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1800 Aguilar

From Wikipedia, the free encyclopedia
Main-belt asteroid

1800 Aguilar
Discovery[1]
Discovered byM. Itzigsohn
Discovery siteLa Plata Obs.
Discovery date12 September 1950
Designations
(1800) Aguilar
Named after
Félix Aguilar(astronomer)[2]
1950 RJ · 1952 BJ
1972 XP2 · 1976 YU7
1977 AE1
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc66.54 yr (24,305 days)
Aphelion2.6778AU
Perihelion2.0362 AU
2.3570 AU
Eccentricity0.1361
3.62yr (1,322 days)
189.20°
0° 16m 20.64s / day
Inclination5.7893°
124.24°
214.46°
Physical characteristics
Dimensions7.384±0.156 km[4][5]
8.18 km(calculated)[3]
2.478±0.002h[a]
0.20(assumed)[3]
0.295±0.047[4][5]
S[3]
12.6[4] · 12.8[1][3] · 13.07±0.05[6]

1800 Aguilar, provisional designation1950 RJ, is a stony Vestianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter.

It was discovered on 12 September 1950, by Argentine astronomerMiguel Itzigsohn atLa Plata Astronomical Observatory in Argentina.[7] The asteroid was named after Argentine astronomerFélix Aguilar.[2]

Orbit and classification

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The stonyS-type asteroid is a member of theVesta family. It orbits the Sun in theinner main-belt at a distance of 2.0–2.7 AU once every 3 years and 7 months (1,322 days). Its orbit has aneccentricity of 0.14 and aninclination of 6° with respect to theecliptic.[1] As noprecoveries were taken, and no prior identifications were made,Aguilar'sobservation arc begins with its official discovery observation.[7]

Physical characteristics

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Rotation period

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In September 2008, a rotationallightcurve ofAguilar was obtained from photometric observations taken by Australian amateur astronomerDavid Higgins. It gave a well-definedrotation period of 2.478 hours with a brightness variation of 0.11 inmagnitude (U=3).[a]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Aguilar measures 7.38 kilometers in diameter, and its surface has analbedo of 0.295,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 8.18 kilometers with anabsolute magnitude of 12.8.[3]

Naming

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Thisminor planet was named for Argentine astronomer Félix Aguilar (1884–1943), former director of the discovering observatory and founder of the University School of Astronomy and Geophysics. He contributed significantly to the development of Argentine astronomy in the first half of the 20th century(also seeFélix Aguilar Observatory).[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3934).[8]

Notes

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  1. ^abHiggins (2011) web: rotation period2.478±0.002 hours with a brightness amplitude of0.11 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1800) Aguilar andDavid Higgins Homepage

References

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  1. ^abcd"JPL Small-Body Database Browser: 1800 Aguilar (1950 RJ)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 20 December 2016. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1800) Aguilar".Dictionary of Minor Planet Names – (1800) Aguilar.Springer Berlin Heidelberg. p. 144.doi:10.1007/978-3-540-29925-7_1801.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1800) Aguilar". Asteroid Lightcurve Database (LCDB). Retrieved19 December 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.
  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. Retrieved19 December 2016.
  6. ^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. Retrieved19 December 2016.
  7. ^ab"1800 Aguilar (1950 RJ)".Minor Planet Center. Retrieved19 December 2016.
  8. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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