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Airfix A11170 Apollo Saturn V 1:144 Scale Series 11 Plastic Model Kit

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By feeding data gathered by the Cassini mission into powerful computer simulations similar to those used to study weather and climate, Yan and Stanley explored what ingredients are necessary to produce the dynamo -- the electromagnetic conversion mechanism -- that could account for Saturn's magnetic field. Russell, Randy (3 June 2003). "Saturn Magnetosphere Overview". Windows to the Universe. Archived from the original on 6 September 2011 . Retrieved 19 July 2011.

Pioneer 11 made the first flyby of Saturn in September 1979, when it passed within 20,000km of the planet's cloud tops. Images were taken of the planet and a few of its moons, although their resolution was too low to discern surface detail. The spacecraft also studied Saturn's rings, revealing the thin F-ring and the fact that dark gaps in the rings are bright when viewed at a high phase angle (towards the Sun), meaning that they contain fine light-scattering material. In addition, Pioneer 11 measured the temperature of Titan. [159] Voyager flybys Cain, Fraser (3 July 2008). "Mass of Saturn". Universe Today. Archived from the original on 26 September 2011 . Retrieved 17 August 2011. Dunbar, Brian (29 November 2007). "NASA – Saturn". NASA. Archived from the original on 29 September 2011 . Retrieved 21 July 2011. Chan, Gary (2000). "Saturn: History Timeline". Archived from the original on 16 July 2011 . Retrieved 16 July 2007.Orton, Glenn S. (September 2009). "Ground-Based Observational Support for Spacecraft Exploration of the Outer Planets". Earth, Moon, and Planets. 105 (2–4): 143–152. Bibcode: 2009EM&P..105..143O. doi: 10.1007/s11038-009-9295-x. S2CID 121930171. How can I use the Saturn V AR Model?: View the Saturn V model through the camera on your device. Take photos of the model in different positions to create a photo story about it blasting off into space. Seligman, Courtney. "Rotation Period and Day Length". Archived from the original on 28 July 2011 . Retrieved 13 August 2009. Walter, Elizabeth (21 April 2003). Cambridge Advanced Learner's Dictionary (Seconded.). Cambridge University Press. ISBN 978-0-521-53106-1.

There are two main hypotheses regarding the origin of the rings. One hypothesis is that the rings are remnants of a destroyed moon of Saturn, for which a research team at MIT has proposed the name " Chrysalis". [124] The second hypothesis is that the rings are left over from the original nebular material from which Saturn was formed. Some ice in the E ring comes from the moon Enceladus's geysers. [125] [126] [127] [128] The water abundance of the rings varies radially, with the outermost ring A being the most pure in ice water. This abundance variance may be explained by meteor bombardment. [129] Kaufman, Marc (22 June 2011). "Saturn′s moon Enceladus shows evidence of an ocean beneath its surface". The Washington Post. Archived from the original on 12 November 2012 . Retrieved 19 July 2011. Rincon, Paul (14 March 2007). "Probe reveals seas on Saturn moon". BBC. Archived from the original on 11 November 2011 . Retrieved 26 September 2007.a b "Starry Night Times". Imaginova Corp. 2006. Archived from the original on 1 October 2009 . Retrieved 5 July 2007.

By the Numbers – Saturn". NASA Solar System Exploration. NASA. Archived from the original on 10 May 2018 . Retrieved 5 August 2020. a b Nemiroff, R.; Bonnell, J., eds. (13 November 2006). "A Hurricane Over the South Pole of Saturn". Astronomy Picture of the Day. NASA . Retrieved 1 May 2013. a b c d "Saturn". National Maritime Museum. 20 August 2015. Archived from the original on 23 June 2008 . Retrieved 6 July 2007.

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The many clouds surrounding Saturn give the planet the appearance of having yellow, brown and grey stripes. The upper atmosphere is extremely windy with gusts reaching an incredible 500m per second. Saturn also experiences pressure strong enough to squeeze gas into liquid! Foust, Jeff (8 January 2016). "NASA Expands Frontiers of Next New Frontiers Competition". SpaceNews. Archived from the original on 18 August 2017 . Retrieved 20 April 2017. Pence, Michael (9 March 2006). "NASA's Cassini Discovers Potential Liquid Water on Enceladus". NASA Jet Propulsion Laboratory. Archived from the original on 11 August 2011 . Retrieved 3 June 2011.

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