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    "info": {
        "author": "Kaloyan Penev",
        "author_email": "kpenev@gmail.com",
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        "description": "===================================================================\nPOET: (P)lanetary (O)orbital (E)volution due to (T)ides on evolving stars :\npython interface\n===================================================================\n\nFor a system consisting of a star and a single planet in a circular orbit\naligned with the stellar rotation, calculate the evolution of the semimajor\naxis and the rotation of the star. If the star has a mass below 1.1 solar\nmasses, the rotation of the radiative core and the convective envelope are\nevolved separately. The following physics is included:\n    * The evolution of the semimajor axis of the orbit due to the tidal\n      dissipation in the star.\n    * The evolution of the angular momentum of the stellar convective\n      envelope by the tidal coupling.\n    * The transfer of angular momentum between the stellar convective and\n      radiative zones.\n    * The effect of the stellar evolution on the tidal dissipation\n      efficiency, and stellar core and envelope spins.\n    * The loss of stellar convective zone angular momentum to a magnetically\n      launched wind.",
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        "name": "POET",
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        "summary": "Calculate the orbital evolution of a planet-star system.",
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