activity
20022010
most citedProspects for Extrasolar "Earths" in Habitable Zones

95 citations · 316 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2010★ 83 cited

Determining Habitability: Which exoEarths should we search for life?

J. Horner, B. W. Jones

Within the next few years, the first Earth-mass planets will be discovered around other stars. Some of those worlds will certainly lie within the classical "habitable zone" of thei…

astro-ph.EP2010★ 41 cited

Habitability of exoplanetary systems with planets observed in transit

Barrie W Jones, P Nick Sleep

(Shortened) We have used the measured properties of the stars in the 79 exoplanetary systems with one or more planets that have been observed in transit, to estimate each system's…

astro-ph.EP2010★ 7 cited

Formation and Dynamical Evolution of the Neptune Trojans - the Influence of the Initial Solar System Architecture

P. S. Lykawka, J. Horner, B. W. Jones +1

In this work, we investigate the dynamical stability of pre-formed Neptune Trojans under the gravitational influence of the four giant planets in compact planetary architectures, o…

astro-ph2006★ 90 cited

Habitability of known exoplanetary systems based on measured stellar properties

Barrie W Jones, P Nick Sleep, David R Underwood

At present, because of observational selection effects, we know of no exoplanetary systems with any planetary masses close to that of the Earth. We have therefore used computer mod…

astro-ph2005★ 95 cited

Prospects for Extrasolar "Earths" in Habitable Zones

B. W. Jones, D. R. Underwood, P. N. Sleep

We have shown that Earth-mass planets could survive in variously restricted regions of the habitable zones (HZs) of most of a sample of nine of the 102 main-sequence exoplanetary s…

astro-ph2002

The Orbits of Terrestrial Planets in the Habitable Zones of Known Exoplanetary Systems

Barrie W Jones, P Nick Sleep

We show that terrestrial planets could survive in variously restricted regions of the habitable zones of 47 Ursae Majoris, Epsilon Eridani, and Rho Coronae Borealis, but nowhere in…