Results 91 to 100 of about 740,794 (260)

Characterizing the Atmospheric Dynamics of HD 209458b-like Hot Jupiters Using AI-driven Image Recognition/Categorization

open access: yesThe Astrophysical Journal, 2023
In order to understand the results of recent observations of exoplanets, models have become increasingly complex. Unfortunately, this increases both the computational cost and output size of said models.
F. Sainsbury-Martinez   +5 more
doaj   +1 more source

Atmospheric Circulation of Terrestrial Exoplanets [PDF]

open access: yes, 2013
The investigation of planets around other stars began with the study of gas giants, but is now extending to the discovery and characterization of super-Earths and terrestrial planets. Motivated by this observational tide, we survey the basic dynamical principles governing the atmospheric circulation of terrestrial exoplanets, and discuss the ...
Showman, Adam P.   +3 more
openaire   +4 more sources

Spectral Retrieval with JWST Photometric data: a Case Study for HIP 65426 b

open access: yesThe Astronomical Journal, 2023
Half of the JWST high-contrast imaging objects will only have photometric data as of Cycle 2. However, to better understand their atmospheric chemistry that informs formation origin, spectroscopic data are preferred.
Ji Wang
doaj   +1 more source

Outstanding Challenges of Exoplanet Atmospheric Retrievals [PDF]

open access: yesSpace Science Reviews, 2020
Spectral retrieval has long been a powerful tool for interpreting planetary remote sensing observations. Flexible, parameterised, agnostic models are coupled with inversion algorithms in order to infer atmospheric properties directly from observations, with minimal reliance on physical assumptions. This approach, originally developed for application to
Kevin Heng   +2 more
openaire   +5 more sources

Exoplanet albedo spectra and colors as a function of planet phase, separation, and metallicity [PDF]

open access: yes, 2010
First generation optical coronagraphic telescopes will obtain images of cool gas and ice giant exoplanets around nearby stars. The albedo spectra of exoplanets at planet-star separations larger than about 1 AU are dominated by reflected light to beyond 1
Ackerman   +58 more
core   +2 more sources

Clouds in Exoplanetary Atmospheres [PDF]

open access: yes, 2020
Today, we know ~4330 exoplanets orbiting their host stars in ~3200 planetary systems. The diversity of these exoplanets is large, and none of the known exoplanets is a twin to any of the solar system planets, nor is any of the known extrasolar planetary systems a twin of the solar system.
arxiv   +1 more source

Controls of Atmospheric Methane on Early Earth and Inhabited Earth-like Terrestrial Exoplanets [PDF]

open access: yes, 2023
Methane (CH4) is a primarily biogenic greenhouse gas. As such, it represents an essential biosignature to search for life on exoplanets. Atmospheric CH4 abundance on Earth-like inhabited exoplanets is likely controlled by marine biogenic production and atmospheric photochemical consumption.
arxiv   +1 more source

The spectrum of hot methane in astronomical objects using a comprehensive computed line list [PDF]

open access: yes, 2014
Hot methane spectra are important in environments ranging from flames to the atmospheres of cool stars and exoplanets. A new spectroscopic line list, 10to10, for $^{12}$CH$_4$ containing almost 10 billion transitions is presented. This comprehensive line
Bailey, Jeremy   +4 more
core   +2 more sources

Retrieving Temperatures and Abundances of Exoplanet Atmospheres with High-resolution Cross-correlation Spectroscopy [PDF]

open access: yesAstronomical Journal, 2018
High-resolution spectroscopy (R ≥ 25,000) has recently emerged as one of the leading methods for detecting atomic and molecular species in the atmospheres of exoplanets.
M. Brogi, M. Line
semanticscholar   +1 more source

Hα Absorption in Transiting Exoplanet Atmospheres [PDF]

open access: yesProceedings of the International Astronomical Union, 2013
AbstractRecent observations by Jensen et al. of Hα absorption by the upper atmosphere of HD189733b have motivated the need for a theoretical understanding of the distribution of n=2 hydrogen within hot Jupiter atmospheres. With this in mind, we model the n=2 state of atomic hydrogen in a hydrostatic atmosphere in thermal and photoionization equilibrium.
Phil Arras, Zhi-Yun Li, Duncan Christie
openaire   +5 more sources

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