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| DOI | 10.1126/science.259.5097.915 |
| Atmospheric evolution of the terrestrial planets | |
| Hunten D.M. | |
| 发表日期 | 1993 |
| ISSN | 0036-8075 |
| 起始页码 | 915 |
| 结束页码 | 920 |
| 卷号 | 259期号:5097 |
| 英文摘要 | The major atmospheric gases on Earth, Venus, and Mars were probably CO2, H2O, and N2. Most of the Earth's CO2 is tied up in minerals such as limestone, and Venus has lost most of its H2O, leaving the CO2 in the atmosphere. Much of Mars' atmosphere may have been eroded in impacts by large meteoroids early in solar-system history. Noble gases are very underabundant everywhere, and must have been lost during an early period; they were probably dragged along during rapid loss of massive amounts of hydrogen. The tenuous atmospheres of Mercury and the moon have lifetimes of a few days or less and must be continuously replenished from internal or external sources. |
| 英文关键词 | atmosphere; carbon dioxide; greenhouse effect; terrestrial planet |
| 语种 | 英语 |
| 来源期刊 | Science
 |
| 文献类型 | 期刊论文 |
| 条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/244104 |
| 作者单位 | Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, United States |
| 推荐引用方式 GB/T 7714 | Hunten D.M.. Atmospheric evolution of the terrestrial planets[J],1993,259(5097). |
| APA | Hunten D.M..(1993).Atmospheric evolution of the terrestrial planets.Science,259(5097). |
| MLA | Hunten D.M.."Atmospheric evolution of the terrestrial planets".Science 259.5097(1993). |
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