Home  

Random  

Nearby  



Log in  



Settings  



Donate  



About Wikipedia  

Disclaimers  



Wikipedia





3787 Aivazovskij





Article  

Talk  



Language  

Watch  

Edit  





3787 Aivazovskij (prov. designation: 1977 RG7) is a stony asteroid of the Itha family, located in the outer region of the asteroid belt. It was discovered by Soviet–Russian astronomer Nikolai Chernykh at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula, on 11 September 1977.[10] The stony S-type asteroid has a rotation period of 3.0 hours and measures approximately 13 kilometers (8.1 miles) in diameter. It was named after painter Ivan Aivazovsky (1817–1900).[2]

3787 Aivazovskij
Shape model of Aivazovskij from its lightcurve
Discovery [1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date11 September 1977
Designations

MPC designation

(3787) Aivazovskij

Named after

Ivan Aivazovsky (painter)[2]

Alternative designations

1977 RG7 · 1931 DM
1967 RO · 1987 UA3

Minor planet category

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)
Aphelion3.2220 AU
Perihelion2.4819 AU

Semi-major axis

2.8519 AU
Eccentricity0.1298

Orbital period (sidereal)

4.82 yr (1,759 days)

Mean anomaly

6.3381°

Mean motion

0° 12m 16.56s / day
Inclination12.055°

Longitude of ascending node

185.88°

Argument of perihelion

305.66°
Physical characteristics

Mean diameter

12.089±0.121 km[5][6]
14.89 km (calculated)[3]

Synodic rotation period

2.97[7]

Geometric albedo

0.20 (assumed)[3]
0.333±0.070[5][6]

Spectral type

S[3][8]

Absolute magnitude (H)

11.4[5] · 11.488±0.002 (R)[9] · 11.5[1][3] · 11.55±0.51[8]

Orbit and classification

edit

When applying the hierarchical clustering method to its proper orbital elements, Aivazovskij is a member of the Itha family,[4] a very small family of asteroids, named after its parent body 918 Itha.[11]: 23  It orbits the Sun in the outer 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 an eccentricity of 0.13 and an inclination of 12° with respect to the ecliptic.[1] The first precovery was taken at Lowell Observatory in 1931, extending the asteroid's observation arc by 46 years prior to its discovery.[10]

Naming

edit

This minor 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 planet 1048 Feodosia is named after this place.[2][12] The official naming citation was published by the Minor Planet Center on 1 September 1993 (M.P.C. 22499).[13]

Physical characteristics

edit

The asteroid has been characterized as a stony S-type asteroidbyPanSTARRS' photometric survey.[3][8] This concurs with the overall spectral type for the Itha family.[11]: 23 

Rotation period

edit

A rotational lightcurveofAivazovskij was obtained from photometric observations made in March 2008, at the Universidad de Monterry Observatory, Mexico. It showed a well-defined rotation periodof2.97 hours with a brightness amplitude of 0.18 in magnitude (U=3).[7] Two additional observations gave a period of 2.9532±0.0005 and 2.980807±0.000005 hours, respectively (U=2/n.a.).[9][14]

Diameter and albedo

edit

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

References

edit
  1. ^ a b c d "JPL Small-Body Database Browser: 3787 Aivazovskij (1977 RG7)" (2017-03-29 last obs.). Jet Propulsion Laboratory. Retrieved 19 June 2017.
  • ^ a b c Schmadel, 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.
  • ^ a b c d e f g "LCDB Data for (3787) Aivazovskij". Asteroid Lightcurve Database (LCDB). Retrieved 3 May 2016.
  • ^ a b "Asteroid 3787 Aivazovskij – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 27 October 2019.
  • ^ a b c d Mainzer, 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. Retrieved 3 May 2016.
  • ^ a b c Masiero, 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. Retrieved 5 December 2016.
  • ^ a b Sada, 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 from the original (PDF) on 17 March 2020. Retrieved 19 March 2020.
  • ^ a b c 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. Retrieved 3 May 2016.
  • ^ a b Waszczak, 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. Retrieved 3 May 2016.
  • ^ a b "3787 Aivazovskij (1977 RG7)". Minor Planet Center. Retrieved 3 May 2016.
  • ^ a b Nesvorný, 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.
  • ^ 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.
  • ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 May 2016.
  • ^ 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.
  • edit

    Retrieved from "https://en.wikipedia.org/w/index.php?title=3787_Aivazovskij&oldid=1205010542"
     



    Last edited on 8 February 2024, at 16:35  





    Languages

     


    العربية
    Deutsch
    Español
    Esperanto
    Euskara
    فارسی
    Français
    Հայերեն
    Italiano
    Latina
    Magyar
    مصرى
    Нохчийн
    Polski
    Português
    Română
    Русский
    Slovenčina
    Српски / srpski
    Svenska
    Татарча / tatarça
    Українська
    Tiếng Vit
    Yorùbá

     

    Wikipedia


    This page was last edited on 8 February 2024, at 16:35 (UTC).

    Content is available under CC BY-SA 4.0 unless otherwise noted.



    Privacy policy

    About Wikipedia

    Disclaimers

    Contact Wikipedia

    Code of Conduct

    Developers

    Statistics

    Cookie statement

    Terms of Use

    Desktop