File:EuropaInterior1.jpg
原始文件 (1,192 × 1,636像素,文件大小:696 KB,MIME类型:image/jpeg)
说明
摘要
[编辑]描述EuropaInterior1.jpg |
Model of Europa's subsurface structure. Original caption released with image: These artist's drawings depict two proposed models of the subsurface structure of the Jovian moon, Europa. Geologic features on the surface, imaged by the Solid State Imaging (SSI) system on NASA's Galileo spacecraft might be explained either by the existence of a warm, convecting ice layer, located several kilometers below a cold, brittle surface ice crust (top model), or by a layer of liquid water with a possible depth of more than 100 kilometers(bottom model). If a 100 kilometer (60 mile) deep ocean existed below a 15 kilometer (10 mile) thick Europan ice crust, it would be 10 times deeper than any ocean on Earth and would contain twice as much water as Earth's oceans and rivers combined. Unlike the Earth, magnesium sulfate might be a major salt component of Europa's water or ice, while the Earth's oceans are salty due to sodium chloride (common salt). While data from various instruments on the Galileo spacecraft indicate that an Europan ocean might exist, no conclusive proof has yet been found. To date Earth is the only known place in the solar system where large masses of liquid water are located close to a solid surface. Other sources are especially interesting since water is a key ingredient for the development of life as we know it. |
日期 |
|
来源 |
Transferred from en.wikipedia to Commons. Transfer was stated to be made by User:Mu301.
|
作者 | NASA/JPL |
其他版本 | Derivative works of this file: EuropaInterior1 cs.jpg |
此标签不表示文件的著作权状态。任何文件在附有此标签的同時还需要一个有效的著作权标签。请参阅许可协议说明页面以了解更多信息。 其他语言:
العربية ∙ беларуская (тарашкевіца) ∙ български ∙ català ∙ čeština ∙ dansk ∙ Deutsch ∙ English ∙ español ∙ فارسی ∙ français ∙ galego ∙ magyar ∙ հայերեն ∙ Bahasa Indonesia ∙ italiano ∙ 日本語 ∙ македонски ∙ മലയാളം ∙ Nederlands ∙ polski ∙ português ∙ русский ∙ sicilianu ∙ slovenščina ∙ Türkçe ∙ українська ∙ 简体中文 ∙ 繁體中文 ∙ +/− |
许可协议
[编辑]Public domainPublic domainfalsefalse |
本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zh、NASA版权方针页面或JPL图片使用方针。) | ||
警告:
|
原始上传日志
[编辑]- 2007-03-13 14:48 RP88 1192×1636×8 (174008 bytes) higher resolution
- 2007-02-23 23:24 Latitude0116 492×676×8 (42637 bytes) Diagram showing Europa's interior (source: [http://photojournal.jpl.nasa.gov/catalog/PIA01669]) {{NASA}}
文件历史
点击某个日期/时间查看对应时刻的文件。
日期/时间 | 缩略图 | 大小 | 用户 | 备注 | |
---|---|---|---|---|---|
当前 | 2019年2月7日 (四) 19:23 | 1,192 × 1,636(696 KB) | Kesäperuna(留言 | 贡献) | 100% JPEG quality from full quality TIFF. | |
2007年12月15日 (六) 02:13 | 1,192 × 1,636(170 KB) | Mu301(留言 | 贡献) | {{Information |Description={{en|Model of Europa's subsurface structure.<br/> ==== Original caption released with image ==== These artist's drawings depict two proposed models of the subsurface structure of the Jovian moon, Europa. Geologic | ||
2007年12月15日 (六) 01:47 | 1,192 × 1,636(170 KB) | Mu301(留言 | 贡献) | == Summary == {{Information | Description = Model of Europa's subsurface structure. | Source = NASA's [http://photojournal.jpl.nasa.gov/index.html Planetary Photojournal], PIA01669: * Source URL: http://photojournal.jpl.nasa.gov/jpe |
您不可以覆盖此文件。
文件用途
以下4个页面使用本文件:
全域文件用途
以下其他wiki使用此文件:
- ar.wikipedia.org上的用途
- azb.wikipedia.org上的用途
- bg.wikipedia.org上的用途
- en.wikipedia.org上的用途
- en.wikibooks.org上的用途
- en.wikiversity.org上的用途
- es.wikipedia.org上的用途
- fa.wikipedia.org上的用途
- fr.wikipedia.org上的用途
- hi.wikipedia.org上的用途
- is.wikipedia.org上的用途
- ja.wikipedia.org上的用途
- kk.wikipedia.org上的用途
- ko.wikipedia.org上的用途
- la.wikipedia.org上的用途
- nn.wikipedia.org上的用途
- no.wikipedia.org上的用途
- pnb.wikipedia.org上的用途
- ro.wikipedia.org上的用途
- sl.wikipedia.org上的用途
- tr.wikipedia.org上的用途
- ur.wikipedia.org上的用途
- vi.wikipedia.org上的用途
- zh.wikipedia.org上的用途