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5335 Damocles

From Wikipedia, the free encyclopedia
Centaur
(5335) Damocles
Discovery
Discovered byR. H. McNaught
Discovery siteSiding Spring Obs.
Discovery date18 February 1991
Designations
(5335) Damocles
Pronunciation/ˈdæməklz/[1]
Named after
Damocles(Greek mythology)[2]
1991 DA
distant[3]
centaur[4] · damocloid[5]
AdjectivesDamoclean (/dæməˈkliːən/)[6]
Symbol (astrological)
Orbital characteristics[4]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 4
Observation arc1.51 yr (551 days)
Aphelion22.078 AU
Perihelion1.5741 AU
11.826 AU
Eccentricity0.8669
40.67 Jyr (14,854 days)
236.35°
0° 1m 27.12s / day
Inclination61.875°
314.14°
191.26°
Mars MOID0.05787 AU[3]
TJupiter1.149
Physical characteristics
Dimensions~ 10 km[7]
26.56[8]
13.3[4][8]

(5335) Damocles/ˈdæməklz/, provisional designation1991 DA, is acentaur and the namesake of thedamocloids, a group ofminor planets which may be inactive nuclei of theHalley-type andlong-period comets. It was discovered on 18 February 1991, by Australian astronomerRobert McNaught atSiding Spring Observatory in Australia. It is named afterDamocles, a figure ofGreek mythology.[2]

Description

[edit]

When Damocles was discovered, it was found to be on anorbit completely different from all others known. Damocles's orbit reached from inside theaphelion ofMars to as far asUranus. It seemed to be in transition from a near-circularouter Solar System orbit to an eccentric orbit taking it to theinner Solar System.[9]Duncan Steel, Gerhard Hahn, Mark Bailey, andDavid Asher carried out projections of its long-term dynamical evolution, and found a good probability that it will become anEarth-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 nearJupiter orSaturn.[10][11]

There is some speculation that Damocles may have ameteor shower associated with it on Mars from the direction ofDraco.[12] The object has a Marsminimum orbit intersection distance (Mars MOID) of 0.057 AU (8,500,000 km; 5,300,000 mi) and a Uranus MOID of 0.3 AU (45,000,000 km; 28,000,000 mi).[3]

As of 2019[update], Damocles is 19.6 AU from the Sun with anapparent magnitude of 26.3.[8] It reached its furthest point from the Sun in 2011.

The adjectival form is Damoclean,/dæməˈkliːən/.[6] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22508).[13]

See also

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

References

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  1. ^Webster, Noah (1884).A Practical Dictionary of the English Language.
  2. ^abSchmadel, Lutz D. (2007). "(5335) Damocles".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 457.doi:10.1007/978-3-540-29925-7_5143.ISBN 978-3-540-00238-3.
  3. ^abc"(5335) Damocles (1991 DA)".Minor Planet Center. Retrieved14 February 2017.
  4. ^abc"1992-08-22 last obs". JPL Small-Body Database Browser. (5335) Damocles (1991 DA).Jet Propulsion Laboratory. Retrieved21 September 2017.
  5. ^Akimasa Nakamura and bas (2 May 2009)."List of Damocloids (Oort cloud asteroids)". Lowell Observatory. Retrieved15 February 2017.
  6. ^abOxford English Dictionary
  7. ^Johnston, Wm. Robert (25 May 2019)."List of known trans-Neptunian objects".Johnston'sArchive.net. Retrieved31 May 2019.
  8. ^abc"AstDyS Damocles Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved21 September 2017.
  9. ^Steel, D. (1995).Rogue Asteroids and Doomsday Comets. Wiley & Sons. pp. 127–128.
  10. ^Asher, David J.; Bailey; Hahn; Steel (1994)."Asteroid (5335) Damocles and its implications for cometary dynamics".Monthly Notices of the Royal Astronomical Society.267: 26.Bibcode:1994MNRAS.267...26A.doi:10.1093/mnras/267.1.26.
  11. ^Asher, David; Bailey, Mark; Hahn, Gerhard; Steel, Duncan (27 May 1993)."Asteroid (5335) Damocles and its implications for cometary dynamics".Monthly Notices of the Royal Astronomical Society.267:26–42.Bibcode:1994MNRAS.267...26A.doi:10.1093/mnras/267.1.26.
  12. ^"Meteor Showers and Their Parent Bodies". Archived fromthe original on 3 October 2008. Retrieved30 December 2006.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved14 February 2017.

External links

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Distant minor planet
Comets
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