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6460 Bassano

From Wikipedia, the free encyclopedia
Main-belt asteroid

6460 Bassano
Discovery[1]
Discovered byU. Quadri
L. Strabla
Discovery siteBassano Bresciano Obs.
Discovery date26 October 1992
Designations
(6460) Bassano
Named after
Bassano Bresciano
(Italian village)[2]
1992 UK6 · 1985 TR2
1989 YM6
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc31.43 yr (11,481 days)
Aphelion2.4975AU
Perihelion2.0183 AU
2.2579 AU
Eccentricity0.1061
3.39yr (1,239 days)
43.163°
0° 17m 25.8s / day
Inclination3.2269°
299.03°
181.72°
Physical characteristics
Dimensions4.252±0.108 km[4][5]
4.94 km(calculated)[3]
2.9131±0.0034h[6]
2.9145±0.0034 h[3]
0.24(assumed)[3]
0.389±0.048[4][5]
S[3]
13.5[4] · 13.576±0.002(R)[6] · 13.7[1][3] · 14.291±0.003(S)[6]

6460 Bassano, provisional designation1992 UK6, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 4.5 kilometers in diameter. The asteroid was discovered on 26 October 1992, by Italian amateur astronomersUlisse Quadri andLuca Strabla at theBassano Bresciano Observatory in northern Italy.[7] It was named for the Italian village ofBassano Bresciano.[2]

Orbit and classification

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TheS-type asteroid is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt.Bassano orbits the Sun in theinner main-belt at a distance of 2.0–2.5 AU once every 3 years and 5 months (1,239 days). Its orbit has aneccentricity of 0.11 and aninclination of 3° with respect to theecliptic.[1]

In October 1985, it was first identified as1985 TR2 at the FrenchCaussols Observatory, extending the body'sobservation arc by 7 years prior to its official discovery observation at Bassano Bresciano.[7]

Physical characteristics

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Rotation period

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Two rotationallightcurves ofBassano were obtained from photometric observations at thePalomar Transient Factory in August 2012. Lightcurve analysis gave arotation period of2.9145 and2.9131 hours with a brightness variation of 0.38 and 0.29magnitude, respectively (U=2/2).[6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Bassano measures 4.3 kilometers in diameter and its surface has a highalbedo of 0.39.[4][5] TheCollaborative Asteroid Lightcurve Link assumes a lower albedo of 0.24 – derived from8 Flora, the principal body and namesake of its orbital family – and hence calculates a larger diameter of 4.9 kilometers.[3]

Naming

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Thisminor planet was named for the location of the discovering observatory,Bassano Bresciano, an ancient village in northern Italy.[2]

The historic village was under Longobard and Frank control during the early Middle Ages, and then ruled by theHouse of Sforza and the Venice republic. In the 16th century the former marshland was regained by the two Italian agronomistsCamillo Tarello andAgostino Gallo. Monuments in the village include Luzzago's palace and Brunelli's villa. Its church has aVia Crucis credited to the school of Venetian painterGiovanni Battista Tiepolo, one of the great Old Masters of that period.[2] The official naming citation was published by theMinor Planet Center on 9 September 1995 (M.P.C. 25655).[8]

References

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  1. ^abcd"JPL Small-Body Database Browser: 6460 Bassano (1992 UK6)" (2017-03-21 last obs.).Jet Propulsion Laboratory. Retrieved21 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(6460) Bassano".Dictionary of Minor Planet Names – (6460) Bassano.Springer Berlin Heidelberg. p. 534.doi:10.1007/978-3-540-29925-7_5883.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (6460) Bassano". Asteroid Lightcurve Database (LCDB). Retrieved17 May 2016.
  4. ^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. Retrieved17 May 2016.
  5. ^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. Retrieved5 December 2016.
  6. ^abcdWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved17 May 2016.
  7. ^ab"6460 Bassano (1992 UK6)".Minor Planet Center. Retrieved30 March 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 May 2016.

External links

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