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Atlas

 
 
Atlas, in astronomy, one of the named moons, or natural satellites, of Saturn. Also known as Saturn XV (or S15), Atlas is a small, irregularly shaped (nonspherical) body measuring about 25 mi (40 km) by 12.5 mi (20 km); it orbits Saturn at a mean distance of 85,544 mi (137,670 km), and has an orbital period of 0.6019 earth days-the rotational period is unknown but is assumed to be the same as the orbital period. Atlas was discovered by Richard J. Terrile in 1980 from photographs taken by Voyager 1 during its flyby of Saturn. Atlas is probably a shepherd satellite (a moon that limits the extent of a planetary ring through gravitational forces) of Saturn's A ring.


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Atlas
Cassini Atlas N00084634 CL.png
Photo taken by Cassini on June 12, 2007, showing Atlas as seen from above its south pole
Discovery
Discovered by Terrile, Voyager 1
Discovery date October, 1980
Designations
Adjective Atlantean
Epoch December 31, 2003 (JD 2453005.5)
Mean orbit radius 137,670 ± 10 km
Eccentricity 0.0012
Orbital period 0.6016947883 d
Inclination 0.003 ± 0.004°
Satellite of Saturn
Physical characteristics
Dimensions 46 × 38 × 19 km[2]
Mean radius 15.3 ± 1.2 km [2]
Surface area ~3,700 km²
Volume ~15,000 km³
Mass 6.6 ± 0.6  × 1015 kg [1]
Mean density 0.44 ± 0.11 g/cm³
Equatorial surface gravity ~0.00083 m/s2
Escape velocity ~0.0062 km/s
Rotation period synchronous
Axial tilt zero
Albedo 0.4
Temperature ~81 K

Atlas (pronounced /ˈætləs/ AT-ləs, or as Greek Άτλας) is an inner satellite of Saturn.

Atlas was discovered by Richard Terrile in 1980 (some time before November 12) from Voyager photos and was designated S/1980 S 28.[3] In 1983 it was officially named after Atlas of Greek mythology, because it "holds the rings on its shoulders" like the Titan Atlas held the sky up above the Earth.[4] It is also designated as Saturn XV.

Atlas is the closest satellite to the sharp outer edge of the A ring, and was long thought to be a shepherd satellite for this ring. However, now it is known that the outer edge of the ring is instead maintained by a 7:6 orbital resonance with the larger but more distant moons Janus and Epimetheus. [5] In 2004 a faint, thin ring, temporarily designated R/2004 S 1, was discovered within Atlas's orbit.[6]

High-resolution images taken in June 2005 by Cassini reveal a saucer-shaped moon with a large smooth equatorial ridge. The most likely explanation for this unusual and prominent structure is that ring material swept up by the moon accumulates on the moon, with a strong preference for the equator due to the ring's thinness. In fact, the size of the equatorial ridge is comparable with the expected size of Atlas's Roche lobe. This would mean that for any further particles attempting to accumulate on the equator, the centrifugal force overcomes Atlas's tiny gravity and they will be lost. [5]

Atlas is significantly perturbed by Prometheus and to a lesser degree by Pandora, leading to excursions in longitude of up to 600 km (~0.25°) away from the precessing keplerian orbit with a rough period of about 3 years. Since the orbits of Prometheus and Pandora are chaotic, it is suspected that Atlas's may be as well.[1]

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Columbia Encyclopedia. The Columbia Electronic Encyclopedia, Sixth Edition Copyright © 2003, Columbia University Press. Licensed from Columbia University Press. All rights reserved. www.cc.columbia.edu/cu/cup/ Read more
Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Atlas (moon)" Read more