Results 71 to 80 of about 2,846 (170)
Unraveling the evolution of hot Jupiter systems under the effect of tidal and magnetic interactions and mass loss [PDF]
Yaroslav A. Lazovik
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Investigating the Origins of Hot Neptunes from Radial Velocity Data
Hot Neptunes are extrasolar planets that are similar in size to Neptune in our solar system but are much closer to their host stars, completing an orbit in 10 days or less. The origin of hot Neptunes is not fully understood.
Sophie Y. Zheng
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Warm Jupiters with orbital periods of ≈10–365 days represent a population of giant planets located well within the water ice line but beyond the region of tidal influence of their host star relevant for high-eccentricity tidal migration.
Marvin Morgan +2 more
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Two-dimensional Models of Microphysical Clouds on Hot Jupiters. I. Cloud Properties
We present a new two-dimensional, bin-scheme microphysical model of cloud formation in the atmospheres of hot Jupiters that includes the effects of longitudinal gas and cloud transport.
Diana Powell, Xi Zhang
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Constraints onTESSalbedos for five hot Jupiters [PDF]
Martin Blažek +12 more
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The ExoEcho project is designed to study the photodynamics of exoplanets by leveraging high-precision transit timing data from ground- and space-based telescopes.
Xinyue Ma +8 more
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A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion [PDF]
David K. Sing +20 more
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The Aligned Orbit of a Hot Jupiter around the M Dwarf TOI-4201
Measuring the obliquities of stars hosting giant planets may shed light on the dynamical history of planetary systems. Significant efforts have been made to measure the obliquities of FGK stars with hot Jupiters, mainly based on observations of the ...
Tianjun Gan +14 more
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