孪生世界,不同命运:斜度如何以不同方式塑造冥王星和海卫一的地貌和气候

Tanguy Bertrand, François Forget, Emmanuel Lellouch
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摘要

海卫一和冥王星被认为有着共同的起源,两者最初都形成于柯伊伯带,但海卫一后来被海王星捕获。这两个天体显示出相似的大小、密度以及大气和表面冰的构成,都存在挥发性冰N2、CH4和CO。然而,它们的外观,包括表面反照率和冰的分布却大相径庭。是什么原因造成了这些不同的表象呢?第一个差异是,由于围绕海王星运行,三体星正经历着显著的潮汐加热,随后重新浮出水面,表面相对平坦,而冥王星没有潮汐作用,显示出明显的地形。在这里,我们使用相同的初始条件和挥发物清单,但根据每个天体的已知轨道和旋转情况,对冥王星和海卫一进行了长期挥发物迁移模拟。该模型一阶再现了冥王星和海卫一上观测到的挥发性冰表面分布。我们的研究结果清楚地表明,倾斜度是冥王星和海卫一表面外观和气候特性差异的主要驱动因素,并进一步支持了这两个天体具有共同起源和不同动力学历史的假设。
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Twin Worlds, Divergent Fates: How Obliquity has differently shaped Pluto's and Triton's landscapes and climates
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.
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