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1088 Mitaka
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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