金星的变形是地厚度和循环循环的驱动力
Julia Semprich1, Justin Filiberto2, Matthew Weller3,4
1AstrobiologyOU, School of Environment, Earth, and Ecosystem Science, The Open University, Milton Keynes, UK. julia.semprich@open.ac.uk.
维纳斯 维纳斯 维纳斯 维纳斯 维纳斯
科学领域:
- 行星科学 行星科学
- 地质地质地质地质地质地
- 地质物理学 地质物理学
背景情况:
- 金星的地厚度和构成仍然不太清楚.
- 热梯度和地力学设置对金星地的影响尚不清楚.
研究的目的:
- 为了确定金星的玄武岩地的最大可能的厚度.
- 研究不同构造体制和热梯度对地厚度的影响.
主要方法:
- 利用变态相位过渡来限制地的厚度.
- 使用融化的开始作为地厚度的限制因素.
主要成果:
- 由于分层,一个停滞的盖子制度与5°C/km的热梯度限制地厚度到~40公里.
- 带有25°C/km的热梯度的移动盖制度限制了地的厚度,由于化,地厚度为~20公里.
- 最大可能的基岩地厚度为~65公里,温度梯度为10°C/公里.
结论:
- 金星的玄武岩地厚度限制在20-65公里之间.
- 超过这些极限将引发分层,地回收或火山活动.
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