411 REFERENCE · Wikipedia
1900 Katyusha
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Stony main-belt asteroid
March 2020
yes
1900 Katyusha
#D6D6D6
001900-asteroid shape model (1900) Katyusha.png
Modelled shape of Katyusha from its lightcurve
T. Smirnova
Crimean Astrophysical Obs.
16 December 1971
(1900) Katyusha
1971 YB1938 WM1941 SS 11950 LS1953 GL 11961 WD1969 DC
Yekaterina Zelenko(Soviet war pilot)
main-beltFlora family
4 September 2017 (JD 2458000.5)
0
63.59 yr (23,226 days)
2.5075 AU
1.9116 AU
2.2096 AU
0.1348
3.28 yr (1,200 days)
354.20°
0.3001 ms / day
6.5426°
281.91°
142.40°
8.820 0.097 km9 km
9.4999 h d on on
0.290.299 0.037
S
12.2
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 and named in honor of Yekaterina Zelenko, the only woman to credited with conducting an aerial ramming.
Orbit and classification
Katyusha is a member of the Flora family, one of the largest groups of stony asteroids in the inner main-belt. 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.
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.
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.
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. Katyusha has been characterized as a S-type asteroid.
References
6
Mainzer, A.
Grav, T.
Masiero, J.
Hand, E.
Bauer, J.
Tholen, D.
McMillan, R. S.
Spahr, T.
Cutri, R. M.
Wright, E.
Watkins, J.
Mo, W.
Maleszewski, C.
November 2011
NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...90M
The Astrophysical Journal
741
2
25
2011ApJ...741...90M
10.1088/0004-637X/741/2/90
23 August 2016 1109.6407
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
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
The Astrophysical Journal Letters
759
1
5
2012ApJ...759L...8M
10.1088/2041-8205/759/1/L8
23 August 2016 1209.5794
Sada
Pedro V.
September 2008
CCD Photometry of Six Asteroids from the Universidad de Monterry Observatory
Minor Planet Bulletin
http://www.minorplanet.info/MPB/issues/MPB_35-3.pdf
35
3
105–107
2008MPBu...35..105S
1052-8091
17 March 2020
20 August 2020
https://web.archive.org/web/20200820104842/http://www.minorplanet.info/MPB/issues/MPB_35-3.pdf
dead
1900
23 August 2016
2016-11-15 last obs.
JPL Small-Body Database Browser: 1900 Katyusha (1971 YB)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001900
https://web.archive.org/web/20200918052102/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001900
dead
18 September 2020
Jet Propulsion Laboratory
14 June 2017
Dictionary of Minor Planet Names – (1900) Katyusha
Schmadel Lutz D.
Springer Berlin Heidelberg
152
2003
978-3-540-29925-7
10.1007/978-3-540-29925-7_1901
(1900) Katyusha
1900 Katyusha (1971 YB)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1900
23 August 2016
6
Joseph R. Masiero
T. Grav
A. K. Mainzer
C. R. Nugent
J. M. Bauer
R. Stevenson
S. Sonnett
August 2014
Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
14 June 2017
External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1900
1899 Crommelin 1900 1901 Moravia
001900
Category:Discoveries by Tamara Mikhaylovna Smirnova
Category:Named minor planets
19711216