TESS Spots a Hot Jupiter with an Inner Transiting Neptune
Journal article, 2020

Hot Jupiters are rarely accompanied by other planets within a factor of a few in orbital distance. Previously, only two such systems have been found. Here, we report the discovery of a third system using data from the Transiting Exoplanet Survey Satellite (TESS). The host star, TOI-1130, is an eleventh magnitude K-dwarf in Gaia G-band. It has two transiting planets: a Neptune-sized planet (3.65 ± 0.10 R\oplus) with a 4.1 days period, and a hot Jupiter (1.50-0.22+0.27 RJ) with an 8.4 days period. Precise radial-velocity observations show that the mass of the hot Jupiter is 0.974-0.044+0.043 MJ. For the inner Neptune, the data provide only an upper limit on the mass of 0.17 MJ (3σ). Nevertheless, we are confident that the inner planet is real, based on follow-up ground-based photometry and adaptive-optics imaging that rule out other plausible sources of the TESS transit signal. The unusual planetary architecture of and the brightness of the host star make TOI-1130 a good test case for planet formation theories, and an attractive target for future spectroscopic observations.

Exoplanet astronomy

Extrasolar rocky planets

Exoplanets

Hot Jupiters

Extrasolar gas giants

Author

Chelsea X. Huang

Massachusetts Institute of Technology (MIT)

S. N. Quinn

Harvard-Smithsonian Center for Astrophysics

A. Vanderburg

University of Texas

Juliette Becker

California Institute of Technology (Caltech)

Joseph E. Rodriguez

Harvard-Smithsonian Center for Astrophysics

Francisco J. Pozuelos

University of Liège

Davide Gandolfi

University of Turin

G. Zhou

Harvard-Smithsonian Center for Astrophysics

Andrew W. Mann

The University of North Carolina System

Karen A. Collins

Harvard-Smithsonian Center for Astrophysics

Ian Crossfield

Massachusetts Institute of Technology (MIT)

Khalid Barkaoui

Cadi Ayyad University

University of Liège

Kevin I. Collins

George Mason University

Malcolm Fridlund

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Michaël Gillon

University of Liège

Erica J. Gonzales

University of California

Maximilian N. Günther

Massachusetts Institute of Technology (MIT)

Todd J. Henry

RECONS Institute

Steve B. Howell

National Aeronautics and Space Administration (NASA)

Hodari-Sadiki James

Georgia State University

Wei-Chun Jao

Georgia State University

Emmanuel Jehin

University of Liège

Eric L. N. Jensen

Swarthmore College

Stephen R. Kane

University of California

Jack J. Lissauer

National Aeronautics and Space Administration (NASA)

Elisabeth Matthews

Massachusetts Institute of Technology (MIT)

Rachel A. Matson

US Naval Observatory

Leonardo A. Paredes

Georgia State University

Joshua E. Schlieder

National Aeronautics and Space Administration (NASA)

K.G. Stassun

Vanderbilt University

Avi Shporer

Massachusetts Institute of Technology (MIT)

Lizhou Sha

Massachusetts Institute of Technology (MIT)

Thiam-Guan Tan

Perth Exoplanet Survey Telescope

Iskra Georgieva

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Savita Mathur

Instituto de Astrofísica de Canarias

Enric Palle

Instituto de Astrofísica de Canarias

Carina Persson

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Vincent Van Eylen

University College London (UCL)

George Ricker

Massachusetts Institute of Technology (MIT)

R. Vanderspek

Massachusetts Institute of Technology (MIT)

D.W. Latham

Harvard-Smithsonian Center for Astrophysics

Joshua N. Winn

Princeton University

S. Seager

Massachusetts Institute of Technology (MIT)

Jon M. Jenkins

National Aeronautics and Space Administration (NASA)

Christopher J. Burke

Massachusetts Institute of Technology (MIT)

Robert Goeke

Massachusetts Institute of Technology (MIT)

Stephen Rinehart

National Aeronautics and Space Administration (NASA)

Mark E. Rose

National Aeronautics and Space Administration (NASA)

E. B. Ting

National Aeronautics and Space Administration (NASA)

Guillermo Torres

Harvard-Smithsonian Center for Astrophysics

Ian Wong

Massachusetts Institute of Technology (MIT)

Astrophysical Journal Letters

2041-8205 (ISSN) 2041-8213 (eISSN)

Vol. 892 1 L7

Exoplanets from space – CHEOPS and PLATO, ESA’s next two projects

Swedish National Space Board (174/18), 2017-01-01 -- 2022-12-31.

Subject Categories (SSIF 2011)

Astronomy, Astrophysics and Cosmology

Roots

Basic sciences

DOI

10.3847/2041-8213/ab7302

More information

Latest update

8/20/2025