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2449 Kenos

From Wikipedia, the free encyclopedia
Mars-crossing asteroid
For the Romanian village Chinuşu, seeKénos.

2449 Kenos
Discovery[1]
Discovered byW. Liller
Discovery siteCerro Tololo
Discovery date8 April 1978
Designations
(2449) Kenos
Named after
Kenos(Selknam mythology)[2]
1978 GC
Mars-crosser[1] · Hungaria[3] · binary
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.93 yr (14,220 days)
Aphelion2.2303AU
Perihelion1.5872 AU
1.9088 AU
Eccentricity0.1685
2.64yr (963 days)
258.57°
0° 22m 25.32s / day
Inclination24.986°
179.86°
102.25°
Physical characteristics
Dimensions2.95 km(calculated)[4]
3.846±0.001 h[5]
3.8481±0.0003 h[6]
3.8492±0.0008 h[7]
4.188±0.007h[8]
0.4(assumed)[4]
Tholen =E[1] · CX[9] · E[4]
B–V = 0.684[1]
U–B = 0.356[1]
14.07±0.09[8] · 14.26[1][4] · 14.46±0.48[9]

2449 Kenos, provisional designation1978 GC, is a bright Hungariaasteroid and medium-sizedMars-crosser from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. It was discovered by American astronomerWilliam Liller atCerro Tololo Inter-American Observatory in Chile, on 8 April 1978, and named afterKenos from Selknam mythology.[2][3] Aminor-planet moon was discovered around the asteroid on 27 February 2015.[10]

Orbit and classification

[edit]

Kenos is a member of theHungaria family, which form the innermost dense concentration of asteroids in the Solar System. IT orbits the Sun in theinner main-belt at a distance of 1.6–2.2 AU once every 2 years and 8 months (963 days). Its orbit has aneccentricity of 0.17 and aninclination of 25° with respect to theecliptic.[1] Based on assumption made by the Collaborative Asteroid Lightcurve Link, the body has a highalbedo of 0.4, which is typical for E-type asteroids with a magnesium silicate surface(also seeEnstatite chondrite).

Physical characteristics

[edit]

In theTholen taxonomy,Kenos is anE-type asteroid.[1]PanSTARRS has characterized it as a CX-type, which transitions between theC-type andX-type asteroids.[9]

Observations performed at the Palmer Divide Observatory (716) in Colorado Springs, Colorado, during 2007 produced alightcurve with a period of3.8492 hours and a brightness range of0.20 inmagnitude.[7] Two more recent observations confirmed the 3.85-hour period.[5][6]

Naming

[edit]

Thisminor planet was named afterKenos, the first man in theSelknam mythology of the Native Americans ofTierra del Fuego, sent by the Supreme Being to bring order into the world. He created the human race by using peat to make male and female organs, taught them language and instructed them in rules to fashion a harmonious society.[2] The official naming citation was published by theMinor Planet Center on 6 February 1993 (M.P.C. 21606).[11]

References

[edit]
  1. ^abcdefghi"JPL Small-Body Database Browser: 2449 Kenos (1978 GC)" (2017-03-14 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 September 2020. Retrieved13 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2449) Kenos".Dictionary of Minor Planet Names – (2449) Kenos.Springer Berlin Heidelberg. pp. 199–200.doi:10.1007/978-3-540-29925-7_2450.ISBN 978-3-540-00238-3.
  3. ^ab"2449 Kenos (1978 GC)".Minor Planet Center. Retrieved6 December 2016.
  4. ^abcd"LCDB Data for (2449) Kenos". Asteroid Lightcurve Database (LCDB). Retrieved6 December 2016.
  5. ^abWarner, Brian D. (October 2010)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2010 March - June".The Minor Planet Bulletin.37 (4):161–165.Bibcode:2010MPBu...37..161W.ISSN 1052-8091. Retrieved6 December 2016.
  6. ^abWarner, Brian D. (July 2015)."Three Unusual Hungaria Asteroids".The Minor Planet Bulletin.42 (3):183–186.Bibcode:2015MPBu...42..183W.ISSN 1052-8091. Retrieved6 December 2016.
  7. ^abWarner, Brian D. (September 2007)."Asteroid Lightcurve Analysis at the Palmer Divide Observatory - December 2006 - March 2007".The Minor Planet Bulletin.34 (3):72–77.Bibcode:2007MPBu...34...72W.ISSN 1052-8091. Retrieved6 December 2016.
  8. ^abWisniewski, W. Z.; Michalowski, T. M.; Harris, A. W.; McMillan, R. S. (March 1995)."Photoelectric Observations of 125 Asteroids".Abstracts of the Lunar and Planetary Science Conference.26: 1511.Bibcode:1995LPI....26.1511W. Retrieved6 December 2016.
  9. ^abcVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007. Retrieved6 December 2016.
  10. ^Johnston, W. R. (29 May 2019)."(2449) Kenos".Asteroids with Satellites Database. Johnston's Archive. Retrieved23 November 2019.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 December 2016.

External links

[edit]
Minor planets
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