Shepherd moon

Prometheus (right) and Pandora both orbit near Saturn's F ring, but only Prometheus is thought to act as a shepherd.
Operation of a shepherd moon– particles are located in front or behind the Moon in its orbit, so these are either accelerated in the direction of the moon and thrown to the outside, or they are slowed down on their path and pulled inwards.

A shepherd moon (also herder moon, watcher moon) is a small natural satellite that clears a gap in planetary-ring material or keeps particles within a ring contained. The name is a result of the fact they limit the "herd" of the ring particles as a shepherd.

Due to their gravitational effect, they pick up particles and deflect them from their original orbits through orbital resonance. This causes gaps in the ring system, such as the particularly striking Cassini Division, as well as other characteristic bands, or strange "twisted" deformation of rings.

Examples

Jupiter

Several of Jupiter's small innermost moons, namely Metis and Adrastea, are within Jupiter's ring system and are also within Jupiter's Roche limit.[1] It is possible that these rings are composed of material that is being pulled off these two bodies by Jupiter's tidal forces, possibly facilitated by impacts of ring material on their surfaces.

Saturn

The complex ring system of Saturn has several such satellites. These include Prometheus (F ring),[2] Daphnis (Keeler Gap),[3] Pan (Encke Gap),[4] Janus, and Epimetheus (both A ring).[5]

Uranus

Uranus also has shepherd moons on its ε ring, Cordelia and Ophelia. They are interior and exterior shepherds, respectively.[6] Both moons are well within Uranus's synchronous orbit radius, and their orbits are therefore slowly decaying due to tidal deceleration.[7]

Neptune

Neptune's rings are very unusual in that they first appeared to be composed of incomplete arcs in Earth-based observations, but Voyager 2's images showed them to be complete rings with bright clumps.[8] It is thought[9] that the gravitational influence of the shepherd moon Galatea and possibly other as-yet undiscovered shepherd moons are responsible for this clumpiness.

Minor planets

Rings around some centaurs have been identified. Chariklo's rings are remarkably well-defined and are suspected to either be very young or kept in place by a shepherd moon similar in mass to the rings.[10] Chiron is also thought to have rings similar in form to those of Chariklo.[11]

See also

References

  1. ↑ Faure, Gunter; Mensing, Teresa (2007). Introduction to Planetary Science: The Geological Perspective. Springer. ISBN 978-1-4020-5233-0.
  2. ↑ "On the masses and motions of mini-moons: Pandora's not a". www.planetary.org. Retrieved 2016-06-14.
  3. ↑ "NASA - Cassini Finds New Saturn Moon That Makes Waves". www.nasa.gov. Retrieved 2016-06-14.
  4. ↑ Showalter, Mark R. (1991-06-27). "Visual detection of 1981S13, Saturn's eighteenth satellite, and its role in the Encke gap". Nature. 351 (6329): 709–713. doi:10.1038/351709a0.
  5. ↑ Moutamid, Maryame El; Nicholson, Philip D.; French, Richard G.; Tiscareno, Matthew S.; Murray, Carl D.; Evans, Michael W.; French, Colleen McGhee; Hedman, Matthew M.; Burns, Joseph A. (2015-10-01). "How Janus' Orbital Swap Affects the Edge of Saturn's A Ring?". arXiv:1510.00434 Freely accessible.
  6. ↑ Esposito, Larry W. (2002-01-01). "Planetary rings". Reports on Progress in Physics. 65 (12): 1741–1783. ISSN 0034-4885. doi:10.1088/0034-4885/65/12/201.
  7. ↑ Karkoschka, Erich (2001-05-01). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus. 151 (1): 69–77. Bibcode:2001Icar..151...69K. doi:10.1006/icar.2001.6597.
  8. ↑ Miner, Ellis D.; Wessen, Randii R.; Cuzzi, Jeffrey N. (2007). "Present knowledge of the Neptune ring system". Planetary Ring System. Springer Praxis Books. ISBN 978-0-387-34177-4.
  9. ↑ Salo, Heikki; Hanninen, Jyrki (1998). "Neptune's Partial Rings: Action of Galatea on Self-Gravitating Arc Particles". Science. 282 (5391): 1102–1104. Bibcode:1998Sci...282.1102S. PMID 9804544. doi:10.1126/science.282.5391.1102.
  10. ↑ Braga-Ribas, F.; Sicardy, B.; Ortiz, J. L.; Snodgrass, C.; Roques, F.; Vieira-Martins, R.; Camargo, J. I. B.; Assafin, M.; Duffard, R. (April 2014). "A ring system detected around the Centaur (10199) Chariklo". Nature. 508 (7494): 72–75. PMID 24670644. doi:10.1038/nature13155.
  11. ↑ Ortiz, J. L.; Duffard, R.; Pinilla-Alonso, N.; Alvarez-Candal, A.; Santos-Sanz, P.; Morales, N.; Fernández-Valenzuela, E.; Licandro, J.; Bagatin, A. Campo. "Possible ring material around centaur (2060) Chiron". Astronomy & Astrophysics. 576: A18. Bibcode:2015A&A...576A..18O. ISSN 0004-6361. arXiv:1501.05911 Freely accessible. doi:10.1051/0004-6361/201424461.

Further reading

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