Orbital Migration Through Atmospheric Mass Loss

Atmospheric mass loss is thought to have strongly shaped the sample of close-in exoplanets. These atmospheres should be lost isotropically, leading to no net migration on the planetary orbit. However, strong stellar winds can funnel the escaping atmosphere into a tail trailing the planet. We derive...

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Main Authors: Benjamin Hanf, William Kincaid, Hilke Schlichting, Livan Cappiello, Daniel Tamayo
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astronomical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-3881/ad944f
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author Benjamin Hanf
William Kincaid
Hilke Schlichting
Livan Cappiello
Daniel Tamayo
author_facet Benjamin Hanf
William Kincaid
Hilke Schlichting
Livan Cappiello
Daniel Tamayo
author_sort Benjamin Hanf
collection DOAJ
description Atmospheric mass loss is thought to have strongly shaped the sample of close-in exoplanets. These atmospheres should be lost isotropically, leading to no net migration on the planetary orbit. However, strong stellar winds can funnel the escaping atmosphere into a tail trailing the planet. We derive a simple kinematic model of the gravitational interaction between the planet and this anisotropic wind, and derive expressions for the expected migration of the planet. Over the expected range of parameters, we find typical migrations of a few tenths to a few percent inward. We argue that this modest migration may be observable for planet pairs near mean motion resonances, which would provide an independent observational constraint on atmospheric mass loss models.
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publishDate 2024-01-01
publisher IOP Publishing
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series The Astronomical Journal
spelling doaj-art-4c92b3f6357f49f2a38026b01b38ea002025-08-20T02:50:08ZengIOP PublishingThe Astronomical Journal1538-38812024-01-0116911910.3847/1538-3881/ad944fOrbital Migration Through Atmospheric Mass LossBenjamin Hanf0https://orcid.org/0009-0008-5746-4179William Kincaid1https://orcid.org/0009-0007-8964-8354Hilke Schlichting2https://orcid.org/0000-0002-0298-8089Livan Cappiello3Daniel Tamayo4https://orcid.org/0000-0002-9908-8705Pomona College , 333 N College Way, Claremont, CA 91711, USAHarvey Mudd College , 301 Platt Boulevard, Claremont, CA 91711, USAUCLA , 595 Charles E. Young Drive East, Los Angeles, CA 90095, USAHarvey Mudd College , 301 Platt Boulevard, Claremont, CA 91711, USAHarvey Mudd College , 301 Platt Boulevard, Claremont, CA 91711, USAAtmospheric mass loss is thought to have strongly shaped the sample of close-in exoplanets. These atmospheres should be lost isotropically, leading to no net migration on the planetary orbit. However, strong stellar winds can funnel the escaping atmosphere into a tail trailing the planet. We derive a simple kinematic model of the gravitational interaction between the planet and this anisotropic wind, and derive expressions for the expected migration of the planet. Over the expected range of parameters, we find typical migrations of a few tenths to a few percent inward. We argue that this modest migration may be observable for planet pairs near mean motion resonances, which would provide an independent observational constraint on atmospheric mass loss models.https://doi.org/10.3847/1538-3881/ad944fExoplanet migration
spellingShingle Benjamin Hanf
William Kincaid
Hilke Schlichting
Livan Cappiello
Daniel Tamayo
Orbital Migration Through Atmospheric Mass Loss
The Astronomical Journal
Exoplanet migration
title Orbital Migration Through Atmospheric Mass Loss
title_full Orbital Migration Through Atmospheric Mass Loss
title_fullStr Orbital Migration Through Atmospheric Mass Loss
title_full_unstemmed Orbital Migration Through Atmospheric Mass Loss
title_short Orbital Migration Through Atmospheric Mass Loss
title_sort orbital migration through atmospheric mass loss
topic Exoplanet migration
url https://doi.org/10.3847/1538-3881/ad944f
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AT williamkincaid orbitalmigrationthroughatmosphericmassloss
AT hilkeschlichting orbitalmigrationthroughatmosphericmassloss
AT livancappiello orbitalmigrationthroughatmosphericmassloss
AT danieltamayo orbitalmigrationthroughatmosphericmassloss