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Evidence of magnetic interaction between late-type stars and close-in giant planets is provided by the observations of stellar hot spots rotating synchronously with the planets and showing an enhancement of chromospheric and X-ray fluxes.…

太阳与恒星天体物理 · 物理学 2015-05-13 A. F. Lanza

The interaction between the magnetic fields of late-type stars and their close-by planets may produce stellar flares as observed in active binary systems. However, in spite of several claims, conclusive evidence is still lacking. We…

地球与行星天体物理 · 物理学 2018-03-07 A. F. Lanza

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

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…

天体物理学 · 物理学 2009-11-13 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 close-in planets through radiation, gravitation, and magnetic fields. We investigate the energy input to a planetary atmosphere by reconnection between stellar and planetary magnetic fields and compare it to the…

地球与行星天体物理 · 物理学 2013-07-10 A. F. Lanza

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

A small percentage of normal stars harbor giant planets that orbit within a few tenths of an astronomical unit. At such distances the potential exists for significant tidal and magnetic field interaction resulting in energy dissipation that…

太阳与恒星天体物理 · 物理学 2015-05-19 Caleb A. Scharf

It has been proposed that magnetic activity could be enhanced due to interactions between close-in massive planets and their host stars. In this article, I present a brief overview of the connection between stellar magnetic activity and…

太阳与恒星天体物理 · 物理学 2017-11-08 A. A. Vidotto

Since the first discovery of an extrasolar planetary system more than a decade ago, hundreds more have been discovered. Surprisingly, many of these systems harbor Jupiter-class gas giants located close to the central star, at distances of…

太阳与恒星天体物理 · 物理学 2014-11-20 O. Cohen , J. J. Drake , V. L. Kashyap , S. H. Saar , I. V. Sokolov , W. B. Manchester , K. C. Hansen , T. I. Gombosi

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…

Magnetic interactions between a star and a close-in planet are postulated to be a source of enhanced emissions and to play a role in the secular evolution of the orbital system. Close-in planets generally orbit in the sub-alfv\'enic region…

地球与行星天体物理 · 物理学 2015-12-23 A. Strugarek , A. S. Brun , S. P. Matt , V. Réville

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

There is growing observational evidence for some kind of interaction between stars and close-in extrasolar giant planets. Shkolnik et al. reported variability in the chromospheric Ca H and K lines of HD 179949 and upsilon And that seemed to…

天体物理学 · 物理学 2007-05-23 Steven R. Cranmer , Steven H. Saar

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

Observations of the coronae of the Sun and of solar-like stars provide complementary information to advance our understanding of stellar magnetic activity, and of the processes leading to the heating of their outer atmospheres. While solar…

太阳与恒星天体物理 · 物理学 2023-07-19 Paola Testa , Steve Saar , Jeremy Drake

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

Magnetic interactions between a planet and its environment are known to lead to aurorae and shocks in the solar system. The large number of close-in exoplanets that have been discovered so far triggered a renewed interest in understanding…

太阳与恒星天体物理 · 物理学 2021-09-17 Antoine Strugarek

Magnetic interactions between close-in planets and their host star can play an important role in the secular orbital evolution of the planets, as well as the rotational evolution of their host. As long as the planet orbits inside the…

地球与行星天体物理 · 物理学 2015-06-22 Antoine Strugarek , Allan Sacha Brun , Sean Patrick Matt , Victor Réville

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
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