Definition
Surface features occurring along the equator.
Subtypes and Regional Variations
- (1)
Spectral feature: equatorial great circle (Rhea)
- (2)
Topographic feature:
- (2.1)
- (2.2)
Equatorial ridge (“flying saucer” bodies): smooth rings around low-gravity small moons orbiting within the main rings of Saturn (Pan, Daphnis, Atlas [Fig. 1]). The ridges are equatorial and are in the same planes as Saturn’s rings. The shape of these bodies is close to the size of the Hills sphere or Roche lobe, which means that a very little disturbance is enough for material to be lost from the satellite’s surface into Saturn orbit. However, for centrifugal forces to balance with gravity forces at the asteroid’s equator, their rotation should be faster. Tidal stresses would produce a body elongate in the radial direction. The presence of the ridges is best explained by accretion from ring particles (Charnoz et al. 2007; Porco et al. 2007; Thomas et al. 2013).
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References
Charnoz S, Brahic A, Thomas PC, Porco CC (2007) The equatorial ridges of Pan and Atlas: terminal accretionary ornaments? Science 318:1622–1624
Porco CC, Thomas PC, Weiss JW, Richardson DC (2007) Saturn’s small inner satellites: clues to their origins. Science 318:1602–1607
Thomas PC, Burns JA, Hedman M, Helfenstein P, Morrison S, Tiscareno MS, Veverka J (2013) The inner small satellites of Saturn: a variety of worlds. Icarus 226(1):999–1019
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Hargitai, H. (2014). Equatorial Features. In: Encyclopedia of Planetary Landforms. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-9213-9_631-1
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DOI: https://doi.org/10.1007/978-1-4614-9213-9_631-1
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