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3787 Aivazovskij

From Wikipedia, the free encyclopedia
Main-belt asteroid

3787 Aivazovskij
Shape model ofAivazovskij from itslightcurve
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date11 September 1977
Designations
(3787) Aivazovskij
Named after
Ivan Aivazovsky(painter)[2]
1977 RG7 · 1931 DM
1967 RO · 1987 UA3
main-belt · (outer)[3]
Itha[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc86.11 yr (31,452 days)
Aphelion3.2220AU
Perihelion2.4819 AU
2.8519 AU
Eccentricity0.1298
4.82yr (1,759 days)
6.3381°
0° 12m 16.56s / day
Inclination12.055°
185.88°
305.66°
Physical characteristics
12.089±0.121 km[5][6]
14.89 km(calculated)[3]
2.97[7]
0.20(assumed)[3]
0.333±0.070[5][6]
S[3][8]
11.4[5] · 11.488±0.002(R)[9] · 11.5[1][3] · 11.55±0.51[8]

3787 Aivazovskij (prov. designation:1977 RG7) is a stonyasteroid of theItha family, located in the outer region of theasteroid belt. It was discovered by Soviet–Russian astronomerNikolai Chernykh at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula, on 11 September 1977.[10] The stonyS-type asteroid has arotation period of 3.0 hours and measures approximately 13 kilometers (8.1 miles) in diameter. It was named after painterIvan Aivazovsky (1817–1900).[2]

Orbit and classification

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When applying thehierarchical clustering method to itsproper orbital elements,Aivazovskij is a member of theItha family,[4] a very smallfamily of asteroids, named after its parent body918 Itha.[11]: 23  It orbits the Sun in theouter main belt at a distance of 2.5–3.2 AU once every 4 years and 10 months (1,759 days;semi-major axis of 2.85 AU). Its orbit has aneccentricity of 0.13 and aninclination of 12° with respect to theecliptic.[1] The firstprecovery was taken atLowell Observatory in 1931, extending the asteroid'sobservation arc by 46 years prior to its discovery.[10]

Naming

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Thisminor planet was named after the Armenian-Russian painter of seascapes,Ivan Aivazovsky (1817–1900), who lived and worked in the Crimean city of Feodosia. The minor planet1048 Feodosia is named after this place.[2][12] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22499).[13]

Physical characteristics

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The asteroid has been characterized as a stonyS-type asteroid byPanSTARRS' photometric survey.[3][8] This concurs with the overallspectral type for the Itha family.[11]: 23 

Rotation period

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A rotationallightcurve ofAivazovskij was obtained from photometric observations made in March 2008, at the Universidad de Monterry Observatory, Mexico. It showed a well-definedrotation period of2.97 hours with a brightness amplitude of 0.18 inmagnitude (U=3).[7] Two additional observations gave a period of2.9532±0.0005 and2.980807±0.000005 hours, respectively (U=2/n.a.).[9][14]

Diameter and albedo

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Based on the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer, the asteroid measure 12.1 kilometers in diameter and its surface has a highalbedo of 0.33,[5][6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20, and calculates a diameter 14.9 kilometers with anabsolute magnitude of 11.5.[3]

References

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  1. ^abcd"JPL Small-Body Database Browser: 3787 Aivazovskij (1977 RG7)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved19 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3787) Aivazovskij".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 320.doi:10.1007/978-3-540-29925-7_3782.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (3787) Aivazovskij". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2016.
  4. ^ab"Asteroid 3787 Aivazovskij – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^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. Retrieved3 May 2016.
  6. ^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.
  7. ^abSada, Pedro V. (October 2008)."CCD Photometry of Three Short-period Asteroids from the Universidad de Monterry Observatory"(PDF).Minor Planet Bulletin.35 (4):161–162.Bibcode:2008MPBu...35..161S.ISSN 1052-8091. Archived fromthe original(PDF) on 17 March 2020. Retrieved19 March 2020.
  8. ^abcVeres, 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. Retrieved3 May 2016.
  9. ^abWaszczak, 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. Retrieved3 May 2016.
  10. ^ab"3787 Aivazovskij (1977 RG7)".Minor Planet Center. Retrieved3 May 2016.
  11. ^abNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  12. ^Schmadel, Lutz D. (2003). "(1048) Feodosia".Dictionary of Minor Planet Names. Springer Berlin Heidelberg. pp. 89–90.doi:10.1007/978-3-540-29925-7_1049.ISBN 978-3-540-29925-7.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2016.
  14. ^Hanuš, J.; Ďurech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016). "New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: A108.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441.ISSN 0004-6361.

External links

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