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Linus (moon)

From Wikipedia, the free encyclopedia
Asteroid moon that orbits 22 Kalliope
Linus
Kalliope and satellite Linus as seen by theW.M. Keck II telescope in 2010
Discovery[1]
Discovered byJean-Luc Margot andMichael E. Brown
Discovery dateAugust 29, 2001
Designations
Kalliope I
Pronunciation/ˈlnəs/
Named after
Linus
S/2001 (22) 1
Main belt
AdjectivesLinian/ˈlɪniən/[2]
Orbital characteristics
1063 ± 23km[3] (1040-1086) 1099 ± 11km[4] (1088-1110)
Eccentricity<0.015[3] <0.005[5]
3.596 ± 0.040d[3] (3.556-3.636) 3.590 ± 0.001d[5] (3.589-3.591)
21.5 m/s
Inclination~0°[3][5]
(undetectable with respect to Kalliope equator)
Satellite of22 Kalliope
Physical characteristics
Dimensions28 ± 2 km[4]
Mass~6×1016 kg(estimate)[3] ~4×1016 kg(estimate)
3.4 g/cm3 (assumed)
Equatorialescape velocity
~20 m/s(estimate)
unknown, probablysynchronous[3][6]
unknown, zero expected
Surfacetemp.minmeanmax
Kelvin~161240
Celsius~ -113−32°
9.7[7]

Linus, formal designation(22) Kalliope I, is anasteroid moon that orbits the largeM-type asteroid22 Kalliope. It was discovered on August 29, 2001, byastronomersJean-Luc Margot andMichael E. Brown with theKeck telescope, inHawaii. Another team also detected the moon with theCanada-France-Hawaii Telescope on September 2, 2001. Both telescopes are onMauna Kea. It received theprovisional designation S/2001 (22) 1,[1] until it was named. The naming proposal appeared in the discovery paper[3] and was approved by theInternational Astronomical Union in July 2003.[8] Although the naming proposal referred to the mythologicalLinus, son of the museCalliope and the inventor of melody and rhythm, the name was also meant to honorLinus Torvalds, inventor of theLinux operating system kernel, andLinus van Pelt, a character in thePeanuts comic strip.[9]

With an estimated28 ± 2 km (17 ± 1 mi) diameter,[4] Linus is very large compared to most asteroid moons, and would be a sizable asteroid by itself. The only known larger moons in themain belt are the smaller components of the double asteroids617 Patroclus and90 Antiope.

It has been estimated that Linus' orbitprecesses at quite a rapid rate, making one cycle in several years. This is attributed primarily to the non-spherical shape of Kalliope.[3][7] Linus's brightness has varied appreciably between observations, which may indicate that its shape is elongated.[7]

Linus may have formed out ofimpactejecta from acollision with Kalliope, or a fragment captured after disruption of a parent asteroid (a proto-Kalliope).

References

[edit]
  1. ^ab"IAUC 7703: S/2001 (22) 1; 2001ed". IAUCentral Bureau for Astronomical Telegrams. September 3, 2001. Retrieved2012-07-18.
  2. ^"linia" = 'of Linus' in Banier (1793)The mythology and fables of the ancients, explain'd from history, v. 1; also inCharles Frederick Partington (1838)The British Cyclopædia of Biography
  3. ^abcdefghJ.L. Margot & M.E. Brown (2003). "A Low-Density M-type Asteroid in the Main Belt".Science.300 (5627):1939–42.Bibcode:2003Sci...300.1939M.doi:10.1126/science.1085844.PMID 12817147.
  4. ^abcDescamps, P.; Marchis, F.; et al. (2008). "New determination of the size and bulk density of the binary asteroid 22 Kalliope from observations of mutual eclipses".Icarus.196 (2):578–600.arXiv:0710.1471.Bibcode:2008Icar..196..578D.doi:10.1016/j.icarus.2008.03.014.
  5. ^abcsynthesis of several observationsArchived 2006-08-29 at theWayback Machine including recent ones with theVLT 8m telescope.
  6. ^Based on a roughtidal locking timescale of several tens of My.
  7. ^abcF. Marchis; et al. (2003). "A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope".Icarus.165 (1): 112.Bibcode:2003Icar..165..112M.doi:10.1016/S0019-1035(03)00195-7.
  8. ^"IAUC 8177: Sats of (22); Sats of Jupiter, Saturn, Uranus". IAUCentral Bureau for Astronomical Telegrams. August 8, 2003. Retrieved2012-07-18.
  9. ^Margot, Jean-Luc (2004)."Adaptive Optics Observations of Kalliope-Linus".UCLA. Retrieved2013-08-30.

External links

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