ORCHARD is a new open code that models planetary evolution and structure across terrestrial to gas giant masses using multiple equations of state and atmospheric boundary conditions.
The Astrophysical Journal756(1), 90 (2012)
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The disk instability model remains viable for explaining giant planets that form early, at large orbital distances, and around M-dwarf stars, supported by updated simulations and observations.
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ORCHARD: A General Planetary Evolution Code
ORCHARD is a new open code that models planetary evolution and structure across terrestrial to gas giant masses using multiple equations of state and atmospheric boundary conditions.
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Giant Planet Formation by Disk Instability
The disk instability model remains viable for explaining giant planets that form early, at large orbital distances, and around M-dwarf stars, supported by updated simulations and observations.