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5196 Bustelli

From Wikipedia, the free encyclopedia

5196 Bustelli
Shape model of Bustelli from itslightcurve
Discovery [1]
Discovered byC. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date30 September 1973
Designations
(5196) Bustelli
Named after
Franz Anton Bustelli[1]
(Italian-Swiss artist)
3102 T-2 · 1982 SY9
1984 DP1 · 1984 FP1
main-belt[1][2] · (middle)
Eunomia[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc46.60yr (17,019 d)
Aphelion3.0788AU
Perihelion2.3183 AU
2.6985 AU
Eccentricity0.1409
4.43 yr (1,619 d)
268.18°
0° 13m 20.28s / day
Inclination13.226°
6.8289°
113.42°
Physical characteristics
5.944±0.091 km[4]
0.146±0.017[5]
SMASS =S[2][6]
12.8[2]

5196 Bustelli (prov. designation:3102 T-2) is a stonyEunomia asteroid from the central regions of theasteroid belt, approximately 6 kilometers (3.7 miles) kilometers in diameter. It was discovered on 30 September 1973, by Dutch astronomersIngrid andCornelis van Houten at Leiden, andTom Gehrels thePalomar Observatory. TheS-type asteroid was named after Italian-Swiss artistFranz Anton Bustelli.[1][2]

Orbit and classification

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Bustelli is a core member of theEunomia family (502),[3] a prominentfamily of stonyS-type asteroid and the largest one in the intermediate main belt with more than 5,000 members.[7] It orbits the Sun in thecentral asteroid belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,619 days;semi-major axis of 2.7 AU). Its orbit has aneccentricity of 0.14 and aninclination of 13° with respect to theecliptic.[2] The body'sobservation arc begins with aprecovery taken at Palomar Observatory in March 1971.[1]

Palomar–Leiden Trojan survey

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Thesurvey designation "T-2" stands for the secondPalomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar andLeiden Observatory in the 1960s and 1970s. 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 is credited with the discovery ofseveral thousand asteroid discoveries.[8]

Naming

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Thisminor planet was named after Italian-Swiss artistFranz Anton Bustelli (1723–1763), a famous modeller of figures for theNymphenburg Porcelain Manufactory. The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22507).[9]

Physical characteristics

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Bustelli has anabsolute magnitude of 12.8. In theSMASS classification, it is a stonyS-type asteroid.[2][6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, Bustelli measures 5.944 kilometers in diameter and its surface has analbedo of 0.146.[4][5]

Rotation period

[edit]

As of 2018, no rotationallightcurve of Bustelli has been obtained fromphotometric observations. The body'srotation period,poles and shape remain unknown.[2]

References

[edit]
  1. ^abcde"5196 Bustelli (3102 T-2)".Minor Planet Center. Retrieved10 April 2018.
  2. ^abcdefgh"JPL Small-Body Database Browser: 5196 Bustelli (3102 T-2)" (2017-10-27 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 17 September 2020. Retrieved10 April 2018.
  3. ^ab"Asteroid 5196 Bustelli – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  4. ^abMasiero, 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. ^abMasiero, 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.
  6. ^abBus, S.; Binzel, R. P. (October 2004). "5196 Bustelli CCD Spectrum".NASA Planetary Data System.Bibcode:2004PDSS....1.....B.
  7. ^Nesvorný, 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.
  8. ^"Minor Planet Discoverers (by number)".Minor Planet Center. 31 March 2018. Retrieved10 April 2018.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 April 2018.

External links

[edit]
Minor planets
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