Results 101 to 110 of about 9,564 (167)
We present high-resolution optical emission spectroscopy observations of the ultrahot Jupiters (UHJs) TOI-1431 b and TOI-1518 b using the PEPSI spectrograph on the LBT.
Sydney Petz +6 more
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Coupled Planetary Interior and Tidal Evolution
We present a new planetary structure/thermal evolution model, designed for use in problems that couple orbital dynamics with planetary structure. We first benchmark our structural/thermal evolution calculations against the MESA stellar evolution code ...
Tim Hallatt, Sarah Millholland
doaj +1 more source
Not All Sub-Neptune Exoplanets Have Magma Oceans
The evolution and structure of sub-Neptunes may be strongly influenced by interactions between the outer gaseous envelope of the planet and a surface magma ocean.
Bodie Breza +2 more
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Puffy Venuses: The Mass–Radius Impact of Carbon-rich Atmospheres on Lava Worlds
The recent advancements in exoplanet observations enable the potential detection of exo-Venuses, rocky planets with carbon-rich atmospheres. How extended these atmospheres can be, given high carbon abundances, has not been studied.
Bo Peng, Diana Valencia
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The JWST Rocky Worlds DDT Program Reveals GJ 3929b to Likely Be a Bare Rock
We report first results from the JWST Rocky Worlds Director’s Discretionary Time program. Two secondary eclipses of the terrestrial exoplanet GJ 3929b were recently observed using MIRI photometric imaging at 15 μ m.
Qiao Xue +16 more
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The disintegrating ultrashort period rocky exoplanet K2-22 b periodically emits dusty clouds in a dynamically chaotic process resulting in a variable transit depth from 0% to 1.3%.
Nick Tusay +14 more
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Magma Ocean Interactions Can Explain JWST Observations of the Sub-Neptune TOI-270 d
Sub-Neptunes with substantial atmospheres may possess magma oceans in contact with the overlying gas, with chemical interactions between the atmosphere and magma playing an important role in shaping atmospheric composition.
Matthew C. Nixon +11 more
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The Uncertainty in Water Mass Fraction of Wet Planets
Planets with masses between Earth and Neptune often have radii that imply the presence of volatiles, suggesting that water may be abundant in their interiors.
Michael Lozovsky
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High-resolution spectroscopy (HRS) of exoplanet atmospheres has successfully detected many chemical species and is quickly moving toward detailed characterization of the chemical abundances and dynamics.
Lennart van Sluijs +6 more
doaj +1 more source
Impact of oxygen fugacity on atmospheric structure and emission spectra of ultra hot rocky exoplanets [PDF]
Fabian L. Seidler +2 more
openalex +1 more source

