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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…

太阳与恒星天体物理 · 物理学 2017-06-23 Jason T. Wright , Brendan P. Miller

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…

太阳与恒星天体物理 · 物理学 2019-05-15 Katja Poppenhaeger

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…

太阳与恒星天体物理 · 物理学 2022-04-13 Nikoleta Ilic , Katja Poppenhaeger , S. Marzieh Hosseini

Stars and their exoplanets evolve together. Depending on the physical characteristics of these systems, such as age, orbital distance and activity of the host stars, certain types of star-exoplanet interactions can dominate during given…

太阳与恒星天体物理 · 物理学 2020-09-30 A. A. Vidotto

Much effort has been invested in recent years, both observationally and theoretically, to understand the interacting processes taking place in planetary systems consisting of a hot Jupiter orbiting its star within 10 stellar radii. Several…

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…

地球与行星天体物理 · 物理学 2025-06-03 A. A. Vidotto

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…

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…

太阳与恒星天体物理 · 物理学 2017-09-20 K. 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…

太阳与恒星天体物理 · 物理学 2014-05-13 K. Poppenhaeger , S. J. Wolk

It is a long-standing question in exoplanet research if Hot Jupiters can influence the magnetic activity of their host stars. While cool stars usually spin down with age and become inactive, an input of angular momentum through tidal…

太阳与恒星天体物理 · 物理学 2015-06-17 K. Poppenhaeger , S. J. Wolk

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…

地球与行星天体物理 · 物理学 2025-02-20 A. Strugarek , E. Shkolnik

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…

太阳与恒星天体物理 · 物理学 2024-12-13 Evgenya L. Shkolnik , Joe Llama

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…

太阳与恒星天体物理 · 物理学 2015-05-30 A. F. Lanza

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…

地球与行星天体物理 · 物理学 2019-02-06 A. Strugarek

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…

地球与行星天体物理 · 物理学 2014-08-27 A. F. Lanza

Stellar magnetic activity is an important factor in the formation and evolution of exoplanets. Magnetic phenomena like stellar flares, coronal mass ejections, and high-energy emission affect the exoplanetary atmosphere and its mass loss…

太阳与恒星天体物理 · 物理学 2017-03-08 K. Poppenhaeger

Stellar variability induce by starspots can hamper the detection of exoplanets and bias planet property estimations. These features can also be used to study star-planet interactions as well as inferring properties from the underlying…

太阳与恒星天体物理 · 物理学 2015-06-17 Conrad Vilela , John Southworth , Carlos del Burgo

The activity levels of stars are influenced by several stellar properties, such as stellar rotation, spectral type and the presence of stellar companions. In analogy to binaries, planetary companions are also thought to be able to cause…

太阳与恒星天体物理 · 物理学 2015-05-28 K. Poppenhaeger , J. H. M. M. Schmitt

The magnetic field of a host star can impact the orbit of a stellar partner, planet, or asteroid if the orbiting body is itself magnetic or electrically conducting. Here, we focus on the instantaneous magnetic forces on an orbiting body in…

地球与行星天体物理 · 物理学 2022-11-09 Benjamin C. Bromley , Scott J. Kenyon

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…

太阳与恒星天体物理 · 物理学 2017-10-04 A. Strugarek , E. Bolmont , S. Mathis , A. S. Brun , V. Réville , F. Gallet , C. Charbonnel
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