Results 81 to 90 of about 1,706 (153)
Context. Modeling how cold giant planets form around M dwarfs remains a challenge, both because their protoplanetary disks can lack sufficient mass and because such planets are expected to migrate inward while interacting with the disk.
Sanchez M. +4 more
doaj +1 more source
We report the discovery and characterization of TIC 350842552 (“Zvrk”), an apparently isolated, rapidly rotating ( P _rot ∼ 99 days) red giant observed by TESS in its southern Continuous Viewing Zone.
J. M. Joel Ong +21 more
doaj +1 more source
The recent discovery of planetesimals orbiting white dwarfs has renewed interest in the final chapters of the evolution of planetary systems. Although observational and theoretical studies have examined the dynamical evolution of these systems, studies ...
Matthew Route
doaj +1 more source
Star-planet interactions: planetary orbital evolution and Engulfment
L'orbite d'une planète peut changer significativement au cours du temps. À cause des forces de marée entre l'étoile et la planète, des échanges entre le moment angulaire orbital de la planète et le moment angulaire rotationnel de l'étoile peuvent survenir.
openaire +2 more sources
Upper Atmosphere Dynamics and Drivers of Volatiles Loss from Terrestrial-Type (Exo)Planets. [PDF]
Kubyshkina D +9 more
europepmc +1 more source
A young progenitor for the most common planetary systems in the Galaxy. [PDF]
Livingston JH +41 more
europepmc +1 more source
Characterization of exoplanets in the James Webb Space Telescope era. [PDF]
Lunine JI, Bahcall N.
europepmc +1 more source
A complex structure of escaping helium spanning more than half the orbit of the ultra-hot Jupiter WASP-121 b. [PDF]
Allart R +21 more
europepmc +1 more source
Exploring exoplanet dynamics with JWST: Tides, rotation, rings, and moons. [PDF]
Millholland SC, Winn JN.
europepmc +1 more source
A first look at rocky exoplanets with JWST. [PDF]
Kreidberg L, Stevenson KB.
europepmc +1 more source

