Triton: Topography and Geology of a Probable Ocean World with Comparison to Pluto and Charon
暂无分享,去创建一个
Jason Hofgartner | Candice Hansen | Dale Cruikshank | Kirby Runyon | Paul Schenk | Chloe Beddingfield | Tanguy Bertrand | Carver Bierson | Ross Beyer | Veronica Bray | William Grundy | Emily Martin | William McKinnon | Jeffrey Moore | Stuart Robbins | Kelsi Singer | John Spencer | S. Stern | Ted Stryk | C. Hansen | J. Moore | R. Beyer | K. Runyon | S. Robbins | D. Cruikshank | W. McKinnon | E. Martin | V. Bray | T. Stryk | J. Hofgartner | K. Singer | T. Bertrand | C. Bierson | C. Beddingfield | J. Spencer | Paul Schenk | S. Stern | William Grundy | P. Schenk
[1] F. Nimmo,et al. Pluto’s ocean is capped and insulated by gas hydrates , 2019, Nature Geoscience.
[2] D. Reuter,et al. Pluto’s global surface composition through pixel-by-pixel Hapke modeling of New Horizons Ralph/LEISA data , 2016, 1604.08468.
[3] S. K. Croft,et al. Voyager 2 at Neptune: Imaging Science Results , 1989, Science.
[4] T. Lauer,et al. A search for temporal changes on Pluto and Charon , 2016, 1711.02750.
[5] Jeffrey S. Kargel,et al. The geology of Triton. , 1995 .
[6] R. Brasser,et al. The origin of the cratering asymmetry on Triton , 2019, Monthly Notices of the Royal Astronomical Society.
[7] R. Canup,et al. ON A GIANT IMPACT ORIGIN OF CHARON, NIX, AND HYDRA , 2011 .
[8] T. Lauer,et al. The geology of Pluto and Charon through the eyes of New Horizons , 2016, Science.
[9] G. A. Macdonald. Pahoehoe, aa, and block lava , 1953 .
[10] Sona Hosseini,et al. The NASA Roadmap to Ocean Worlds , 2018, Astrobiology.
[11] D. Reuter,et al. Geology before Pluto: Pre-encounter considerations , 2014 .
[12] W. Grundy,et al. Near-infrared spectral monitoring of Triton with IRTF/SpeX II: Spatial distribution and evolution of ices , 2009, 0908.2623.
[13] Douglas P. Hamilton,et al. Neptune's capture of its moon Triton in a binary–planet gravitational encounter , 2006, Nature.
[14] W. McKinnon,et al. On the origin of Triton and Pluto , 1984, Nature.
[15] J. Moore,et al. Topography and geology of Uranian mid-sized icy satellites in comparison with Saturnian and Plutonian satellites , 2020, Philosophical Transactions of the Royal Society A.
[16] O. Umurhan,et al. Convection in a volatile nitrogen-ice-rich layer drives Pluto’s geological vigour , 2016, Nature.
[17] S. Kieffer,et al. Triton's plumes: Discovery, characteristics, and models , 1995 .
[18] Tod R. Lauer,et al. Basins, fractures and volcanoes: Global cartography and topography of Pluto from New Horizons , 2018, Icarus.
[19] N. Awasthi,et al. Toothpaste lava from the Barren Island volcano (Andaman Sea) , 2011 .
[20] T. Spohn,et al. Subsurface oceans and deep interiors of medium-sized outer planet satellites and large trans-neptunian objects , 2006 .
[21] F. Nimmo,et al. Evidence for a hot start and early ocean formation on Pluto , 2020, Nature Geoscience.
[22] R. Canup,et al. A Giant Impact Origin of Pluto-Charon , 2005, Science.
[23] R. Brasser,et al. Reassessing the origin of Triton , 2011, 1105.1179.
[24] B. Buratti,et al. The spatial distribution of UV-absorbing regions on Triton , 1996 .
[25] P. Spudis,et al. Impact melt flows at Lowell crater , 2014 .
[26] P. Thomas. The Shape of Triton from Limb Profiles , 2000 .
[27] J. Veverka,et al. Large Quasi-Circular Features Beneath Frost on Triton , 1992, Science.
[28] K. Zahnle,et al. On the negligible surface age of Triton , 2007 .
[29] A. McEwen,et al. Surface and Airborne Evidence for Plumes and Winds on Triton , 1990, Science.
[30] R. H. Brown,et al. Triton's Geyser-Like Plumes: Discovery and Basic Characterization , 1990, Science.
[31] B. J. Holler,et al. On the surface composition of Triton’s southern latitudes , 2015, 1508.05924.
[32] J. Moore,et al. The nature and origin of Charon's smooth plains , 2018, Icarus.
[33] H. Melosh,et al. Vigorous convection as the explanation for Pluto’s polygonal terrain , 2016, Nature.
[34] T. Lauer,et al. Breaking up is hard to do: Global cartography and topography of Pluto's mid-sized icy Moon Charon from New Horizons , 2018, Icarus.
[35] F. Forget,et al. Observed glacier and volatile distribution on Pluto from atmosphere–topography processes , 2016, Nature.
[36] O. Umurhan,et al. Pluto: Pits and mantles on uplands north and east of Sputnik Planitia , 2017 .
[37] T. Lauer,et al. Impact craters on Pluto and Charon indicate a deficit of small Kuiper belt objects , 2016, Science.
[38] James Roberts,et al. Sustainability of a subsurface ocean within Triton's interior , 2012 .
[39] D. E. Jennings,et al. Surface compositions across Pluto and Charon , 2016, Science.
[40] W. McKinnon,et al. Triton’s Surface Age and Impactor Population Revisited in Light of Kuiper Belt Fluxes: Evidence for Small Kuiper Belt Objects and Recent Geological Activity , 1999, astro-ph/9910435.
[41] D. Cruikshank. Triton, Pluto, Centaurs, and Trans-Neptunian Bodies , 2005 .
[42] F. Nimmo,et al. Powering Triton's recent geological activity by obliquity tides: Implications for Pluto geology , 2014 .
[43] T. Owen,et al. Ices on the Surface of Triton , 1993, Science.