The Twin Sister Planets Venus and Earth: Why are they so different?
This book explains how it came to be that Venus and Earth, while very similar in chemical composition, zonation, size and heliocentric distance from the Sun, are very different in surface environmental conditions. It is argued here that these differences can be accounted for by planetoid capture pro...
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| Ngôn ngữ: | English |
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Springer
2016
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| Truy cập trực tuyến: | https://scholar.dlu.edu.vn/thuvienso/handle/DLU123456789/59955 |
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oai:scholar.dlu.edu.vn:DLU123456789-599552023-11-11T06:57:23Z The Twin Sister Planets Venus and Earth: Why are they so different? Malcuit, Robert Geography Earth Venus This book explains how it came to be that Venus and Earth, while very similar in chemical composition, zonation, size and heliocentric distance from the Sun, are very different in surface environmental conditions. It is argued here that these differences can be accounted for by planetoid capture processes and the subsequent evolution of the planet-satellite system. Venus captured a one-half moon-mass planetoid early in its history in the retrograde direction and underwent its “fatal attraction scenario” with its satellite (Adonis). Earth, on the other hand, captured a moon-mass planetoid (Luna) early in its history in prograde orbit and underwent a benign estrangement scenario with its captured satellite. 2016-03-31T02:14:38Z 2016-03-31T02:14:38Z 2015 Book 978-3-319-11388-3 978-3-319-11387-6 https://scholar.dlu.edu.vn/thuvienso/handle/DLU123456789/59955 en application/pdf Springer |
| institution |
Thư viện Trường Đại học Đà Lạt |
| collection |
Thư viện số |
| language |
English |
| topic |
Geography Earth Venus |
| spellingShingle |
Geography Earth Venus Malcuit, Robert The Twin Sister Planets Venus and Earth: Why are they so different? |
| description |
This book explains how it came to be that Venus and Earth, while very similar in chemical composition, zonation, size and heliocentric distance from the Sun, are very different in surface environmental conditions. It is argued here that these differences can be accounted for by planetoid capture processes and the subsequent evolution of the planet-satellite system. Venus captured a one-half moon-mass planetoid early in its history in the retrograde direction and underwent its “fatal attraction scenario” with its satellite (Adonis). Earth, on the other hand, captured a moon-mass planetoid (Luna) early in its history in prograde orbit and underwent a benign estrangement scenario with its captured satellite. |
| format |
Book |
| author |
Malcuit, Robert |
| author_facet |
Malcuit, Robert |
| author_sort |
Malcuit, Robert |
| title |
The Twin Sister Planets Venus and Earth:
Why are they so different? |
| title_short |
The Twin Sister Planets Venus and Earth:
Why are they so different? |
| title_full |
The Twin Sister Planets Venus and Earth:
Why are they so different? |
| title_fullStr |
The Twin Sister Planets Venus and Earth:
Why are they so different? |
| title_full_unstemmed |
The Twin Sister Planets Venus and Earth:
Why are they so different? |
| title_sort |
twin sister planets venus and earth:
why are they so different? |
| publisher |
Springer |
| publishDate |
2016 |
| url |
https://scholar.dlu.edu.vn/thuvienso/handle/DLU123456789/59955 |
| _version_ |
1819766430736842752 |