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The Role of Atmospheric Composition in Defining the Habitable Zone Limits and Supporting E. coli Growth [PDF]

open access: yesLife
Studying exoplanet atmospheres is essential for assessing their potential to host liquid water and their capacity to support life (their habitability).
Asena Kuzucan   +6 more
doaj   +2 more sources

Model atmospheres of irradiated exoplanets: The influence of stellar parameters, metallicity, and the C/O ratio [PDF]

open access: yes, 2015
Many parameters constraining the spectral appearance of exoplanets are still poorly understood. We therefore study the properties of irradiated exoplanet atmospheres over a wide parameter range including metallicity, C/O ratio and host spectral type.
Dullemond, Cornelis Petrus   +4 more
core   +2 more sources

Observations of Exoplanet Atmospheres [PDF]

open access: yes, 2015
Detailed characterization of an extrasolar planet's atmosphere provides the best hope for distinguishing the makeup of its outer layers, and the only hope for understanding the interplay between initial composition, chemistry, dynamics & circulation, and
Crossfield, Ian J. M.
core   +2 more sources

Earth shaped by primordial H_2 atmospheres [PDF]

open access: yesNature, 2023
Thermodynamic modelling shows that Earth’s water, core density and overall oxidation state can be explained by the formation of Earth from planetary embryos with hydrogen-rich primary atmospheres and underlying magma oceans.
E. Young, A. Shahar, H. Schlichting
semanticscholar   +1 more source

The Sonora Brown Dwarf Atmosphere and Evolution Models. I. Model Description and Application to Cloudless Atmospheres in Rainout Chemical Equilibrium [PDF]

open access: yesAstrophysical Journal, 2021
We present a new generation of substellar atmosphere and evolution models, appropriate for application to studies of L-, T-, and Y-type brown dwarfs and self-luminous extrasolar planets.
M. Marley   +10 more
semanticscholar   +1 more source

Atmospheres of Rocky Exoplanets [PDF]

open access: yes, 2021
Rocky planets are common around other stars, but their atmospheric properties remain largely unconstrained. Thanks to a wealth of recent planet discoveries and upcoming advances in observing capability, we are poised to characterize the atmospheres of ...
R. Wordsworth, L. Kreidberg
semanticscholar   +1 more source

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) [PDF]

open access: yesAstronomy & Astrophysics, 2020
Ultra-hot Jupiters offer interesting prospects for expanding our theories on dynamical evolution and the properties of extremely irradiated atmospheres.
V. Bourrier   +23 more
semanticscholar   +1 more source

The Surprising Roles of Turbulence in Tropical Cyclone Physics

open access: yesAtmosphere, 2023
Tropical cyclones have long been known to be powered by turbulent enthalpy fluxes from the ocean’s surface and slowed by turbulent momentum fluxes into the surface.
Kerry Emanuel   +2 more
doaj   +1 more source

How Well do We Understand the Planck Feedback?

open access: yesJournal of Advances in Modeling Earth Systems, 2023
A reference or “no‐feedback” radiative response to warming is fundamental to understanding how much global warming will occur for a given change in greenhouse gases or solar radiation incident on the Earth.
Timothy W. Cronin, Ishir Dutta
doaj   +1 more source

Light absorption by pollution, dust, and biomass burning aerosols: a global model study and evaluation with AERONET measurements [PDF]

open access: yesAnnales Geophysicae, 2009
Atmospheric aerosol distributions from 2000 to 2007 are simulated with the Goddard Chemistry Aerosol Radiation and Transport (GOCART) model to attribute light absorption by aerosol to its composition and sources from pollution, dust, and biomass ...
Mian Chin   +9 more
doaj   +1 more source

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