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3936 Elst

From Wikipedia, the free encyclopedia
Stony Vestian asteroid from the inner regions of the asteroid belt
3936 Elst
Discovery[1]
Discovered byC. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date16 October 1977
Designations
(3936) Elst
Named after
Eric W. Elst(Belgian astronomer)[2]
2321 T-3 · 1972 GY
1973 TC · 1976 JG1
1980 MB · 1981 WA2
1984 MT · 1985 WS
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc45.05 yr (16,455 days)
Aphelion2.7424AU
Perihelion2.1139 AU
2.4281 AU
Eccentricity0.1294
3.78yr (1,382 days)
282.61°
0° 15m 37.8s / day
Inclination5.6458°
240.74°
38.474°
Physical characteristics
Dimensions4.593±0.073 km[4]
4.939±0.048 km[5]
7.46 km(calculated)[3]
6.6322±0.0002h[a]
0.20(assumed)[3]
0.4607±0.0712[5]
0.509±0.096[4]
S[3]
13.0[1][3][5] · 13.36±0.24[6]

3936 Elst, provisional designation2321 T-3, is a stony Vestianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. The asteroid was discovered on 16 October 1977, by Dutch astronomer coupleIngrid andCornelis van Houten at Leiden, on photographic plates taken by Dutch–American astronomerTom Gehrels atPalomar Observatory in California, United States.[7] It was named after Belgian astronomerEric W. Elst.[2]

Orbit and classification

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Elst is a stonyS-type asteroid and member of theVesta family. It orbits the Sun in theinner main-belt at a distance of 2.1–2.7 AU once every 3 years and 9 months (1,382 days). Its orbit has aneccentricity of 0.13 and aninclination of 6° with respect to theecliptic.[1] It was first identified as1972 GY and1973 TC atCrimea–Nauchnij, extending the body'sobservation arc by 4 years prior to its official discovery observation at Palomar.[7]

Physical characteristics

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Lightcurve

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In August 2007, a rotationallightcurve ofElst was obtained from photometric observations by Czech astronomerPetr Pravec atOndřejov Observatory. Lightcurve analysis gave a well-definedrotation period of 6.6322 hours with a brightness amplitude of 0.13magnitude (U=3).[a]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Elst measures 4.593 and 4.939 kilometers in diameter and its surface has analbedo of 0.4607 and 0.509, respectively,[5][4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a larger diameter of 7.46 kilometers based on anabsolute magnitude of 13.0.[3]

Survey designation

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Thesurvey designation "T-3" stands for the thirdPalomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar andLeiden Observatory conducted in 1977. Gehrels used Palomar'sSamuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped thephotographic plates to Ingrid and Cornelis van Houten at Leiden Observatory whereastrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[8]

Naming

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Thisminor planet was named in honor of Belgian astronomerEric Walter Elst, one of the world's topdiscoverer of minor planets atUccle Observatory in Belgium.[2] The official naming citation was published by theMinor Planet Center on 28 April 1991 (M.P.C. 18138).[9]

Notes

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  1. ^abPravec (2007) web: rotation period6.6322±0.0002 hours with a brightness amplitude of0.13 magnitude and a Quality Code of 3 (see lightcurve plot). Summary figures for (3936) Elst atCollaborative Asteroid Lightcurve Link (CALL) andOndřejov Asteroid Photometry Project website

References

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  1. ^abcd"JPL Small-Body Database Browser: 3936 Elst (2321 T-3)" (2017-05-01 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3936) Elst".Dictionary of Minor Planet Names – (3936) Elst.Springer Berlin Heidelberg. p. 335.doi:10.1007/978-3-540-29925-7_3925.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3936) Elst". Asteroid Lightcurve Database (LCDB). Retrieved9 March 2017.
  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. Retrieved9 March 2017.
  5. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90.
  6. ^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. Retrieved9 March 2017.
  7. ^ab"3936 Elst (2321 T-3)".Minor Planet Center. Retrieved9 March 2017.
  8. ^"Minor Planet Discoverers".Minor Planet Center. 24 April 2016. Retrieved9 March 2017.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 March 2017.

External links

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