Английская Википедия:5335 Damocles

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Шаблон:Infobox planet

(5335) Damocles Шаблон:IPAc-en, provisional designation Шаблон:Mp, is a centaur and the namesake of the damocloids, a group of minor planets which may be inactive nuclei of the Halley-type and long-period comets. It was discovered on 18 February 1991, by Australian astronomer Robert McNaught at Siding Spring Observatory in Australia. It is named after Damocles, a figure of Greek mythology.[1]

Description

When Damocles was discovered, it was found to be on an orbit completely different from all others known. DamoclesШаблон:'s orbit reached from inside the aphelion of Mars to as far as Uranus. It seemed to be in transition from a near-circular outer Solar System orbit to an eccentric orbit taking it to the inner Solar System.[2] Duncan Steel, Gerhard Hahn, Mark Bailey, and David Asher carried out projections of its long-term dynamical evolution, and found a good probability that it will become an Earth-crosser asteroid, and may spend a quarter of its life in such an orbit. Damocles has a stable orbit for tens of thousands of years before and after the present, because its highly inclined orbit does not take it near Jupiter or Saturn.[3][4]

There is some speculation that Damocles may have a meteor shower associated with it on Mars from the direction of Draco.[5] The object has a Mars minimum orbit intersection distance (Mars MOID) of Шаблон:Convert and a Uranus MOID of Шаблон:Convert.[6]

Шаблон:As of, Damocles is 19.6 AU from the Sun with an apparent magnitude of 26.3 .[7] It reached its furthest point from the Sun in 2011.

The adjectival form is Damoclean, Шаблон:IPA.[8] The official naming citation was published by the Minor Planet Center on 1 September 1993 (Шаблон:Small).[9]

See also

  • The sword of Damocles – an over-hanging threat, a long-standing political metaphor from ancient Greece.

References

Шаблон:Reflist

External links

Шаблон:Minor planets navigator Шаблон:Small Solar System bodies Шаблон:Authority control

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