2009 Voloshina

Carbonaceous asteroid Ukrainian surname Voloshin October 2019 yes 2009 Voloshina #D6D6D6 1968 10 22 T. Smirnova Crimean Astrophysical Obs. (2009) Voloshina 1968 UL1926 FF1929 TO1957 WF 21959 EC1970 EL 11973 SP 61973 SU 3 Vera Danilovna Voloshina(Soviet WWII partisan) main-belt(outer) 4 September 2017 (JD 2458000.5) 0 90.65 yr (33,111 days) 3.5594 AU 2.6725 AU 3.1160 AU 0.1423 5.50 yr (2,009 days) 261.36° 2.8609° 107.55° 6.2038° 21.19 9.05 km26.558 0.476 km28.04 0.72 km34.67 km (derived)34.8 km (IRAS) 2.94 0.010 h5.896 0.002 h5.907 0.0547 h 0.0487 (derived)0.0698 0.0090.11 0.110.118 0.0070.120 0.024 C 10.810.870 0.120 (R)10.944 0.002 (R)11.211.29 0.32 2009 Voloshina, provisional designation 1968 UL, is a carbonaceous asteroid from the outer regions of the asteroid belt, approximately 27 kilometers in diameter. It was discovered on 22 October 1968, by Russian astronomer Tamara Smirnova at the Crimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula. The asteroid was named for WWII partisan Vera Voloshina. Classification and orbit Voloshina orbits the Sun in the outer main-belt at a distance of 2.7–3.6 AU once every 5 years and 6 months (2,009 days). Its orbit has an eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. In March 1926, Voloshina was first observed as 1926 FF at Yerkes Observatory and one day later at Heidelberg Observatory. Its observation arc begins at Heidelberg, 62 years prior to its official discovery observation. Physical characteristics Voloshina has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey. Lightcurves In May 2009, a rotational lightcurve of Voloshina was obtained from photometric observations by astronomers at the Oakley Southern Sky Observatory (E09) in Australia. Lightcurve analysis gave a rotation period of 5.896 hours with a brightness variation of 0.40 magnitude (U=3-). In January and February 2014, astronomers at the Palomar Transient Factory found a period of 2.94 and 5.907 hours with an amplitude of 0.32 and 0.27 magnitude, respectively (U=2/2). Diameter and albedo According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Voloshina measures between 21.19 and 34.8 kilometers in diameter and its surface has an albedo between 0.0698 and 0.120. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0487 and calculates a diameter of 34.67 kilometers based on an absolute magnitude of 11.2. An occultation of a star by 2009 Voloshina was observed in 2021. Naming This minor planet was named in honor of Vera Danilovna Voloshina (1919–1941), a partisan of the Soviet Great Patriotic War (1941–1945), also known as the Eastern Front of the Second World War. The official 2009 naming citation was published by the Minor Planet Center on 1 September 1978 (M.P.C. 4481). References 30em 2016-11-11 last obs. JPL Small-Body Database Browser: 2009 Voloshina (1968 UL) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002009 Jet Propulsion Laboratory 3 July 2017 Dictionary of Minor Planet Names – (2009) Voloshina Schmadel Lutz D. Springer Berlin Heidelberg 163 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_2010 (2009) Voloshina 2009 Voloshina (1968 UL) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=2009 3 July 2017 Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008) Appendix – Publication Dates of the MPCs Schmadel Lutz D. Springer Berlin Heidelberg 221 978-3-642-01964-7 10.1007/978-3-642-01965-4 6 Joseph R. Masiero A. K. Mainzer T. Grav J. M. Bauer R. M. Cutri J. Dailey P. R. M. Eisenhardt R. S. McMillan T. B. Spahr M. F. Skrutskie D. Tholen R. G. Walker E. L. Wright E. DeBaun D. Elsbury T. IV Gautier S. Gomillion A. Wilkins November 2011 Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M The Astrophysical Journal 741 2 20 2011ApJ...741...68M 10.1088/0004-637X/741/2/68 1109.4096 3 July 2017 E. F. Tedesco P. V. Noah M. Noah S. D. Price October 2004 IRAS Minor Planet Survey V6.0 https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab NASA Planetary Data System 12 IRAS-A-FPA-3-RDR-IMPS-V6.0 2004PDSS...12.....T 22 October 2019 2009 3 July 2017 6 Fumihiko Usui Daisuke Kuroda Thomas G. Müller Sunao Hasegawa Masateru Ishiguro Takafumi Ootsubo Daisuke Ishihara Hirokazu Kataza Satoshi Takita Shinki Oyabu Munetaka Ueno Hideo Matsuhara Takashi Onaka October 2011 Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey Publications of the Astronomical Society of Japan 63 5 1117–1138 2011PASJ...63.1117U 10.1093/pasj/63.5.1117 (online, AcuA catalog p. 153) 6 A. Mainzer T. Grav J. Masiero E. Hand J. Bauer D. Tholen R. S. McMillan T. Spahr R. M. Cutri E. Wright J. Watkins W. Mo C. Maleszewski November 2011 NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results The Astrophysical Journal 741 2 25 2011ApJ...741...90M 10.1088/0004-637X/741/2/90 1109.6407 6 C. R. Nugent A. Mainzer J. Masiero J. Bauer R. M. Cutri T. Grav E. Kramer S. Sonnett R. Stevenson E. L. Wright December 2015 NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N The Astrophysical Journal 814 2 13 2015ApJ...814..117N 10.1088/0004-637X/814/2/117 1509.02522 3 July 2017 Richard Ditteon Elaine Kirkpatrick Katelyn Doering January 2010 Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2009 April - May http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2010MPBu...37....1D The Minor Planet Bulletin 37 1 1–3 1052-8091 2010MPBu...37....1D 3 July 2017 6 Chan-Kao Chang Wing-Huen Ip Ip Wing-huen Hsing-Wen Lin Yu-Chi Cheng Chow-Choong Ngeow Ting-Chang Yang Adam Waszczak Shrinivas R. Kulkarni David Levitan Branimir Sesar Russ Laher Jason Surace Thomas. A. Prince August 2015 Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJS..219...27C The Astrophysical Journal Supplement Series 219 2 19 2015ApJS..219...27C 10.1088/0067-0049/219/2/27 1506.08493 3 July 2017 6 Adam Waszczak Chan-Kao Chang Eran O. Ofek Russ Laher Frank Masci David Levitan Jason Surace Yu-Chi Cheng Wing-Huen Ip Daisuke Kinoshita George Helou Thomas A. Prince Shrinivas Kulkarni September 2015 Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W The Astronomical Journal 150 3 35 2015AJ....150...75W 10.1088/0004-6256/150/3/75 1504.04041 3 July 2017 6 Peter Veres Robert Jedicke Alan Fitzsimmons Larry Denneau Mikael Granvik Bryce Bolin Serge Chastel Richard J. Wainscoat William S. Burgett Kenneth C. Chambers Heather Flewelling Nick Kaiser Eugen A. Magnier Jeff S. Morgan Paul A. Price John L. Tonry Christopher Waters November 2015 Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V Icarus 261 34–47 2015Icar..261...34V 10.1016/j.icarus.2015.08.007 1506.00762 3 July 2017 External links 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 2008 Konstitutsiya 2009 2010 Chebyshev 002009 Category:Discoveries by Tamara Mikhaylovna Smirnova Category:Named minor planets 19681022