1022 Olympiada

Near-Earth asteroid March 2018 yes 1022 Olympiada #D6D6D6 001022-asteroid shape model (1022) Olympiada.png Shape model of Olympiada from its lightcurve V. Albitzkij Simeiz Obs. 23 June 1924 (1022) Olympiada 1924 RT1928 FQ1948 QO1957 OC1961 JF1962 QKA910 NA Olimpiada Albitskaya(discoverer's mother) main-belt(outer)background 23 March 2018 (JD 2458200.5) 0 106.79 yr (39,006 d) 3.2959 AU 2.3144 AU 2.8051 AU 0.1749 4.70 yr (1,716 d) 10.487° 0.2098 ms / day 21.054° 111.97° 124.74° 26.39 2.2 km26.65 km (derived)32.88 0.76 km34.30 0.99 km 3.822 0.006 h3.833 0.005 hlightcurve-plot-Warner3.8331 0.0006 h3.83359 0.00005 h3.834 0.001 h3.835 0.0016 h4.589 0.002 h (retracted) 0.105 0.0050.125 0.0170.1600 0.0300.2069 (derived) SMASS X 10.053 0.001 (R)10.2010.46 0.2610.50 1022 Olympiada, provisional designation 1924 RT, is a background asteroid from the central regions of the asteroid belt, approximately 30 km mi off us in diameter. It was discovered at the Simeiz Observatory on the Crimean peninsula on 23 June 1924, by Soviet astronomer Vladimir Albitsky, who named it after his mother, Olimpiada Albitskaya. The X-type asteroid has a short rotation period of 3.83 hours. Orbit and classification Olympiada is a non-family asteroid from the main belt's background population. It orbits the Sun in the central asteroid belt at a distance of 2.3–3.3 AU once every 4 years and 8 months (1,716 days; semi-major axis of 2.81 AU). Its orbit has an eccentricity of 0.17 and an inclination of 21° with respect to the ecliptic. The body's observation arc begins with its first observation as A910 NA at Heidelberg Observatory in July 1910, or nearly 14 years prior to its official discovery observation at Simeiz. Naming This minor planet was named after Olimpiada Albitskaya, mother of the discoverer Vladimir Albitsky (1891–1952). No accurate naming citation was given for this asteroid in The Names of the Minor Planets. The author of the Dictionary of Minor Planets, Lutz Schmadel, learned about the naming circumstances from Nikolai Chernykh (1931–2004), a prolific long-time astronomer at Nauchnij, Crimea. Physical characteristics In the SMASS classification, Olympiada is an X-type asteroid. Rotation period Several rotational lightcurves of Olympiada have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado. Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a consolidated brightness variation between 0.27 and 0.66 magnitude (U=3),lightcurve-plot-Warner while the period of his first 1999-observation was later revised from 4.589 to 3.822 hours. For an asteroid of its size, it has a rather fast spin-rate. This period is also in good agreement with other observations obtained by astronomers at the Belgrade Astronomical Observatory (3.8331 h; Δ0.35 mag) in March 2008, by astronomers at the Palomar Transient Factory (3.835 h; Δ0.46 mag) in January 2012, and by a group of Italian astronomers (3.834 h; Δ0.66 mag) in March 2017 (U=3/2/3). Poles In 2011, a modeled lightcurve using data from the Uppsala Asteroid Photometric Catalogue and other sources gave a concurring sidereal period 3.83359 hours, as well as two poles at (46.0°, 10.0°) and (242.0°, 52.0°) in ecliptic coordinates (λ, β) (Q=2+). Brian Warner also determined two spin axes at (40.0°, 18.0°) and (250.0°, 71.0°) using his data set from 2008 (Q=2). Diameter and albedo According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Olympiada measures between 26.39 and 34.30 kilometers in diameter and its surface has an albedo between 0.105 and 0.1600. The Collaborative Asteroid Lightcurve Link derives an untypically high albedo of 0.2069 and a diameter of 26.65 kilometers based on an absolute magnitude of 10.2. Notes lightcurve-plot-Warner Lightcurve plot of (1022) Olympiada, Palmer Divide Observatory, B. D. Warner (2008). Rotation period 3.833 0.006 hours with a brightness amplitude of 0.34 0.02 mag. Quality code of 3. Summary figures at the LCDB References 30em 2017-04-30 last obs. JPL Small-Body Database Browser: 1022 Olympiada (1924 RT) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001022 Jet Propulsion Laboratory 15 March 2018 Dictionary of Minor Planet Names Schmadel Lutz D. Springer Berlin Heidelberg (1022) Olympiada 88 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_1023 1022 Olympiada (1924 RT) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=1022 15 March 2018 Asteroid 1022 Olympiada – Nesvorny HCM Asteroid Families V3.0 Small Bodies Data Ferret https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1022+Olympiada 24 October 2019 October 2026 InternetArchiveBot 1022 15 March 2018 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 Joseph R. Masiero A. K. Mainzer T. Grav J. M. Bauer R. M. Cutri C. Nugent M. S. Cabrera 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 1209.5794 15 March 2018 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 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 15 March 2018 6 Hanus, J. Durech, J. Broz, M. Warner, B. D. Pilcher, F. Stephens, R. Oey, J. Bernasconi, L. Casulli, S. Behrend, R. Polishook, D. Henych, T. Lehký, M. Yoshida, F. Ito, T. June 2011 A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011A&A...530A.134H Astronomy & Astrophysics 530 16 2011A&A...530A.134H 10.1051/0004-6361/201116738 1104.4114 15 March 2018 Warner, B. D. December 1999 Asteroid Photometry at the Palmer Divide Observatory http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1999MPBu...26...31W The Minor Planet Bulletin 26. 31 1999MPBu...26...31W 15 March 2018 Warner, Brian D. June 2005 Revised lightcurve analysis for 1022 Olympiada and 3285 Ruth Wolfe http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005MPBu...32...26W The Minor Planet Bulletin 32 2 26 1052-8091 2005MPBu...32...26W 15 March 2018 Brian D. Warner Josef Durech Michael Fauerbach Scott Marks October 2008 Shape and Spin Models for Four Asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35..167W The Minor Planet Bulletin 35 4 167–171 1052-8091 2008MPBu...35..167W 15 March 2018 6 Lorenzo Franco Giorgio Baj Vito Tinella Mauro Bachini Giacomo Succi Giovanni Battista Casalnuovo Paolo Bacci October 2017 Rotation Periods for Three Main-belt Asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2017MPBu...44..311F The Minor Planet Bulletin 44 4 311–312 1052-8091 2017MPBu...44..311F 15 March 2018 Vladimir Benishek Vojislava Protitch-Benishek April 2009 CCD Photometry of Asteroids at the Belgrade Astronomical Observatory: 2008 January–September http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2009MPBu...36...35B The Minor Planet Bulletin 36 2 35–37 1052-8091 2009MPBu...36...35B 15 March 2018 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 15 March 2018 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 – Geneva Observatory, Raoul Behrend Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center 1022 1021 Flammario 1022 1023 Thomana 001022 Category:Discoveries by Vladimir Albitsky Category:Named minor planets 001022 19240623