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1585 Union

From Wikipedia, the free encyclopedia
Dark background asteroid

1585 Union
Discovery[1]
Discovered byE. L. Johnson
Discovery siteUnion Obs.
Discovery date7 September 1947
Designations
(1585) Union
Named after
Union Observatory
(aka Johannesburg Obs.)[2]
1947 RG · 1929 DB
1937 QF · 1939 CD1
1944 DG · 1949 EE
1952 QA1 · 1952 SD
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc78.37 yr (28,624 days)
Aphelion3.8332AU
Perihelion2.0231 AU
2.9281 AU
Eccentricity0.3091
5.01yr (1,830 days)
304.39°
0° 11m 48.12s / day
Inclination26.187°
150.10°
264.54°
Physical characteristics
Dimensions49.01±18.07 km[4]
50.42±1.6 km[3][5]
50.68±0.88 km[6]
55.271±0.243 km[7]
55.42±18.20 km[8]
56.014±0.292 km[9]
9.38h[10]
24 h(fragmentary)[11]
0.0304±0.0028[9]
0.031±0.004[7]
0.0378±0.003[3][5]
0.038±0.001[6]
0.04±0.04[8]
0.05±0.02[4]
P[9] · C[3]
B–V = 0.590[1]
U–B = 0.290[1]
10.33±0.22[12] · 10.35[8] · 10.66[1][4][5][6] · 10.67[3][9][10]

1585 Union, provisional designation1947 RG, is a dark backgroundasteroid from the outer regions of theasteroid belt, approximately 52 kilometers in diameter. It was discovered on 7 September 1947, by South African astronomerErnest Johnson at theUnion Observatory in Johannesburg, South Africa.[13] The asteroid was named after the discovering observatory.[2]

Orbit and classification

[edit]

Union is not a member of any knownasteroid family. It orbits the Sun in theouter main belt at a distance of 2.0–3.8 AU once every 5.01 years (1,830 days). Its orbit has aneccentricity of 0.31 and aninclination of 26° with respect to theecliptic.[1]

In 1929, the asteroid was first identified as1929 DB at theUccle Observatory in Belgium. The body'sobservation arc begins at the FinnishTurku Observatory in February 1939, more than 17 years prior to its official discovery observation at Johannesburg.[13]

Physical characteristics

[edit]

Union has been characterized as aP-type asteroid by theWide-field Infrared Survey Explorer (WISE), while the LCDB assumes a generic carbonaceousC-type.[3][9]

Rotation period

[edit]

In March 1984, a rotationallightcurve ofUnion was obtained from photometric observations by American astronomerRichard Binzel. Lightcurve analysis gave arotation period of 9.38 hours with a brightness variation of 0.22magnitude (U=2).[10] In addition, a fragmentary lightcurve with a period of 24 hours was obtained by French amateur astronomerLaurent Bernasconi in 2004 (U=1).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA's WISE telescope,Union measures between 49.01 and 56.014 kilometers in diameter and its surface has analbedo between 0.0304 and 0.05.[4][5][6][7][8][9]

TheCollaborative Asteroid Lightcurve Link adopt the results obtained by IRAS, that is, an albedo of 0.0378 and a diameter of 50.42 kilometers. CALL also takes anabsolute magnitude of 10.67 from Richard Binzel.[3]

Naming

[edit]

Thisminor planet was named after the discovering Union Observatory, also known as theJohannesburg Observatory, Transvaal Observatory (1909–1912) and Republic Observatory (1961–1971). The officialnaming citation was published by theMinor Planet Center in June 1953 (M.P.C. 941).[14]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1585 Union (1947 RG)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved30 August 2017.
  2. ^abSchmadel, Lutz D. (2007). "(1585) Union".Dictionary of Minor Planet Names – (1585) Union.Springer Berlin Heidelberg. p. 125.doi:10.1007/978-3-540-29925-7_1586.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1585) Union". Asteroid Lightcurve Database (LCDB). Retrieved30 August 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117.S2CID 9341381. Retrieved30 August 2017.
  5. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved17 October 2019.
  6. ^abcdUsui, 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. (online,AcuA catalog p. 153)
  7. ^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.S2CID 119293330. Retrieved30 August 2017.
  8. ^abcdNugent, 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.
  9. ^abcdefMainzer, 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.S2CID 35447010.
  10. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved30 August 2017.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1585) Union".Geneva Observatory. Retrieved30 August 2017.
  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.S2CID 53493339. Retrieved30 August 2017.
  13. ^ab"1585 Union (1947 RG)".Minor Planet Center. Retrieved30 August 2017.
  14. ^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.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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Distant minor planet
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