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  1. AU="S. Alan Stern"
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  3. AU="Claude, Pierre-Abel"
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  5. AU="Larkin, J"
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  1. Artikel ; Online: Triton

    Paul M. Schenk / Chloe B. Beddingfield / Tanguy Bertrand / Carver Bierson / Ross Beyer / Veronica J. Bray / Dale Cruikshank / William M. Grundy / Candice Hansen / Jason Hofgartner / Emily Martin / William B. McKinnon / Jeffrey M. Moore / Stuart Robbins / Kirby D. Runyon / Kelsi N. Singer / John Spencer / S. Alan Stern / Ted Stryk

    Remote Sensing, Vol 13, Iss 3476, p

    Topography and Geology of a Probable Ocean World with Comparison to Pluto and Charon

    2021  Band 3476

    Abstract: The topography of Neptune’s large icy moon Triton could reveal important clues to its internal evolution, but has been difficult to determine. New global digital color maps for Triton have been produced as well as topographic data for <40% of the surface ...

    Abstract The topography of Neptune’s large icy moon Triton could reveal important clues to its internal evolution, but has been difficult to determine. New global digital color maps for Triton have been produced as well as topographic data for <40% of the surface using stereogrammetry and photoclinometry. Triton is most likely a captured Kuiper Belt dwarf planet, similar though slightly larger in size and density to Pluto, and a likely ocean moon that exhibited plume activity during Voyager 2′s visit in 1989. No surface features or regional deviations of greater than ±1 km amplitude are found. Volatile ices in the southern terrains may take the form of extended lobate deposits 300–500 km across as well as dispersed bright materials that appear to embay local topography. Limb hazes may correlate with these deposits, indicating possible surface–atmosphere exchange. Triton’s topography contrasts with high relief up to 6 km observed by New Horizons on Pluto. Low relief of (cryo)volcanic features on Triton contrasts with high-standing massifs on Pluto, implying different viscosity materials. Solid-state convection occurs on both and at similar horizontal scales but in very different materials. Triton’s low relief is consistent with evolution of an ice shell subjected to high heat flow levels and may strengthen the case of an internal ocean on this active body.
    Schlagwörter Triton ; ocean world ; Neptune ; topography ; cartography ; Pluto ; Science ; Q
    Thema/Rubrik (Code) 551
    Sprache Englisch
    Erscheinungsdatum 2021-09-01T00:00:00Z
    Verlag MDPI AG
    Dokumenttyp Artikel ; Online
    Datenquelle BASE - Bielefeld Academic Search Engine (Lebenswissenschaftliche Auswahl)

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  2. Artikel ; Online: Large-scale cryovolcanic resurfacing on Pluto

    Kelsi N. Singer / Oliver L. White / Bernard Schmitt / Erika L. Rader / Silvia Protopapa / William M. Grundy / Dale P. Cruikshank / Tanguy Bertrand / Paul M. Schenk / William B. McKinnon / S. Alan Stern / Rajani D. Dhingra / Kirby D. Runyon / Ross A. Beyer / Veronica J. Bray / Cristina Dalle Ore / John R. Spencer / Jeffrey M. Moore / Francis Nimmo /
    James T. Keane / Leslie A. Young / Catherine B. Olkin / Tod R. Lauer / Harold A. Weaver / Kimberly Ennico-Smith

    Nature Communications, Vol 13, Iss 1, Pp 1-

    2022  Band 9

    Abstract: Giant icy volcanos (cryovolcanos) on Pluto are unique in the imaged solar system and provide evidence for unexpected, active geology late in Pluto’s history. ...

    Abstract Giant icy volcanos (cryovolcanos) on Pluto are unique in the imaged solar system and provide evidence for unexpected, active geology late in Pluto’s history.
    Schlagwörter Science ; Q
    Sprache Englisch
    Erscheinungsdatum 2022-03-01T00:00:00Z
    Verlag Nature Portfolio
    Dokumenttyp Artikel ; Online
    Datenquelle BASE - Bielefeld Academic Search Engine (Lebenswissenschaftliche Auswahl)

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