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4324 Bickel

From Wikipedia, the free encyclopedia
Main-belt asteroid

4324 Bickel
Discovery[1]
Discovered byL. G. Taff
Discovery siteLincoln Laboratory ETS
Discovery date24 December 1981
Designations
(4324) Bickel
Named after
Wolf Bickel
(amateur astronomer)[2]
1981 YA1 · 1932 UD
1932 WE · 1948 SD
1948 TK2 · 1964 PE
1966 DC · 1972 NF
1973 YR3 · 1985 XX
A924 YC
main-belt · (middle)
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc92.44 yr (33,765 days)
Aphelion3.0537AU
Perihelion2.0373 AU
2.5455 AU
Eccentricity0.1996
4.06yr (1,483 days)
320.50°
0° 14m 33.72s / day
Inclination7.7760°
292.79°
108.71°
Physical characteristics
Dimensions11.65±0.56 km[3]
12.39 km(calculated)[4]
16h[5]
26.5 h[6]
26.592±0.003 h[5]
0.20(assumed)[4]
0.248±0.020[3]
S[4]
11.80[3] · 11.9[1][4] · 12.37±0.29[7]

4324 Bickel, provisional designation1981 YA1, is a stonyasteroid from the middle region of theasteroid belt, approximately 12 kilometers in diameter. It was discovered on 24 December 1981, by American astronomer Laurence Taff atLincoln Laboratory's Experimental Test Site in Socorro, New Mexico, United States. The asteroid was named after amateur astronomerWolf Bickel.[2]

Orbit and classification

[edit]

Bickel orbits the Sun in thecentral main-belt at a distance of 2.0–3.1 AU once every 4 years and 1 month (1,483 days). Its orbit has aneccentricity of 0.20 and aninclination of 8° with respect to theecliptic.[1] It was first identified asA924 YC atHeidelberg Observatory in 1924, extending the body'sobservation arc by 57 years prior to its official discovery observation at Socorro.[2]

Physical characteristics

[edit]

Bickel has been characterized as a commonS-type asteroid.[4]

Rotation period

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In September 2001, the first ever conducted photometric observation ofBickel at theRozhen Observatory, Bulgaria, rendered a rotationallightcurve with a longer-than-averageperiod of26.5 hours and a brightness variation of 0.63magnitude (U=2).[6] A more refined lightcurve was obtained in October 2005, by astronomers Raymond Poncy,Laurent Bernasconi and Rui Goncalves, which gave a well-defined period of26.592±0.003 hours with an amplitude of 0.72 magnitude (U=3).[5]

Diameter and albedo

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According to observations by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Bickel measures 11.7 kilometers in diameter and its surface has analbedo of 0.248,[3] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a slightly larger diameter of 12.4 kilometers with anabsolute magnitude of 11.9.[4]

Naming

[edit]

Thisminor planet was named in honor of German amateur astronomerWolf Bickel (born 1942) who began observing minor planets at his privateBergisch Gladbach Observatory in 1995.[2]

At the time this minor planet was named, he had discovered more than 540 numbered minor planets.[2] The official naming citation was published by theMinor Planet Center on 22 July 2013 (M.P.C. 84378).[8] Bickel has become Germany's most prolific discoverer of asteroids, ahead of (professional) astronomerFreimut Börngen, the first time in 150 years, that an amateur astronomer is ranking first among the German top discoverers.[9] His total number of discoveries has since increased to more than 600.[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4324 Bickel (1981 YA1)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcde"4324 Bickel (1981 YA1)".Minor Planet Center. Retrieved5 April 2016.
  3. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved17 May 2016.
  4. ^abcdef"LCDB Data for (4324) Bickel". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  5. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (4324) Bickel".Geneva Observatory. Retrieved17 May 2016.
  6. ^abIvanova, V. G.; Apostolovska, G.; Borisov, G. B.; Bilkina, B. I. (November 2002)."Results from photometric studies of asteroids at Rozhen National Observatory, Bulgaria".In: Proceedings of Asteroids:505–508.Bibcode:2002ESASP.500..505I. Retrieved17 May 2016.
  7. ^Veres, 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. Retrieved17 May 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.
  9. ^"Bickel überholt Börngen – die erfolgreichsten deutschen Kleinplanetenentdecker" [Bickel overtakes Börgen – Most prolific German discoverers of minor planets](PDF).VdS-Journal – Vereinigung der Sternfreunde. April 2013. pp. 80–83. Retrieved5 April 2016.
  10. ^"Minor Planet Discoverers (by number)".Minor Planet Center. 23 March 2016. Retrieved5 April 2016.

External links

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