Pan amid the rings of Saturn. The 'side' view gives Pan the appearance of being embedded in the rings, although it actually travels within the Encke Gap.
|Discovered by||M. R. Showalter|
|Discovery date||July 16, 1990|
|Longest distance from the center of its orbital path
|How long it takes to complete an orbit||0.575050718 days (13.801217 hours)|
|Angle above the reference plane
|What it orbits||Saturn|
|Size and other qualities|
|Measurements||34.4 × 31.4 × 20.8 km|
|Average radius||14.1 ± 1.3 km|
|Mass||4.95 ± 0.75 ×1015 kg|
|Average density||0.42 ± 0.15 g/cm³|
|Surface gravity||0.0001–0.0018 m/s2|
|Escape velocity||~0.006 km/s|
|Angle at which it turns
(in relation to its orbit)
|How much light it reflects||0.5|
|Avg. surface temp.||~78 K|
Pan is a moon of Saturn. It is the closest moon to the planet, orbiting 133,600 km above Saturn's cloud tops. It was discovered in 1990 by Mark Showalter. He discovered Pan when he was analysing the photos taken by Voyager 2. It orbits inside the Encke gap which it has made Saturn's A Ring.
Its mass is in the range .
References[change | change source]
- Jacobson, R. A.; et al. (2008). "Revised orbits of Saturn's small inner satellites". Astronomical Journal 135 (1): 261–263. doi:10.1088/0004-6256/135/1/261.
- Thomas, P. C. (July 2010). "Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission". Icarus 208 (1): 395–401. doi:10.1016/j.icarus.2010.01.025. http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf.
- IAUC 5052: Saturn 1990 July 16 (discovery)
- IAUC 5347: Satellites of Saturn and Neptune 1991 September 16 (naming the moon)
- "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 2007-09-14.
- Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission