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فائل:EuropaInterior1.jpg

اصل فائل ‏(1,192 × 1,636 پکسل، فائل کا حجم: 696 کلوبائٹ، MIME قسم: image/jpeg)

یہ فائل ویکی ذخائر کی ہے اور دیگر منصوبوں کے زیر استعمال ہوسکتی ہے۔ فائل کے صفحہ تعارف پر موجود تعارف ذیل میں موجود ہے۔

خلاصہ

تفصیل

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.
تاریخ


(Original text: 1999-01-18)
ماخذ

Transferred from en.wikipedia to Commons. Transfer was stated to be made by User:Mu301.
(Original text : NASA's Planetary Photojournal, PIA01669:

مصنف NASA/JPL
دوسرے نسخے Derivative works of this file:  EuropaInterior1 cs.jpg
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA01669.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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اجازہ کاری

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
Warnings:

اولین اپلوڈ کا نوشتہ

فائل کی تفصیلات کا اصل صفحہ یہاں تھا۔ درج ذیل تمام صارفین en.wikipedia کے ہیں۔
  • 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}}

فائل کا تاریخچہ

کسی خاص وقت یا تاریخ میں یہ فائل کیسی نظر آتی تھی، اسے دیکھنے کے لیے اس وقت/تاریخ پر کلک کریں۔

تاریخ/وقتتھمب نیلابعادصارفتبصرہ
رائج الوقت19:23، 7 فروری 2019ءمورخہ 19:23، 7 فروری 2019ء کا تھمب نیل1,192 × 1,636 (696 کلوبائٹ)Kesäperuna100% JPEG quality from full quality TIFF.
02:13، 15 دسمبر 2007ءمورخہ 02:13، 15 دسمبر 2007ء کا تھمب نیل1,192 × 1,636 (170 کلوبائٹ)Mu301{{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
01:47، 15 دسمبر 2007ءمورخہ 01:47، 15 دسمبر 2007ء کا تھمب نیل1,192 × 1,636 (170 کلوبائٹ)Mu301== 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

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