C/2001 OG108

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C/2001 OG108 (LONEOS)
Discovery
Discovered by M. E. Van Ness[1]
LONEOS telescope at Lowell Observatory
Discovery date 28 July 2001[2]
Orbital characteristics A
Epoch 15 December 2001[3]
(JD 2452258.5)
Aphelion 25.606 AU (Q)
Perihelion 0.99404 AU (q)
Semi-major axis 13.300 AU (a)
Eccentricity 0.92526
Orbital period 48.51 yr
Inclination 80.245°
Last perihelion 2002-Mar-15[3]
Next perihelion 2050-Jun-06[4]

C/2001 OG108 (LONEOS) is a Halley-type comet with an orbital period of 48.51 years.[3] It was discovered on 28 July 2001 by the LONEOS telescope at Lowell Observatory.[2]

Observations taken in January and February 2002 showed that the "asteroid" had developed a small amount of cometary activity as it approached perihelion.[1] It was subsequently reclassified as a comet.[1] The comet came to perihelion (closest approach to the Sun) on 15 March 2002.[3] The next perihelion passage is calculated to be on 6 June 2050.[4]

The comet has a rotational period of 2.38 ± 0.02 days (57.12 hr).[1][3]

In 2003, the comet was estimated to have a mean absolute V magnitude (H) of 13.05 ± 0.10, with an albedo of 0.03, giving an effective radius of 8.9 ± 0.7 km.[1] Using data from Fernandez (2004–2005) JPL lists the comet with an albedo of 0.05 and a diameter of 13.6 ± 1.0 km.[3]

This comet probably represents the transition between typical Halley-family/long-period comets and extinct comets.[1] Damocloids have been studied as possible extinct cometary candidates due to the similarity of their orbital parameters with those of Halley-family comets.[1]

See also

References

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External links