TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment

Abstract We report the discovery and characterization of TOI-2005 b, a warm Jupiter on an eccentric ( e ∼ 0.59), 17.3 days orbit around a V mag = 9.867 rapidly rotating F-star. The object was detected as a candidate by Transiting Exoplanet Survey Satellite and the planetary nature of TOI-2005 b was then confirmed via a series of ground-based photometric, spectroscopic, and diffraction-limited imaging observations. The planet was found to reside in a low sky-projected stellar obliquity orbit ( λ = <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mn>4</mml:mn> <mml:mo>.</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>8</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>2.5</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>2.3</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> degrees) via a transit spectroscopic observation using the Magellan Magellan Inamori Kyocera Echelle spectrograph. TOI-2005 b is one of a few planets known to have a low-obliquity high-eccentricity orbit, which may be the result of high-eccentricity coplanar migration. The planet has a periastron equilibrium temperature of ∼2100 K, similar to some highly irradiated hot Jupiters where atomic metal species have been detected in transmission spectroscopy, and varies by almost 1000 K during its orbit. Future observations of the atmosphere of TOI-2005b can inform us about its radiative timescales thanks to the rapid heating and cooling of the planet.

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Publication Details

Journal
The Astronomical Journal
Published
2025-04-24
DOI
https://doi.org/10.3847/1538-3881/adc441
Citations
4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
4.62

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article

TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment

Samuel N. Quinn, Thiam-Guan Tan, Jon M. Jenkins, Lyu Abe et al.
4 citations
The Astronomical Journal
Stellar, planetary, and galactic studies
4.62
article

TOI-2005b: An Eccentric Warm Jupiter in Spin-orbit Alignment

Samuel N. Quinn, Thiam-Guan Tan, Jon M. Jenkins, Lyu Abe, Jiayin Dong, Cristilyn N. Watkins, David W. Latham, Rafael Brahm, J. Villaseñor, Karen A. Collins, T. Guillot, Zahra Essack, A. H. M. J. Triaud, Eric B. Ting, Jack Schulte, Sara Seager, Richard P. Schwarz, Olga Suárez, K. Horne, Andrew Vanderburg, G. Ricker, Knicole D. Colón, Chelsea X. Huang, Andrés Jordán, D. J. Osip, Carl Ziegler, L. C. Mayorga, Avi Shporer, Y. Beletsky, George Zhou, Noah Vowell, Jason D. Eastman, Brad Carter, Thomas Henning, Joseph E. Rodriguez, Mélissa J. Hobson, Allyson Bieryla, M. I. Jones, Joshua N. Winn
article en
4 citations

Abstract

Abstract We report the discovery and characterization of TOI-2005 b, a warm Jupiter on an eccentric ( e ∼ 0.59), 17.3 days orbit around a V mag = 9.867 rapidly rotating F-star. The object was detected as a candidate by Transiting Exoplanet Survey Satellite and the planetary nature of TOI-2005 b was then confirmed via a series of ground-based photometric, spectroscopic, and diffraction-limited imaging observations. The planet was found to reside in a low sky-projected stellar obliquity orbit ( λ = <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mn>4</mml:mn> <mml:mo>.</mml:mo> <mml:msubsup> <mml:mrow> <mml:mn>8</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>2.5</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> <mml:mn>2.3</mml:mn> </mml:mrow> </mml:msubsup> </mml:math> degrees) via a transit spectroscopic observation using the Magellan Magellan Inamori Kyocera Echelle spectrograph. TOI-2005 b is one of a few planets known to have a low-obliquity high-eccentricity orbit, which may be the result of high-eccentricity coplanar migration. The planet has a periastron equilibrium temperature of ∼2100 K, similar to some highly irradiated hot Jupiters where atomic metal species have been detected in transmission spectroscopy, and varies by almost 1000 K during its orbit. Future observations of the atmosphere of TOI-2005b can inform us about its radiative timescales thanks to the rapid heating and cooling of the planet.

The Astronomical JournalVol. 169(5)
Ames Research Center (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), University of Illinois Urbana-Champaign (US), University of St Andrews (GB), University of New Mexico (US), University of Southern Queensland (AU), Princeton University (US), Stephen F. Austin State University (US), Adolfo Ibáñez University (CL), Johns Hopkins University Applied Physics Laboratory (US), Millennium Institute of Astrophysics (CL), Perth Exoplanet Survey Telescope Observatory (AU), Max Planck Institute for Astronomy (DE), Center for Astrophysics Harvard & Smithsonian (US), Observatoire de la Côte d’Azur (FR), European Southern Observatory (CL), Las Campanas Observatory (CL), Flatiron Health (United States) (US), Flatiron Institute (US), Data Observatory Foundation, American Institute of Aeronautics and Astronautics (US), Massachusetts Institute of Technology (US), University of Birmingham (GB), Michigan State University (US)
National Science Foundation, National Aeronautics and Space Administration, Simons Foundation, California Institute of Technology, European Space Agency, Flatiron Health, European Commission, Agence Nationale de la Recherche, Ministry of Science, ICT and Future Planning, Institut Polaire Français Paul Emile Victor, Agencia Nacional de Investigación y Desarrollo, Ames Research Center, Science Mission Directorate, Science and Technology Facilities Council
Openalex Percentile: Top 6%
Stellar, planetary, and galactic studies
4.62
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