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1648 Shajna

From Wikipedia, the free encyclopedia
Stony asteroid from the inner regions of the asteroid belt

1648 Shajna
Shape model ofShajna from itslightcurve
Discovery[1]
Discovered byP. Shajn
Discovery siteSimeiz Obs.
Discovery date5 September 1935
Designations
(1648) Shajna
Named after
Couple of astronomers
(Pelageya andGrigory)[2]
1935 RF · 1934 CK1
1938 MC · 1941 FD
1948 LC · 1951 EX2
1952 SX · 1952 UW
1955 QT · 1955 RP
A921 GB · A924 EQ
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc95.99 yr (35,061 days)
Aphelion2.6971AU
Perihelion1.7737 AU
2.2354 AU
Eccentricity0.2065
3.34yr (1,221 days)
250.93°
0° 17m 41.64s / day
Inclination4.5723°
130.42°
134.71°
Physical characteristics
Dimensions8.26±1.47 km[4]
8.30±0.30 km[5]
9.23 km(calculated)[3]
9.450±0.141 km[6][7]
6.41368±0.00001h[8]
6.41369±0.00005 h[9]
6.4140±0.0002 h[10]
6.4140±0.0164 h(R)[11]
6.4248±0.0164 h(S)[11]
0.191±0.016[6][7]
0.20(assumed)[3]
0.247±0.049[5]
0.35±0.13[4]
Tholen =S[1] · S[3]
B–V = 0.792[1]
U–B = 0.497[1]
11.838±0.003(R)[11] · 12.21[4] · 12.54[1][3][5][6]

1648 Shajna, provisional designation1935 RF, is a stonyasteroid from the inner regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 5 September 1935, by Russian astronomerPelageya Shajn atSimeiz Observatory on the Crimean peninsula.[12] Two weeks later, it was independently discovered byCyril Jackson atJohannesburg Observatory, South Africa. It was later named after the discoverer and her husband, Russian astronomersGrigory Shajn.[2]

Orbit and classification

[edit]

Shajna orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,221 days). Itswell-determined orbit has aneccentricity of 0.21 and aninclination of 5° with respect to theecliptic.[1] In 1921,Shajna was first identified as1921 GB atHeidelberg Observatory. Its first used observation was taken atUccle in 1934, when it was identified as1934 CK1, extending the body'sobservation arc by one year prior to its official discovery observation.[12]

Rotation period

[edit]

In July 2005, a rotationallightcurve of was obtained by French amateur astronomerLaurent Bernasconi. It gave a well-definedrotation period of 6.4140 hours with a brightness variation of 0.65magnitude (U=3).[10] Two modeled lightcurves from various surveys including the Lowell photometric database gave similar periods of 6.41368 and 6.41369 hours (U=n.a.).[8][9] Photometric observations at thePalomar Transient Factory in September 2012, gave nearly identical periods of 6.4140 and 6.4248 hours in the R- and S-band, respectively (U=2/2).[11]

Diameter and albedo

[edit]

According to the surveys carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Shajna measures between 8.26 and 9.45 kilometers in diameter, and its surface has analbedo between 0.191 and 0.35.[4][5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 9.23 kilometers with anabsolute magnitude of 12.54.[3]

Naming

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Thisminor planet was named in honor of the late couple of Russian astronomersGrigory Shajn (1892–1956) and the discoverer herself,Pelageya Shajn (1894–1956), first woman ever to discover a minor planet. The asteroid1190 Pelagia is also named after her, while her husband is honored by the lunar craterShayn.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1962 (M.P.C. 2117).[13]

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 1648 Shajna (1935 RF)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1648) Shajna".Dictionary of Minor Planet Names – (1648) Shajna.Springer Berlin Heidelberg. p. 131.doi:10.1007/978-3-540-29925-7_1649.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1648) Shajna". Asteroid Lightcurve Database (LCDB). Retrieved26 December 2016.
  4. ^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.
  5. ^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.S2CID 46350317. Retrieved26 December 2016.
  6. ^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.S2CID 35447010.
  7. ^abcMasiero, 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.S2CID 118745497. Retrieved26 December 2016.
  8. ^abDurech, J.; Hanus, J.; Oszkiewicz, D.; Vanco, R. (March 2016)."Asteroid models from the Lowell photometric database".Astronomy and Astrophysics.587: 6.arXiv:1601.02909.Bibcode:2016A&A...587A..48D.doi:10.1051/0004-6361/201527573.S2CID 118427201. Retrieved26 December 2016.
  9. ^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.S2CID 119112278.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1648) Shajna".Geneva Observatory. Retrieved26 December 2016.
  11. ^abcdWaszczak, 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.S2CID 8342929. Retrieved26 December 2016.
  12. ^ab"1648 Shajna (1935 RF)".Minor Planet Center. Retrieved26 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.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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