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Related papers: Star-Planet Interactions

200 papers

Planets interact with their host stars through gravity, radiation and magnetic fields, and for those giant planets that orbit their stars within ~10 stellar radii (~0.1 AU for a sun-like star), star-planet interactions (SPI) are observable…

Solar and Stellar Astrophysics · Physics 2024-12-13 Evgenya L. Shkolnik , Joe Llama

The interaction between planets and their host stars is governed by the forces of gravity, radiation, and magnetic fields. For planets orbiting their stars at distances of approximately 10 stellar radii or less, these effects are…

Earth and Planetary Astrophysics · Physics 2025-02-20 A. Strugarek , E. Shkolnik

Hot Jupiters (HJs) are massive gaseous planets orbiting close to their host stars. Due to their physical characteristics and proximity to the central star, HJs are the natural laboratories to study the process of star-planet interaction…

Earth and Planetary Astrophysics · Physics 2022-05-25 Salvatore Colombo , Ignazio Pillitteri , Salvatore Orlando , Giuseppina Micela

The distribution of hot Jupiters, for which star-planet interactions can be significant, questions the evolution of exosystems. We aim to follow the orbital evolution of a planet along the rotational and structural evolution of the host…

Close-in massive planets interact with their host stars through tidal and magnetic mechanisms. In this paper, we review circumstantial evidence for star-planet interaction as revealed by the photospheric magnetic activity in some of the…

Solar and Stellar Astrophysics · Physics 2015-05-30 A. F. Lanza

There are several physical processes that mediate the interaction between an exoplanet and its host star, with the four main ones being due to magnetic, particle (stellar outflow), radiative and tidal interactions. These interactions can be…

Earth and Planetary Astrophysics · Physics 2025-06-03 A. A. Vidotto

Magnetic interactions between a planet and its environment are known to lead to phenomena such as aurorae and shocks in the solar system. The large number of close-in exoplanets that were discovered triggered a renewed interest in magnetic…

Earth and Planetary Astrophysics · Physics 2019-02-06 A. Strugarek

The architecture of many exoplanetary systems is different from the solar system, with exoplanets being in close orbits around their host stars and having orbital periods of only a few days. We can expect interactions between the star and…

Solar and Stellar Astrophysics · Physics 2017-09-20 K. Poppenhaeger

Stars interact with their planets through gravitation, radiation, and magnetic fields. I shall focus on the interactions between late-type stars with an outer convection zone and close-in planets, i.e., with an orbital semimajor axis…

Earth and Planetary Astrophysics · Physics 2014-08-27 A. F. Lanza

Tidal interaction between an exoplanet and its host star is a possible pathway to transfer angular momentum between the planetary orbit and the stellar spin. In cases where the planetary orbital period is shorter than the stellar rotation…

Solar and Stellar Astrophysics · Physics 2022-04-13 Nikoleta Ilic , Katja Poppenhaeger , S. Marzieh Hosseini

The magnetic activity levels of planet host stars may differ from that of stars not known to host planets in several ways. Hot Jupiters may induce activity in their hosts through magnetic interactions, or through tidal interactions by…

Solar and Stellar Astrophysics · Physics 2017-06-23 Jason T. Wright , Brendan P. Miller

Evidence suggesting an observable magnetic interaction between a star and its hot Jupiter appears as a cyclic variation of stellar activity synchronized to the planet's orbit. In this study, we monitored the chromospheric activity of 7…

Recent observations suggest that stellar magnetic activity may be influenced by the presence of a close-by giant planet. Specifically, chromospheric hot spots rotating in phase with the planet orbital motion have been observed during some…

Astrophysics · Physics 2009-11-13 A. F. Lanza

Planets may have effects on their host stars by tidal or magnetic interaction. Such star-planet interactions are thought to enhance the activity level of the host star. However, stellar activity also affects the sensitivity of planet…

Solar and Stellar Astrophysics · Physics 2013-03-05 K. Poppenhaeger , J. H. M. M. Schmitt

Magnetic (or tidal) interactions between "hot Jupiters" and their host stars can potentially enhance chromospheric and coronal activity. An ideal testbed for investigating this effect is provided by the extreme WASP-18 system, which…

Earth and Planetary Astrophysics · Physics 2015-06-05 Brendan P. Miller , Elena Gallo , Jason T. Wright , Andrea K. Dupree

The architecture of exoplanetary systems is often different from the solar system, with some exoplanets being in close orbits around their host stars and having orbital periods of only a few days. In analogy to interactions between stars in…

Solar and Stellar Astrophysics · Physics 2019-05-15 Katja Poppenhaeger

The magnetic activity of planet-hosting stars is an important factor to estimate the atmospheric stability of close-in exoplanets and the age of their host stars. It has long been speculated that close-in exoplanets can influence the…

Solar and Stellar Astrophysics · Physics 2014-05-13 K. Poppenhaeger , S. J. Wolk

The stellar rotation has an essential role in modifying the structure of the star and, therefore, the way these different interplays arise. On the other hand, changes in orbits impact the star's rotation and its evolution. The evolution of…

Earth and Planetary Astrophysics · Physics 2024-04-11 Thiago M. Santiago , Sarah G. A. Barbosa , Francisco J. Cavalcante , Daniel B. de Freitas

Gravitational tidal interactions drive long-term rotational and orbital evolution in planetary systems, in multiple (particularly close binary) star systems and in planetary moon systems. Dissipation of tidal flows in Earth's oceans is…

Earth and Planetary Astrophysics · Physics 2025-04-16 Adrian J. Barker

Planets in close-in orbits interact magnetically and tidally with their host stars. These interactions lead to a net torque that makes close-in planets migrate inward or outward depending on their orbital distance. We compare systematically…

Solar and Stellar Astrophysics · Physics 2017-10-04 A. Strugarek , E. Bolmont , S. Mathis , A. S. Brun , V. Réville , F. Gallet , C. Charbonnel
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