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LHS 1815b: The First Thick-disk Planet Detected by TESS

Gan, Tianjun; Shporer, Avi; Livingston, John H.; Collins, Karen A.; Mao, Shude; Trani, Alessandro A.; Gandolfi, Davide; Hirano, Teruyuki; Luque, Rafael; Stassun, Keivan G.; Ziegler, Carl; Howell, Steve B.; Hellier, Coel; Irwin, Jonathan M.; Winters, Jennifer G.; Anderson, David R.; Briceño, César; Law, Nicholas; Mann, Andrew W.; Bonfils, Xavier; Astudillo-Defru, Nicola; Jensen, Eric L. N.; Anglada-Escudé, Guillem; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Furesz, Gabor; Guerrero, Natalia M.; Quintana, Elisa; Twicken, Joseph D.; Caldwell, Douglas A.; Tenenbaum, Peter; Huang, Chelsea X.; Rowden, Pamela; Rojas-Ayala, Bárbara

Authors

Tianjun Gan

Avi Shporer

John H. Livingston

Karen A. Collins

Shude Mao

Alessandro A. Trani

Davide Gandolfi

Teruyuki Hirano

Rafael Luque

Keivan G. Stassun

Carl Ziegler

Steve B. Howell

Jonathan M. Irwin

Jennifer G. Winters

David R. Anderson

César Briceño

Nicholas Law

Andrew W. Mann

Xavier Bonfils

Nicola Astudillo-Defru

Eric L. N. Jensen

Guillem Anglada-Escudé

George R. Ricker

Roland Vanderspek

David W. Latham

Sara Seager

Joshua N. Winn

Jon M. Jenkins

Gabor Furesz

Natalia M. Guerrero

Elisa Quintana

Joseph D. Twicken

Douglas A. Caldwell

Peter Tenenbaum

Chelsea X. Huang

Pamela Rowden

Bárbara Rojas-Ayala



Abstract

We report the first discovery of a thick-disk planet, LHS 1815b (TOI-704b, TIC 260004324), detected in the Transiting Exoplanet Survey Satellite (TESS) survey. LHS 1815b transits a bright (V = 12.19 mag, K = 7.99 mag) and quiet M dwarf located 29.87 ± 0.02 pc away with a mass of 0.502 ± 0.015 M⊙ and a radius of 0.501 ± 0.030 R⊙. We validate the planet by combining space- and ground-based photometry, spectroscopy, and imaging. The planet has a radius of 1.088 ± 0.064 R⊕ with a 3σ mass upper limit of 8.7 M⊕. We analyze the galactic kinematics and orbit of the host star LHS 1815 and find that it has a large probability (Pthick/Pthin = 6482) to be in the thick disk with a much higher expected maximal height (Zmax = 1.8 kpc) above the Galactic plane compared with other TESS planet host stars. Future studies of the interior structure and atmospheric properties of planets in such systems using, for example, the upcoming James Webb Space Telescope, can investigate the differences in formation efficiency and evolution for planetary systems between different Galactic components (thick disks, thin disks, and halo).

Citation

Gan, T., Shporer, A., Livingston, J. H., Collins, K. A., Mao, S., Trani, A. A., …Rojas-Ayala, B. (in press). LHS 1815b: The First Thick-disk Planet Detected by TESS. Astronomical Journal, 159(4), 160. https://doi.org/10.3847/1538-3881/ab775a

Journal Article Type Article
Acceptance Date Feb 16, 2020
Online Publication Date Mar 18, 2020
Deposit Date Jun 16, 2023
Journal The Astronomical Journal
Print ISSN 0004-6256
Publisher IOP Publishing
Peer Reviewed Peer Reviewed
Volume 159
Issue 4
Pages 160
DOI https://doi.org/10.3847/1538-3881/ab775a
Keywords Space and Planetary Science; Astronomy and Astrophysics
Additional Information Journal title: The Astronomical Journal; Article type: paper; Article title: LHS 1815b: The First Thick-disk Planet Detected by TESS; Copyright information: © 2020. The American Astronomical Society. All rights reserved.; Date received: 2019-12-22; Date accepted: 2020-02-16; Online publication date: 2020-03-18