S. Lectez

most citedA

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32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko

25 citations · 25 across the 1 of their papers we have counts for

collaborators

2 papers

astro-ph.EP2016

Martian zeolites as a source of atmospheric methane

Olivier Mousis, Jean-Marc Simon, Jean-Pierre Bellat +7

The origin of the martian methane is still poorly understood. A plausible explanation is that methane could have been produced either by hydrothermal alteration of basaltic crust o…

astro-ph.EP2015★ 25 cited

A $\sim$ 32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko

S. Lectez, J. M. Simon, O. Mousis +4

Grand Canonical Monte Carlo simulations are used to reproduce the N $_{2}$ /CO ratio ranging between 1.7 $\times$ 10 $^{- 3}$ and 1.6 $\times$ 10 $^{- 2}$ observed {\it in situ} in the Jup…

Martian zeolites as a source of atmospheric methane

A ∼32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko

A $\sim$ 32-70 K formation temperature range for the ice grains agglomerated by comet 67P/Churyumov-Gerasimenko