冰川的静态调整揭示了火星的内部粘度结构
A Broquet1, A-C Plesa2, V Klemann3
1Institute for Planetary Research, German Aerospace Center, DLR, Berlin, Germany. adrien.broquet@dlr.de.
Nature
|February 26, 2025
概括
火星
科学领域:
- 星球科学
- 地质学
- 冰川学
背景情况:
- 冰川静态调整 (GIA) 是理解行星粘度的关键.
- 在其他行星上,由于观测数据有限,GIA研究很罕见.
- 火星的北极帽是GIA分析的独特特征.
研究的目的:
- 调查火星北极冰盖的位置.
- 确定火星当前的内部粘度结构.
- 限制使用新数据的GIA模型.
主要方法:
- 综合热进化模型
- 粘弹性变形计算
- 对雷达观测,重力场数据和地震数据的分析.
主要成果:
- 在火星的北方地区持续下降.
- 需要高粘度 (2-6 × 10^22 Pa·s在500公里以下).
- 模型与厚厚的地 (>40公里) 和枯竭的地幔 (>90%的放射性元素) 相一致.
结论:
- 火星的北极帽形成于1.7×12.0亿年前.
- 石质层变形小于0.13毫米/年.
- 未来的重力任务将进一步限制火星GIA.
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