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3174 Alcock

From Wikipedia, the free encyclopedia
Asteroid

3174 Alcock
Shape model ofAlcock from itslightcurve
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date26 October 1984
Designations
(3174) Alcock
Named after
George Alcock
(amateur astronomer)[2]
1984 UV · 1962 YD
1969 BB · 1973 YO1
1975 EO3 · 1978 RB1
1978 TJ3 · 1979 YR8
1980 AH · 1981 GF
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc47.71 yr (17,426 days)
Aphelion3.6932AU
Perihelion2.5991 AU
3.1462 AU
Eccentricity0.1739
5.58yr (2,038 days)
296.20°
0° 10m 35.76s / day
Inclination2.3715°
72.244°
4.6082°
Physical characteristics
18.66±0.80 km[4]
18.71 km(calculated)[3]
7.05±0.01 h[5]
0.08(assumed)[3]
0.102±0.009[4]
C(assumed)[3]
12.0[1][3] · 11.80[4]

3174 Alcock (prov. designation:1984 UV) is a carbonaceousThemistian asteroid from the outer region of theasteroid belt. It was discovered by American astronomerEdward Bowell at Lowell's U.S.Anderson Mesa Station in Flagstaff, Arizona, on 26 October 1984.[6] The likelyC-type asteroid has arotation period of 7.1 hours and measures approximately 19 kilometers (12 miles) in diameter. It was named after British amateur astronomerGeorge Alcock (1912–2000).

Orbit and classification

[edit]

The darkC-type asteroid is a member of theThemis family, a dynamical family of outer-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,038 days). Its orbit has aneccentricity of 0.17 and aninclination of 2° with respect to theecliptic.[1] The first used observation was taken atCrimea–Nauchnij in 1973, when the body was identified as1973 YO1, extending itsobservation arc by 11 years prior to the official discovery observation. However, the first images were already taken at the U.S.Goethe Link Observatory in 1962, while it was identified as1962 YD.[6]

Naming

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Thisminor planet was named by the discoverer for prolific British amateur astronomerGeorge Alcock (1912–2000), who visually discovered 5comets and 4novae.[2] Thenaming was published by theMinor Planet Center on 5 November 1987 (M.P.C. 12458).[7]

Physical characteristics

[edit]

A rotationallightcurve of this asteroid was obtained from photometric observations made by French astronomer René Roy in February 2008. The lightcurve gave arotation period of7.05±0.01 hours with a brightness variation of 0.65 inmagnitude (U=3-).[5]

According to the spaced-based survey carried out by the JapaneseAkari satellite, the asteroid measures 18.66 kilometers in diameter and its surface has analbedo of 0.102,[4] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.08 and calculates a diameter of 18.71 kilometers.[3]

References

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  1. ^abcd"JPL Small-Body Database Browser: 3174 Alcock (1984 UV)" (2016-10-06 last obs.).Jet Propulsion Laboratory. Retrieved16 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3174) Alcock".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 263.doi:10.1007/978-3-540-29925-7_3175.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3174) Alcock". Asteroid Lightcurve Database (LCDB). Retrieved7 May 2016.
  4. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  5. ^abBehrend, Raoul."Asteroids and comets rotation curves – (3174) Alcock".Geneva Observatory. Retrieved7 May 2016.
  6. ^ab"3174 Alcock (1984 UV)".Minor Planet Center. Retrieved7 May 2016.
  7. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 May 2016.

External links

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