太极星的晚期形成与早期火星的影响
Sylvain Bouley1,2, David Baratoux3,4, Isamu Matsuyama5
1GEOPS-Géosciences Paris Sud, Université Paris-Sud, CNRS, Université Paris-Saclay, Rue du Belvédère, Bâtiment 504-509, 91405 Orsay, France.
Nature
|March 3, 2016
概括
火星的塔尔西斯火山区域可能没有影响早期的山谷网络. 新模型表明,在塔尔西斯形成之前,地形学解释了早期火星上的山谷方位和水分分布.
科学领域:
- 星球科学
- 地质学
- 气候科学
背景情况:
- 太阳系最大的火山群, 经过数十亿年的发展.
- 它的巨大质量被认为导致了真正的极地流浪 (TPW),重新定位了火星,并将塔尔西斯定位在赤道附近.
- 之前的理论提出了Tharsis影响了早期火星山谷网络的方向.
研究的目的:
- 探究塔尔西斯火山负载对早期火星山谷网络方向的影响.
- 为了重建火星的地形和旋转图形,
- 测试Tharsis前的地形是否可以解释观测到的山谷网络模式.
主要方法:
- 在 Tharsis 形成之前计算了火星的旋转图形 (平衡形状).
- 在Tharsis之前重建了地球表面的地形,
- 分析了地形梯度,并将它们与观测到的山谷网络方向进行了比较.
主要成果:
- 观测到的山谷网络方向与火星上的地形梯度一致.
- 在TPW前的框架中,山谷分布与南半球的度带保持一致.
- 基于TPW前的地形,气候模型预测了该带的偏好冰/水积累.
结论:
- 不需要太西斯载荷来解释早期火星山谷网络的方向.
- 达尔西斯的晚期生长阶段与谷间的切割同时发生,对火星的早期地质和气候有重大影响.
- 这一修订的时间表表明了潜在的冰川环境,并将火山排气与地表水的稳定性联系起来.
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