MNRAS, 304, 793.CrossRefGoogle Scholar
Chyba, C.F. 1993, Geochim. Cosmochim. Acta 57, 3351.CrossRefGoogle Scholar
Kasting, J.F., Whitmire, D.P., & Reynolds, R.T. 1993, Icarus 101, 108.CrossRefGoogle Scholar