- Hyperion (moon)
name = Hyperion
alt_names = Saturn VII
adjectives = Hyperionian
bgcolour = #a0ffa0
discovery = yes
discoverer = W. C. Bond, G. P. Bond & W. Lassell
September 16, 1848
semimajor = 1 481 009 km [Computed from period, using the [http://cfa-www.harvard.edu/iau/NatSats/NaturalSatellites.html IAU-MPC NSES] µ value]
eccentricity = 0.123 006 1 [ [http://home.gwi.net/~pluto/mpecs/ss07.htm#elements Pluto Project pseudo-MPEC for Saturn VII] ]
period = 21.276 61 d
inclination = 0.43° (to Saturn's equator) [ [http://sse.jpl.nasa.gov/planets/profile.cfm?Object=Sat_Hyperion&Display=Facts&System=Metric NASA's Solar System Exploration: Saturn: Moons: Hyperion: Facts & Figures] ] [ [http://www.mira.org/fts0/planets/100/text/txt002x.htm MIRA's Field Trips to the Stars Internet Education Program: Saturn] ]
satellite_of = Saturn
physical_characteristics = yes
dimensions = 360×280×225 km [ [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Hyperion NASA's Solar System Exploration: Saturn: Moons: Hyperion] ]
mass = (0.558 4 ± 0.006 8)e|19 kgcite journal| last=Jacobson| first=R. A.| coauthors=Antreasian, P. G.; Bordi, J. J.; Criddle, K. E.; et al.| title=The Gravity Field of the Saturnian System from Satellite Observations and Spacecraft Tracking Data| journal=The Astronomical Journal| month=December| year=2006| volume=132| pages=2520–2526| doi=10.1086/508812]
density = 0.566 7 ± 0.102 5 g/cm³
surface_grav = 0.017-0.021 m/s² depending on location cite journal| last=Thomas| first=P. C.| coauthors="et al."| title=Hyperion's sponge-like appearance| journal=Nature| year=2007| volume=448| pages=50–56 | doi=10.1038/nature05779 ]
escape_velocity = 45-99 m/s depending on location .
rotation = chaotic
axial_tilt = variable
albedo = 0.3cite web|first=David R.|last=Williams|date=
18 September 2006|title=Saturnian Satellite Fact Sheet|work=NASA|url=http://nssdc.gsfc.nasa.gov/planetary/factsheet/saturniansatfact.html|accessdate=2007-11-04]
Hyperion (pronEng|haɪˈpɪəriən respell|hye|PEER|ee-ən, or as in Greek "Ὑπερίων)" is a moon of Saturn discovered by
William Cranch Bond, George Phillips Bondand William Lassellin 1848. It is distinguished by its irregular shape, its chaotic rotation, and its unexplained sponge-like appearance.
Hyperion's discovery came shortly after
John Herschelhad suggested names for the seven previously-known satellites of Saturn in his 1847 publication "Results of Astronomical Observations made at the Cape of Good Hope". [As reported by William Lassell, [http://adsabs.harvard.edu//full/seri/MNRAS/0008//0000042.000.html Monthly Notices of the Royal Astronomical Society, Vol. 8, No. 3, pp. 42–43] 1848 January 14)] Lassell, who saw Hyperion two days after Bond, had already endorsed Herschel's naming scheme and suggested the name Hyperion in accordance with it. [Lassell, W.; [http://adsabs.harvard.edu//full/seri/MNRAS/0008//0000195.000.html "Discovery of a New Satellite of Saturn"] , Monthly Notices of the Royal Astronomical Society, Vol. 8, No. 9 (November 1848), pp. 195–197 ] He also beat Bond to publication. [Bond, W. C.; [http://adsabs.harvard.edu//full/seri/MNRAS/0009//0000001.000.html "Discovery of a new satellite of Saturn"] , Monthly Notices of the Royal Astronomical Society, Vol. 9, No. 1 ( November 10, 1848) pp. 1–2]
Hyperion is one of the largest highly irregular (non-spherical) bodies in the
solar system(second to Proteus). The largest crater on Hyperion is approximately 121.57 km in diameter and 10.2 km deep. A possible explanation for the irregular morphology is that Hyperion is a fragment of a larger body that was broken by a large impact in the distant past, an event which has been linked to the enigmatic darkening of Iapetus.Matthews, R. A. J.; [http://adsabs.harvard.edu/abs/1992QJRAS..33..253M "The Darkening of Iapetus and the Origin of Hyperion"] , Quarterly Journal of the Royal Astronomical Society, Vol. 33 (September 1992), pp. 253–258]
Like most of Saturn's moons, Hyperion's low
densityindicates that it is composed largely of water ice with only a small amount of rock. It is thought that Hyperion may be similar to a loosely accreted pile of rubble in its physical composition. However, unlike most of Saturn's moons, Hyperion has a low albedo(0.2–0.3), indicating that it is covered by at least a thin layer of dark material. This may be material from Phoebe (which is much darker) that got past Iapetus. Hyperion is redder than Phoebe and closely matches the color of the dark material on Iapetus.
Voyager 2" passed through the Saturn system but photographed Hyperion only from a distance. It discerned individual craters and an enormous ridge but was not able to make out the texture of the moon's surface. Early images from the "Cassini" orbiter suggested an unusual appearance, but it was not until "Cassini"'s sole targeted flyby of Hyperion on September 25, 2005that the moon's oddness was revealed in full.
Hyperion's surface is covered with deep, sharp-edged craters that give it the appearance of a giant sponge. Dark material fills the bottom of each crater. The reddish substance contains long chains of
carbonand hydrogenand appears very similar to material found on other Saturnian satellites, most notably Iapetus.
The latest analyses of data obtained by
NASA's "Cassini" spacecraft during its flybys of Hyperion in 2005 and 2006 show that about 40 percent of the moon is empty space. It was suggested in July 2007 that this porosityallows craters to remain nearly unchanged over the eons.The new analyses also confirmed that Hyperion is composed mostly of water ice with very little rock. "We find that water ice is the main constituent of the surface, but it's dirty water ice," said Dale Cruikshank, a researcher at NASA Ames Research Center. [cite web
title=Key to Giant Space Sponge Revealed | work=space.com
Voyager 2images and subsequent ground based photometry indicate that Hyperion's rotation is chaotic, that is, its axis of rotation wobbles so much that its orientation in space is unpredictable. Hyperion is the only known moon in the solar system that rotates chaotically, but simulations suggest that other irregular satellites may have done so in the past.It is unique among the large moons in that it is very irregularly shaped, has a fairly eccentric orbit, and is near another large moon, Titan. These factors combine to restrict the set of conditions under which a stable rotation is possible. The 3:4 orbital resonancebetween Titan and Hyperion may also make a chaotic rotation more likely. The odd rotation probably accounts for the relative uniformity of Hyperion's surface, in contrast to many of Saturn's other moons which have contrastive trailing and leading hemispheres. [cite journal | author=J. Wisdom, S.J. Peale, F. Mignard | title=The chaotic rotation of Hyperion | journal=(IAU, COSPAR, NASA, et al., Colloquium on Natural Satellites, 77th, Cornell University, Ithaca, NY, July 5-9, 1983) Icarus (ISSN 0019-1035) | month=May | year=1984 | volume=58 | pages=137–152 | url=http://adsabs.harvard.edu/abs/1984Icar...58..137W | doi=10.1016/0019-1035(84)90032-0 ]
Hyperion has been imaged several times from moderate distances by the Cassini orbiter. There was one close targeted fly-by, at a distance of 500 km on
2005 September 26; there are no plans for any others.
* [http://saturn.jpl.nasa.gov/science/moons/moonDetails.cfm?pageID=6 Cassini mission Hyperion page]
* [http://solarsystem.nasa.gov/planets/profile.cfm?Object=Sat_Hyperion Hyperion Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]
* [http://www.planetary.org/explore/topics/our_solar_system/saturn/hyperion.html The Planetary Society: Hyperion]
* [http://www.nasa.gov/multimedia/imagegallery/image_feature_749.html NASA: Saturn's Hyperion, A Moon With Odd Craters]
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