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20112026
most citedSeven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1

1.6k citations · 6.6k across the 83 of their papers we have counts for

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Showing 2023Show all

7 papers · 1 filter

astro-ph.IM2023★ 8 cited

Ground-breaking Exoplanet Science with the ANDES spectrograph at the ELT

Enric Palle, Katia Biazzo, Emeline Bolmont +56

In the past decade the study of exoplanet atmospheres at high-spectral resolution, via transmission/emission spectroscopy and cross-correlation techniques for atomic/molecular mapp…

astro-ph.EP2023★ 43 cited

A cool runaway greenhouse without surface magma ocean

Franck Selsis, Jérémy Leconte, Martin Turbet +2

Water vapour atmospheres with content equivalent to the Earth's oceans, resulting from impacts or a high insolation, were found to yield a surface magma ocean. This was, however, a…

astro-ph.EP2023★ 36 cited

A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

TRAPPIST-1 JWST Community Initiative, :, Julien de Wit +80

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most prominen…

astro-ph.EP2023★ 11 cited

First exploration of the runaway greenhouse transition with a GCM

G. Chaverot, E. Bolmont, M. Turbet

Even if their detection is for now challenging, observation of small terrestrial planets will be easier in a near future thanks to continuous improvements of detection and characte…

astro-ph.EP2023★ 37 cited

Water Condensation Zones around Main Sequence Stars

Martin Turbet, Thomas J. Fauchez, Jeremy Leconte +10

Understanding the set of conditions that allow rocky planets to have liquid water on their surface -- in the form of lakes, seas or oceans -- is a major scientific step to determin…

astro-ph.EP2023★ 3 cited

Potential Atmospheric Compositions of TRAPPIST-1 c constrained by JWST/MIRI Observations at 15 m

Andrew P. Lincowski, Victoria S. Meadows, Sebastian Zieba +13

The first JWST observations of TRAPPIST-1 c showed a secondary eclipse depth of 421+/-94 ppm at 15 um, which is consistent with a bare rock surface or a thin, O2-dominated, low CO2…