Hot Spot Offset Variability from Magnetohydrodynamical Thermoresistive Instability in Hot Jupiters
Hot Jupiter (HJ) atmospheres are possibly subject to a thermoresistive instability (TRI). Such an instability may develop as the ohmic heating increases the electrical conductivity in a positive feedback loop, which ultimately leads to a runaway of the ...
Raphaël Hardy +2 more
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CHES: An astrometry mission searching for nearby habitable planets. [PDF]
Ji J, Wang S, Li H, Fang L, Li D.
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ATMOSPHERIC CHARACTERIZATION OF FIVE HOT JUPITERS WITH THE WIDE FIELD CAMERA 3 ON THEHUBBLE SPACE TELESCOPE [PDF]
Sukrit Ranjan +6 more
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Measuring the abundances of carbon- and oxygen-bearing molecules has been a primary focus in studying the atmospheres of hot Jupiters, as doing so can help constrain the carbon-to-oxygen (C/O) ratio.
Dare Bartelt +10 more
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CHEMICAL CONSEQUENCES OF THE C/O RATIO ON HOT JUPITERS: EXAMPLES FROM WASP-12b, COROT-2b, XO-1b, AND HD 189733b. [PDF]
Moses JI +3 more
europepmc +1 more source
Stellar clustering shapes the architecture of planetary systems. [PDF]
Winter AJ +3 more
europepmc +1 more source
Hints of a close outer companion to the ultra-hot Jupiter TOI-2109 b [PDF]
Jan‐Vincent Harre +88 more
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THERMAL PROCESSES GOVERNING HOT-JUPITER RADII [PDF]
David S. Spiegel, Adam Burrows
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The rotational and divergent components of atmospheric circulation on tidally locked planets. [PDF]
Hammond M, Lewis NT.
europepmc +1 more source
Strict Upper Limits on the Carbon-to-Oxygen Ratios of Eight Hot Jupiters from Self-Consistent Atmospheric Retrieval [PDF]
Björn Benneke
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