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6793 Palazzolo

From Wikipedia, the free encyclopedia
Main-belt asteroid discovered by Italian astronomers

6793 Palazzolo
Discovery[1]
Discovered byU. Quadri
L. Strabla
Discovery siteBassano Bresciano Obs.
Discovery date30 December 1991
Designations
(6793) Palazzolo
Named after
Palazzolo sull'Oglio
(Italian city)[2]
1991 YE · 1982 YS2
1990 SZ23
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc33.90 yr (12,382 days)
Aphelion3.1007AU
Perihelion2.2594 AU
2.6800 AU
Eccentricity0.1569
4.39yr (1,603 days)
273.56°
0° 13m 28.56s / day
Inclination4.9244°
106.38°
46.196°
Physical characteristics
Dimensions8.01 km(calculated)[3]
9.882±0.051 km[4][5]
6.190±0.040h[6]
6.2308±0.0072 h[3][7]
6.2323±0.0072 h[7]
0.083±0.004[4][5]
0.10(assumed)[3]
S[3]
13.6[1] · 13.78±0.23[8] · 13.520±0.110[6] · 13.3[4] · 14.143±0.005(S)[7] · 13.709±0.002(R)[7]

6793 Palazzolo, provisional designation1991 YE, is a stonyasteroid from the middle region of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 30 December 1991, by Italian amateur astronomersUlisse Quadri andLuca Strabla at theBassano Bresciano Observatory in northern Italy.[9] The asteroid was named after the Italian city ofPalazzolo sull'Oglio.[2]

Orbit and classification

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Palazzolo orbits the Sun in thecentral main-belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,603 days). Its orbit has aneccentricity of 0.16 and aninclination of 5° with respect to theecliptic.[1]

In 1982, the asteroid was first identified as1982 YS2 atCrimea–Nauchnij. Itsobservation arc begins 1990, with its identification as1990 SZ23 at ESO'sLa Silla Observatory, 1 year prior to its official discovery observation at Bassano Bresciano.[9]

Physical characteristics

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Palazzolo is an assumedS-type asteroid.[3]

Rotation period

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In 2012, a rotationallightcurve ofPalazzolo was obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of6.2308 hours with a brightness amplitude of 0.16 inmagnitude (U=2).[7]

Follow-up observations in 2013 and 2014, gave a similar period of6.190 and6.2323 hours with an amplitude of 0.16 and 0.14, respectively (U=2/2).[7][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,Palazzolo has a diameter of 9.9 kilometers and analbedo of 0.083,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and calculates a diameter of 8.0 kilometers.[3]

Naming

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Thisminor planet is named after the Italian city ofPalazzolo sull'Oglio, located between Brescia and Bergamo, in northern parts of the country. Known for its industries, including the first Italian factories producing cement and buttons, the city is now famous for its of spinning machines and zippers. It was founded on the banks of riverOglio, with archaeological findings dating back to the Roman era.[2] The approved naming citation was published by theMinor Planet Center on 4 April 1996 (M.P.C. 26933).[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 6793 Palazzolo (1991 YE)" (2016-11-15 last obs.).Jet Propulsion Laboratory. Retrieved21 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(6793) Palazzolo".Dictionary of Minor Planet Names – (6793) Palazzolo.Springer Berlin Heidelberg. p. 557.doi:10.1007/978-3-540-29925-7_6105.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (6793) Palazzolo". 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. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved17 May 2016.
  7. ^abcdefWaszczak, 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.
  8. ^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.
  9. ^ab"6793 Palazzolo (1991 YE)".Minor Planet Center. Retrieved29 March 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved17 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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