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2325 Chernykh

From Wikipedia, the free encyclopedia
Themistian asteroid

2325 Chernykh
Discovery[1]
Discovered byA. Mrkos
Discovery siteKlet Obs.
Discovery date25 September 1979
Designations
(2325) Chernykh
Named after
Lyudmila Chernykh
Nikolai Chernykh
(Russian astronomers)[1]
1979 SP · 1957 UJ
1959 CH · 1971 FR
1974 WD1 · 1974 XN
1979 UG3
main-belt[1][2] · (outer)
Themis[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc62.03yr (22,658 d)
Aphelion3.6909AU
Perihelion2.5870 AU
3.1389 AU
Eccentricity0.1758
5.56 yr (2,031 d)
281.91°
0° 10m 37.92s / day
Inclination1.9199°
139.94°
267.37°
Physical characteristics
22.789±0.194 km[4]
0.065±0.012[4]
11.9[2]

2325 Chernykh, provisional designation1979 SP, is a dark Themistianasteroid from the outer regions of theasteroid belt, approximately 23 kilometers (14 miles) in diameter. It was discovered on 25 September 1979, by Czech astronomerAntonín Mrkos at theKlet Observatory in the Czech Republic. The asteroid was named after Russian astronomer coupleLyudmila Chernykh andNikolai Chernykh.[1]

Orbit and classification

[edit]

Chernykh is a Themistian asteroid that belongs to theThemis family (602),[3] a very largefamily of carbonaceous asteroids, named after24 Themis.[5] It orbits the Sun in theouter main-belt at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,031 days;semi-major axis of 3.14 AU). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[2] The body'sobservation arc begins with its firstprecovery observation atPalomar Observatory in May 1955.[1]

Physical characteristics

[edit]

Although the asteroid'sspectral type is unknown, its albedo indicates acarbonaceous composition, which also agrees withC-type classification for the Themistian asteroids.[5]: 23 

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Chernykh measures 22.789 kilometers in diameter and its surface has analbedo of 0.065.[4] As of 2018, no rotationallightcurve ofChernykh has been obtained fromphotometric observations. The body'srotation period,pole and shape remain unknown.[2]

Naming

[edit]

Thisminor planet was named after the Russian astronomersLyudmila Chernykh (1935–2017) andNikolai Chernykh (1931–2004), prolificdiscoverers of minor planets who lead the extensive astrometric program at the discoveringCrimean Astrophysical Observatory.[1] The official naming citation was published by theMinor Planet Center on 1 June 1981 (M.P.C. 6060).[6]

References

[edit]
  1. ^abcdef"2325 Chernykh (1979 SP)".Minor Planet Center. Retrieved26 March 2018.
  2. ^abcde"JPL Small-Body Database Browser: 2325 Chernykh (1979 SP)" (2017-06-03 last obs.).Jet Propulsion Laboratory. Retrieved26 March 2018.
  3. ^ab"Asteroid 2325 Chernykh – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  4. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.
  5. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  6. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 March 2018.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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