Results 131 to 140 of about 15,442 (228)
JWST/NIRISS Reveals the Water-rich “Steam World” Atmosphere of GJ 9827 d
With sizable volatile envelopes but smaller radii than the solar system ice giants, sub-Neptunes have been revealed as one of the most common types of planet in the galaxy. While the spectroscopic characterization of larger sub-Neptunes (2.5–4 R _⊕ ) has
Caroline Piaulet-Ghorayeb +32 more
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Seasonal Changes in the Atmosphere of HD 80606 b Observed with JWST’s NIRSpec/G395H
High-eccentricity gas giant planets serve as unique laboratories for studying the thermal and chemical properties of H/He-dominated atmospheres. One of the most extreme cases is HD 80606 b—a hot Jupiter orbiting a Sun-like star with an eccentricity of 0 ...
James T. Sikora +13 more
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Challenge of direct imaging of exoplanets within structures: disentangling real signal from point source from background light [PDF]
Jialin Li +21 more
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Limb-resolved transmission spectroscopy has the potential to transform our understanding of exoplanetary atmospheres. By separately measuring the transmission spectra of the evening and morning limbs, these atmospheric regions can be individually ...
Matthew M. Murphy +18 more
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Aerosols and clouds are expected to be ubiquitous in exoplanet and brown dwarf atmospheres, where they can have a significant impact on transmission and emission spectra.
Matt G. Lodge +4 more
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Structure and evolution of the first CoRoT exoplanets: probing the brown dwarf/planet overlapping mass regime [PDF]
Jérémy Leconte +4 more
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TOI-6324 b: An Earth-mass Ultra-short-period Planet Transiting a Nearby M Dwarf
We report the confirmation of TOI-6324 b, an Earth-sized (1.059 ± 0.041 R _⊕ ) ultra-short-period (USP) planet orbiting a nearby (∼20 pc) M dwarf. Using the newly commissioned Keck Planet Finder spectrograph, we have measured the mass of TOI-6324 b 1.17 ±
Rena A. Lee +73 more
doaj +1 more source
Potential Interior Structures and Habitability of Super-Earth Exoplanets LHS 1140 b, K2-18 b, TOI-1452 b and TOI-1468 c [PDF]
Mangesh Daspute +5 more
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Exoplanet Technosignature Detection of Orbital Terraforming Mirror Structures
The search for technosignatures no longer rests solely on radio signals. Modern wide-field surveys now make it possible to detect engineered structures at interstellar distances. Among the most promising of these are space-based mirrors, as large reflective constructs designed to manipulate planetary climates by increasing or reducing incoming sunlight.
openaire +1 more source

