Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? [PDF]
Life (Basel), 2023 Glidden A +3 more
europepmc +1 more source
Atmospheric escape from exoplanets: recent observations and theoretical models [PDF]
arXivThe review aims to give an overview of atmospheric escape processes from exoplanets. I briefly discuss the physics of various escape processes responsible for atmospheric escape across different types of exoplanets. Transmission spectroscopy is one of the major workhorses to observe the escaping atmosphere from exoplanets. I discuss recent observations
arxiv
WASP-69b’s Escaping Envelope Is Confined to a Tail Extending at Least 7 Rp
The Astrophysical JournalStudying the escaping atmospheres of highly irradiated exoplanets is critical for understanding the physical mechanisms that shape the demographics of close-in planets.
Dakotah Tyler +3 more
doaj +1 more source
The Impact-driven Atmospheric Loss of Super-Earths around Different Spectral Types of Host Stars
The Astrophysical JournalA 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
The Astrophysical JournalTerrestrial 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
The Formation of Double Hot Jupiter Systems through von Zeipel–Lidov–Kozai Migration
The Astrophysical JournalThe 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
Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? [PDF]
, 2022 C. Swastik +7 more
openalex +1 more source
Separating Super-puffs versus Hot Jupiters among Young Puffy Planets
The Astrophysical JournalDiscoveries 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
Structure and evolution of super-Earth to super-Jupiter exoplanets [PDF]
, 2008 I. Baraffe, G. Chabrier, Travis Barman
openalex +1 more source
Observational Signatures of a Previous Dynamical Instability in Multi-planet M-dwarf Systems
The Astrophysical JournalWe 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