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1789 Dobrovolsky

From Wikipedia, the free encyclopedia
Main-belt asteroid

1789 Dobrovolsky
Shape model ofDobrovolsky from itslightcurve
Discovery[1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date19 August 1966
Designations
(1789) Dobrovolsky
Named after
Georgy Dobrovolsky
(cosmonaut)[2]
1966 QC · 1936 KK
1939 GR · 1943 SG
1946 NA · 1953 TC2
1953 VX3 · 1955 EJ
1956 PD · 1956 RT
1969 OF
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc73.51 yr (26,850 days)
Aphelion2.6309AU
Perihelion1.7952 AU
2.2131 AU
Eccentricity0.1888
3.29yr (1,203 days)
195.44°
0° 17m 57.84s / day
Inclination1.9761°
102.09°
214.93°
Physical characteristics
Dimensions7.809±0.077 km[4]
7.922±0.099[5]
9.85 km(calculated)[3]
11.23±0.37 km[6]
4.800±0.020h[7]
4.811096±0.000005 h[8]
4.8111±0.0025 h[9]
4.812±0.001 h[a]
5.8 h[10]
0.1825±0.0243[4]
0.185±0.031[6][5]
0.24(assumed)[3]
S[3][11]
11.05±1.53[11] · 11.800±0.080(R)[7] · 11.922±0.001(R)[9] · 12.2[1][3][6] · 13.0[4]

1789 Dobrovolsky (prov. designation:1966 QC) is aFlora asteroid from the inner regions of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 19 August 1966, by Russian astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula.[12] The asteroid was named after cosmonautGeorgy Dobrovolsky.[2]

Orbit and classification

[edit]

Dobrovolsky is a member of theFlora family, a large group of stonyS-type asteroids in the inner main-belt. It orbits the Sun in theinner main-belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,203 days). Its orbit has aneccentricity of 0.19 and aninclination of 2° with respect to theecliptic.[1] First identified as1936 KK atJohannesburg, the body's first used observation was taken atNice Observatory in 1943, whenDobrovolsky was identified as1943 SG, extending itsobservation arc by 23 years prior to its official discovery observation.[12]

Naming

[edit]

Thisminor planet was named in honor of Ukrainian–Soviet cosmonautGeorgy Dobrovolsky, commander of theSoyuz 11 spacecraft, who died on 30 June 1971 during the vehicle's return to Earth after completing the flight program of the first crewed orbital station,Salyut. The subsequently numbered minor planets1790 Volkov and1791 Patsayev were named in honour of his dead crew members.[2]

The names of all three cosmonauts are also engraved on the plaque next to the sculpture of theFallen Astronaut on the Moon, which was placed there during theApollo 15 mission, containing the names of eight American astronauts and six Soviet cosmonauts, who had all died in service. The officialnaming citation was published by theMinor Planet Center on 1 July 1972 (M.P.C. 3296).[13]

Physical characteristics

[edit]

Rotation period

[edit]

The so-far best rated rotationallightcurve ofDobrovolsky was obtained from photometric observations by American astronomerBrian A. Skiff in March 2011. It gave arotation period of 4.812 hours with a brightness variation of 0.13magnitude (U=3).[a] Other lightcurves were obtained byClaes-Ingvar Lagerkvist (in 1973) and at thePalomar Transient Factory (in 2014), giving a period of 5.8, 4.800 and 4.8111 hours, respectively (U=2/2/2).[7][9][10] An international study from February 2016, published a modeled period of 4.811096 hours (U=n.a.).[8]

Diameter and albedo

[edit]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Dobrovolsky measures 7.92 kilometers in diameter and its surface has analbedo of 0.185 (best result),[4][5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, the largest member and namesake of its family – and calculates a diameter of 9.85 kilometers with anabsolute magnitude of 12.2.[3]

Notes

[edit]
  1. ^abSkiff, B.A. (2011) web: rotation period4.812±0.001 hours with a brightness amplitude of0.13 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1746) Brouwer

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1789 Dobrovolsky (1966 QC)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1789) Dobrovolsky".Dictionary of Minor Planet Names – (1789) Dobrovolsky.Springer Berlin Heidelberg. p. 143.doi:10.1007/978-3-540-29925-7_1790.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1789) Dobrovolsky". 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.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved19 December 2016.
  6. ^abcdMasiero, 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. Retrieved19 December 2016.
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved19 December 2016.
  8. ^abHanus, J.; Durech, 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: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441. Retrieved19 December 2016.
  9. ^abcWaszczak, 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. Retrieved19 December 2016.
  10. ^abLagerkvist, C.-I. (March 1978)."Photographic photometry of 110 main-belt asteroids".Astronomy and Astrophysics Supplement Series.31:361–381.Bibcode:1978A&AS...31..361L. Retrieved19 December 2016.
  11. ^abVeres, 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.
  12. ^ab"1789 Dobrovolsky (1966 QC)".Minor Planet Center. Retrieved19 December 2016.
  13. ^Schmadel, Lutz D. (2009). "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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