Suggested Topics within your search.
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Water, to feed the planet
Published 2014-07-01“… Water, to feed the planet …”
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A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey
Published 2025-01-01“…The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. …”
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The Epoch of Giant Planet Migration Planet Search Program. III. The Occurrence Rate of Young Giant Planets inside the Water Ice Line
Published 2025-01-01“…We present statistical results from the Epoch of Giant Planet Migration RV planet search program. This survey was designed to measure the occurrence rate of giant planets interior to the water ice line of young Sun-like stars, compare this to the prevalence of giant planets at older ages, and provide constraints on the timescale and dominant inward migration mechanism of giant planets. …”
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Secular Resonances in Planet-hosting Binary Stars. II. Application to Terrestrial Planet Formation
Published 2025-01-01Subjects: Get full text
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Prospects for the characterization of habitable planets
Published 2023-08-01Subjects: “…planets…”
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Crater Dimensions on the Dwarf Planets
Published 2025-01-01“…The icy dwarf planets of Pluto, Charon, and Ceres provide important geologic comparisons for each other as they possess similar gravities and experience impacts of similar velocities compared to larger planets and moons. …”
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Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ
Published 2025-01-01“…In this work, we attempt to amplify eccentricity tides with three previously ignored effects. (1) Planets tend to be inflated when they were younger. (2) Kepler-like planets likely form as resonant chains parked at the disk inner edge; overlooked inner planets could have contributed to tidal dissipation of the whole system. (3) Disk migration captures planets into first-order MMR with nonzero initial deviation Δ, thereby lowering the amount of dissipation needed. …”
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Planet–Planet Scattering and Von Zeipel–Lidov–Kozai Migration—The Dynamical History of HAT-P-11
Published 2025-01-01“…Here we propose a two-step dynamical process that can reproduce all intriguing aspects of the system. We first invoke planet–planet scattering to generate significant eccentricities and mutual inclinations between the planets. …”
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The True Stellar Obliquity of a Sub-Saturn Planet from the Tierras Observatory and the Keck Planet Finder
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Concealing Circumbinary Planets with Tidal Shrinkage
Published 2025-01-01“…Of the 14 transiting planets that have been detected orbiting eclipsing binaries (“circumbinary planets”), none have been detected with stellar binary orbital periods shorter than 7 days, despite such binaries existing in abundance. …”
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