411 REFERENCE · Wikipedia
1467 Mashona
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Asteroid
October 2019
yes
1467 Mashona
#D6D6D6
30 July 1938
C. Jackson
Johannesburg Obs.
(1467) Mashona
1938 OE1930 DL1936 DK1936 FA 11948 EGA923 CB
Shona people (Mashona)(natives of Mashonaland)
main-belt(outer)
4 September 2017 (JD 2458000.5)
0
94.41 yr (34,483 days)
3.8268 AU
2.9485 AU
3.3877 AU
0.1296
6.24 yr (2,277 days)
255.30°
0.1581 ms / day
21.910°
326.50°
349.55°
89.160 0.728 km90.93 28.77 km95.08 1.30 km104.119 1.062 km107.54 km (calculated)
9.740 0.0029 h9.744 0.001 h9.76 h
0.05 0.030.057 (assumed)0.0609 0.01110.074 0.0020.083 0.014
Tholen = GCGCB–V = 0.743U–B = 0.373
8.515 0.001 (R)8.57
1467 Mashona, provisional designation 1938 OE, is a rare-type carbonaceous asteroid from the outer regions of the asteroid belt, approximately 100 kilometers in diameter, making it one of the top 200 largest asteroids currently known to exist. It was discovered on 30 July 1938, by South African astronomer Cyril Jackson at the Johannesburg Observatory in South Africa. It was later named after the native Shona people of Zimbabwe.
Classification and orbit
Mashona orbits the Sun in the outer main-belt at a distance of 2.9–3.8 AU once every 6 years and 3 months (2,277 days). Its orbit has an eccentricity of 0.13 and an inclination of 22° with respect to the ecliptic. It is a member of the Cybele asteroid group.
In February 1923, it was first identified as 1923 CB at Heidelberg Observatory in Germany. The body's observation arc begins at Johannesburg, 5 days after its official discovery observation.
Mashona was the highest numbered asteroid used in calculating the future orbit of 101955 Bennu.
Physical characteristics
In the Tholen classification, Mashona is a rare GC-type, a spectral type that transitions between the common C and rare G-type asteroids.
Lightcurves
Until April 2010, three rotational lightcurves of Mashona have been obtained from photometric observations. Lightcurve analysis gave a well-defined rotation period between 9.74 and 9.76 hours with a brightness amplitude varying from 0.24 to 0.31 magnitude (U=3/2/3).
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Mashona measures between 89.160 and 104.119 kilometers in diameter and its surface has an albedo between 0.05 and 0.083. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 107.54 kilometers based on an absolute magnitude of 8.57. Among nearly half a million asteroids, Mashona belongs to the 200 largest bodies.
Naming
This minor planet was named for the Shona people (Mashona), natives of Mashonaland in Zimbabwe, then Rhodesia. The official 1467 naming citation was published by the Minor Planet Center in April 1953 (M.P.C. 909).
References
2017-07-05 last obs.
JPL Small-Body Database Browser: 1467 Mashona (1938 OE)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001467
Jet Propulsion Laboratory
24 July 2017
Dictionary of Minor Planet Names – (1467) Mashona
Schmadel Lutz D.
Springer Berlin Heidelberg
117
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1468 (1467) Mashona
1467 Mashona (1938 OE)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1467
24 July 2017
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
2009
https://archive.org/details/dictionaryminorp2008schm
limited
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
Asteroids and comets rotation curves – (1467) Mashona
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001467
24 July 2017
3 August 2003
https://web.archive.org/web/20030803183423/http://obswww.unige.ch/~behrend/page4cou.html#001467
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
24 July 2017
The largest asteroids and outer solar system objects
Wm. Robert Johnston
Johnston's Archive
http://www.johnstonsarchive.net/astro/largestasteroids.html
7 February 2015
24 July 2017
1467
24 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
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
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
24 July 2017
Claes-Ingvar Lagerkvist
Anders Erikson
Felix Lahulla
Mario De Martino
Andreas Nathues
Mats Dahlgren
January 2001
A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2001Icar..149..190L
Icarus
149
1
190–197
2001Icar..149..190L
10.1006/icar.2000.6507
24 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
24 July 2017
A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids
Lagerkvist Claes-Ingvar
Erikson Anders
Lahulla Felix
De Martino Mario
Nathues Andreas
Dahlgren Mats
1
Icarus
149
1
190–197
January 2001
10.1006/icar.2000.6507
2001Icar..149..190L
.
Farnocchia Davide Chesley Steven R. Takahashi Yu
Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data
Icarus 2021
10.1016/j.icarus.2021.114594 free
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
1467
1466 Mündleria 1467 1468 Zomba
001467
Category:Discoveries by Cyril Jackson (astronomer)
Category:Named minor planets
001467
19380730