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== Orbital resonances ==
== Orbital resonances ==


A number of features in [[Saturn's rings]] are related to [[orbital resonance|resonances]] with Mimas. Mimas is responsible for clearing the material from the [[Cassini Division]], the gap between Saturn's two widest rings, the [[A Ring]] and [[B Ring]]. Particles in the [[Rings of Saturn#Huygens Gap|Huygens Gap]] at the inner edge of the Cassini division are in a 2:1 [[orbital resonance|resonance]] with Mimas. They orbit twice for each orbit of Mimas. The repeated pulls by Mimas on the Cassini division particles, always in the same direction in space, force them into new orbits outside the gap. The boundary between the C and B ring is in a 3:1 resonance with Mimas. Recently, the [[Rings of Saturn#G Ring|G Ring]] was found to be in a 7:6 co-rotation eccentricity resonance{{Clarify|date=November 2012}} with Mimas; the ring's inner edge is about {{convert|15000|km|abbr=on}} inside Mimas's orbit.{{citation needed|date=November 2011}}
A number of features in [[Saturn's rings]] are related to [[orbital resonance|resonances]] with Mimas. Mimas is responsible for clearing the material from the [[Cassini Division]], the gap between Saturn's two widest rings, the [[A Ring]] and [[B Ring]]. Particles in the [[Rings of Saturn#Huygens Gap|Huygens Gap]] at the inner edge of the Cassini division are in a 2:1 orbital resonance with Mimas. They orbit twice for each orbit of Mimas. The repeated pulls by Mimas on the Cassini division particles, always in the same direction in space, force them into new orbits outside the gap. The boundary between the C and B ring is in a 3:1 resonance with Mimas. Recently, the [[Rings of Saturn#G Ring|G Ring]] was found to be in a 7:6 co-rotation eccentricity resonance{{Clarify|date=November 2012}} with Mimas; the ring's inner edge is about {{convert|15000|km|abbr=on}} inside Mimas's orbit.{{citation needed|date=November 2011}}


Mimas is also in a 2:1 [[Orbital resonance#Mean-motion resonances in the Solar System|mean-motion resonance]] with the larger moon [[Tethys (moon)|Tethys]], and in a 2:3 resonance with the outer [[F Ring]] [[Planetary ring|shepherd]] moonlet, [[Pandora (moon)|Pandora]].
Mimas is also in a 2:1 [[Orbital resonance#Mean-motion resonances in the Solar System|mean-motion resonance]] with the larger moon [[Tethys (moon)|Tethys]], and in a 2:3 resonance with the outer [[F Ring]] [[Planetary ring|shepherd]] moonlet, [[Pandora (moon)|Pandora]].

Revision as of 22:03, 30 March 2018

Mimas
Mimas with its large crater Herschel. Other bright-walled craters include Ban just left of center near top, and Percivale two thirds of the way left of Herschel. (Cassini, 2010)
Discovery
Discovered byWilliam Herschel
Discovery date17 September 1789[1]
Designations
Pronunciation/ˈmaɪməs/ or /ˈmiːməs/[citation needed]
Saturn I
AdjectivesMimantean, Mimantian
Orbital characteristics [2]
Periapsis181902 km
Apoapsis189176 km
185539 km
Eccentricity0.0196
0.942 d
14.28 km/s (calculated)
Inclination1.574° (to Saturn's equator)
Satellite ofSaturn
Physical characteristics
Dimensions415.6 × 393.4 × 381.2 km
(0.0311 Earths)[3]
198.2±0.4 km [3]
490000–500000 km2
Volume32600000±200000 km3
Mass(3.7493±0.0031)×1019 kg [4][5]
(6.3×10−6 Earths)
Mean density
1.1479±0.007 g/cm3 [3]
0.064 m/s2 (0.00648 g)
0.159 km/s
synchronous
zero
Albedo0.962±0.004 (geometric)[6]
Temperature≈ 64 K
12.9 [7]

Mimas is a moon of Saturn which was discovered in 1789 by William Herschel.[8] It is named after Mimas, a son of Gaia in Greek mythology, and is also designated Saturn I.

With a diameter of 396 kilometres (246 mi) it is the smallest astronomical body that is known to be rounded in shape because of self-gravitation.

Discovery

Mimas was discovered by the astronomer William Herschel on 17 September 1789. He recorded his discovery as follows: "The great light of my forty-foot [12 m] telescope was so useful that on the 17th of September, 1789, I remarked the seventh satellite, then situated at its greatest western elongation."[9]

Name

Mimas is named after one of the Giants in Greek mythology, Mimas. The names of all seven then-known satellites of Saturn, including Mimas, were suggested by William Herschel's son John in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope.[10][11] He named them after Titans specifically because Saturn (the Roman equivalent of Cronus in Greek mythology), was the leader of the Titans and ruler of the world for some time. Mimas was a son of the Greek goddess Gaia.

Physical characteristics

Further information: List of geological features on Mimas
Cassini view of Mimas's trailing hemisphere, showing craters up to 6 km deep and 1-km-deep chasmata (grooves). The large crater near center is Morgan; Arthur is close to the lower right limb. Pelion Chasma is faintly visible as a horizontal trough left of Arthur and below Morgan.

The surface area of Mimas is slightly less than the land area of Spain. The low density of Mimas, 1.15 g/cm3, indicates that it is composed mostly of water ice with only a small amount of rock. Due to the tidal forces acting on it, Mimas is noticeably prolate; its longest axis is about 10% longer than the shortest. The ellipsoidal shape of Mimas is especially noticeable in some recent images from the Cassini probe.

Mimas's most distinctive feature is a giant impact crater 130 km (81 mi) across, named Herschel after the discoverer of Mimas. Herschel's diameter is almost a third of Mimas's own diameter; its walls are approximately 5 km (3 mi) high, parts of its floor measure 10 km (6 mi) deep, and its central peak rises 6 km (4 mi) above the crater floor. If there were a crater of an equivalent scale on Earth (in relative size) it would be over 4,000 km (2,500 mi) in diameter, wider than Australia. The impact that made this crater must have nearly shattered Mimas: fractures can be seen on the opposite side of Mimas that may have been created by shock waves from the impact travelling through Mimas's body.[12]

The Mimantean surface is saturated with smaller impact craters, but no others are anywhere near the size of Herschel. Although Mimas is heavily cratered, the cratering is not uniform. Most of the surface is covered with craters larger than 40 km (25 mi) in diameter, but in the south polar region, there are generally no craters larger than 20 km (12 mi) in diameter.

Three types of geological features are officially recognized on Mimas: craters, chasmata (chasms) and catenae (crater chains).

Mimas maps – June 2017
North pole
Global map
South pole
Credit: NASA/JPL-Caltech/Space Science Institute
Mimas maps – November 2014 (enhanced-color)
Northern and southern hemispheres
Trailing and leading hemispheres
Credit: NASA / JPL-Caltech / Space Science Institute / Lunar and Planetary Institute
Mimas maps – November 2014 (enhanced-color)
Global map
Credit: NASA / JPL-Caltech / Space Science Institute / Lunar and Planetary Institute

Orbital resonances

A number of features in Saturn's rings are related to resonances with Mimas. Mimas is responsible for clearing the material from the Cassini Division, the gap between Saturn's two widest rings, the A Ring and B Ring. Particles in the Huygens Gap at the inner edge of the Cassini division are in a 2:1 orbital resonance with Mimas. They orbit twice for each orbit of Mimas. The repeated pulls by Mimas on the Cassini division particles, always in the same direction in space, force them into new orbits outside the gap. The boundary between the C and B ring is in a 3:1 resonance with Mimas. Recently, the G Ring was found to be in a 7:6 co-rotation eccentricity resonance[clarification needed] with Mimas; the ring's inner edge is about 15,000 km (9,300 mi) inside Mimas's orbit.[citation needed]

Mimas is also in a 2:1 mean-motion resonance with the larger moon Tethys, and in a 2:3 resonance with the outer F Ring shepherd moonlet, Pandora.

Anomalous libration

In 2014, researchers noted that the librational motion of Mimas has a component that cannot be explained by its orbit alone, and concluded that it was due to either an interior that is not in hydrostatic equilibrium (an elongated core) or an internal ocean.[13] However, in 2017 it was concluded that an ocean would lead to surface tidal stresses comparable to or greater than those on tectonically active Europa. Thus, the lack of evidence for surface cracking or other tectonic activity on Mimas argues against the presence of such an ocean.[14] Since formation of a core would likely have led to formation of an internal ocean in the past, probably leading to geologic activity, this explanation for the libration is also problematic. The presence of an asymmetric mass anomaly associated with the crater Herschel is another possible explanation for the libration.[14]

Exploration

Pioneer 11 flew by Saturn in 1979, and its closest approach to Mimas was 104,263 km on September 1, 1979.[15] Voyager 1 flew by in 1980, and Voyager 2 in 1981.

Mimas has been imaged several times by the Cassini orbiter, which entered into orbit around Saturn in 2004. A close flyby occurred on February 13, 2010, when Cassini passed by Mimas at 9,500 km (5,900 mi).

When seen from certain angles, Mimas resembles the Death Star, a fictional space station and superweapon known from the 1977 film Star Wars. Herschel resembles the concave disc of the Death Star's "superlaser". This is coincidental, as the film was made nearly three years before Mimas was resolved well enough to see the crater.[16]

In 2010, NASA revealed a temperature map of Mimas, using images obtained by Cassini. The warmest regions, which are along one edge of Mimas, create a shape similar to the video game character Pac-Man, with Herschel Crater assuming the role of an "edible dot" or "power pellet" known from Pac-Man gameplay.[17][18][19]

  • Mimas is the tiny white dot in the lower left. (Click to enlarge view.)
    Mimas is the tiny white dot in the lower left. (Click to enlarge view.)
  • Mimas, silhouetted against Saturn's northern latitudes.
    Mimas, silhouetted against Saturn's northern latitudes.
  • Mimas, behind the F Ring.
    Mimas, behind the F Ring.
  • Mimas viewed by Cassini looking distinctly egg-shaped.
    Mimas viewed by Cassini looking distinctly egg-shaped.
  • Mimas and mountain (October 22, 2016).
    Mimas and mountain
    (October 22, 2016).
  • Mimas before Saturn's limb (color added) (February 13, 2010).
    Mimas before Saturn's limb (color added)
    (February 13, 2010).
  • Mimas mosaic with mostly high resolution.
    Mimas mosaic with mostly high resolution.
  • Mimas displays subtle color differences (false-color).
    Mimas displays subtle color differences
    (false-color).
  • Mimas' albedo features on crater walls (Herschel at lower right)
    Mimas' albedo features on crater walls (Herschel at lower right)

See also

References

  1. ^ "Imago Mundi: La Découverte des satellites de Saturne" (in French).
  2. ^ Harvey, Samantha (April 11, 2007). "NASA: Solar System Exploration: Planets: Saturn: Moons: Mimas: Facts & Figures". NASA. Retrieved 2007-10-10.
  3. ^ a b c Roatsch, T.; Jaumann, R.; Stephan, K.; Thomas, P. C. (2009). "Cartographic Mapping of the Icy Satellites Using ISS and VIMS Data". Saturn from Cassini-Huygens. pp. 763–781. doi:10.1007/978-1-4020-9217-6_24. ISBN 978-1-4020-9216-9.
  4. ^ Jacobson, R. A.; Antreasian, P. G.; Bordi, J. J.; Criddle, K. E.; Ionasescu, R.; Jones, J. B.; Mackenzie, R. A.; Meek, M. C.; Parcher, D.; Pelletier, F. J.; Owen, Jr., W. M.; Roth, D. C.; Roundhill, I. M.; Stauch, J. R. (December 2006). "The Gravity Field of the Saturnian System from Satellite Observations and Spacecraft Tracking Data". The Astronomical Journal. 132 (6): 2520–2526. Bibcode:2006AJ....132.2520J. doi:10.1086/508812.
  5. ^ Jacobson, R. A.; Spitale, J.; et al. (2005). "The GM values of Mimas and Tethys and the libration of Methone" (PDF). Astronomical Journal. 132 (2): 711–713. Bibcode:2006AJ....132..711J. doi:10.1086/505209.
  6. ^ Verbiscer, A.; French, R.; Showalter, M.; Helfenstein, P. (9 February 2007). "Enceladus: Cosmic Graffiti Artist Caught in the Act". Science. 315 (5813): 815. Bibcode:2007Sci...315..815V. doi:10.1126/science.1134681. PMID 17289992. Retrieved 20 December 2011. (supporting online material, table S1)
  7. ^ Observatorio ARVAL (April 15, 2007). "Classic Satellites of the Solar System". Observatorio ARVAL. Retrieved 2011-12-17.
  8. ^ Herschel, W. (1790). "Account of the Discovery of a Sixth and Seventh Satellite of the Planet Saturn; With Remarks on the Construction of Its Ring, Its Atmosphere, Its Rotation on an Axis, and Its Spheroidical Figure". Philosophical Transactions of the Royal Society of London. 80 (0): 1–20. doi:10.1098/rstl.1790.0001.
  9. ^ Herschel, William Philosophical Transactions of the Royal Society of London, Vol. 80, reported by Arago, M. (1871). "Herschel". Annual Report of the Board of Regents of the Smithsonian Institution: 198–223. Archived from the original on 2016-01-13. Retrieved 2006-11-26. {{cite journal}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  10. ^ As reported by William Lassell, Monthly Notices of the Royal Astronomical Society, Vol. 8, No. 3, pp. 42–43 (January 14, 1848)
  11. ^ Lassell, William (1848). "Satellites of Saturn: Observations of Mimas, the closest and most interior Satellite of Saturn". Monthly Notices of the Royal Astronomical Society. 8: 42–43. Bibcode:1848MNRAS...8...42L. doi:10.1093/mnras/8.3.42. Retrieved 2006-11-26.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  12. ^ Elkins-Tanton, Linda E. (2006). Jupiter and Saturn. Infobase Publishing. p. 144. ISBN 9781438107257.
  13. ^ Tajeddine, R.; Rambaux, N.; Lainey, V.; Charnoz, S.; Richard, A.; Rivoldini, A.; Noyelles, B. (2014-10-17). "Constraints on Mimas' interior from Cassini ISS libration measurements". Science. 346 (6207): 322–324. Bibcode:2014Sci...346..322T. doi:10.1126/science.1255299.
  14. ^ a b Rhoden, A. R.; Henning, W.; Hurford, T. A.; Patthoff, D. A.; Tajeddine, R. (2017-02-24). "The implications of tides on the Mimas ocean hypothesis". Journal of Geophysical Research: Planets. Bibcode:2017JGRE..122..400R. doi:10.1002/2016JE005097.
  15. ^ "Pioneer 11 Full Mission Timeline". Dmuller.net. Retrieved 2012-02-26.
  16. ^ Young, Kelly (2005-02-11). "Saturn's moon is Death Star's twin". New Scientist. Retrieved 2008-08-21. Saturn's diminutive moon, Mimas, poses as the Death Star – the planet-destroying space station from the movie Star Wars – in an image recently captured by NASA's Cassini spacecraft.
  17. ^ Cook, Jia-Rui C. (2010-03-29). "1980s Video Icon Glows on Saturn Moon". NASA. Retrieved 2010-04-02.
  18. ^ "Bizarre Temperatures on Mimas". NASA. 2010-03-29. Retrieved 2010-04-02.
  19. ^ "Saturn moon looks like Pac-Man in image taken by Nasa spacecraft". The Daily Telegraph. 2010-03-30. Retrieved 2010-04-02.
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