Discovery and Characterization of the TOI-4468 Planetary System: A Transiting Hot Jupiter with a Lone Nearby Outer Companion

Abstract We report the discovery of two planets, a hot Jupiter (HJ) and a nearby outer sub-Neptune, orbiting the star TOI-4468. This system is unique among the current exoplanet census in that it features a close outer companion to a HJ without an accompanying inner companion. By jointly fitting radial velocity (RV) measurements taken with the NEID spectrograph and transit photometry from the Transiting Exoplanet Survey Satellite (TESS) and several ground-based observatories, we constrain the orbital periods, masses, and radii of these two planets. We confirm the planetary nature of the HJ TOI-4468 b ( R = 1.01 R J , m = 0.54 M J , P = 2.77 days). We also validate the outer planet TOI-4468 c ( R = 0.28 R J , P = 7.01 days) statistically, incorporating constraints from ground-based observations. We also identify, but cannot confirm, an additional RV signal that may be due to an outer giant in this system with an orbital period of 624 days. From the observed geometry of this system, we argue that it must never have encountered an early secular resonance that is thought to excite the mutual inclination of other HJ/outer companion systems. We discuss the possibility of an undetected inner companion, as well as potential implications for HJ formation.

Authors

Institutions

Publication Details

Journal
The Astronomical Journal
Published
2026-10-29
DOI
https://doi.org/10.3847/1538-3881/aeaee4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Discovery and Characterization of the TOI-4468 Planetary System: A Transiting Hot Jupiter with a Lone Nearby Outer Companion

Ivan A. Strakhov, Robert Aloisi, Benjamin J. Hord, H. Parviainen et al.
2 links
The Astronomical Journal
Stellar, planetary, and galactic studies
article

Discovery and Characterization of the TOI-4468 Planetary System: A Transiting Hot Jupiter with a Lone Nearby Outer Companion

Ivan A. Strakhov, Robert Aloisi, Benjamin J. Hord, H. Parviainen, Karen A. Collins, Adam Popowicz, Richard P. Schwarz, Andrew M. Vanderburg, Thomas G. Beatty, Melinda Soares-Furtado, Guđmundur Stefánsson, Lizhou Sha, Joseph R. Livesey, Joseph E. Rodriguez, Keivan Guadalupe Stassun, Manfred Raetz, Alyssa R. Jankowski, Fabian Rodriguez Frustaglia, Eva Stafne, Juliette Becker, Maxwell A. Kroft, Thomas MacLean, Judith Korth, Chelsea X. Huang, Khalid Barkaoui, Coleman Nelson, Elise Koo, Paul Foster, Zijun He, Kinga Kasprzyk, Devansh Mathur
article en

Abstract

Abstract We report the discovery of two planets, a hot Jupiter (HJ) and a nearby outer sub-Neptune, orbiting the star TOI-4468. This system is unique among the current exoplanet census in that it features a close outer companion to a HJ without an accompanying inner companion. By jointly fitting radial velocity (RV) measurements taken with the NEID spectrograph and transit photometry from the Transiting Exoplanet Survey Satellite (TESS) and several ground-based observatories, we constrain the orbital periods, masses, and radii of these two planets. We confirm the planetary nature of the HJ TOI-4468 b ( R = 1.01 R J , m = 0.54 M J , P = 2.77 days). We also validate the outer planet TOI-4468 c ( R = 0.28 R J , P = 7.01 days) statistically, incorporating constraints from ground-based observations. We also identify, but cannot confirm, an additional RV signal that may be due to an outer giant in this system with an orbital period of 624 days. From the observed geometry of this system, we argue that it must never have encountered an early secular resonance that is thought to excite the mutual inclination of other HJ/outer companion systems. We discuss the possibility of an undetected inner companion, as well as potential implications for HJ formation.

The Astronomical JournalVol. 172(5)
Silesian University of Technology (PL), California Institute of Technology (US), Goddard Space Flight Center (US), University of Wisconsin–Madison (US), University of Liège (BE), Universidad de La Laguna (ES), University of Southern Queensland (AU), Lund University (SE), Lomonosov Moscow State University (RU), Vanderbilt University (US), Princeton University (US), California State University Los Angeles (US), Center for Astrophysics Harvard & Smithsonian (US), Instituto de Astrofísica de Canarias (ES), Massachusetts Institute of Technology (US), Michigan State University (US), University of Amsterdam (NL), Netherlands Institute for Radio Astronomy (NL), Stanford University (US)
National Science Foundation, National Aeronautics and Space Administration, Wisconsin Alumni Research Foundation, Oak Ridge Associated Universities, University of Pennsylvania, California Institute of Technology, University of Wisconsin-Madison, Pennsylvania State University, NASA Exoplanet Science Institute, Universidad de La Laguna, European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Ministry of Science, ICT and Future Planning, Vetenskapsrådet, Ministerio de Ciencia e Innovación, Lomonosov Moscow State University, Goddard Space Flight Center, Science Mission Directorate, Office of the Vice Chancellor for Research, University of Illinois at Chicago, Ministerio de Universidades
Openalex Percentile: Top 34%
Stellar, planetary, and galactic studies
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon