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1146 Biarmia
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Metallic main-belt asteroid
October 2019
yes
1146 Biarmia
#D6D6D6
G. Neujmin
Simeiz Obs.
7 May 1929
(1146) Biarmia
1929 JF1941 WD 1A913 KA
b i ' ɑr m i ə'Biarmian' in Eduard Muret (1891) Encyclopædic English–German and German–English Dictionary
Bjarmaland (Permia)(territory in Norse sagas)
main-belt(outer)
4 September 2017 (JD 2458000.5)
0
87.88 yr (32,098 days)
3.8212 AU
2.2678 AU
3.0445 AU
0.2551
5.31 yr (1,940 days)
184.40°
0.1855 ms / day
17.067°
213.89°
63.801°
21.59 1.52 km31.14 1.2 km32.39 0.97 km32.925 0.148 km38.567 0.735 km
5.33 0.01 h5.468 0.004 h5.4700 0.0002 hlightcurve-plot11.514 0.004 h21.6 h (retracted)lcdb-Behrend 2008
0.1436 0.01470.196 0.0240.219 0.0150.2190 0.0180.455 0.096
Tholen XMB–V 0.690U–B 0.247
9.809.99 0.33
1146 Biarmia, provisional designation 1929 JF, is a metallic background asteroid from the outer regions of the asteroid belt, approximately 32 kilometers in diameter. It was discovered on 7 May 1929, by Russian astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula. The asteroid was named for the Bjarmaland mentioned in Norse sagas.
Orbit and classification
Biarmia is not a member of any known asteroid family. It orbits the Sun in the outer main-belt at a distance of 2.3–3.8 AU once every 5 years and 4 months (1,940 days). Its orbit has an eccentricity of 0.26 and an inclination of 17° with respect to the ecliptic.
The asteroid was first identified as A913 KA at Winchester Observatory (799) in June 1913. The body's observation arc begins with its official discovery observation at Simeiz.
Physical characteristics
Biarmia has been characterized in several observations as a metallic M-type asteroid. In the Tholen classification, it is an X-type asteroid which also includes the M-types as a subgroup.
Rotation period
The best-rated rotational lightcurves of Biarmia were obtained from photometric observations at the Etscorn Observatory (719), New Mexico, and at the S.O.S. Observatory (H39) in Minnesota, United States. Lightcurve analysis gave a rotation period of 5.468 and 5.4700 hours with a brightness amplitude of 0.22 and 0.20 magnitude, respectively (U=3/3).lightcurve-plot
Other observations received a lower rating or have since been retracted.lcdb-Behrend 2008 Warner's period of 11.514 hours was later revised to 5.33 (U=2).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, Biarmia measures between 21.59 and 38.567 kilometers in diameter and its surface has an albedo between 0.1436 and 0.455.
The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, a stony albedo of 0.2190 and a diameter of 31.14 kilometers based on an absolute magnitude of 9.80.
Naming
This minor planet was named for the Bjarmaland mentioned in Norse sagas. This legendary territory probably refers to the Russian region around Arkhangelsk on the White Sea near the Finnish border. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 107).
Notes
lightcurve-plot Lightcurve plot of 1146 Biarmia with a period of 5.47 hours. Brian D. Warner. Note by Warner: "Originally reported in MPB 27, 4-6 with P = 11.514 and A = 0.32. Reanalysis found revised period of P = 5.33, which disagrees with the 5.47 found by Durkee. The curve above is plotted to the Durkee period, which does give a better fit than with 5.33 h."
lcdb-Behrend 2008 Behrend (2008) web: obs. date: 27 January 2008. Rotation period 21.6 hours with a brightness amplitude of 0.07 mag. Summary figures for (1146) Biarmia at Collaborative Asteroid Lightcurve Link (CALL). Lightcurve was removed from website by Raoul Behrend.
References
30em 2017-03-24 last obs.
JPL Small-Body Database Browser: 1146 Biarmia (1929 JF)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001146
https://web.archive.org/web/20200810194756/https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001146
10 August 2020
Jet Propulsion Laboratory
8 September 2017
Dictionary of Minor Planet Names – (1146) Biarmia
Schmadel Lutz D.
Springer Berlin Heidelberg
97
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1147 (1146) Biarmia
1146 Biarmia (1929 JF)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1146
8 September 2017
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
The Astrophysical Journal
791
2
11
2014ApJ...791..121M
10.1088/0004-637X/791/2/121
1406.6645
1146
8 September 2017
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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
The Astrophysical Journal Letters
759
1
5
2012ApJ...759L...8M
10.1088/2041-8205/759/1/L8
1209.5794
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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)
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P. V. Noah
M. Noah
S. D. Price
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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
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J. Masiero
E. Hand
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D. Tholen
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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
Warner, B.
March 2000
Asteroid Photometry at the Palmer Divide Observatory
The Minor Planet Bulletin
27
4–6
2000MPBu...27....4W
Durkee, Russell I.
October 2009
The Lightcurves of 1146 Biarmia and 5598 Carlmurray
The Minor Planet Bulletin
36
4
170
1052-8091
2009MPBu...36..170D
Warner, Brian D.
January 2011
Upon Further Review: III. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory
The Minor Planet Bulletin
38
1
21–23
1052-8091
2011MPBu...38...21W
Daniel A. III Klinglesmith
Jesse Hanowell
Curtis Alan Warren
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Lightcurves for Inversion Model Candidates
The Minor Planet Bulletin
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4
206–208
1052-8091
2014MPBu...41..206K
6
I. N. Belskaya
S. Fornasier
G. P. Tozzi
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A. Cellino
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Yu. N. Krugly
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S. Faggi
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Icarus
284
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2017Icar..284...30B
10.1016/j.icarus.2016.11.003
11336/63617
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1105.3380
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Peter Veres
Robert Jedicke
Alan Fitzsimmons
Larry Denneau
Mikael Granvik
Bryce Bolin
Serge Chastel
Richard J. Wainscoat
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261
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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
1146
1145 Robelmonte 1146 1147 Stavropolis
001146
Category:Discoveries by Grigory Neujmin
Category:Named minor planets
001146
19290507