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Related papers: Limits on Clouds and Hazes for the TRAPPIST-1 Plan…

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Recently, four additional Earth-mass planets were discovered orbiting the nearby ultracool M8 dwarf TRAPPIST-1, making a remarkable total of seven planets with equilibrium temperatures compatible with the presence of liquid water on their…

Solar and Stellar Astrophysics · Physics 2017-07-26 Cecilia Garraffo , Jeremy J. Drake , Ofer Cohen , Julian D. Alvarado-Gomez , Sofia P. Moschou

Context. Planetary mass and radius data are showing a wide variety in densities of low-mass exoplanets. This includes sub-Neptunes, whose low densities can be explained with the presence of a volatile-rich layer. Water is one of the most…

Earth and Planetary Astrophysics · Physics 2021-03-10 Lorena Acuña , Magali Deleuil , Olivier Mousis , Emmanuel Marcq , Maëva Levesque , Artyom Aguichine

Rocky exoplanets orbiting in the habitable zone (HZ) of nearby M dwarfs provide unique opportunities for characterizing their atmospheres and searching for biosignature gases. TRAPPIST-1e, a temperate Earth-sized exoplanet in the HZ of a…

Earth and Planetary Astrophysics · Physics 2022-09-13 Zifan Lin , Lisa Kaltenegger

The James Webb Space Telescope (JWST) will offer the first opportunity to characterize terrestrial exoplanets with sufficient precision to identify high mean molecular weight atmospheres, and TRAPPIST-1's seven known transiting Earth-sized…

Earth and Planetary Astrophysics · Physics 2019-06-26 Jacob Lustig-Yaeger , Victoria S. Meadows , Andrew P. Lincowski

The atmospheres of late M stars represent a significant challenge in the characterization of any transiting exoplanets due to the presence of strong molecular features in the stellar atmosphere. TRAPPIST-1 is an ultra-cool dwarf, host to…

Context. New estimates of the masses and radii of the seven planets orbiting the ultracool M-dwarf TRAPPIST-1 star permit improved modelling of their compositions, heating by tidal dissipation, and removal of tidal heat by solid-state…

Earth and Planetary Astrophysics · Physics 2019-04-03 Vera Dobos , Amy C. Barr , László L. Kiss

The TRAPPIST-1 system is remarkable for its seven planets that are similar in size, mass, density, and stellar heating to the rocky planets Venus, Earth, and Mars in our own Solar System (Gillon et al. 2017). All TRAPPIST-1 planets have…

Earth and Planetary Astrophysics · Physics 2023-06-02 Thomas P. Greene , Taylor J. Bell , Elsa Ducrot , Achrène Dyrek , Pierre-Olivier Lagage , Jonathan J. Fortney

TRAPPIST-1e is a potentially habitable terrestrial exoplanet orbiting an ultra-cool M Dwarf star and is a key target for observations with the James Webb Space Telescope (JWST). One-dimensional photochemical modelling of terrestrial…

Earth and Planetary Astrophysics · Physics 2023-09-28 Gregory Cooke , Dan Marsh , Catherine Walsh , Allison Youngblood

The TRAPPIST-1 planets have become prime targets for studying the atmospheric and geophysical properties of planets around M-dwarf stars. To effectively identify their atmospheric composition, we first must understand their geological…

Earth and Planetary Astrophysics · Physics 2025-11-17 Junellie Perez , Laura K. Schaefer , Edward Schwieterman , Kevin B. Stevenson , Howard Chen , Jacob Lustig-Yaeger

The TRAPPIST-1 planetary system is a favorable target for the atmospheric characterization of temperate earth-sized exoplanets by means of transmission spectroscopy with the forthcoming James Webb Space Telescope (JWST). A possible obstacle…

TRAPPIST-1 is an ultracool dwarf star transited by seven Earth-sized planets, for which thorough characterization of atmospheric properties, surface conditions encompassing habitability and internal compositions is possible with current and…

The Trappist-1 planets provide a unique opportunity to test the current understanding of rocky planet evolution. The James Webb Space Telescope is expected to characterize the atmospheres of these planets, potentially detecting CO$_2$, CO,…

Earth and Planetary Astrophysics · Physics 2022-07-12 Joshua Krissansen-Totton , Jonathan J. Fortney

Recent transmission spectroscopy has revealed that clouds and hazes are common in the atmospheres of close-in exoplanets. In this study, using the photochemical, microphysical, and transmission spectrum models for close-in warm ($\lesssim$…

Earth and Planetary Astrophysics · Physics 2019-11-06 Yui Kawashima , Masahiro Ikoma

In this work we aim to determine the atmospheric survivability of the TRAPPIST-1 planets by modelling the response of the upper atmosphere to incoming stellar high-energy radiation. Through this case study, we also aim to learn more about…

Earth and Planetary Astrophysics · Physics 2024-01-31 Gwenaël Van Looveren , Manuel Güdel , Sudeshna Boro Saikia , Kristina Kislyakova

Ly-$\alpha$ observations provide a powerful probe of stellar activity and atmospheric escape in exoplanetary systems. We present here an analysis of 104 HST/STIS orbits monitoring the TRAPPIST-1 system between 2017 and 2022, covering 3--5…

With the discovery of rocky planets in the temperate habitable zone (HZ) of the close-by cool star TRAPPIST-1 the question of whether such planets could harbour life arises. Habitable planets around red dwarf stars can orbit in radiation…

Earth and Planetary Astrophysics · Physics 2017-05-10 J. T. O'Malley-James , L. Kaltenegger

The James Webb Space Telescope (JWST) will provide an opportunity to investigate the atmospheres of potentially habitable planets. Aerosols, significantly mute molecular features in transit spectra because they prevent light from probing…

Earth and Planetary Astrophysics · Physics 2022-07-28 Dhvani Doshi , Nicolas B. Cowan , Yi Huang

The TRAPPIST-1 system is comprised of seven Earth-sized rocky planets in small orbits around a Jupiter-sized ultracool dwarf star 12 parsec away. These planets cover an irradiation range similar to the range of the inner solar system. Three…

Earth and Planetary Astrophysics · Physics 2024-01-23 Michaël Gillon

Context. The TRAPPIST-1 system hosts seven Earth-sized, temperate exoplanets orbiting an ultra-cool dwarf star. As such, it represents a remarkable setting to study the formation and evolution of terrestrial planets that formed in the same…