Results 41 to 50 of about 1,706 (153)

Star‐planet interactions and selection effects from planet detection methods [PDF]

open access: yesAstronomische Nachrichten, 2011
AbstractPlanets 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 detection methods.
Poppenhaeger, K., Schmitt, J. H. M. M.
openaire   +2 more sources

The Spin–Orbit Misalignment of TOI-1842b: The First Measurement of the Rossiter–McLaughlin Effect for a Warm Sub-Saturn around a Massive Star

open access: yesThe Astrophysical Journal Letters, 2023
The mechanisms responsible for generating spin–orbit misalignments in exoplanetary systems are still not fully understood. It is unclear whether these misalignments are related to the migration of hot Jupiters or are a consequence of general star and ...
Kyle Hixenbaugh   +3 more
doaj   +1 more source

Interaction of free-floating planets with a star–planet pair [PDF]

open access: yesCelestial Mechanics and Dynamical Astronomy, 2012
The recent discovery of free-floating planets and their theoretical interpretation as celestial bodies, either condensed independently or ejected from parent stars in tight clusters, introduced an intriguing possibility. Namely, that some exoplanets are not condensed from the protoplanetary disk of their parent star.
Varvoglis, Harry   +2 more
openaire   +2 more sources

An Earth-sized Planet on the Verge of Tidal Disruption

open access: yesThe Astronomical Journal
TOI-6255 b (GJ 4256) is an Earth-sized planet (1.079 ± 0.065 R _⊕ ) with an orbital period of only 5.7 hr. With the newly commissioned Keck Planet Finder and CARMENES spectrographs, we determine the planet’s mass to be 1.44 ± 0.14 M _⊕ .
Fei Dai   +96 more
doaj   +1 more source

Chasing Star–Planet Magnetic Interactions: The Case of Kepler-78 [PDF]

open access: yesThe Astrophysical Journal, 2019
Abstract Observational evidence of star–planet magnetic interactions (SPMIs) in compact exosystems have been looked for in the past decades. Indeed, planets in close-in orbit can be magnetically connected to their host star and can channel Alfvén waves carrying large amounts of energy toward the central star.
A. Strugarek   +4 more
openaire   +4 more sources

Capture into Apsidal Resonance and the Decimation of Planets around Inspiraling Binaries

open access: yesThe Astrophysical Journal Letters
Transiting circumbinary planets (CBPs) are conspicuously rare and entirely absent around stellar binaries with periods ≤7 days. Here we exploit a secular resonance to stimulate the orbit of a CBP into strong, disruptive interactions with the host binary.
Mohammad Farhat, Jihad Touma
doaj   +1 more source

Carving the Edges of the Rocky Planet Population

open access: yesThe Astrophysical Journal Letters
Short-period planets provide ideal laboratories for testing star–planet interaction. Planets that are smaller than  ∼2 R _⊕ are considered to be largely rocky, either having been stripped of or never having acquired the gaseous envelope.
Eve J. Lee, James E. Owen
doaj   +1 more source

High-eccentricity Migration with Disk-induced Spin–Orbit Misalignment: A Preference for Perpendicular Hot Jupiters

open access: yesThe Astrophysical Journal Letters, 2023
High-eccentricity migration is a likely formation mechanism for many observed hot Jupiters, particularly those with a large misalignment between the stellar spin axis and orbital angular momentum axis of the planet.
Michelle Vick, Yubo Su, Dong Lai
doaj   +1 more source

Atmospheric Escape From Three Terrestrial Planets in the L 98-59 System

open access: yesThe Astrophysical Journal
A critically important process affecting the climate evolution and potential habitability of an exoplanet is atmospheric escape, in which high-energy radiation from a star drives the escape of hydrogen atoms and other light elements from a planet’s ...
Emeline F. Fromont   +8 more
doaj   +1 more source

Tidal Migration of Exoplanets around M Dwarfs: Frequency-dependent Tidal Dissipation

open access: yesThe Astrophysical Journal
The orbital architectures of short-period exoplanet systems are shaped by tidal dissipation in their host stars. For low-mass M dwarfs whose dynamical tidal response comprises a dense spectrum of inertial modes at low frequencies, resolving the frequency
Samantha C. Wu   +2 more
doaj   +1 more source

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