1900 Katyusha

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1900 Katyusha
001900-asteroid shape model (1900) Katyusha.png
Modelled shape of Katyusha from its lightcurve
Discovery [1]
Discovered by T. Smirnova
Discovery site Crimean Astrophysical Obs.
Discovery date16 December 1971
Designations
(1900) Katyusha
Named after
 Yekaterina Zelenko
(Soviet 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 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 63.59 yr (23,226 days)
Aphelion 2.5075 AU
Perihelion 1.9116 AU
2.2096 AU
Eccentricity 0.1348
3.28 yr (1,200 days)
354.20°
0° 18m 0.36s / day
Inclination 6.5426°
281.91°
142.40°
Physical characteristics
8.820±0.097 km [4]
9 km [5] [6]
9.4999  h (0.39583  d) [1]
0.29 [5] [6]
0.299±0.037 [4]
S [3]
12.2 [1]

    1900 Katyusha (prov. designation: 1971 YB) is a stony background asteroid from the inner asteroid belt, approximately 9 kilometers in diameter. It was discovered on 16 December 1971, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula [7] and named in honor of Yekaterina Zelenko, the only woman to credited with conducting an aerial ramming. [2]

    Contents

    Orbit and classification

    Katyusha is a member of the Flora family, one of the largest groups of stony asteroids in the inner main-belt. [3] It orbits the Sun in the inner main-belt at a distance of 1.9–2.5  AU once every 3 years and 3 months (1,200 days). Its orbit has an eccentricity of 0.13 and an inclination of 7° with respect to the ecliptic. [1]

    Naming

    This minor planet was named in honor of Ukrainian Yekaterina 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]

    Physical characteristics

    It rotates around its axis with a period of 9.4999 hours and with a brightness variation of 0.72 magnitude, indicating a non-spheroidal shape. [8]

    According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Katyusha measures between 8.820 and 9 kilometers in diameter and its surface has an albedo between 0.29 and 0.299. [4] [5] [6] Katyusha has been characterized as a S-type asteroid. [3]

    References

    1. 1 2 3 4 5 "JPL Small-Body Database Browser: 1900 Katyusha (1971 YB)" (2016-11-15 last obs.). Jet Propulsion Laboratory. Archived from the original on 18 September 2020. Retrieved 14 June 2017.
    2. 1 2 3 Schmadel, Lutz D. (2003). "(1900) Katyusha". Dictionary of Minor Planet Names – (1900) Katyusha. Springer Berlin Heidelberg. p. 152. doi:10.1007/978-3-540-29925-7_1901. ISBN   978-3-540-29925-7.
    3. 1 2 3 4 "LCDB Data for (1900) Katyusha". Asteroid Lightcurve Database (LCDB). Retrieved 23 August 2016.
    4. 1 2 3 Masiero, 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 . Retrieved 14 June 2017.
    5. 1 2 3 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.
    6. 1 2 3 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.
    7. ↑ "1900 Katyusha (1971 YB)". Minor Planet Center. Retrieved 23 August 2016.
    8. ↑ Sada, Pedro V. (September 2008). "CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory" (PDF). Minor Planet Bulletin. 35 (3): 105–107. Bibcode:2008MPBu...35..105S. ISSN   1052-8091 . Retrieved 17 March 2020.
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