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Probing the terrestrial planet TRAPPIST-1c for the presence of an atmosphere

Probing the terrestrial planet TRAPPIST-1c for the presence of an atmosphere
Probing the terrestrial planet TRAPPIST-1c for the presence of an atmosphere
Since the discovery of the first exoplanets, a prime aspiration has been characterization of planets akin to our own Earth. JWST will, for the first time, enable observations of the atmospheres of terrestrial planets, allowing us to understand the nature and diversity and ultimately the habitability of Earth-like worlds. Facilitated by the broad spectral coverage of the NIRSpec Prism, we propose to characterize the atmosphere of the terrestrial-sized exoplanet TRAPPIST-1c, which is one of the most favorable such targets due to its significant transit depth and proximity to Earth. The seven terrestrial planets in the TRAPPIST-1 system receive between 0.1 to 4 times the irradiation of Earth and thus form a unique natural laboratory for testing and understanding planetary environments, their composition and their habitability. Planets b, d, e, and f are part of GTO programs and observations of planet c will thus allow comparative atmospheric characterization of all the inner planets in the TRAPPIST-1 system. Our program will enable the detection of the most probable types of clear atmospheres for TRAPPIST-1c, and its atmospheric constituents. Distinguishing between a cloudy/hazy atmosphere and no atmosphere is extremely challenging for any terrestrial planet, including planet c, and will require occupying JWST for close to 100 hours. We submit that the most fruitful use of JWST will be to reveal the clear-atmosphere Earth-like planets early, using short visits like this proposal, enabling ground-breaking exhaustive characterization of the most favorable Earth-like planets with clear atmospheres before the end of JWST's lifetime.
Rathcke, Alexander
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Bello-Arufe, Aaron
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Buchhave, Lars A.
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Burgasser, Adam J.
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Diamond-Lowe, Hannah
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Espinoza, Nestor
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Fisher, Chloe
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Gibson, Neale
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Guzman Mesa, Andrea
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Heng, Kevin
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Hoeijmakers, Jens
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Hooton, Matthew
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Kitzmann, Daniel
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Kozakis, Thea
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Lopez-Morales, Mercedes
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Mendonca, Joao Manuel
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Morris, Brett M.
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Rathcke, Alexander
4f2c25a8-9c69-48fb-b6b9-46f3738ed40c
Bello-Arufe, Aaron
18871deb-dd2e-403d-8eab-b5bf5e04c84d
Buchhave, Lars A.
09bc47d1-865f-4f71-b25a-51ad6371e3f8
Burgasser, Adam J.
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Diamond-Lowe, Hannah
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Espinoza, Nestor
9568eed4-6b09-488c-9622-596302c0d842
Fisher, Chloe
1a9ff10b-56d7-421d-95d3-e3b62c09cf22
Gibson, Neale
2f15791e-26e6-4380-93d4-0b172d40f9de
Guzman Mesa, Andrea
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Heng, Kevin
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Hoeijmakers, Jens
544bdbbf-3dde-46f5-ac74-0b2697dfcc69
Hooton, Matthew
ae6563d9-21fe-49db-9268-f439836b92fc
Kitzmann, Daniel
af1659b8-c27f-4d1b-b7a2-afaeb944af07
Kozakis, Thea
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Lopez-Morales, Mercedes
832e1868-95c2-4139-b418-ecf6d522b292
Mendonca, Joao Manuel
cb29fe08-eb94-4fad-8eba-eac1c5de491b
Morris, Brett M.
3b4ef40b-0a97-4c7a-b616-e70218353e0b

Rathcke, Alexander, Bello-Arufe, Aaron, Buchhave, Lars A., Burgasser, Adam J., Diamond-Lowe, Hannah, Espinoza, Nestor, Fisher, Chloe, Gibson, Neale, Guzman Mesa, Andrea, Heng, Kevin, Hoeijmakers, Jens, Hooton, Matthew, Kitzmann, Daniel, Kozakis, Thea, Lopez-Morales, Mercedes, Mendonca, Joao Manuel and Morris, Brett M. (2021) Probing the terrestrial planet TRAPPIST-1c for the presence of an atmosphere.

Record type: Other

Abstract

Since the discovery of the first exoplanets, a prime aspiration has been characterization of planets akin to our own Earth. JWST will, for the first time, enable observations of the atmospheres of terrestrial planets, allowing us to understand the nature and diversity and ultimately the habitability of Earth-like worlds. Facilitated by the broad spectral coverage of the NIRSpec Prism, we propose to characterize the atmosphere of the terrestrial-sized exoplanet TRAPPIST-1c, which is one of the most favorable such targets due to its significant transit depth and proximity to Earth. The seven terrestrial planets in the TRAPPIST-1 system receive between 0.1 to 4 times the irradiation of Earth and thus form a unique natural laboratory for testing and understanding planetary environments, their composition and their habitability. Planets b, d, e, and f are part of GTO programs and observations of planet c will thus allow comparative atmospheric characterization of all the inner planets in the TRAPPIST-1 system. Our program will enable the detection of the most probable types of clear atmospheres for TRAPPIST-1c, and its atmospheric constituents. Distinguishing between a cloudy/hazy atmosphere and no atmosphere is extremely challenging for any terrestrial planet, including planet c, and will require occupying JWST for close to 100 hours. We submit that the most fruitful use of JWST will be to reveal the clear-atmosphere Earth-like planets early, using short visits like this proposal, enabling ground-breaking exhaustive characterization of the most favorable Earth-like planets with clear atmospheres before the end of JWST's lifetime.

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More information

Published date: March 2021

Identifiers

Local EPrints ID: 497593
URI: http://eprints.soton.ac.uk/id/eprint/497593
PURE UUID: abe056ac-3822-4927-b53f-0391e76b3c18
ORCID for Joao Manuel Mendonca: ORCID iD orcid.org/0000-0002-6907-4476

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Date deposited: 28 Jan 2025 17:40
Last modified: 29 Jan 2025 03:16

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Contributors

Author: Alexander Rathcke
Author: Aaron Bello-Arufe
Author: Lars A. Buchhave
Author: Adam J. Burgasser
Author: Hannah Diamond-Lowe
Author: Nestor Espinoza
Author: Chloe Fisher
Author: Neale Gibson
Author: Andrea Guzman Mesa
Author: Kevin Heng
Author: Jens Hoeijmakers
Author: Matthew Hooton
Author: Daniel Kitzmann
Author: Thea Kozakis
Author: Mercedes Lopez-Morales
Author: Joao Manuel Mendonca ORCID iD
Author: Brett M. Morris

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