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Linus (moon)

Linus, formal designation (22) Kalliope I Linus, is an asteroid moon that orbits the large M-type asteroid 22 Kalliope. It was discovered on August 29, 2001, by astronomers Jean-Luc Margot and Michael E. Brown with the Keck telescope, in Hawaii. Another team also detected the moon with the Canada-France-Hawaii Telescope on September 2, 2001. Both telescopes are on Mauna Kea. It received the provisional designation S/2001 (22) 1,[1] until it was named. The naming proposal appeared in the discovery paper[3] and was approved by the International Astronomical Union in July 2003.[8] Although the naming proposal referred to the mythological Linus, son of the muse Calliope and the inventor of melody and rhythm, the name was also meant to honor Linus Torvalds, inventor of the Linux operating system kernel, and Linus van Pelt, a character in the Peanuts comic strip.[9]

Linus
Kalliope and satellite Linus as seen by the W.M. Keck II telescope in 2010
Discovery[1]
Discovered byJean-Luc Margot and Michael 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 ± 23 km[3] (1040-1086) 1099 ± 11 km[4] (1088-1110)
Eccentricity<0.015 [3] <0.005 [5]
3.596 ± 0.040 d[3] (3.556-3.636) 3.590 ± 0.001 d[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)
Mean density
3.4 g/cm3 (assumed)
Equatorial escape velocity
~20 m/s (estimate)
unknown, probably synchronous[3][6]
unknown, zero expected
Surface temp. min mean max
Kelvin ~161 240
Celsius ~ -113 −32°
9.7 [7]

With an estimated 28 ± 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 the main belt are the smaller components of the double asteroids 617 Patroclus and 90 Antiope.

It has been estimated that Linus' orbit precesses 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 of impact ejecta from a collision with Kalliope, or a fragment captured after disruption of a parent asteroid (a proto-Kalliope).

References edit

  1. ^ a b "IAUC 7703: S/2001 (22) 1; 2001ed". IAU Central Bureau for Astronomical Telegrams. September 3, 2001. Retrieved 2012-07-18.
  2. ^ "linia" = 'of Linus' in Banier (1793) The mythology and fables of the ancients, explain'd from history, v. 1; also in Charles Frederick Partington (1838) The British Cyclopædia of Biography
  3. ^ a b c d e f g h J.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. ^ a b c Descamps, 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. ^ a b c synthesis of several observations 2006-08-29 at the Wayback Machine including recent ones with the VLT 8m telescope.
  6. ^ Based on a rough tidal locking timescale of several tens of My.
  7. ^ a b c F. 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". IAU Central Bureau for Astronomical Telegrams. August 8, 2003. Retrieved 2012-07-18.
  9. ^ Margot, Jean-Luc (2004). "Adaptive Optics Observations of Kalliope-Linus". UCLA. Retrieved 2013-08-30.

External links edit

  • IAUC 7703: S/2001 (22) 1, announcing Linus' discovery (2001 September 3)
  • IAUC 8177: Sats of (22); Sats of Jupiter, Saturn, Uranus, announcing Linus' naming (2003 August 8)
  • Link to the Linus discovery paper , "A Low-Density M-type Asteroid in the Main Belt"
  • very well resolved with the 8m VLT
  • another image of Kalliope and Linus

linus, moon, linus, formal, designation, kalliope, linus, asteroid, moon, that, orbits, large, type, asteroid, kalliope, discovered, august, 2001, astronomers, jean, margot, michael, brown, with, keck, telescope, hawaii, another, team, also, detected, moon, wi. Linus formal designation 22 Kalliope I Linus is an asteroid moon that orbits the large M type asteroid 22 Kalliope It was discovered on August 29 2001 by astronomers Jean Luc Margot and Michael E Brown with the Keck telescope in Hawaii Another team also detected the moon with the Canada France Hawaii Telescope on September 2 2001 Both telescopes are on Mauna Kea It received the provisional designation S 2001 22 1 1 until it was named The naming proposal appeared in the discovery paper 3 and was approved by the International Astronomical Union in July 2003 8 Although the naming proposal referred to the mythological Linus son of the muse Calliope and the inventor of melody and rhythm the name was also meant to honor Linus Torvalds inventor of the Linux operating system kernel and Linus van Pelt a character in the Peanuts comic strip 9 LinusKalliope and satellite Linus as seen by the W M Keck II telescope in 2010Discovery 1 Discovered byJean Luc Margot and Michael E BrownDiscovery dateAugust 29 2001DesignationsMPC designationKalliope IPronunciation ˈ l aɪ n e s Named afterLinusAlternative designationsS 2001 22 1Minor planet categoryMain beltAdjectivesLinian ˈ l ɪ n i e n 2 Orbital characteristicsSemi major axis1063 23 km 3 1040 1086 1099 11 km 4 1088 1110 Eccentricity lt 0 015 3 lt 0 005 5 Orbital period sidereal 3 596 0 040 d 3 3 556 3 636 3 590 0 001 d 5 3 589 3 591 Average orbital speed21 5 m sInclination 0 3 5 undetectable with respect to Kalliope equator Satellite of22 KalliopePhysical characteristicsDimensions28 2 km 4 Mass 6 1016 kg estimate 3 4 1016 kg estimate Mean density3 4 g cm3 assumed Equatorial escape velocity 20 m s estimate Synodic rotation periodunknown probably synchronous 3 6 Axial tiltunknown zero expectedSurface temp min mean maxKelvin 161 240Celsius 113 32 Absolute magnitude H 9 7 7 With an estimated 28 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 the main belt are the smaller components of the double asteroids 617 Patroclus and 90 Antiope It has been estimated that Linus orbit precesses 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 of impact ejecta from a collision with Kalliope or a fragment captured after disruption of a parent asteroid a proto Kalliope References edit a b IAUC 7703 S 2001 22 1 2001ed IAU Central Bureau for Astronomical Telegrams September 3 2001 Retrieved 2012 07 18 linia of Linus in Banier 1793 The mythology and fables of the ancients explain d from history v 1 also in Charles Frederick Partington 1838 The British Cyclopaedia of Biography a b c d e f g h J L Margot amp 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 a b c Descamps 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 a b c synthesis of several observations Archived 2006 08 29 at the Wayback Machine including recent ones with the VLT 8m telescope Based on a rough tidal locking timescale of several tens of My a b c F 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 IAUC 8177 Sats of 22 Sats of Jupiter Saturn Uranus IAU Central Bureau for Astronomical Telegrams August 8 2003 Retrieved 2012 07 18 Margot Jean Luc 2004 Adaptive Optics Observations of Kalliope Linus UCLA Retrieved 2013 08 30 External links editIAUC 7703 S 2001 22 1 announcing Linus discovery 2001 September 3 IAUC 8177 Sats of 22 Sats of Jupiter Saturn Uranus announcing Linus naming 2003 August 8 Link to the Linus discovery paper A Low Density M type Asteroid in the Main Belt Kalliope and Linus very well resolved with the 8m VLT orbit diagram for Linus Information on Kalliope Linus orbit and several images A different VLT image of Kalliope and Linus another image of Kalliope and Linus Retrieved from https en wikipedia org w index php title Linus moon amp oldid 1212860393, wikipedia, wiki, book, books, library,

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