Results 101 to 110 of about 16,128 (220)
The Impact-driven Atmospheric Loss of Super-Earths around Different Spectral Types of Host Stars
A planet’s mass loss is important for the its formation and evolution. The radius valley (RV) is believed to be triggered by evaporation-induced mass loss.
Wei Zhong+3 more
doaj +1 more source
Evolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years [PDF]
Trevor J. David+10 more
openalex +1 more source
EUCLID : Dark Universe Probe and Microlensing planet Hunter
There is a remarkable synergy between requirements for Dark Energy probes by cosmic shear measurements and planet hunting by microlensing. Employing weak and strong gravitational lensing to trace and detect the distribution of matter on cosmic and ...
Batista, V+15 more
core
Terrestrial planets currently in the habitable zone around M dwarfs are estimated to have been in runaway greenhouse conditions for up to ∼1 Gyr due to the long-term pre-main-sequence phase of M dwarfs.
Yo Kawamura+7 more
doaj +1 more source
Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? [PDF]
C. Swastik+7 more
openalex +1 more source
The Formation of Double Hot Jupiter Systems through von Zeipel–Lidov–Kozai Migration
The von Zeipel–Lidov–Kozai (ZLK) mechanism with tidal friction has been demonstrated as a promising avenue to generate hot Jupiters in stellar binary systems.
Yurou Liu, Tiger Lu, Malena Rice
doaj +1 more source
Structure and evolution of super-Earth to super-Jupiter exoplanets [PDF]
I. Baraffe, G. Chabrier, Travis Barman
openalex +1 more source
Separating Super-puffs versus Hot Jupiters among Young Puffy Planets
Discoveries of close-in young puffy ( R _p ≳ 6 R _⊕ ) planets raise the question of whether they are bona fide hot Jupiters or puffed-up Neptunes, potentially placing constraints on the formation location and timescale of hot Jupiters.
Amalia Karalis+2 more
doaj +1 more source
Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems
We identify observational signatures suggesting a history of dynamical instability in 26 out of 34 M-dwarf multi-planet systems containing no large planets.
Anna C. Childs+4 more
doaj +1 more source
The study of lava planets has attracted significant attention recently because of their close proximity to their host stars, which enhances their detectability for atmospheric characterization.
Zhuo-Yang Song, Feng Ding, Wanying Kang
doaj +1 more source