When you wish upon a planet: the encapsulating tail of KELT-9b
When you wish upon a planet: the encapsulating tail of KELT-9b
Irradiated Jovian atmospheres are complex, dynamic, and can undergo temporal variations that are closely influenced by their parent stars. Of the Jovian planets that have been catalogued to date, KELT-9b is the hottest known, with an equilibrium temperature of 4050 K. We probe the temporal variability of transmission spectroscopic signatures from KELT-9b via a set of archival multi-year ground-based transit observations. Our observations confirm atomic detections of H-alpha, Fe, Fe+ and Mg over multiple epochs, and that the H-alpha transit light curve deviates from a standard transit in shape. The H-alpha transit can be well described via a "cometary" tail that streams away from the planet in the direction of the observer, perpendicular to the planetary orbit. We discuss the temporal stability of this evaporative tail, and its implications on modelling the dynamics of the KELT-9b atmosphere. These multi-epoch observations, performed with the TRES facility on the 1.5 m reflector at FLWO, highlight the capabilities of small telescopes to provide temporal monitoring of the dynamics of exoplanet atmospheres.
Lowson, Nataliea
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Zhou, George
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Huang, Chelsea
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Wright, Duncan
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Mendonca, Joao
cb29fe08-eb94-4fad-8eba-eac1c5de491b
Latham, David
07caab57-fb83-4b32-b5c3-10b97421f7a5
June 2022
Lowson, Nataliea
d5463f56-3886-46a9-b858-ff3378999d5a
Zhou, George
0a35a8dd-ee84-436b-992b-d56a78cfe3b1
Huang, Chelsea
938a9901-728a-4c60-a4ee-5430ae703887
Wright, Duncan
590a24ae-cbd2-44c2-87a8-a5c076d6cfff
Mendonca, Joao
cb29fe08-eb94-4fad-8eba-eac1c5de491b
Latham, David
07caab57-fb83-4b32-b5c3-10b97421f7a5
Lowson, Nataliea, Zhou, George, Huang, Chelsea, Wright, Duncan, Mendonca, Joao and Latham, David
(2022)
When you wish upon a planet: the encapsulating tail of KELT-9b.
Bulletin of the AAS, 54 (5).
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Abstract
Irradiated Jovian atmospheres are complex, dynamic, and can undergo temporal variations that are closely influenced by their parent stars. Of the Jovian planets that have been catalogued to date, KELT-9b is the hottest known, with an equilibrium temperature of 4050 K. We probe the temporal variability of transmission spectroscopic signatures from KELT-9b via a set of archival multi-year ground-based transit observations. Our observations confirm atomic detections of H-alpha, Fe, Fe+ and Mg over multiple epochs, and that the H-alpha transit light curve deviates from a standard transit in shape. The H-alpha transit can be well described via a "cometary" tail that streams away from the planet in the direction of the observer, perpendicular to the planetary orbit. We discuss the temporal stability of this evaporative tail, and its implications on modelling the dynamics of the KELT-9b atmosphere. These multi-epoch observations, performed with the TRES facility on the 1.5 m reflector at FLWO, highlight the capabilities of small telescopes to provide temporal monitoring of the dynamics of exoplanet atmospheres.
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Published date: June 2022
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Local EPrints ID: 497556
URI: http://eprints.soton.ac.uk/id/eprint/497556
ISSN: 0002-7537
PURE UUID: 936e5f46-b0a7-40b9-92e1-c64c198d99f1
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Date deposited: 27 Jan 2025 17:56
Last modified: 28 Jan 2025 03:15
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Contributors
Author:
Nataliea Lowson
Author:
George Zhou
Author:
Chelsea Huang
Author:
Duncan Wright
Author:
Joao Mendonca
Author:
David Latham
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