The Discovery of Five Hot Jupiters by TESS
Journal article, 2026

Despite decades of research on hot Jupiters, there are still several theories for their formation. Perhaps hot Jupiters form in several ways. Atmospheric and dynamical studies have the capability to constrain the formation scenarios. However, potential targets have to be well characterized before these observations can further constrain the theories. We present the confirmation and characterization of five hot and warm Jupiters discovered by the TESS space mission. Using TESS data combined with ground-based observations, we determine the masses, radii, and other parameters of TOI-2040 b, TOI-2049 b, TOI-2578 b, TOI-4427 b, and TOI-4458 b. Three of the planets have equilibrium temperatures of about 1800 K while two have temperatures of about 1000 K. Particularly interesting for future atmospheric characterizations are TOI-2578 b and TOI-4427 b, because of their low density and large transmission spectroscopy metric. TOI-4458 b is of special interest because it is in the northern PLATO field. It appears that TOI-2040 b has a small, but measurable eccentricity.

Exoplanet atmospheres (487)

Author

E. W. Guenther

Thüringer Landessternwarte Tautenburg

William D. Cochran

University of Texas

P. MacQueen

University of Texas

E. Goffo

University of Turin

Hanna Kellermann

Ludwig Maximilian University of Munich (LMU)

Benard Nsamba

Max Planck Society

Kyambogo University

M. Endl

University of Texas

D. Sebastian

Thüringer Landessternwarte Tautenburg

University of Birmingham

D. Gandolfi

University of Turin

Cyrille Aumasson

Observatoire des Baronnies Provençales

O. Barragán

University of Oxford

Slawomir Bednarz

Silesian University of Technology

Krzysztof Bernacki

Silesian University of Technology

Allyson Bieryla

Harvard-Smithsonian Center for Astrophysics

P. Bosch-Cabot

University of Lethbridge

Ilaria Carleo

Instituto de Astrofísica de Canarias

Wesleyan University

D. R. Ciardi

California Institute of Technology (Caltech)

Clark Catherine A. Clark

California Institute of Technology (Caltech)

Szilard Csizmadia

German Aerospace Center (DLR)

H. Deeg

Instituto de Astrofísica de Canarias

Parker Duke

University of Texas

Gareb Enoc Fernández Rodríguez

Instituto de Astrofísica de Canarias

Juliana Ehrhardt

Ludwig Maximilian University of Munich (LMU)

M.E. Everett

NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab)

Malcolm Fridlund

Leiden University

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

Iskra Georgieva

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Frank Grupp

Ludwig Maximilian University of Munich (LMU)

T. Hirano

National Institutes of Natural Sciences

The Graduate University for Advanced Studies (SOKENDAI)

National Astronomical Observatory of Japan

Petr Kabath

Czech Academy of Sciences

Juma Kamulali

Kyambogo University

University of Porto

Max Planck Society

Yugo Kawai

University of Tokyo

J. F. Kielkopf

University of Louisville

Judith Korth

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Lund University

Lacedelli Gaia

University of La Laguna

Instituto de Astrofísica de Canarias

K. W.F. Lam

Technische Universität Berlin

D. W. Latham

Harvard-Smithsonian Center for Astrophysics

J.H. Livingston

The Graduate University for Advanced Studies (SOKENDAI)

National Institutes of Natural Sciences

M. B. Lund

California Institute of Technology (Caltech)

Priscilla Muheki

Mbarara University of Science & Technology

F. Murgas

University of La Laguna

Instituto de Astrofísica de Canarias

Norio Narita

University of La Laguna

Instituto de Astrofísica de Canarias

University of Tokyo

National Institutes of Natural Sciences

Greg Olmschenk

National Aeronautics and Space Administration (NASA)

Enric Palle

Instituto de Astrofísica de Canarias

Carina Persson

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Adam Popowicz

Silesian University of Technology

Teznie Pugh

University of Texas

Manfred Rätz

Volkssternwarte Kirchheim

S. Redfield

Wesleyan University

Arno Riffeser

Ludwig Maximilian University of Munich (LMU)

Marek Skarka

Czech Academy of Sciences

L. M. Serrano

University of Turin

A. M.S. Smith

German Aerospace Center (DLR)

G. Srdoc

Kotizarovci Observatory

Vincent Van Eylen

University College London (UCL)

Julian Van Eyken

California Institute of Technology (Caltech)

Anäel Wünsche

Observatoire des Baronnies Provençales

Astronomical Journal

0004-6256 (ISSN) 1538-3881 (eISSN)

Vol. 172 1 54

Subject Categories (SSIF 2025)

Astronomy, Astrophysics, and Cosmology

DOI

10.3847/1538-3881/ae6449

More information

Latest update

7/6/2026 8