1900 Katyusha

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1900 Katyusha
Discovery [1]
Discovered byT. Smirnova
Discovery siteCrAO (Nauchnyj)
Discovery date16 December 1971
Designations
1900 Katyusha
Named after
Yekaterina Zelenko
(war pilot)[2]
1971 YB · 1938 WM
1941 SS1 · 1950 LS
1953 GL1 · 1961 WD
1969 DC
main-belt · Flora family[3]
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc62.09 yr (22678 days)
Aphelion2.5073 AU (375.09 Gm)
Perihelion1.9109 AU (285.87 Gm)
2.2091 AU (330.48 Gm)
Eccentricity0.13497
3.28 yr (1199.3 d)
174.01°
0° 18m 0.648s / day
Inclination6.5434°
281.92°
142.51°
Earth MOID0.928604 AU (138.9172 Gm)
Jupiter MOID2.771 AU (414.5 Gm)
TJupiter3.638
Physical characteristics
Dimensions9 km[4][5]
9.4999 h (0.39583 d)
0.29[4][5]
S (LCDB)[3]
12.2

1900 Katyusha, provisional designation 1971 YB, is a small but bright stony asteroid of the inner main-belt. It was discovered on December 16, 1971, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj[6] and measures about 9 kilometers in diameter. Its albedo of 0.29 has been determined by spectrophotometric observations made by NEOWISE in 2010–2011.[4][5]

The asteroid orbits the Sun at a distance of 1.9–2.5 AU once every 3 years and 3 months (1,200 days)[1] and rotates around its axis with a period of nine and a half hours (9.4999±0.0001 h, 0.72±0.02 mag).[7] It is an assumed S-type asteroid belonging to the Flora family.[3]

Named in honor of Ukrainian Ekaterina Ivanovna Zelenko (1916–1941), a war pilot and Hero of the Soviet Union, known for being the only woman who had ever executed an aerial ramming. The asteroid's name "Katyusha" is a petname for Ekaterina.[2]

References

  1. ^ a b c "JPL Small-Body Database Browser: 1900 Katyusha (1971 YB)" (2015-05-17 last obs.). Jet Propulsion Laboratory. Retrieved 20 April 2016.
  2. ^ a b Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1900) Katyusha. Springer Berlin Heidelberg. p. 152. ISBN 978-3-540-29925-7. Retrieved 23 August 2016.
  3. ^ a b c "LCDB Data for (1900) Katyusha". Asteroid Lightcurve Database (LCDB). Retrieved 23 August 2016.
  4. ^ a b c Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; Cabrera, M. S. (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. Retrieved 23 August 2016.
  5. ^ a b c Mainzer, 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. Retrieved 23 August 2016.
  6. ^ "1900 Katyusha (1971 YB)". Minor Planet Center. Retrieved 23 August 2016.
  7. ^ Sada, Pedro V. (September 2008). "CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory". The Minor Planet Bulletin. 35 (3): 105–107. Bibcode:2008MPBu...35..105S. ISSN 1052-8091. Retrieved 23 August 2016.

External links