Skip to main content

  | मौसम…

411 समाचार
Public archive edition · Attributed source reporting with original dates · AI drafts are excluded

411 REFERENCE · Wikipedia

1088 Mitaka

Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.

Asteroid October 2019 yes 1088 Mitaka #D6D6D6 001088-asteroid shape model (1088) Mitaka.png Modelled shape of Mitaka from its lightcurve O. Oikawa Tokyo Astronomical Obs. 17 November 1927 (1088) Mitaka 1927 WA1942 FR1953 VW 31971 BEA917 RA Mitaka (Japanese village) main-belt(inner) background 4 September 2017 (JD 2458000.5) 0 88.22 yr (32,224 days) 2.6328 AU 1.7722 AU 2.2025 AU 0.1954 3.27 yr (1,194 days) 200.92° 0.3015 ms / day 7.6514° 54.495° 319.50° 11.33 2.51 km13.35 0.75 km15.137 0.131 km15.957 0.030 km16.016 km16.02 km (taken) 3.027 0.003 h3.0353 0.0005 h3.035377 h3.035378 0.000005 h3.0354 0.0002 h3.0361 0.0007 h3.049 0.005 h (115.0°, 46.0°) (λ1/β1) (278.0°, −72.0°) (λ2/β2) 0.15490.1588 0.02040.173 0.0250.276 0.0340.37 0.16 Tholen S SMASS S B–V 0.947 U–B 0.594 11.3911.5511.6211.62 0.08 1088 Mitaka (prov. designation: 1927 WA) is a bright background asteroid from the inner regions of the asteroid belt. It was discovered on 17 November 1927, by Japanese astronomer Okuro Oikawa at the old Tokyo Astronomical Observatory in Japan. The stony S-type asteroid has a notably short rotation period of 3.0 hours and measures approximately 15 km mi off 2 us in diameter. It was named after the Japanese village of Mitaka. Orbit and classification Mitaka is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements. It orbits the Sun in the inner asteroid belt at a distance of 1.8–2.6 AU once every 3 years and 3 months (1,194 days). Its orbit has an eccentricity of 0.20 and an inclination of 8° with respect to the ecliptic. The asteroid was first observed as A917 RA at the Simeiz Observatory on 11 September 1917. The body's observation arc begins at Tokyo in December 1927, one month after its official discovery observation. Naming This minor planet was named after the Japanese village of Mitaka, where the discovering Tokyo Astronomical Observatory was located. Nowadays the city of Mitaka hosts the headquarters of the National Astronomical Observatory of Japan with the Tokyo Photoelectric Meridian Circle, public relation and data centers, and several telescopes. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 103). Physical characteristics Mitaka is a common, stony S-type asteroid in both the Tholen and Bus–Binzel SMASS classification. Rotation period and poles Several rotational lightcurves of Mitaka have been obtained from photometric observations since 1989. Analysis of the best rated lightcurve by French amateur astronomer Pierre Antonini gave a rotation period of 3.0361 hours with a consolidated brightness variation of 0.23 to 0.62 magnitude (U=3). In 2009 and 2011, modelling of Mitakas lightcurve using photometric data from the US Naval Observatory, the Uppsala Asteroid Photometric Catalogue (UAPC), the Palmer Divide Observatory's archive, the Palomar Transient Factory survey, and from individual observers, gave a concurring rotation period of 3.035377 and 3.035378 hours. The modeled lightcurves also gave a spin axis of (115.0°, 46.0°) and (278.0°, −72.0°), as well as (280.0°, −71.0°) in ecliptic coordinates (λ, β). Diameter and albedo According to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Mitaka measures between 11.33 and 16.016 kilometers in diameter and its surface has an albedo between 0.1549 and 0.37. The Collaborative Asteroid Lightcurve Link adopts Petr Pravec's revised WISE results with an albedo of 0.1549 and takes a diameter of 16.02 kilometers based on an absolute magnitude of 11.62. References 30em 2017-07-05 last obs. JPL Small-Body Database Browser: 1088 Mitaka (1927 WA) https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001088 Jet Propulsion Laboratory 27 September 2017 Dictionary of Minor Planet Names – (1088) Mitaka Schmadel Lutz D. Springer Berlin Heidelberg (1088) Mitaka 93 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_1089 1088 Mitaka (1927 WA) Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=1088 27 September 2017 Asteroids and comets rotation curves – (1088) Mitaka Behrend Raoul Geneva Observatory http://obswww.unige.ch/~behrend/page3cou.html#001088 27 September 2017 3 December 2002 https://web.archive.org/web/20021203214643/http://obswww.unige.ch/~behrend/page3cou.html#001088 dead 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 119293330 27 September 2017 1088 27 September 2017 Petr Pravec Alan W. Harris Peter Kusnirák Adrián Galád Kamil Hornoch September 2012 Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012Icar..221..365P Icarus 221 1 365–387 2012Icar..221..365P 10.1016/j.icarus.2012.07.026 27 September 2017 6 C. R. Nugent A. Mainzer J. Bauer R. M. Cutri E. A. Kramer T. Grav J. Masiero S. Sonnett E. L. Wright September 2016 NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos The Astronomical Journal 152 3 12 2016AJ....152...63N 10.3847/0004-6256/152/3/63 1606.08923 free 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 free (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 35447010 W. Z. Wisniewski T. M. Michalowski A. W. Harris R. S. McMillan March 1995 Photoelectric Observations of 125 Asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1995LPI....26.1511W Abstracts of the Lunar and Planetary Science Conference 26 1511 1995LPI....26.1511W 27 September 2017 6 J. Durech M. Kaasalainen B. D. Warner M. Fauerbach S. A. Marks S. Fauvaud M. Fauvaud J.-M. Vugnon F. Pilcher L. Bernasconi R. Behrend January 2009 Asteroid models from combined sparse and dense photometric data https://www.aanda.org/articles/aa/pdf/2009/01/aa10393-08.pdf Astronomy and Astrophysics 493 1 291–297 2009A&A...493..291D 10.1051/0004-6361:200810393 24 August 2017 free 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 27 September 2017 6 A. Kryszczynska F. Colas M. Polinska R. Hirsch V. Ivanova G. Apostolovska B. Bilkina F. P. Velichko T. Kwiatkowski P. Kankiewicz F. Vachier V. Umlenski T. Michalowski A. Marciniak A. Maury K. Kaminski M. Fagas W. Dimitrov W. Borczyk K. Sobkowiak J. Lecacheux R. Behrend A. Klotz L. Bernasconi R. Crippa F. Manzini R. Poncy P. Antonini D. Oszkiewicz T. Santana-Ros October 2012 Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region Astronomy and Astrophysics 546 51 2012A&A...546A..72K 10.1051/0004-6361/201219199 free Macias, Amadeo Aznar January 2015 Asteroid Lightcurve Analysis at Isaac Aznar Observatory Aras De Los Olmos, Valencia, Spain http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015MPBu...42....4M The Minor Planet Bulletin 42 1 4–6 1052-8091 2015MPBu...42....4M 27 September 2017 Asteroid 1088 Mitaka Small Bodies Data Ferret https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1088+Mitaka 13 March 2020 https://web.archive.org/web/20201003195001/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1088+Mitaka 3 October 2020 dead Asteroid 1088 Mitaka – Proper Elements AstDyS-2, Asteroids – Dynamic Site https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1088 13 March 2020 External links Lightcurve Database Query (LCDB), at www.minorplanet.info 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 1088 1087 Arabis 1088 1089 Tama 001088 Category:Discoveries by Okuro Oikawa Category:Named minor planets 001088 001088 19271117