The Open UniversitySkip to content
 

Prospects for habitable "earths" in known exoplanetary systems

Jones, Barrie W.; Underwood, David R. and Sleep, P. Nick (2005). Prospects for habitable "earths" in known exoplanetary systems. Astrophysical Journal, 622(2, Part 1) pp. 1091–1101.

URL: http://www.journals.uchicago.edu/ApJ/journal/issue...
DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1086/428108
Google Scholar: Look up in Google Scholar

Abstract

We have examined whether putative Earth-mass planets could remain confined to the habitable zones (HZs) of the 111 exoplanetary systems confirmed by 2004 August. We find that in about half of these systems there could be confinement for at least the past 1000 Myr, though in some cases only in variously restricted regions of the HZ. The HZ migrates outward during the main-sequence lifetime, and we find that in about two-thirds of the systems an Earth-mass planet could be confined to the HZ for at least 1000 Myr sometime during the main-sequence lifetime. Clearly, these systems should be high on the target list for exploration for terrestrial planets. We have reached our conclusions by detailed investigations of seven systems, which has resulted in an estimate of the distance from the giant planet within which orbital stability is unlikely for an Earth-mass planet. This distance is given by nR(H), where R-H is the Hill radius of the giant planet and n is a multiplier that depends on the giant's orbital eccentricity and on whether the Earth-mass planet is interior or exterior to the giant planet. We have estimated n for each of the seven systems by launching Earth-mass planets in various orbits and following their fate with a hybrid orbital integrator. We have then evaluated the habitability of the other exoplanetary systems using nR(H) derived from the giant's orbital eccentricity without carrying out time-consuming orbital integrations. A stellar evolution model has been used to obtain the HZs throughout the main-sequence lifetime.

Item Type: Journal Article
ISSN: 1538-4357
Keywords: astrobiology; planetary systems; planets and satellites;
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 6342
Depositing User: Astrid Peterkin
Date Deposited: 19 Jan 2007
Last Modified: 02 Dec 2010 19:56
URI: http://oro.open.ac.uk/id/eprint/6342
Share this page:

Actions (login may be required)

View Item
Report issue / request change

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340   general-enquiries@open.ac.uk