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在冥王星上的Sputnik Planitia中以升华驱动的对流
Adrien Morison1, Stéphane Labrosse2, Gaël Choblet3
1Physics and Astronomy, University of Exeter, Exeter, UK.
Nature
|December 16, 2021
概括
化驱动的对流解释了Sputnik Planitia在冥王星上的多边形表面模式. 这个过程需要较低的基底热流或较高的粘度对比度在冰层内.
科学领域:
- 星球科学
- 地质学
- 表面过程
背景情况:
- 冥王星上的Sputnik Planitia具有独特的多边形表面图案.
- 以往涉及固态对流的模型未能复制观察到的平面多边形和窄槽的地形.
研究的目的:
- 调查表面化在Sputnik Planitia的冰盆内推动对流的作用.
- 为了使对流模型与观察到的表面形态相协调.
主要方法:
- 在冥王星的Sputnik Planitia中对流过程的数值建模.
- 对不同基底热量流和冰粘度对比对表面图案的影响的分析.
主要成果:
- 化驱动的对流成功地重现了观察到的多边形结构.
- 该模型表明基底热量比以前接受的值低 (~0.3 mW m-2).
- 另外,通常接受的热流量 (2-3 mW m−2) 可以维持这些模式,具有显著更高的粘度对比度 (~3,000).
结论:
- 表面升华是推动对流和塑造Sputnik Planitia表面的一个关键机制.
- 这些发现表明我们对冥王星冰中的热流和物质特性有了更好的理解.
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