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20729 Opheltius
Trojan asteroid From Wikipedia, the free encyclopedia
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20729 Opheltius (provisional designation 1999 XS143) is a Jupiter trojan from the Greek camp, approximately 51 kilometers (32 miles) in diameter. It was discovered on 15 December 1999, by American astronomer Charles Juels at the Fountain Hills Observatory in Arizona.[1] The dark Jovian asteroid has a short rotation period of 5.72 hours and belongs to the 90 largest Jupiter trojans.[7]
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Orbit and classification
Opheltius is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's L4 Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance .[3] It is also a non-family asteroid in the Jovian background population.[4]
It orbits the Sun at a distance of 4.9–5.5 AU once every 11 years and 11 months (4,352 days; semi-major axis of 5.22 AU). Its orbit has an eccentricity of 0.06 and an inclination of 22° with respect to the ecliptic.[2]
The body's observation arc begins with a precovery published by the Digitized Sky Survey and taken at the Palomar Observatory in February 1953, almost 47 years prior to its official discovery observation at Fountain Hills.[1]
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Numbering and naming
This minor planet was numbered on 9 January 2001 (M.P.C. 41908).[8] It was named in April 2025 after Opheltius, the name of two mythological figures; one an Achean killed by Hector, and the other a defender of Troy.[9]
Physical characteristics
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Opheltius is an assumed carbonaceous C-type asteroid. It has a high V–I color index of 1.00 (see table below).[7]
Rotation period
In September 2008, a rotational lightcurve of Opheltius was obtained from photometric observations. Lightcurve analysis gave a rotation period of 5.72±0.02 hours with a brightness variation of 0.33 magnitude (U=2).[6][7]
Observations by Stefano Mottola at the Calar Alto Observatory in October 2009 showed a divergent period of 7.631 hours with an amplitude of 0.20 magnitude (U=2).[7][10]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Opheltius is 50.96 kilometers in diameter and its surface has an albedo of 0.052,[5] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 46.30 kilometers based on an absolute magnitude of 10.4.[7] The object was neither observed by IRAS nor the Akari satellite.
100+ largest Jupiter trojans
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References
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