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1916 Boreas

From Wikipedia, the free encyclopedia
Near-Earth asteroid

1916 Boreas
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date1 September 1953
Designations
(1916) Boreas
Pronunciation/ˈbɔːriəs/[2]
Named after
Boreas(Greek mythology)[3]
1953 RA
NEO · Amor[1][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.73 yr (23,279 days)
Aphelion3.2944AU
Perihelion1.2506 AU
2.2725 AU
Eccentricity0.4497
3.43yr (1,251 days)
252.13°
0° 17m 15.72s / day
Inclination12.884°
340.64°
335.83°
Earth MOID0.2520 AU · 98.2LD
Physical characteristics
Dimensions3.07 km(calculated)[5]
3.5 km[1]
3.4741±0.0003h[6][a]
3.4746 h[7]
3.4746±0.0010 h[a]
3.4748±0.0010 h[a]
3.49±0.01 h[8]
0.15(assumed)[1]
0.20(assumed)[5]
S(Tholen),S(SMASS)
S[9] · Sw[5][10][11]
B–V = 0.852
U–B = 0.407
14.86±0.112[5][12] · 14.93[1][11]

1916 Boreas, provisional designation1953 RA, is an eccentric, stonyasteroid andnear-Earth object of theAmor group, approximately 3 kilometers in diameter. After its discovery in 1953, it became alost asteroid until 1974. It was named afterBoreas from Greek mythology.

Discovery

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Boreas was discovered on 1 September 1953, by Belgian astronomerSylvain Arend at theRoyal Observatory of Belgium in Uccle.[4] The asteroid was observed for 2 months and then with time became alost asteroid. It was recovered in 1974, by Richard Eugene McCrosky, G. Schwartz and JH Bulger based on a predicted position byBrian G. Marsden.[b][13]

Orbit and classification

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Boreas orbits the Sun at a distance of 1.3–3.3 AU once every 3 years and 5 months (1,251 days). Its orbit has aneccentricity of 0.45 and aninclination of 13° with respect to theecliptic.[1]

Thenear-Earth asteroid has anEarthminimum orbit intersection distance of 0.2520 AU (37,700,000 km),[1] which corresponds to 98.2lunar distances. Itsobservation arc begins with it official discovery observation at Uccle in 1953.[4]

Physical characteristics

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On theTholen andSMASS taxonomic scheme,Boreas is classified as a commonS-type asteroid with a stony composition.[1] It has also been characterized as a Sw-subtype.[5][10][11]

Several rotationallightcurves gave arotation period between 3.4741 and 3.49 hours with a brightness variation between 0.25 and 0.35magnitude (U=2/2/3/n.a.).[6][7][8][a]

In 1994, astronomerTom Gehrels estimatedBoreas to measure 3.5 kilometers in diameter, based on an assumedalbedo of 0.15.[1] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.07 kilometers with anabsolute magnitude of 14.93.[5]

Naming

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Thisminor planet is named after the Greek god of the north wind,Boreas, as the asteroid was discovered moving rapidly northward after passing the ascending node of its orbit.[3] The official naming citation was published by theMinor Planet Center on 8 April 1982 (M.P.C. 6833).[14]

Notes

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  1. ^abcdPravec (2001) web: rotation period3.4748±0.0010 hours with a brightness amplitude of0.28 mag. Behrend (2001) web: rotation period3.4741±0.0003 hours with a brightness amplitude of0.29 mag. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (1916) Boreas
  2. ^Central Bureau for Astronomical Telegrams – 1953 RA This member of the Amor group, not observed since 1953 (cf. Minor Planet Circ. No. 3015), has been recovered by McCrosky, Schwartz and Bulger with the 155-cm reflector some 0o.3 from an unpublished prediction by B. G. MarsdenInternational Astronomical Union Circular 2710 for (1953 RA)

References

[edit]
  1. ^abcdefghij"JPL Small-Body Database Browser: 1916 Boreas (1953 RA)" (2017-05-27 last obs.).Jet Propulsion Laboratory. Retrieved9 June 2017.
  2. ^"Boreas".Dictionary.com Unabridged (Online). n.d.
  3. ^abSchmadel, Lutz D. (2007). "(1916) Boreas".Dictionary of Minor Planet Names – (1916) Boreas.Springer Berlin Heidelberg. p. 154.doi:10.1007/978-3-540-29925-7_1917.ISBN 978-3-540-00238-3.
  4. ^abc"1916 Boreas (1953 RA)".Minor Planet Center. Retrieved10 December 2016.
  5. ^abcdef"LCDB Data for (1916) Boreas". Asteroid Lightcurve Database (LCDB). Retrieved10 December 2016.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1916) Boreas".Geneva Observatory. Retrieved18 May 2016.
  7. ^abKrugly, Yu. N.; Belskaya, I. N.; Chiorny, V. G.; Shevchenko, V. G.; Gaftonyuk, N. M. (November 2002)."CCD photometry of near-Earth asteroids in 2001".In: Proceedings of Asteroids.500:903–906.Bibcode:2002ESASP.500..903K. Retrieved10 December 2016.
  8. ^abRobinson, L. E. (June 2002)."Lightcurve Photometry of 551 Ortrud, 1118 Hanskya, and 1916 Boreas from Sunflower Observatory".The Minor Planet Bulletin.29:37–38.Bibcode:2002MPBu...29...37R. Retrieved10 December 2016.
  9. ^Dandy, C. L.; Fitzsimmons, A.; Collander-Brown, S. J. (June 2003)."Optical colors of 56 near-Earth objects: trends with size and orbit".Icarus.163 (2):363–373.Bibcode:2003Icar..163..363D.doi:10.1016/S0019-1035(03)00087-3. Retrieved10 December 2016.
  10. ^abThomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014)."Physical characterization of Warm Spitzer-observed near-Earth objects".Icarus.228:217–246.arXiv:1310.2000.Bibcode:2014Icar..228..217T.doi:10.1016/j.icarus.2013.10.004.hdl:2060/20140012047.S2CID 119278697. Retrieved10 December 2016.
  11. ^abcCarry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016)."Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry".Icarus.268:340–354.arXiv:1601.02087.Bibcode:2016Icar..268..340C.doi:10.1016/j.icarus.2015.12.047.S2CID 119258489. Retrieved10 December 2016.
  12. ^Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved10 December 2016.
  13. ^Brian G. Marsden (24 October 1974)."International Astronomical Union Circular 2710". Central Bureau for Astronomical Telegrams. Retrieved5 July 2011.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 December 2016.

External links

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