Pan (Moon)

colspan="2" |
bgcolor="#a0ffa0" colspan="2" | Discovery
align="left" | Discovered by M.R. Showalter
align="left" | Discovered in 1990
bgcolor="#a0ffa0" colspan="2" | Orbital characteristics
align="left" | Semimajor axis 133,584 km
align="left" | Eccentricity 0.00021 +/- 0.00008
align="left" | Orbital period 13 h 48 min
align="left" | Inclination 0.007 +/- 0.002°
align="left" | Is a satellite of Saturn
bgcolor="#a0ffa0" colspan="2" | Physical characteristics
align="left" | Mean diameter 20 km
align="left" | Mass 2.7×1015 kg
align="left" | Mean density 0.6 g/cm3
align="left" | Surface gravity 0.002 m/s2
align="left" | Rotation period unknown
align="left" | Axial tilt 0 °
align="left" | Albedo 0.5
align="left" | Atmosphere none
Pan (pan) is a moon of Saturn, named after the god Pan. It was discovered by Mark R. Showalter in 1990 from analysis of old Voyager probe photos. Pan is within the Encke division in Saturn's A Ring; it acts as a shepherd and is responsible for keeping the Encke gap open. Its gravity produces wave patterns in the rings that indicated Pan's presence and led to the reexamination of Voyager photographs of its predicted location. Other undiscovered moons may exist within Saturn's rings. The existence of such a moon in the Encke division was first predicted by Jeffrey N. Cuzzi and Jeffrey N. Scargle in 1985. Then Showalter et al. inferred its orbit and mass in 1986 by modeling its "wake", or gravitational disturbance. They arrived at a very precise prediction of 133,603 ± 10 km for the semimajor axis and a mass of 5–10 × 10-12 Saturn masses, and inferred that there was only a single moon within the Encke gap. http://www.sciencedirect.com/science?_ob=ArticleURL&_udi=B6WGF-470F4DX-C0&_coverDate=05%2F31%2F1986&_alid=185908849&_rdoc=1&_fmt=&_orig=search&_qd=1&_cdi=6821&_sort=d&view=c&_acct=C000050221&_version=1&_urlVersion=0&_userid=10&md5=e8b6d7c23048e402cf78d5e7817650d4 http://ringmaster.arc.nasa.gov/showalter/1986_wakes.html The actual semi-major axis is 133,583 km and the mass is 2.7 × 1015 kg, or 4.7 × 10-12 of Saturn's mass of 5.688 × 1026 kg. The moon was later found within 1° of the predicted position. The search was undertaken by considering all Voyager 2 images and using a computer calculation to predict whether the moon would be visible under sufficiently favorable conditions in each one. Every qualifying Voyager 2 image with resolution better than ~50 km/pixel shows Pan clearly. In all, it appears in eleven Voyager 2 images. http://adsabs.harvard.edu//full/seri/BAAS./0022//0001040.000.html After the discovery it received a temporary designation S/1981 S 13. It is also designated as Saturn XVIII. There is also an asteroid called 4450 Pan.

References

External links


Saturn | 'Pan' | Atlas | ...

 

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