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1309 Hyperborea
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Carbonaceous background asteroid
October 2019
yes
1309 Hyperborea
#D6D6D6
G. Neujmin
Simeiz Obs.
11 October 1931
(1309) Hyperborea
1931 TO1934 GT1971 SG 11973 AW 4A919 RBA919 SH
h aɪ p ər ˈ b ɔər iː əhyperborean
Hyperborea(Greek mythology)
main-belt(outer)background
4 September 2017 (JD 2458000.5)
0
98.23 yr (35,880 days)
3.6888 AU
2.7251 AU
3.2069 AU
0.1503
5.74 yr (2,098 days)
292.38°
0.1716 ms / day
10.279°
206.08°
244.90°
55.14 14.34 km55.48 13.26 km57.11 km (derived)57.15 3.9 km57.570 0.349 km57.99 0.72 km61.605 1.019 km64.40 2.03 km
13.858 0.004 h13.87 0.00213.88 0.02 h13.95 0.02 h
0.03 0.020.032 0.0070.0387 0.00540.04 0.030.0411 (derived)0.043 0.0050.044 0.0010.0450 0.007
C
10.2010.3010.30 0.1110.4010.43
1309 Hyperborea h aɪ p ər ˈ b ɔər iː ə is a carbonaceous background asteroid from the outermost regions of the asteroid belt, approximately 57 kilometers in diameter. It was discovered on 11 October 1931, by Soviet astronomer Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula, and given the provisional designation 1931 TO. The asteroid was named after Hyperborea, the northern homeland of a Greek mythical race of giants.
Orbit and classification
Hyperborea is a non-family asteroid of the main belt's background population. It orbits the Sun in the outermost asteroid belt at a distance of 2.7–3.7 AU once every 5 years and 9 months (2,098 days; semi-major axis of 3.21 AU). Its orbit has an eccentricity of 0.15 and an inclination of 10° with respect to the ecliptic.
The body's observation arc begins at Heidelberg Observatory with its first observations as A919 RB in September 1919, or 12 years prior to its official discovery observation at Simeiz.
Physical characteristics
Hyperborea has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey.
Rotation period
Between 2002 and 2017, four rotational lightcurves of Hyperborea were obtained from photometric observations by astronomers Francisco Sold and Pierre Antonini, as well as by astronomers at the Oakley Southern Sky and Rozhen Observatory in Australia and Bulgaria, respectively (U=2+/n.a./3/2). The consolidated lightcurve gave a rotation period of 13.88 hours with a brightness amplitude between 0.34 and 0.41 magnitude.
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, Hyperborea measures between 55.14 and 64.40 kilometers in diameter and its surface has an albedo between 0.03 and 0.0450.
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0411 and a diameter of 57.11 kilometers based on an absolute magnitude of 10.3.
Naming
This minor planet was named after Hyperborea, the homeland of the Hyperboreans, a Greek mythical race of giants associated with the cult of Apollo. Herodotus placed the region far to the north of Thrace beyond the North Wind. It was therefore believed to be a region of perpetual sunshine. Lutz Schmadel, the author of the Dictionary of Minor Planets, learned about the naming from Russian astronomer Nataliya Sergeevna Samoilova-Yakhontova (see 1653 1653 Yakhontovia).
References
30em 2017-11-25 last obs.
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https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001309
Jet Propulsion Laboratory
15 December 2017
Dictionary of Minor Planet Names – (1309) Hyperborea
Schmadel Lutz D.
Springer Berlin Heidelberg
107
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10.1007/978-3-540-29925-7_1310 (1309) Hyperborea
1309 Hyperborea (1931 TO)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1309
15 December 2017
Asteroids and comets rotation curves – (1309) Hyperborea
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001309
15 December 2017
3 August 2003
https://web.archive.org/web/20030803183423/http://obswww.unige.ch/~behrend/page4cou.html#001309
dead
6
Joseph R. Masiero
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The Astrophysical Journal
791
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2014ApJ...791..121M
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Asteroid 1309 Hyperborea – Proper Elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1309
29 October 2019
1309
15 December 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
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Publications of the Astronomical Society of Japan
63
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http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
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6
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741
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1109.6407 35447010
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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
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22 October 2019
6
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The Astronomical Journal
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3
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C. R. Nugent
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814
2
13
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1509.02522
9341381 15 December 2017
Gordana Apostolovska
Violeta Ivanova
Galin Borisov
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Lightcurves and rotational periods of 1474 Beira, 1309 Hyperborea, and 2525 O'Steen
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2004MPBu...31...44A
The Minor Planet Bulletin
31
2
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35
4
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6
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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
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External links
(1309) Hyperborea at AstDyS-2
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
1309
1308 Halleria 1309 1310 Villigera
001309
Category:Discoveries by Grigory Neujmin
Category:Named minor planets
19311011
Category:Hyperborea