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2175 Andrea Doria

From Wikipedia, the free encyclopedia
Stony Florian asteroid

2175 Andrea Doria
Discovery[1]
Discovered byP. Wild
Discovery siteZimmerwald Obs.
Discovery date12 October 1977
Designations
(2175) Andrea Doria
Named after
Andrea Doria
(16th-century admiral)[2]
1977 TY · 1964 VY1
1967 RS · 1967 TE
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.18 yr (24,171 days)
Aphelion2.6751AU
Perihelion1.7560 AU
2.2155 AU
Eccentricity0.2074
3.30yr (1,205 days)
44.452°
0° 17m 56.04s / day
Inclination3.7056°
222.09°
143.68°
Physical characteristics
Dimensions3.86±0.14 km[4]
3.922±0.042[5]
4.013±0.021 km[6]
4.50 km(calculated)[3]
4.880±0.001h[a]
0.24(assumed)[3]
0.392±0.067[4]
0.3997±0.0568[6]
0.417±0.057[5]
S[3][7]
13.6[6] · 13.70[4] · 13.9[1][3] · 14.28±0.29[7]

2175 Andrea Doria, provisional designation1977 TY, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter.

It was discovered on 12 October 1977, by Swiss astronomerPaul Wild atZimmerwald Observatory near Bern, Switzerland, and named after 16th-century Genoese admiralAndrea Doria.[2][8]

Orbit and classification

[edit]

Andrea Doria is a member of theFlora family, one of the largest families ofstony asteroids in the main belt. It orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,205 days). Its orbit has aneccentricity of 0.21 and aninclination of 4° with respect to theecliptic.[1] A firstprecovery was taken atPalomar Observatory in 1950, extending the body'sobservation arc by 27 years prior to its official discovery observation at Zimmerwald.[8]

Physical characteristics

[edit]

In October 2010, a rotationallightcurve ofAndrea Doria was obtained from photometric observations by American amateur astronomer Ralph Megna. Lightcurve analysis gave a well-definedrotation period of 4.880 hours with a brightness variation of 0.25magnitude (U=3).[a]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Andrea Doria measures between 3.86 and 4.013 kilometers in diameter and its surface has analbedo between 0.392 and 0.417.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, aS-type asteroid and the family's largest member and namesake – and calculates a diameter of 4.50 kilometers with anabsolute magnitude of 13.9.[3]

Naming

[edit]

Thisminor planet was named after Genoese admiralAndrea Doria (1466–1560), popularized in Friedrich Schiller's dramaFiesco.[2] Several ships, including theSS Andrea Doria, famous for its sinking off the coast of New England, had also been named after the admiral. The official naming citation was published by theMinor Planet Center on 22 September 1983 (M.P.C. 8151).[9]

Notes

[edit]
  1. ^abMegna (2011) web:lightcurve plot of (2175) Andrea Doria, Megna, R. (2011) with a rotation period4.880±0.001 hours with a brightness amplitude of0.25 mag. Quality code of 3. Summary figures atCollaborative Asteroid Lightcurve Link

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2175 Andrea Doria (1977 TY)" (2016-08-18 last obs.).Jet Propulsion Laboratory. Retrieved12 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2175) Andrea Doria".Dictionary of Minor Planet Names – (2175) Andrea Doria.Springer Berlin Heidelberg. p. 177.doi:10.1007/978-3-540-29925-7_2176.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2175) Andrea Doria". Asteroid Lightcurve Database (LCDB). Retrieved29 March 2017.
  4. ^abcdMasiero, 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. Retrieved29 March 2017.
  5. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved29 March 2017.
  6. ^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.
  7. ^abVeres, 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. Retrieved29 March 2017.
  8. ^ab"2175 Andrea Doria (1977 TY)".Minor Planet Center. Retrieved29 March 2017.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 March 2017.

External links

[edit]
Minor planets
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Authority control databasesEdit this at Wikidata
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