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3176 Paolicchi

From Wikipedia, the free encyclopedia
Main-belt asteroid

3176 Paolicchi
Discovery[1]
Discovered byZ. Knežević
Discovery sitePiszkéstető Stn.
Discovery date13 November 1980
Designations
(3176) Paolicchi
Named after
Paolo Paolicchi(astrophysicist)[2]
1980 VR1 · 1931 UP
1941 WC · 1941 WG1
1951 XF1 · 1956 XD
1965 UD · 1968 HM1
1975 XU · 1978 JG
1978 LQ · A902 WG
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc114.53 yr (41,832 days)
Aphelion2.9658AU
Perihelion2.7854 AU
2.8756 AU
Eccentricity0.0314
4.88yr (1,781 days)
170.54°
0° 12m 7.56s / day
Inclination18.114°
53.209°
25.596°
Physical characteristics
Dimensions31.84±0.68 km[4]
33.83 km(derived)[3]
33.94±2.8 km(IRAS 15)[1]
41.33±0.36 km[5]
20.4±0.5h[6]
0.038±0.007[5]
0.0511(derived)[3]
0.0669±0.012(IRAS 15)[1]
0.081±0.004[4]
C[3]
10.90[4] · 11.10[5] · 11.2[1][3] · 11.47±0.24[7]

3176 Paolicchi, provisional designation1980 VR1, is a carbonaceousasteroid from the outer region of theasteroid belt, about 34 kilometers in diameter. It was discovered on 13 November 1980, by Serbian astronomerZoran Knežević at the Konkoly Observatory'sPiszkéstető Station northeast of Budapest, Hungary.[8]

Orbit and classification

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The darkC-type asteroid orbits the Sun in theouter main-belt at a distance of 2.8–3.0 AU once every 4 years and 11 months (1,781 days). Its orbit has aneccentricity of 0.03 and aninclination of 18° with respect to theecliptic.[1] First identified asA902 WG atHeidelberg Observatory in 1902, the first used observation was made at the U.S.Lowell Observatory in 1931, whenPaolicchi was identified as1931 UP, extending itsobservation arc by 49 years prior to its official discovery observation.[8]

Physical characteristics

[edit]

It has arotation period of 20.400 hours[6] and analbedo in the range of 0.04–0.08, according to the surveys carried out by the Infrared Astronomical Satellite,IRAS, the JapaneseAkari satellite, and theWide-field Infrared Survey Explorer with its subsequentNEOWISE mission.[4][5] The Collaborative Asteroid Lightcurve Link derives an albedo of 0.05.[3] Estimated diameters forPaolicchi range between 31.8 and 41.3 kilometers.[1][3][4][5]

Naming

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Thisminor planet was named in honor of Italian astrophysicistPaolo Paolicchi (b. 1950) at theUniversity of Pisa, whose research activity included the study on the dynamical and collisional history ofSmall Solar System bodies and the origin of planetary and stellar systems. Paolicchi's work on minor planets has focused on the modeling of catastrophic breakup events and on the evolution of their rotational properties.[2] The official naming citation was published by theMinor Planet Center on 7 September 1987 (M.P.C. 12209).[9]

References

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  1. ^abcdefg"JPL Small-Body Database Browser: 3176 Paolicchi (1980 VR1)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Retrieved16 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3176) Paolicchi".Dictionary of Minor Planet Names – (3176) Paolicchi.Springer Berlin Heidelberg. p. 263.doi:10.1007/978-3-540-29925-7_3177.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (3176) Paolicchi". Asteroid Lightcurve Database (LCDB). Retrieved6 December 2016.
  4. ^abcdeUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  5. ^abcdeMasiero, 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. Retrieved6 December 2016.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (3176) Paolicchi".Geneva Observatory. Retrieved6 December 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. Retrieved6 December 2016.
  8. ^ab"3176 Paolicchi (1980 VR1)".Minor Planet Center. Retrieved6 December 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 December 2016.

External links

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