[{WikipediaArticle oldid='223161045'}]
[{VerifyArticle user='eertl' template='Standard' date='21. November 2014' page-date='2014' comment='Überprüft, nach Jaros, A., Nussbaumer, A., Nussbaumer, P., Physik compact. Basiswissen 7RG; Ranzini, G., Atlas des Universums. Sonnensystem-Galaxien-Sternbilder' funder='66' }]
[{ALLOW edit Admin}][{ALLOW view All}][{ALLOW comment All}][{ALLOW verify eertl}]
----
Die Anzahl der Monde variiert zwischen den verschiedenen Quellen und unterscheidet sich von dem Artikel in der Wikipedia.
-- [Ertl Elisabeth|User/Ertl Elisabeth], Sonntag, 23. November 2014, 10:49%%information
%%(font-size: 80%;)
!!!License Information of Images on page
||Image Description||Credit||Artist||License Name||File
| Four Saturn moons as seen from Cassini. Dione transits Titan by the en:rings of Saturn . Prometheus transits the rings. In a rare moment, the Cassini spacecraft captured this enduring portrait of a near-alignment of four of Saturn's restless moons. Timing is critical when trying to capture a view of multiple bodies, like this one. All four of the moons seen here were on the far side of the rings from the spacecraft when this image was taken; and about an hour later, all four had disappeared behind Saturn. Seen here are Titan (5,150 kilometers, or 3,200 miles across) and Dione (1,126 kilometers, or 700 miles across) at bottom; Prometheus (102 kilometers, or 63 miles across) hugs the rings at center; Telesto (24 kilometers, or 15 miles across) is a mere speck in the darkness above center. The image was taken in visible light with the Cassini narrow-angle camera on Oct. 17, 2005 at a distance of approximately 3.4 million kilometers (2.1 million miles) from Dione and 2.5 million kilometers (1.6 million miles) from Titan. The image scale is 16 kilometers (10 miles) per pixel on Dione and 21 kilometers (13 miles) per pixel on Titan.| http://photojournal.jpl.nasa.gov/catalog/PIA07644| NASA| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Cassini - four Saturn Moons.jpg
| The Wikimedia Commons logo, SVG version.| Original created by Reidab ( PNG version ) SVG version was created by Grunt and cleaned up by 3247 . Re-creation with SVG geometry features by Pumbaa , using a proper partial circle and SVG geometry features. (Former versions used to be slightly warped.)| Reidab , Grunt , 3247 , Pumbaa| [{Image src='https://www.austria-forum.org/cc/images/slim/by-sa.png' alt='CC BY-SA 3.0' align='center' link='https://www.austria-forum.org/cc/by-sa-30.html' target='_blank'}]| Datei:Commons-logo.svg
| Illustration of Jupiter and Saturn from “Ars Magna Lucis et Umbrae”| https://archive.org/details/athanasiikirche00kirc/page/n9/mode/2up| Athanasius Kircher| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Illustration of Jupiter and Saturn from “Ars Magna Lucis et Umbrae”.jpg
| Cassini stares deep into the swirling hurricane-like vortex at Saturn's south pole, where the vertical structure of the clouds is highlighted by shadows. Such a storm, with a well-developed eye ringed by towering clouds, is a phenomenon never before seen on another planet. This image shows a swirling cloud mass centered on the south pole, around which winds blow at 550 kilometers (350 miles) per hour. The frames have been aligned to make the planet appear stationary, while the sun appears to revolve about the pole in a counterclockwise direction. The clouds inside the dark, inner circle are lower than the surrounding clouds, which cast a shadow that follows the sun. The width of the shadow and the height of the sun above the local horizon yield a crude estimate of the height of the surrounding clouds relative to the clouds in the center. The shadow-casting clouds tower 30 to 75 kilometers (20 to 45 miles) above those in the center. This is two to five times greater than the tallest terrestrial thunderstorms and two to five times the height of clouds surrounding the eye of a terrestrial hurricane. Such a height difference arises because Saturn's hydrogen-helium atmosphere is less dense at comparable pressures than Earth's atmosphere, and is therefore more distended in the vertical dimension. The south polar storm, which displays two spiral arms of clouds extending from the central ring and spans the dark area inside a thick, brighter ring of clouds, is approximately 8,000 kilometers (5,000 miles) across, which is considerably larger than a terrestrial hurricane. Eye-wall clouds are a distinguishing feature of hurricanes on Earth. They form where moist air flows inward across the ocean's surface, rising vertically and releasing a load of precipitation around an interior circular region of descending air, which is the eye itself. Though it is uncertain whether moist convection is driving this storm, as is the case with Earthly hurricanes, the dark 'eye' at the pole, the eye-wall clouds and the spiral arms together indicate a hurricane-like system. The distinctive eye-wall clouds especially have not been seen on any planet beyond Earth. Even Jupiter's Great Red Spot, much larger than Saturn's polar storm, has no eye, no eye-wall, and is relatively calm at the center. This giant Saturnian storm is apparently different from hurricanes on Earth because it is locked to the pole, does not drift around like terrestrial hurricanes and because it does not form over liquid water oceans. The images were acquired over a period of three hours on Oct. 11, 2006, when Cassini was approximately 340,000 kilometers (210,000 miles) from Saturn. Image scale is about 17 kilometers (11 miles) per pixel. The images were taken with the wide-angle camera using a spectral filter sensitive to wavelengths of infrared light centered at 752 nanometers. All frames have been contrast enhanced using digital image processing techniques. The unprocessed images show an oblique view toward the pole, and have been reprojected to show the planet from a perspective directly over the south pole.| https://photojournal.jpl.nasa.gov/catalog/PIA08332 ( image link )| NASA/JPL/Space Science Institute| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Looking saturn in the eye.jpg
| Saturn from 60 degrees by Cassini| http://photojournal.jpl.nasa.gov/catalog/PIA08361| NASA /JPL/Space Science Institute| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:PIA08361 Ring World.png
| Regions of saturn's magnetosphere| Eigenes Werk, basierend auf: Plasma magnet saturn.jpg :| Original: CWitte Vektor: Mrmw| [{Image src='https://www.austria-forum.org/cc/images/slim/cc-zero.png' alt='CC0' align='center' link='https://www.austria-forum.org/cc/cc0-10.html' target='_blank'}]| Datei:Plasma magnet saturn.svg
| Das Zeichen wird dazu genutzt, besonders gut geschriebene Artikel in der deutschsprachigen Wikipedia zu kennzeichnen| File:Qsicon exzellent.png| User:Niabot| [{Image src='https://www.austria-forum.org/cc/images/slim/by-sa.png' alt='CC BY-SA 3.0' align='center' link='https://www.austria-forum.org/cc/by-sa-30.html' target='_blank'}]| Datei:Qsicon Exzellent.svg
| Satellite picture of the "hexagon on saturn"—It is a hexagon twice as wide as Earth around Saturn's north pole. First observed by the Voyager 1 probe in the 1980s, the hexagon has been sighted still by the Cassini probe| Converted from original GIF as follows: download http://www.nasa.gov/images/content/172324main_pia09187.gif linked from http://www.nasa.gov/mission_pages/cassini/multimedia/pia09187.html mplayer.exe 172324main_pia09187.gif -vo yuv4mpeg ffmpeg2theora-20100316/ffmpeg2theora.exe stream.yuv --inputfps 5 --framerate 5 --videoquality 5 --output stream20100316ifps5fr5vq5.ogv upload stream20100316ifps5fr5vq5.ogv as File:Rotatingsaturnhexagon_gif_vq5.ogv 2006-11-10 (imaged by space probe) 2007-03-27 (published by NASA); 2010-05-05 (converted to Theora OGG video)| Credit: NASA/JPL/University of Arizona| [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:Rotatingsaturnhexagon gif vq5.ogv
| Interner Aufbau des Saturns und Größenvergleich mit Erde.| Selbst erstellt (aus Bild:Gas Giant Interiors-de.png)| FrancescoA| [{Image src='https://www.austria-forum.org/cc/images/slim/by-sa.png' alt='CC BY-SA 3.0' align='center' link='https://www.austria-forum.org/cc/by-sa-30.html' target='_blank'}]| Datei:Saturn-Internal-de.png
| | | | [{Image src='https://www.austria-forum.org/cc/images/slim/publicdomain.png' alt='Public domain' align='center' link='https://www.austria-forum.org/cc/public-domain-10.html' target='_blank'}]| Datei:SaturnInBadTelescope.jpg
%%
%%