冥王星冰壳的厚度来自于Sputnik Planitia前盖的弹性变形:是对填充载荷的响应还是撞击事件的遗迹?

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
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引用次数: 0

摘要

行星岩石圈上的荷载通常会形成一个清晰的挠曲隆起,包括一个永久性(或持久性)的前隆起,它保留了关于荷载力和岩石圈本身特性的重要信息。在冥王星上,外层冰壳(即岩石圈)的各方面情况越来越容易确定,因为最近利用 "新视野 "号太空探测器的数据所做的工作揭示了正在进行的地表低温火山活动和地下水海的证据。然而,冰壳的确切厚度和弹性尚待完全确定。Sputnik Planitia 是冥王星上最大的表面特征之一,是一个椭圆形凹陷,可能是在撞击事件中形成的,随后被氮冰填充。它的特点是有一个光滑的、径向不对称的前凸起,沿着凹陷边界的一些地方还保留着前凸起。然而,冲击荷载和填充物引起的荷载对前凸形成的影响比例仍然未知。在此,我们报告了对 Sputnik Planitia 前凸起的分析结果,以探索冰壳和氮填充物的特征。通过在冥王星的材料和环境参数范围内利用多重聚合蒙特卡洛(CMC)模拟,最佳拟合挠曲面能够从十个剖面图中复制挠曲(包括前凸起)的地形。结果显示冰壳厚度在 65 至 90 千米之间,平均为 78 千米。冰壳的密度比地下水洋的密度低 50 千克/立方米。我们证明,如果前冰盖的形成完全是由氮冰填充负荷造成的,那么填充厚度必须达到 18 千米。此外,东南-西北中心对称负载可能是由东南-西北轨迹的撞击物体产生的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Thickness of Pluto's Ice Shell from elastic deformation of the Sputnik Planitia forebulge: Response to infill load or vestige of impact event?

Load on a planet's lithosphere can often form a well-defined flexural bulge, including a permanent (or long-lasting) forebulge, which preserves important information on the force of the load and properties of the lithosphere itself. On Pluto, aspects of the outer ice shell (i.e. the lithosphere) have become increasingly ascertainable, as recent work using data from the New Horizons space probe has revealed evidence of ongoing surface cryovolcanism and a subsurface water ocean. However, the precise thickness and elasticity of the ice shell has yet to be fully established. Sputnik Planitia, one of the largest surface features on Pluto, is an elliptical depression that may have formed during an impact event and subsequently infilled with nitrogen ice. It is characterized by a smooth, radially asymmetrical, forebulge which has been retained in places along the border of the depression. However, the proportion of influence on the formation of the forebulge between the impact load and the load induced by the infill remains unknown. Here, we report results from the analysis of the forebulge of Sputnik Planitia to explore the characteristics of the ice shell and the nitrogen infill. By utilizing multiple Converging Monte Carlo (CMC) simulations within the material and environmental parameters of Pluto, the best fit flexure surface was able to replicate the topography of the flexure (including the forebulge) from ten profiles. Results show an ice shell thickness ranging from 65 to 90 km, with an average of 78 km. The density of the ice shell is 50 kg/m3 less than the density of the subsurface water ocean. We demonstrate that if the formation of the forebulge occurs solely from the nitrogen ice infill load, the infill must reach >18 km of thickness. Furthermore, a southeast-northwest central load symmetry may have been produced by an impacting object with a southeast-northwest trajectory.

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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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