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  1. 1

    The Water Planet / by Feather, Ralph M.

    View in OPAC
    Book
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    Digital Planet : tomorrow's technology and you / by Beekman, George

    Published 2014
    View in OPAC
    Book
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    Planet City by Liam Young

    Published 2021-12-01
    Subjects:
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    Article
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    Water, to feed the planet by Romano Prodi

    Published 2014-07-01
    “… Water, to feed the planet …”
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    Article
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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 by Quang H. Tran, Brendan P. Bowler, William D. Cochran, Chad F. Bender, Samuel Halverson, Suvrath Mahadevan, Joe P. Ninan, Paul Robertson, Arpita Roy, Guðmundur Stefánsson, Ryan C. Terrien

    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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    Article
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    Crater Dimensions on the Dwarf Planets by Veronica J. Bray, Michael F. Zeilnhofer, S. J. Robbins, P. M. Schenk, Kelsi M. Singer, O. L. White, S. A. Stern, S. D. Benecchi, K. A. Durfey, H. A. Weaver, C. B. Olkin, J. R. Spencer, the New Horizons Geology and Geophysics Investigation Team

    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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    Article
  15. 15

    Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ by Yuancheng Xu, Fei Dai

    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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    PlanetPlanet Scattering and Von Zeipel–Lidov–Kozai Migration—The Dynamical History of HAT-P-11 by Tiger Lu, Qier An, Gongjie Li, Sarah C. Millholland, Malena Rice, G. Mirek Brandt, Timothy D. Brandt

    Published 2025-01-01
    “…Here we propose a two-step dynamical process that can reproduce all intriguing aspects of the system. We first invoke planetplanet scattering to generate significant eccentricities and mutual inclinations between the planets. …”
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    Article
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    Concealing Circumbinary Planets with Tidal Shrinkage by Saahit Mogan, J.J. Zanazzi

    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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    Article