Results 91 to 100 of about 1,944 (221)
Exoplanet atmospheres at high spectral resolution [PDF]
The spectrum of an exoplanet reveals the physical, chemical, and biological processes that have shaped its history and govern its future. However, observations of exoplanet spectra are complicated by the overwhelming glare of their host stars.
Birkby, Jayne
core +1 more source
Do Super-puffs Defy Core Accretion? Population-wide Interior Structure Constraints
Sub-Saturn mass planets with extremely low bulk densities ( ρ ≲ 0.3 g cm ^−3 ), or “super-puffs,” are one of the most interesting and least understood populations of exoplanets.
Nicholas T. Marston +2 more
doaj +1 more source
The need for laboratory work to aid in the understanding of exoplanetary atmospheres [PDF]
Advancements in our understanding of exoplanetary atmospheres, from massive gas giants down to rocky worlds, depend on the constructive challenges between observations and models.
Wang, Sharon X. +33 more
core
Exoplanet mass and radius inferences fundamentally rely on host star mass and radius inferences. Despite the importance of host star mass, radius, and elemental abundance inferences for the derivation of exoplanet internal structure constraints ...
Alejandra Ross +4 more
doaj +1 more source
Statistical Trends in JWST Transiting Exoplanet Atmospheres [PDF]
Our brains are hardwired for pattern recognition as correlations are useful for predicting and understanding nature. As more exoplanet atmospheres are being characterized with JWST, we are starting to unveil their properties on a population level.
David K. Sing +15 more
core +1 more source
Evolution of Steam Worlds: Energetic Aspects
Sub-Neptunes occupy an intriguing region of planetary mass–radius space, where theoretical models of interior structure predict that they could be water-rich, where water is in steam and supercritical state.
Artyom Aguichine +5 more
doaj +1 more source
A global map of the atmospheric circulation and thermal structure for an ultrahot exoplanet [PDF]
WASP-121b is one of the standout exoplanets available for atmospheric characterization, both in transmission and emission, due to its large radius (1.8 Jupiter radii), high temperature ( 2700K), and bright host star (H=9.4mag).
Barstow, Joanna +13 more
core
Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet's Cores
Some exoplanets have much higher densities than expected from stellar abundances of planet-forming elements. There are two theories—metal-rich formation hypothesis and naked core hypothesis—that explain how formation and evolution can alter the ...
Zifan Lin, Saverio Cambioni, Sara Seager
doaj +1 more source
Fleeting but Not Forgotten: The Imprint of Escaping Hydrogen Atmospheres on Super-Earth Interiors
Small, close-in exoplanets are divided into two subpopulations: super-Earths and sub-Neptunes. Most super-Earths are thought to have lost their primordially accreted hydrogen-dominated atmospheres via thermally driven winds.
James G. Rogers +2 more
doaj +1 more source
APPLE: An Evolution Code for Modeling Giant Planets
We introduce APPLE , a novel planetary evolution code designed specifically for the study of giant exoplanet and Jovian planet evolution in the era of Galileo, Juno, and Cassini. With APPLE , state-of-the-art equations of state for hydrogen, helium, ice,
Ankan Sur +4 more
doaj +1 more source

