Tanguy Bertrand, François Forget, Emmanuel Lellouch
{"title":"Twin Worlds, Divergent Fates: How Obliquity has differently shaped Pluto's and Triton's landscapes and climates","authors":"Tanguy Bertrand, François Forget, Emmanuel Lellouch","doi":"arxiv-2409.01122","DOIUrl":null,"url":null,"abstract":"Triton and Pluto are believed to share a common origin, both forming\ninitially in the Kuiper Belt but Triton being later captured by Neptune. Both\nobjects display similar sizes, densities, and atmospheric and surface ice\ncomposition, with the presence of volatile ices N2, CH4 and CO. Yet their\nappearance, including their surface albedo and ice distribution strongly\ndiffer. What can explain these different appearances? A first disparity is that\nTriton is experiencing significant tidal heating due to its orbit around\nNeptune, with subsequent resurfacing and a relatively flat surface, while Pluto\nis not tidally activated and displays a pronounced topography. Here we present\nlong-term volatile transport simulations of Pluto and Triton, using the same\ninitial conditions and volatile inventory, but with the known orbit and\nrotation of each object. The model reproduces, to first order, the observed\nvolatile ice surface distribution on Pluto and Triton. Our results\nunambiguously demonstrate that obliquity is the main driver of the differences\nin surface appearance and in climate properties on Pluto and Triton, and give\nfurther support to the hypothesis that both objects had a common origin\nfollowed by a different dynamical history.","PeriodicalId":501209,"journal":{"name":"arXiv - PHYS - Earth and Planetary Astrophysics","volume":"50 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Earth and Planetary Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.01122","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Triton and Pluto are believed to share a common origin, both forming
initially in the Kuiper Belt but Triton being later captured by Neptune. Both
objects display similar sizes, densities, and atmospheric and surface ice
composition, with the presence of volatile ices N2, CH4 and CO. Yet their
appearance, including their surface albedo and ice distribution strongly
differ. What can explain these different appearances? A first disparity is that
Triton is experiencing significant tidal heating due to its orbit around
Neptune, with subsequent resurfacing and a relatively flat surface, while Pluto
is not tidally activated and displays a pronounced topography. Here we present
long-term volatile transport simulations of Pluto and Triton, using the same
initial conditions and volatile inventory, but with the known orbit and
rotation of each object. The model reproduces, to first order, the observed
volatile ice surface distribution on Pluto and Triton. Our results
unambiguously demonstrate that obliquity is the main driver of the differences
in surface appearance and in climate properties on Pluto and Triton, and give
further support to the hypothesis that both objects had a common origin
followed by a different dynamical history.