1783 Albitskij

1783 Albitskij, provisional designation 1935 FJ, is a carbonaceous Adeonian asteroid from the middle region of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 24 March 1935, by Georgian–Russian astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula.[13] The asteroid was named after Soviet astronomer Vladimir Albitzky.[2]

1783 Albitskij
Discovery [1]
Discovered byG. Neujmin
Discovery siteSimeiz Obs.
Discovery date24 March 1935
Designations
(1783) Albitskij
Named after
Vladimir Albitzky [2]
(Soviet/Russian astronomer)
1935 FJ · 1933 TB
1952 BP1 · 1952 DP
1970 GA1
main-belt · (middle)
Eunomia [3] · Adeona [4]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.12 yr (29,993 days)
Aphelion3.0132 AU
Perihelion2.3124 AU
2.6628 AU
Eccentricity0.1316
4.35 yr (1,587 days)
23.419°
0° 13m 36.48s / day
Inclination11.506°
189.51°
315.93°
Physical characteristics
Dimensions20.47±6.78 km[5]
21.34 km (derived)[3]
21.36±2.4 km (IRAS:3)[6]
24.268±0.093 km[7]
24.64±7.83 km[8]
24.68±0.76 km[9]
25.642±0.178 km[10]
12 h[11]
0.033±0.003[10]
0.051±0.048[8]
0.0546±0.0091[7]
0.057±0.004[9]
0.06±0.07[5]
0.0706 (derived)[3]
0.0738±0.019 (IRAS:3)[6]
SMASS = Ch [1] · C [3][12]
11.80[6][9] · 11.85[3][7][11] · 11.90[8] · 12.0[1] · 12.01[5] · 12.14±0.00[12]

    Orbit and classification

    Albitskij is a member of the Adeona family (505),[4] a large family of carbonaceous asteroids, when applying the Hierarchical Clustering Method to its proper orbital elements. It has also been dynamically classified as a member of the Eunomia family (as many other members of the Adeona family), which can be ruled out, due to the fact, that this family consist of stony rather than carbonaceous asteroid.[3][14]:23

    The asteroid orbits the Sun in the central main belt at a distance of 2.3–3.0 AU once every 4 years and 4 months (1,587 days). Its orbit has an eccentricity of 0.13 and an inclination of 12° with respect to the ecliptic.[1]

    In 1933, it was first identified as 1933 TB at the U.S. Oak Ridge Observatory in Massachusetts, two years prior to its discovery. The body's observation arc begins one month after its official discovery with the first used observation made at Uccle Observatory in Belgium.[13]

    Physical characteristics

    In the SMASS taxonomic scheme, Albitskij is a Ch-subtype, a hydrated C-type asteroid.[1] It has also been characterized as a common carbonaceous C-type by Pan-STARRS photometric survey.[12] This agrees with the overall spectral type of the Adeona family (505).[14]:23

    Rotation period

    Published by Cláudia Angeli and Maria Barucci, a rotational lightcurve was obtained for this asteroid from photometric observations made at the French Haute-Provence and Pic du Midi observatories by astronomers at Meudon in the early 1990s. It gave a rotation period of 12 hours with a brightness amplitude of 0.4 magnitude (U=2).[11]

    Diameter and albedo

    According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Albitskij measures between 20.47 and 25.6 kilometers in diameter and its surface has an albedo between 0.03 and 0.07.[5][6][7][8][9][10]

    The Collaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS and derives an albedo of 0.07 and a diameter of 21.3 kilometers, based on an absolute magnitude of 11.85.[3]

    Naming

    This minor planet is named after Soviet astronomer, discoverer of minor planets and head of Simeiz Observatory, Vladimir Albitzky (1891–1952). His research included variable stars and the measurement of radial velocities.[2] The official naming citation was published by the Minor Planet Center on 1 June 1980 (M.P.C. 5357).[15]

    gollark: So that you can flatten a binary tree by unhooking it and enabling gravity.
    gollark: Idea: 2D memory with objects with rigid body mechanics.
    gollark: Use basename or whatever on it.
    gollark: I read some work using GPT-3 to automatically generalise to all Greek letters.
    gollark: Fun animations and characters?

    References
    1. "JPL Small-Body Database Browser: 1783 Albitskij (1935 FJ)" (2017-05-05 last obs.). Jet Propulsion Laboratory. Retrieved 8 June 2017.
    2. Schmadel, Lutz D. (2007). "(1783) Albitskij". Dictionary of Minor Planet Names – (1783) Albitskij. Springer Berlin Heidelberg. p. 143. doi:10.1007/978-3-540-29925-7_1784. ISBN 978-3-540-00238-3.
    3. "LCDB Data for (1783) Albitskij". Asteroid Lightcurve Database (LCDB). Retrieved 3 November 2016.
    4. "Asteroid 1783 Albitskij – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
    5. Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv:1606.08923. Bibcode:2016AJ....152...63N. doi:10.3847/0004-6256/152/3/63. Retrieved 27 October 2017.
    6. Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T. Retrieved 22 October 2019.
    7. 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.
    8. Masiero, 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. Retrieved 3 November 2016.
    9. Usui, 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. Retrieved 17 October 2019. (online, AcuA catalog p. 153)
    10. 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 8 September 2016.
    11. Angeli, C. A.; Barucci, M. A. (March 1996). "CCD observations: rotational properties of 13 small asteroids". Planetary and Space Science. 44 (3): 181–186. Bibcode:1996P&SS...44..181A. doi:10.1016/0032-0633(95)00124-7. Retrieved 3 November 2016.
    12. 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 November 2016.
    13. "1783 Albitskij (1935 FJ)". Minor Planet Center. Retrieved 3 November 2016.
    14. 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 9780816532131.
    15. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 November 2016.

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