Constraining an exoplanet’s magnetic field using star-planet interactions

Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observable as an optical or radio stellar activity signal synchronised with the planet's orbital period. We analyze 18 years of high-resolution optical spectroscopy of GJ 436, a low mass star orbited by a Neptune-sized exoplanet on a polar eccentric orbit. Stellar activity indicators show enhancements at a period corresponding to the exoplanet orbit, modulated by stellar rotation, and the star's 8-year magnetic cycle. We interpret this as a signal of star-planet magnetic interaction. Using a geometric model, we reproduce these periods if GJ 436 b has a magnetic field strength of 6 to 110 Gauss.

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Publication Details

Journal
Science
Published
2026-06-25
DOI
https://doi.org/10.1126/science.adv3075
Primary Topic
Astrophysics and Star Formation Studies
Type
article
Field-Weighted Citation Impact
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article

Constraining an exoplanet’s magnetic field using star-planet interactions

A. Reiners, R. Luque, P. Schöfer, Ε. Πάλλη et al.
Science
Astrophysics and Star Formation Studies
article

Constraining an exoplanet’s magnetic field using star-planet interactions

A. Reiners, R. Luque, P. Schöfer, Ε. Πάλλη, M. R. Zapatero Osorio, A. F. Lanza, J. A. Caballero, P. J. Amado, Daniele Viganò, M. Á. Pérez-Torres, S. Zucker, S. V. Jeffers, A. P. Hatzes, I. Ribas, Daniel Revilla, Simranpreet Kaur, L. Peña-Moñino, A. Binnenfeld, A. Quirrenbach, G. W. Henry
article en

Abstract

Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observable as an optical or radio stellar activity signal synchronised with the planet's orbital period. We analyze 18 years of high-resolution optical spectroscopy of GJ 436, a low mass star orbited by a Neptune-sized exoplanet on a polar eccentric orbit. Stellar activity indicators show enhancements at a period corresponding to the exoplanet orbit, modulated by stellar rotation, and the star's 8-year magnetic cycle. We interpret this as a signal of star-planet magnetic interaction. Using a geometric model, we reproduce these periods if GJ 436 b has a magnetic field strength of 6 to 110 Gauss.

Science
Universitat Autònoma de Barcelona (ES), Universidad de La Laguna (ES), Tel Aviv University (IL), European University Cyprus (CY), Heidelberg University (DE), University of Chicago (US), Institut d'Estudis Espacials de Catalunya (ES), Exact Sciences (United States) (US), Osservatorio Astrofisico di Catania (IT), Centro de Astrobiología (ES), Instituto de Astrofísica de Canarias (ES), Institut de Ciència de Materials de Barcelona (ES), Thüringer Landessternwarte Tautenburg (DE), Fundació Universitat-Empresa de les Illes Balears (ES), Instituto de Astrofísica de Andalucía (ES), Universitat de les Illes Balears (ES), University of Göttingen (DE), Tennessee State University (US), National Institute for Astrophysics (IT)
Openalex Percentile: Top 6%
Astrophysics and Star Formation Studies
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