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1 Classification and orbit  



1.1  Retrograde orbit  







2 Naming  





3 Physical characteristics  





4 References  





5 External links  














20461 Dioretsa






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From Wikipedia, the free encyclopedia
 


20461 Dioretsa
Discovery [1]
Discovered byLINEAR
Discovery siteLincoln Lab ETS
Discovery date8 June 1999
Designations

MPC designation

(20461) Dioretsa
Pronunciation/d.əˈrɛtsə/

Named after

Asteroid[2]
(spelled backwards)

Alternative designations

1999 LD31

Minor planet category

centaur[3] · damocloid[4]
unusual[5] · distant[1]
Symbol (astrological)
Orbital characteristics[3]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter2
Observation arc2.54 yr (927 d)
Aphelion45.404 AU
Perihelion2.4021 AU

Semi-major axis

23.903 AU
Eccentricity0.8995

Orbital period (sidereal)

116.87 yr (42,686 d)

Mean anomaly

59.873°

Mean motion

0° 0m 30.24s / day
Inclination160.43°

Longitude of ascending node

297.77°

Argument of perihelion

103.13°
Jupiter MOID0.1907 AU
TJupiter-1.5470
Physical characteristics

Mean diameter

14±km[4][6]

Geometric albedo

0.03±0.01[4][6]

Absolute magnitude (H)

13.8[1][3]

20461 Dioretsa /d.əˈrɛtsə/ is a centaur and damocloid on a retrograde, cometary-like orbit from the outer Solar System. It was discovered on 8 June 1999, by members of the LINEAR team at the Lincoln Laboratory Experimental Test Site near Socorro, New Mexico, United States.[1] The highly eccentric unusual object measures approximately 14 kilometers (8.7 miles) in diameter.[4][6] It was named Dioretsa, the word "asteroid" spelled backwards.[1]

Classification and orbit[edit]

Dioretsa is a member of the damocloids,[4] with a retrograde orbit and a negative TJupiter of −1.547. It is also a centaur, as its orbit has a semi-major axis in between that of Jupiter (5.5 AU) Neptune (30.1 AU).[3] The Minor Planet Center lists it as a critical object and (other) unusual minor planet due to an orbital eccentricity of more than 0.5.[5]

It orbits the Sun at a distance of 2.4–45.4 AU once every 116 years and 10 months (42,686 days; semi-major axis of 23.9 AU). Its orbit has an eccentricity of 0.90 and an inclination of 160° with respect to the ecliptic.[3] Its observation arc begins 12 months prior to its official discovery observation, with a precovery taken by SpacewatchatSteward Observatory in June 1998.[1] As of 2021, it was last observed in 2000 and its orbit still has an uncertainty of 2.[3]

Retrograde orbit[edit]

An inclination of greater than 90° means that a body moves in a retrograde orbit. Dioretsa's orbit is otherwise similar to that of a comet. This has led to speculation that Dioretsa was originally an object from the Oort cloud.[citation needed]

Naming[edit]

The minor planet's name "Dioretsa" is the word "asteroid" spelled backwards, and is the first numbered of currently 136 known (see Data Base Search of the Minor Planet Center) minor planets with a retrograde motion in the Solar System.[2] The approved naming citation was published by the Minor Planet Center on 1 May 2003 (M.P.C. 48396).[7]

Physical characteristics[edit]

According to observations made with the 10-meter Keck Telescope, Dioretsa measures 14 kilometers in diameter and its surface has a low albedo of 0.03.[6] It has an absolute magnitude of 13.8.[3] As of 2018, Dioretsa's spectral type as well as its rotation period and shape remain unknown.[3][8]

References[edit]

  1. ^ a b c d e f "20461 Dioretsa (1999 LD31)". Minor Planet Center. Retrieved 20 November 2018.
  • ^ a b Schmadel, Lutz D. (2006). "(20461) Dioretsa [24.4, 0.90, 160.2]". Dictionary of Minor Planet Names – (20461) Dioretsa, Addendum to Fifth Edition: 2003–2005. Springer Berlin Heidelberg. p. 152. doi:10.1007/978-3-540-34361-5_1728. ISBN 978-3-540-34360-8.
  • ^ a b c d e f g h "JPL Small-Body Database Browser: 20461 Dioretsa (1999 LD31)" (2000-12-29 last obs.). Jet Propulsion Laboratory. Retrieved 20 November 2018.
  • ^ a b c d e Johnston, Wm. Robert (7 October 2018). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 20 January 2018.
  • ^ a b "List Of Other Unusual Objects". Minor Planet Center. 14 November 2018. Retrieved 20 November 2018.
  • ^ a b c d Harris, Alan W.; Delbó, Marco; Binzel, Richard P.; Davies, John K.; Roberts, Julie; Tholen, David J.; et al. (October 2001). "Visible to Thermal-Infrared Spectrophotometry of a Possible Inactive Cometary Nucleus". Icarus. 153 (2): 332–337. Bibcode:2001Icar..153..332H. doi:10.1006/icar.2001.6687. Retrieved 4 April 2016.
  • ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 20 November 2018.
  • ^ "LCDB Data for (20461) Dioretsa". Asteroid Lightcurve Database (LCDB). Retrieved 27 June 2017.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=20461_Dioretsa&oldid=1218342330"

    Categories: 
    Minor planet object articles (numbered)
    Centaurs (small Solar System bodies)
    Damocloids
    Unusual minor planets
    Discoveries by LINEAR
    Named minor planets
    Astronomical objects discovered in 1999
    Minor planets with a retrograde orbit
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    Articles with short description
    Short description is different from Wikidata
    Use dmy dates from June 2014
    Articles containing potentially dated statements from 2021
    All articles containing potentially dated statements
    All articles with unsourced statements
    Articles with unsourced statements from June 2017
    Webarchive template wayback links
    Articles with JPL SBDB identifiers
    Articles with MPC identifiers
     



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