Mallama, Anthony; Krobusek, Bruce; Pavlov, Hristo (2017). "Comprehensive wide-band magnitudes and albedos for the planets, with applications to exo-planets and Planet Nine". Icarus. 282: 19–33. arXiv: 1609.05048. Bibcode: 2017Icar..282...19M. doi: 10.1016/j.icarus.2016.09.023. S2CID 119307693. The CD will become Saturn's rings. Usually one side of the CD has printing on it. This is the side you will decorate with glitter. a b Dyches, Preston; etal. (28 July 2014). "Cassini Spacecraft Reveals 101 Geysers and More on Icy Saturn Moon". NASA. Archived from the original on 14 July 2017 . Retrieved 29 July 2014.

Build as a single unit, ignoring the internal detail and focusing on the main external detail, and permanently join (including filling and sanding the gaps) of the sections together. Shiga, David (20 September 2007). "Faint new ring discovered around Saturn". NewScientist.com. Archived from the original on 3 May 2008 . Retrieved 8 July 2007. Beyond the main rings, at a distance of 12million km from the planet is the sparse Phoebe ring. It is tilted at an angle of 27° to the other rings and, like Phoebe, orbits in retrograde fashion. [130] Yes, there is ice beyond Earth! In fact, ice can be found on several planets and moons in our solar system. explore Sánchez-Lavega, A.; etal. (8 October 2002). "Hubble Space Telescope Observations of the Atmospheric Dynamics in Saturn's South Pole from 1997 to 2002". Bulletin of the American Astronomical Society. 34: 857. Bibcode: 2002DPS....34.1307S. Archived from the original on 30 June 2010 . Retrieved 6 July 2007.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. Saturn". Universe Guide. Archived from the original on 23 February 2013 . Retrieved 29 March 2009. [ unreliable source?] 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.

Observing Saturn". National Maritime Museum. 20 August 2015. Archived from the original on 22 April 2007 . Retrieved 6 July 2007. Saturn's usually bland atmosphere occasionally exhibits long-lived ovals and other features common on Jupiter. In 1990, the Hubble Space Telescope imaged an enormous white cloud near Saturn's equator that was not present during the Voyager encounters, and in 1994 another smaller storm was observed. The 1990 storm was an example of a Great White Spot, a short-lived phenomenon that occurs once every Saturnian year, roughly every 30 Earth years, around the time of the northern hemisphere's summer solstice. [63] Previous Great White Spots were observed in 1876, 1903, 1933 and 1960, with the 1933 storm being the best observed. [64] The latest giant storm was observed in 2010. In 2015, researchers used Very Large Array telescope to study Saturnian atmosphere, and reported that they found "long-lasting signatures of all mid-latitude giant storms, a mixture of equatorial storms up to hundreds of years old, and potentially an unreported older storm at 70°N". [65] Michtchenko, T. A.; Ferraz-Mello, S. (February 2001). "Modeling the 5: 2 Mean-Motion Resonance in the Jupiter-Saturn Planetary System". Icarus. 149 (2): 357–374. Bibcode: 2001Icar..149..357M. doi: 10.1006/icar.2000.6539.Seligman, Courtney. "Rotation Period and Day Length". Archived from the original on 28 July 2011 . Retrieved 13 August 2009.