Fil:Punga_Mare_crop.jpg
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![Fil:Punga Mare crop.jpg](http://upload.wikimedia.org/wikipedia/commons/thumb/4/44/Punga_Mare_crop.jpg/660px-Punga_Mare_crop.jpg)
Opprinnelig fil (1 100 × 1 000 piksler, filstørrelse: 1,32 MB, MIME-type: image/jpeg)
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Beskrivelse
BeskrivelsePunga Mare crop.jpg |
English: This is a segment of a colorized mosaic from NASA's Cassini mission that shows the most complete view yet of Titan's northern land of lakes and seas. Saturn's moon Titan is the only world in our solar system other than Earth that has stable liquid on its surface. The liquid in Titan's lakes and seas is mostly methane and ethane.
Seas and major lakes are labeled in the annotated version. The data were obtained by Cassini's radar instrument from 2004 to 2013. In this color scheme, liquids appear blue and black depending on the way the radar bounced off the surface. Land areas appear yellow to white. Punga Mare is just below the north pole. Most of the bodies of liquid on Titan occur in the northern hemisphere. In fact nearly all the lakes and seas on Titan fall into a box covering about 600 by 1,100 miles (900 by 1,800 kilometers). Only 3 percent of the liquid at Titan falls outside of this area. Scientists are trying to identify the geologic processes that are creating large depressions capable of holding major seas in this limited area. A prime suspect is regional extension of the crust, which on Earth leads to the formation of faults creating alternating basins and roughly parallel mountain ranges. This process has shaped the Basin and Range province of the western United States, and during the period of cooler climate 13,000 years ago much of the present state of Nevada was flooded with Lake Lahontan, which (though smaller) bears a strong resemblance to the region of closely packed seas on Titan. An unannotated version and a version with explanatory text are also available in Figures 1 and 2. A related flyover can be seen at PIA17656. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, DC. The Cassini orbiter was designed, developed and assembled at JPL. The radar instrument was built by JPL and the Italian Space Agency, working with team members from the United States and several European countries. For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini. The original NASA image has been modified by cropping and removing the labels. |
Dato | |
Kilde | http://photojournal.jpl.nasa.gov/catalog/PIA17655 |
Opphavsperson | NASA / JPL-Caltech / Agenzia Spaziale Italiana / USGS |
Andre versjoner | Image:PIA17655 Punga Mare crop.jpg - Larger version (2,300 × 2,000 pixels, 891 KB) with label |
Lisensiering
Public domainPublic domainfalsefalse |
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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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Dato/klokkeslett | Miniatyrbilde | Dimensjoner | Bruker | Kommentar | |
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nåværende | 10. feb. 2014 kl. 03:17 | ![]() | 1 100 × 1 000 (1,32 MB) | WolfmanSF | tweak image |
10. feb. 2014 kl. 03:03 | ![]() | 1 100 × 1 000 (1,31 MB) | WolfmanSF | remove labels | |
8. feb. 2014 kl. 12:14 | ![]() | 1 100 × 1 000 (1,32 MB) | WolfmanSF | User created page with UploadWizard |
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Kort tittel |
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Retning | Normal |
Horisontal oppløsning | 300 dpi |
Vertikal oppløsning | 300 dpi |
Programvare brukt | Adobe Photoshop Elements 9.0 Windows |
Dato og tid for filendring | 9. feb. 2014 kl. 17:17 |
Fargerom | sRGB |
Bildebredde | 1 100 px |
Bildehøyde | 1 000 px |
Dato og tid for digitalisering | 7. feb. 2014 kl. 21:46 |
Dato metadata sist ble endret | 9. feb. 2014 kl. 09:17 |
Opphavsrettsstatus | Opphavsrettstatus er ikke angitt |
Unik ID for originaldokumentet | xmp.did:347C442EA890E311BA40C060E31765E8 |
IIM-versjon | 2 |