ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution

Exoplanet atmosphere studies are often enriched by synergies with brown dwarf analogs. However, many key molecules commonly seen in brown dwarfs have yet to be confirmed in exoplanet atmospheres. An important example is chromium hydride (CrH), which is often used to probe atmospheric...

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Main Authors: Laura Flagg, Jake D. Turner, Emily Deibert, Andrew Ridden-Harper, Ernst de Mooij, Ryan J. MacDonald, Ray Jayawardhana, Neale Gibson, Adam Langeveld, David Sing
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal Letters
Subjects:
Online Access:https://doi.org/10.3847/2041-8213/ace529
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author Laura Flagg
Jake D. Turner
Emily Deibert
Andrew Ridden-Harper
Ernst de Mooij
Ryan J. MacDonald
Ray Jayawardhana
Neale Gibson
Adam Langeveld
David Sing
author_facet Laura Flagg
Jake D. Turner
Emily Deibert
Andrew Ridden-Harper
Ernst de Mooij
Ryan J. MacDonald
Ray Jayawardhana
Neale Gibson
Adam Langeveld
David Sing
author_sort Laura Flagg
collection DOAJ
description Exoplanet atmosphere studies are often enriched by synergies with brown dwarf analogs. However, many key molecules commonly seen in brown dwarfs have yet to be confirmed in exoplanet atmospheres. An important example is chromium hydride (CrH), which is often used to probe atmospheric temperatures and classify brown dwarfs into spectral types. Recently, tentative evidence for CrH was reported in the low-resolution transmission spectrum of the hot Jupiter WASP-31b. Here, we present high spectral resolution observations of WASP-31b’s transmission spectrum from GRACES/Gemini North and UVES/Very Large Telescope. We detect CrH at 5.6 σ confidence, representing the first metal hydride detection in an exoplanet atmosphere at high spectral resolution. Our findings constitute a critical step in understanding the role of metal hydrides in exoplanet atmospheres.
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spelling doaj.art-99cc7258541c418bbfac3f739d8b04822024-09-25T10:17:18ZengIOP PublishingThe Astrophysical Journal Letters2041-82052023-01-019532L1910.3847/2041-8213/ace529ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral ResolutionLaura Flagg0https://orcid.org/0000-0001-6362-0571Jake D. Turner1https://orcid.org/0000-0001-7836-1787Emily Deibert2https://orcid.org/0000-0001-9796-2158Andrew Ridden-Harper3https://orcid.org/0000-0002-5425-2655Ernst de Mooij4https://orcid.org/0000-0001-6391-9266Ryan J. MacDonald5https://orcid.org/0000-0003-4816-3469Ray Jayawardhana6https://orcid.org/0000-0001-5349-6853Neale Gibson7https://orcid.org/0000-0002-9308-2353Adam Langeveld8https://orcid.org/0000-0002-4451-1705David Sing9https://orcid.org/0000-0001-6050-7645Department of Astronomy and Carl Sagan Institute, Cornell University , Ithaca, NY 14853, USA ; laura.s.flagg@gmail.comDepartment of Astronomy and Carl Sagan Institute, Cornell University , Ithaca, NY 14853, USA ; laura.s.flagg@gmail.comGemini Observatory , NSF’s NOIRLab, Casilla 603, La Serena, ChileLas Cumbres Observatory , 6740 Cortona Drive, Suite 102, Goleta, CA 93117, USAAstrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast , University Road, Belfast BT7 1NN, UKDepartment of Astronomy and Carl Sagan Institute, Cornell University , Ithaca, NY 14853, USA ; laura.s.flagg@gmail.com; Department of Astronomy, University of Michigan , Ann Arbor, MI 48109, USADepartment of Astronomy, Cornell University , Ithaca, NY 14853, USASchool of Physics, Trinity College Dublin, The University of Dublin , Dublin 2, IrelandDepartment of Astronomy and Carl Sagan Institute, Cornell University , Ithaca, NY 14853, USA ; laura.s.flagg@gmail.comDepartment of Earth & Planetary Sciences, Johns Hopkins University , Baltimore, MD 21218, USAExoplanet atmosphere studies are often enriched by synergies with brown dwarf analogs. However, many key molecules commonly seen in brown dwarfs have yet to be confirmed in exoplanet atmospheres. An important example is chromium hydride (CrH), which is often used to probe atmospheric temperatures and classify brown dwarfs into spectral types. Recently, tentative evidence for CrH was reported in the low-resolution transmission spectrum of the hot Jupiter WASP-31b. Here, we present high spectral resolution observations of WASP-31b’s transmission spectrum from GRACES/Gemini North and UVES/Very Large Telescope. We detect CrH at 5.6 σ confidence, representing the first metal hydride detection in an exoplanet atmosphere at high spectral resolution. Our findings constitute a critical step in understanding the role of metal hydrides in exoplanet atmospheres.https://doi.org/10.3847/2041-8213/ace529Exoplanet atmospheresExoplanetsHigh resolution spectroscopyTransmission spectroscopy
spellingShingle Laura Flagg
Jake D. Turner
Emily Deibert
Andrew Ridden-Harper
Ernst de Mooij
Ryan J. MacDonald
Ray Jayawardhana
Neale Gibson
Adam Langeveld
David Sing
ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
The Astrophysical Journal Letters
Exoplanet atmospheres
Exoplanets
High resolution spectroscopy
Transmission spectroscopy
title ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
title_full ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
title_fullStr ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
title_full_unstemmed ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
title_short ExoGemS Detection of a Metal Hydride in an Exoplanet Atmosphere at High Spectral Resolution
title_sort exogems detection of a metal hydride in an exoplanet atmosphere at high spectral resolution
topic Exoplanet atmospheres
Exoplanets
High resolution spectroscopy
Transmission spectroscopy
url https://doi.org/10.3847/2041-8213/ace529
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