activity
20062019
most cited3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds

346 citations · 813 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2019★ 20 cited

Subsistence of ice-covered lakes during the Hesperian at Gale crater, Mars

Alexandre M. Kling, Robert M. Haberle, Christopher P. McKay +2

Sedimentary deposits characterized by the Mars Science Laboratory Curiosity rover provide evidence that Gale crater, Mars intermittently hosted a fluvio-lacustrine environment duri…

astro-ph.EP2016

Detection and Quantification of Volatiles at Mars using a multispectral LIDAR

Adrian J. Brown, Timothy Michaels, Lori Fenton +14

We present a concept for using a polarization sensitive multispectral lidar to map the seasonal distribution and exchange of volatiles among the reservoirs of the Martian surface a…

astro-ph.EP2012★ 346 cited

3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds

Francois Forget, Robin Wordsworth, Ehouarn Millour +5

On the basis of geological evidence, it is often stated that the early martian climate was warm enough for liquid water to flow on the surface thanks to the greenhouse effect of a…

astro-ph.EP2011★ 103 cited

Suppression of the water ice and snow albedo feedback on planets orbiting red dwarf stars and the subsequent widening of the habitable zone

M. Joshi, R. Haberle

M-stars comprise 80% of main-sequence stars, and so their planetary systems provide the best chance for finding habitable planets, i.e.: those with surface liquid water. We have mo…

astro-ph2006★ 344 cited

A Re-appraisal of the Habitability of Planets Around M Dwarf Stars

Jill C. Tarter, Peter R. Backus, Rocco L. Mancinelli +29

Stable, hydrogen-burning, M dwarf stars comprise about 75% of all stars in the Galaxy. They are extremely long-lived and because they are much smaller in mass than the Sun (between…