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Linus (moon)
From Wikipedia, the free encyclopedia
| Discovery[1] and Designation | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Discovered by: | Jean-Luc Margot and Michael E. Brown | |||||||||
| Discovery date: | August 29, 2001 | |||||||||
| Orbital characteristics | ||||||||||
| Semi-major axis: | 1065 ± 8 km[2] [3][4] | |||||||||
| Eccentricity: | < 0.005 [2] | |||||||||
| Orbital period: | 3.590 ± 0.001 d [2] | |||||||||
| Avg. orbital speed: | 21.5 m/s | |||||||||
| Inclination: | 9 ± 1° [2] (with respect to Kalliope equator) |
|||||||||
| Satellite of: | 22 Kalliope | |||||||||
| Physical characteristics | ||||||||||
| Dimensions: | 38 ± 6 km [4][5] | |||||||||
| Mass: | ~6×1016 kg (estimate) [4] | |||||||||
| Equatorial Escape velocity: | ~20 m/s (estimate) | |||||||||
| Rotation period: | unknown, probably synchronous[6] | |||||||||
| Axial tilt: | unknown, zero expected | |||||||||
| Surface temp.: Kelvin Celsius |
|
|||||||||
| Absolute magnitude: | 9.7 [4] | |||||||||
(22) Kalliope I Linus is an asteroid moon that orbits the large M-type asteroid 22 Kalliope.
With an estimated 38±6 km diameter [4], Linus is very large compared to most asteroid moons, and in fact would be a sizeable asteroid by itself. The only known larger moons in the Main belt are the two components of the double asteroid 90 Antiope.
On August 29, 2001, astronomers Jean-Luc Margot and Michael E. Brown discovered Linus orbiting 22 Kalliope with the Keck telescope. 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, and was named on August 8, 2003 after the mythological Linus, son of the muse Calliope and the inventor of melody and rhythm.
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][4]. Linus's brightness has varied appreciably between observations, which may indicate that its shape is elongated [4].
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).
- ^ IAUC 7703
- ^ a b c d synthesis of several observations including recent ones with the VLT 8m telescope.
- ^ a b J.L. Margot & M.E. Brown (2003). "A Low-Density M-type Asteroid in the Main Belt". Science 300: 1939.
- ^ a b c d e f g F. Marchis et al (2003). "A three-dimensional solution for the orbit of the asteroidal satellite of 22 Kalliope". Icarus 165: 112.
- ^ Assuming the same albedo as Kalliope.
- ^ Based on a rough tidal locking timescale of several tens of My.
- IAUC 7703, announcing Linus' discovery
- IAUC 8177, announcing Linus' naming
- 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
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| Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Neptune Trojans · Comets · Trans-Neptunians (Kuiper belt • Scattered disc objects • Oort cloud) |
| For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons, meteoroids and the Solar System. For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |