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Atlas (moon)
Moon of Saturn
Moon of Saturn
| Field | Value |
|---|---|
| name | Atlas |
| mpc_name | Saturn XV |
| alt_names | S/1980 S 28 |
| adjectives | Atlantean |
| pronounced | |
| named_after | Ἄτλας Ātlās |
| image | Atlas color PIA21449.png |
| caption | Color photo taken by Cassini on 12 April 2017 |
| discoverer | Terrile, Voyager 1 |
| discovered | October, 1980 |
| orbit_ref | |
| epoch | December 31, 2003 (JD ) |
| mean_orbit_radius | |
| eccentricity | |
| period | |
| inclination | |
| satellite_of | Saturn |
| group | Outer shepherd moon of the A Ring |
| dimensions | km |
| (± km) | |
| mean_diameter | |
| volume | |
| mass | |
| density | |
| surface_grav | |
| escape_velocity | km/s at longest axis |
| to km/s at poles | |
| rotation | synchronous |
| axial_tilt | zero |
| albedo | 0.4 |
| single_temperature | ≈ 81 K |
(± km) to km/s at poles
Atlas is an inner satellite of Saturn which was discovered by Richard Terrile in 1980 from Voyager photos and was designated S/1980 S 28. 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. It is also designated 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 (which was probably the reason for its name). 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. In 2004 a faint, thin ring, temporarily designated R/2004 S 1, was discovered in the Atlantean orbit.
High-resolution images taken in June 2005 by Cassini revealed Atlas to have a roughly spherical centre surrounded by 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. The size of the equatorial ridge is comparable with the expected Roche lobe of the moon, which means that for any additional particles impacting the equator, the centrifugal force will nearly overcome Atlas's tiny gravity, and they will probably be lost.
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. This causes the orbit of Atlas to be chaotic, with a Lyapunov time of 10 years.
Gallery
File:Cassini Atlas N00084634 CL.png|Atlas from above its south pole (June 12, 2007) File:Atlas Rev09.2x.jpg|Atlas - Cassini (June 8, 2005). File:Atlas with rings.jpg|Atlas - A and F rings (June 30, 2006). File:PIA17206-SaturnMoon-Atlas-Flyby-20151206.jpg|Atlas near the A ring (December 6, 2015). File:F Ring and Atlas PIA10448.jpg|Atlas near the F ring (May 9, 2005).
References
Notes
Citations
Sources
- {{cite journal | access-date = 2011-12-30
- {{cite web | access-date = 2011-12-30
- {{cite journal |access-date=2011-12-30
|archive-url=https://web.archive.org/web/20111213152218/http://www.cbat.eps.harvard.edu/iauc/03500/03539.html |archive-date=2011-12-13
- {{cite journal | access-date = 2011-12-30
- {{cite journal
- {{cite journal |doi-access = free
References
- {{OED. Atlantean
- Ciarniello, Mauro. (2024-09-17). "The Origin and Composition of Saturn’s Ring Moons". Space Science Reviews.
- Cooper, N. J.. (2014-12-24). "SATURNʼS INNER SATELLITES: ORBITS, MASSES, AND THE CHAOTIC MOTION OF ATLAS FROM NEW CASSINI IMAGING OBSERVATIONS". The Astronomical Journal.
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