Fil:Tortola Facula Cassini c12.jpg

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English: Tortola Facula (formerly interpreted as cryovolcano) on Saturn moon Titan in false color, taken by the Cassini space probe with ultraviolet and infrared camera.
Deutsch: Tortola Facula auf Titan, fotografiert von Cassini, 2004.
Dato
Kilde NASA planetary photojournal: PIA07965
Forfatter NASA/JPL/Space Science Institute
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(Genbrug af denne fil)
Copyright information from http://www.jpl.nasa.gov/images/policy/index.cfm - Unless otherwise noted, images and video on JPL public web sites (public sites ending with a jpl.nasa.gov address) may be used for any purpose without prior permission [...]


Public domain Denne fil er i offentligt domæne i USA fordi den udelukkende er skabt af NASA. NASAs ophavsretspolitik erklærer at materiale udgivet af NASA ikke er omfattet af ophavsret medmindre andet er nævnt. (Se også Template:PD-USGov, NASAs ophavsretspolitik eller JPLs politik for brug af billeder.)
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Original Caption Released with Image:

This false-color mosaic of Saturn's largest moon Titan, obtained by Cassini's visual and infrared mapping spectrometer, shows what scientists interpret as an icy volcano (see inset). The mosaic was constructed using six medium-resolution infrared images, obtained during Cassini's flyby of the hazy moon on Oct. 26, 2004.

The colors correspond to atmospheric (red) and surface (green and blue) features that are not visible to the human eye. The inset shows a high-resolution image taken using a 2.3 micron filter near the point of Cassini's closest approach to Titan at 1,200 kilometers (746 miles). The resolution in this inset image is 2 kilometers (1.2 miles) per pixel. The image scale of the large image is 25 kilometers (16 miles) per pixel.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The visual and infrared mapping spectrometer team is based at the University of Arizona.

For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov. The visual and infrared mapping spectrometer team homepage is at http://wwwvims.lpl.arizona.edu archive copy at the Wayback Machine.

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Dato/tidMiniaturebilledeDimensionerBrugerKommentar
nuværende28. feb. 2010, 09:46Miniature af versionen fra 28. feb. 2010, 09:467.458 × 4.035 (838 KB)Nova13higher resolution
10. jun. 2005, 10:19Miniature af versionen fra 10. jun. 2005, 10:19724 × 484 (48 KB)Wricardoh~commonswiki{{Information| |Description = Icy volcanos on Saturn moon Titan in False Color, taken by the Cassini space probe with ultraviolet and infrared camera. |Source = NASA planetary photojournal * [http://photojournal.jpl.nasa.gov/catalog/P

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