5145 Pholus

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5145 Pholus
Discovery
Discovered by Spacewatch
(David L. Rabinowitz)
Discovery date January 9, 1992
Designations
Alternative names 1992 AD
Minor planet
category
Centaur, Asteroid
Epoch November 26, 2005 (JD 2453700.5)
Aphelion 4806.533 Gm (32.130 AU)
Perihelion 1306.224 Gm (8.732 AU)
Semi-major axis 3056.379 Gm (20.431 AU)
Eccentricity 0.573
Orbital period 33730.363 d (92.35 a)
Average orbital speed 6.01 km/s
Mean anomaly 55.230°
Inclination 24.685°
Longitude of ascending node 119.332°
Argument of perihelion 355.225°
Physical characteristics
Dimensions 185±16 km [1]
Mass ~6.6×1018 kg
Mean density 2.0? g/cm³
Equatorial surface gravity ~0.052 m/s²
Escape velocity ~0.098 km/s
Rotation period 9.983 hours
Albedo 0.046±0.02
Temperature ~62 K
Spectral type (red) B-V=1.19; V-R=0.78 [1]
Absolute magnitude 7.64

5145 Pholus (pronounced /ˈfoʊləs/ foe'-ləs, from Greek: Φόλος) is a centaur in an eccentric orbit, with a perihelion near the orbit of Saturn and aphelion near the orbit of Neptune. It is believed to have originated as a Kuiper belt object.

It was discovered by David L. Rabinowitz, then of the University of Arizona's Spacewatch Project, and named after Pholus, the brother of the mythological Chiron, after which 2060 Chiron was named in order to follow the tradition of naming this class of outer planet crossing objects after Centaurs.

Pholus was the second centaur type asteroid to be discovered and was quickly found to be quite red in color, for which it has been occasionally nicknamed "Big Red". The color has been speculated to be due to organic compounds on its surface (Wilson, et al., 1994).

The surface composition of Pholus has been estimated from its reflectance spectrum using two spatially segregated components (Cruikshank, et al., 1998): dark amorphous carbon and an intimate mixture of water ice, methanol ice, olivine grains, and complex organic compounds (tholins). The carbon black component was used to match the low albedo of the object.

Unlike the first Centaur, 2060 Chiron, Pholus has shown no signs of cometary activity.

The diameter of Pholus is estimated to be 185±16 km [2].

[edit] References

  1. ^ Tegler, Stephen C. (2006-01-26). Kuiper Belt Object Magnitudes and Surface Colors. Retrieved on 2006-11-05.
  • Cruikshank DP, and 14 colleagues (1998). "The Composition of Centaur 5145 Pholus". Icarus 135: 389-407. doi:10.1006/icar.1998.5997.