Hostname: page-component-5c6d5d7d68-7tdvq Total loading time: 0 Render date: 2024-08-19T03:22:45.869Z Has data issue: false hasContentIssue false
  • English
  • Français

Terrestrial planet orbits in the habitable zones of exoplanetary system

Published online by Cambridge University Press:  26 May 2016

B. W. Jones  and
P. N. Sleep
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

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.

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
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 199 - 201
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