Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1029/2020GL092128 |
Seeing Through the Atmosphere of Venus: What's on the Surface? | |
E. A. Cloutis | |
2021-01-12 | |
发表期刊 | Geophysical Research Letters |
出版年 | 2021 |
英文摘要 | The exploration of the surface geology of Venus has been hampered by its inhospitable conditions and thick and opaque atmosphere. Fundamental properties, such as crustal composition and heterogeneity remain poorly constrained. Multiple analytical techniques are required to better understand its geology. A spectroscopy‐based study laboratory study of the emissivity properties of Venus‐relevant igneous rocks, measured at 440 °C by Dyar et al. (2020b; https://doi.org/10.1029/2020GL090497) shows that the use of multiple atmospheric windows in the 1‐µm region can provide strong constraints on the FeO content of Venus‐relevant igneous rocks, and by extension, the type of igneous rock. These results will improve our ability to map the surface geology of Venus remotely. |
领域 | 气候变化 |
URL | 查看原文 |
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文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/311343 |
专题 | 气候变化 |
推荐引用方式 GB/T 7714 | E. A. Cloutis. Seeing Through the Atmosphere of Venus: What's on the Surface?[J]. Geophysical Research Letters,2021. |
APA | E. A. Cloutis.(2021).Seeing Through the Atmosphere of Venus: What's on the Surface?.Geophysical Research Letters. |
MLA | E. A. Cloutis."Seeing Through the Atmosphere of Venus: What's on the Surface?".Geophysical Research Letters (2021). |
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