1783 Albitskij

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1783 Albitskij
Discovery [1]
Discovered by G. Neujmin
Discovery site Simeiz Obs.
Discovery date 24 March 1935
Designations
MPC designation 1783 Albitskij
Named after
Vladimir Albitzky
(astronomer)[2]
1935 FJ · 1933 TB
1952 BP1 · 1952 DP
1970 GA1
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc 81.60 yr (29,804 days)
Aphelion 3.0121 AU
Perihelion 2.3124 AU
2.6623 AU
Eccentricity 0.1314
4.34 yr (1,587 days)
338.07°
0° 13m 36.84s / day
Inclination 11.506°
189.51°
315.89°
Physical characteristics
Dimensions 21.34 km (derived)[3]
21.36±2.4 km (IRAS:3)[4]
24.268±0.093 km[5]
24.64±7.83 km[6]
24.68±0.76 km[7]
25.642±0.178 km[8]
12 h[9]
0.033±0.003[8]
0.051±0.048[6]
0.0546±0.0091[5]
0.057±0.004[7]
0.0706 (derived)[3]
0.0738±0.019 (IRAS:3)[4]
SMASS = Ch [1] · C[3][10]
11.80[4][7] · 11.85[3][5][9] · 11.90[6] · 12.0[1] · 12.14±0.00[10]

1783 Albitskij, provisional designation 1935 FJ, is a carbonaceous Eunomian asteroid from the middle region of the asteroid belt, approximately 23 kilometers in diameter. It was discovered on 24 March 1935, by Soviet–Russian astronomer Grigory Neujmin at Simeiz Observatory on the Crimean peninsula.[11]

The C-type asteroid – classified as a Ch-subtype in the SMASS taxonomic scheme – orbits the Sun 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.[11]

The asteroid is a member of the Eunomia family, a large group of typically stony S-type asteroids and a prominent family in the intermediate main-belt. Since the asteroid's spectral type is that of a carbonaceous C-type, rather than of a stony S-type body, it is considered to be an interloper (see Eunomia family § Interlopers).[12]

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, the asteroid measures between 21.4 and 25.6 kilometers in diameter and its surface has an albedo between 0.03 and 0.07.[4][5][6][7][8] 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]

Published by Cláudia Angeli and Maria A. Barucci, a rotational light-curve 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).[9]

The 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] Naming citation was published on 1 June 1980 (M.P.C. 5357).[13]

References[edit]

  1. ^ a b c d e "JPL Small-Body Database Browser: 1783 Albitskij (1935 FJ)" (2016-11-07 last obs.). Jet Propulsion Laboratory. Retrieved 8 December 2016. 
  2. ^ a b Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (1783) Albitskij. Springer Berlin Heidelberg. p. 143. ISBN 978-3-540-00238-3. Retrieved 3 November 2016. 
  3. ^ a b c d e f "LCDB Data for (1783) Albitskij". Asteroid Lightcurve Database (LCDB). Retrieved 3 November 2016. 
  4. ^ a b c d Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. Bibcode:2004PDSS...12.....T. Retrieved 3 November 2016. 
  5. ^ 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" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407Freely accessible. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 3 November 2016. 
  6. ^ a b c d 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:1209.5794Freely accessible. Bibcode:2012ApJ...759L...8M. doi:10.1088/2041-8205/759/1/L8. Retrieved 3 November 2016. 
  7. ^ a b c d 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" (PDF). Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. Retrieved 3 November 2016. 
  8. ^ 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:1109.4096Freely accessible. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68. Retrieved 8 September 2016. 
  9. ^ a b c 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. 
  10. ^ a b 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:1506.00762Freely accessible. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. Retrieved 3 November 2016. 
  11. ^ a b "1783 Albitskij (1935 FJ)". Minor Planet Center. Retrieved 3 November 2016. 
  12. ^ Lazzaro, Daniela; Mothé-Diniz, Thaís.; Carvano, Jorge M.; Angeli, Cláudia A.; Betzler, Alberto S.; Florczak, Marcos; et al. (December 1999). "The Eunomia Family: A Visible Spectroscopic Survey". Icarus. 142 (2): 445–453. Bibcode:1999Icar..142..445L. doi:10.1006/icar.1999.6213. Retrieved 25 December 2015. 
  13. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 3 November 2016. 

External links[edit]