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Datoteka:Ligeia Mare in false color (PIA17031).jpg

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Opis
English: Ligeia Mare, shown here in a false-color image from NASA's Cassini mission, is the second largest known body of liquid on Saturn's moon Titan. It is filled with liquid hydrocarbons, such as ethane and methane, and is one of the many seas and lakes that bejewel Titan's north polar region. Cassini has yet to observe waves on Ligeia Mare and will look again during its next encounter on May 23, 2013. The image is a false-color mosaic of synthetic aperture radar images obtained by the Cassini spacecraft between February 2006 and April 2007. Dark areas (low radar return) are colored black while bright regions (high radar return) are colored yellow to white. In this color scheme, liquids, which are dark to the radar, end up appearing black and the solid surface of Titan, which appears bright to the radar, ends up appearing yellow.
Datum između veljače 2006. i travnja 2007.
date QS:P,+2006-00-00T00:00:00Z/8,P1319,+2006-02-00T00:00:00Z/10,P1326,+2007-04-00T00:00:00Z/10
Izvor http://photojournal.jpl.nasa.gov/catalog/PIA17031
Autor NASA/JPL-Caltech/ASI/Cornell
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA17031.

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Licencija

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.)
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Datum/VrijemeMinijaturaDimenzijeSuradnikKomentar
sadašnja06:36, 25. svibnja 2013.Minijatura za inačicu od 06:36, 25. svibnja 2013.1.581 × 1.507 (668 KB)Huntster{{Information |Description={{en|1= Ligeia Mare, shown here in a false-color image from NASA's Cassini mission, is the second largest known body of liquid on Saturn's moon Titan. It is filled with liquid hydrocarbons, such as ethane and methane, and is ...

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