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词条 1309 Hyperborea
释义

  1. Orbit and classification

  2. Physical characteristics

      Rotation period    Diameter and albedo  

  3. Naming

  4. References

  5. External links

{{Infobox planet
| minorplanet = yes
| name = 1309 Hyperborea
| background = #D6D6D6
| image =
| image_size =
| caption =
| discovery_ref =  
| discoverer = G. Neujmin
| discovery_site = Simeiz Obs.
| discovered = 11 October 1931
| mpc_name = (1309) Hyperborea
| alt_names = 1931 TO{{·}}1934 GT
{{mp|1971 SG|1}}{{·}}{{mp|1973 AW|4}}
A919 RB{{·}}A919 SH
| pronounced =
| named_after = Hyperborea [2]
{{small|(Greek mythology)}}
| mp_category = main-belt{{·}}{{small|(outer)}} [4]
background [5]
| orbit_ref =  
| epoch = 4 September 2017 (JD 2458000.5)
| uncertainty = 0
| observation_arc = 98.23 yr (35,880 days)
| aphelion = 3.6888 AU
| perihelion = 2.7251 AU
| semimajor = 3.2069 AU
| eccentricity = 0.1503
| period = 5.74 yr (2,098 days)
| mean_anomaly = 292.38°
| mean_motion = {{Deg2DMS|0.1716|sup=ms}} / day
| inclination = 10.279°
| asc_node = 206.08°
| arg_peri = 244.90°
| dimensions = {{val|55.14|14.34}} km[7]
{{val|55.48|13.26}} km[8]
57.11 km {{small|(derived)}}[4]
{{val|57.15|3.9}} km[10]
{{val|57.570|0.349}} km[11]
{{val|57.99|0.72}} km[12]
{{val|61.605|1.019}} km[13]
{{val|64.40|2.03}} km[14]
| rotation = {{val|13.858|0.004}} h[15]
{{val|13.87|0.002}}[15]
{{val|13.88|0.02}} h[17]
{{val|13.95|0.02}} h[18]
| albedo = {{val|0.03|0.02}}[7]
{{val|0.032|0.007}}[14]
{{val|0.0387|0.0054}}[13]
{{val|0.04|0.03}}[8]
0.0411 {{small|(derived)}}[4]
{{val|0.043|0.005}}[11]
{{val|0.044|0.001}}[12]
{{val|0.0450|0.007}}[10]
| spectral_type = C [4][28]
| abs_magnitude = 10.20[10][12][13]{{·}}10.30[4][14]{{·}}{{val|10.30|0.11}}[28]{{·}}10.40[7]{{·}}10.43[8]
}}1309 Hyperborea, provisional designation {{mp|1931 TO}}, 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.[38] The asteroid was named after Hyperborea, the northern homeland of a Greek mythical race of giants.[2]

Orbit and classification

Hyperborea is a non-family asteroid of the main belt's background population.[5] 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 {{mp|A919 RB}} in September 1919, or 12 years prior to its official discovery observation at Simeiz.[38]

Physical characteristics

Hyperborea has been characterized as a carbonaceous C-type asteroid by Pan-STARRS photometric survey.[28]

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 ({{small|U=2+/n.a./3/2}}).[15][17][18] The consolidated lightcurve gave a rotation period of 13.88 hours with a brightness amplitude between 0.34 and 0.41 magnitude.[4]

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.[7][8][10][11][12][13][14]

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.[4]

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 {{MoMP|1653|1653 Yakhontovia}}).[2]

References

1. ^{{cite book |title = Dictionary of Minor Planet Names – (1309) Hyperborea |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 107 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1310 |chapter = (1309) Hyperborea }}
2. ^{{cite web |title = 1309 Hyperborea (1931 TO) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1309 |accessdate = 15 December 2017}}
3. ^{{cite web |title = Asteroids and comets rotation curves – (1309) Hyperborea |last = Behrend |first = Raoul |publisher = Geneva Observatory |url = http://obswww.unige.ch/~behrend/page4cou.html#001309 |accessdate = 15 December 2017}}
4. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = T. |last2 = Grav |first3 = A. K. |last3 = Mainzer |first4 = C. R. |last4 = Nugent |first5 = J. M. |last5 = Bauer |first6 = R. |last6 = Stevenson |first7 = S. |last7 = Sonnett |date = August 2014 |title = Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos |journal = The Astrophysical Journal |volume = 791 |issue = 2 |page = 11 |bibcode = 2014ApJ...791..121M |doi = 10.1088/0004-637X/791/2/121 |arxiv = 1406.6645 }}
5. ^{{cite web |title = Small Bodies Data Ferret |work = Nesvorny HCM Asteroid Families V3.0 |url = https://sbntools.psi.edu/ferret/PropertySearch/familyForm.action |accessdate = 15 December 2017}}
6. ^{{cite web |title = LCDB Data for (1309) Hyperborea |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1309%7CHyperborea |accessdate = 15 December 2017}}
7. ^{{cite journal |display-authors = 6 |first1 = Fumihiko |last1 = Usui |first2 = Daisuke |last2 = Kuroda |first3 = Thomas G. |last3 = Müller |first4 = Sunao |last4 = Hasegawa |first5 = Masateru |last5 = Ishiguro |first6 = Takafumi |last6 = Ootsubo |first7 = Daisuke |last7 = Ishihara |first8 = Hirokazu |last8 = Kataza |first9 = Satoshi |last9 = Takita |first10 = Shinki |last10 = Oyabu |first11 = Munetaka |last11 = Ueno |first12 = Hideo |last12 = Matsuhara |first13 = Takashi |last13 = Onaka |date = October 2011 |title = Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey |url = http://pasj.oxfordjournals.org/content/63/5/1117.full.pdf+html |journal = Publications of the Astronomical Society of Japan |volume = 63 |issue = 5 |pages = 1117–1138 |bibcode = 2011PASJ...63.1117U |doi = 10.1093/pasj/63.5.1117 |access-date= 15 December 2017}}
8. ^{{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. K. |last2 = Mainzer |first3 = T. |last3 = Grav |first4 = J. M. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = C. |last6 = Nugent |first7 = M. S. |last7 = Cabrera |date = November 2012 |title = Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M |journal = The Astrophysical Journal Letters |volume = 759 |issue = 1 |page = 5 |bibcode = 2012ApJ...759L...8M |doi = 10.1088/2041-8205/759/1/L8 |arxiv = 1209.5794 |access-date= 15 December 2017}}
9. ^{{cite journal |display-authors = 6 |first1 = A. |last1 = Mainzer |first2 = T. |last2 = Grav |first3 = J. |last3 = Masiero |first4 = E. |last4 = Hand |first5 = J. |last5 = Bauer |first6 = D. |last6 = Tholen |first7 = R. S. |last7 = McMillan |first8 = T. |last8 = Spahr |first9 = R. M. |last9 = Cutri |first10 = E. |last10 = Wright |first11 = J. |last11 = Watkins |first12 = W. |last12 = Mo |first13 = C. |last13 = Maleszewski |date = November 2011 |title = NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 25 |bibcode = 2011ApJ...741...90M |doi = 10.1088/0004-637X/741/2/90 |arxiv = 1109.6407 }}
10. ^{{cite journal |first1 = E. F. |last1 = Tedesco |first2 = P. V. |last2 = Noah |first3 = M. |last3 = Noah |first4 = S. D. |last4 = Price |date = October 2004 |title = IRAS Minor Planet Survey V6.0 |url = https://sbn.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab |journal = NASA Planetary Data System |pages = IRAS-A-FPA-3-RDR-IMPS-V6.0 |bibcode = 2004PDSS...12.....T |access-date = 15 December 2017 |archive-url = https://web.archive.org/web/20160603231123/http://sbn.psi.edu/pds/asteroid/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab |archive-date = 2016-06-03 |dead-url = yes |df = }}
11. ^{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Bauer |first4 = R. M. |last4 = Cutri |first5 = E. A. |last5 = Kramer |first6 = T. |last6 = Grav |first7 = J. |last7 = Masiero |first8 = S. |last8 = Sonnett |first9 = E. L. |last9 = Wright |date = September 2016 |title = NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016AJ....152...63N |journal = The Astronomical Journal |volume = 152 |issue = 3 |page = 12 |bibcode = 2016AJ....152...63N |doi = 10.3847/0004-6256/152/3/63 |arxiv = 1606.08923 |access-date= 15 December 2017}}
12. ^{{cite journal |display-authors = 6 |first1 = C. R. |last1 = Nugent |first2 = A. |last2 = Mainzer |first3 = J. |last3 = Masiero |first4 = J. |last4 = Bauer |first5 = R. M. |last5 = Cutri |first6 = T. |last6 = Grav |first7 = E. |last7 = Kramer |first8 = S. |last8 = Sonnett |first9 = R. |last9 = Stevenson |first10 = E. L. |last10 = Wright |date = December 2015 |title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N |journal = The Astrophysical Journal |volume = 814 |issue = 2 |page = 13 |bibcode = 2015ApJ...814..117N |doi = 10.1088/0004-637X/814/2/117 |arxiv = 1509.02522 |access-date= 15 December 2017}}
13. ^{{Cite journal |first1 = Gordana |last1 = Apostolovska |first2 = Violeta |last2 = Ivanova |first3 = Galin |last3 = Borisov |date = June 2004 |title = Lightcurves and rotational periods of 1474 Beira, 1309 Hyperborea, and 2525 O'Steen |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2004MPBu...31...44A |journal = The Minor Planet Bulletin |volume = 31 |issue = 2 |pages = 44–45 |issn = 1052-8091 |bibcode = 2004MPBu...31...44A |access-date= 15 December 2017}}
14. ^{{Cite journal |first1 = Robert Lemke |last1 = Oliver |first2 = Heath |last2 = Shipley |first3 = Richard |last3 = Ditteon |date = October 2008 |title = Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2008 March |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35..149O |journal = The Minor Planet Bulletin |volume = 35 |issue = 4 |pages = 149–150 |issn = 1052-8091 |bibcode = 2008MPBu...35..149O |access-date= 15 December 2017}}
15. ^{{cite journal |display-authors = 6 |first1 = Peter |last1 = Veres |first2 = Robert |last2 = Jedicke |first3 = Alan |last3 = Fitzsimmons |first4 = Larry |last4 = Denneau |first5 = Mikael |last5 = Granvik |first6 = Bryce |last6 = Bolin |first7 = Serge |last7 = Chastel |first8 = Richard J. |last8 = Wainscoat |first9 = William S. |last9 = Burgett |first10 = Kenneth C. |last10 = Chambers |first11 = Heather |last11 = Flewelling |first12 = Nick |last12 = Kaiser |first13 = Eugen A. |last13 = Magnier |first14 = Jeff S. |last14 = Morgan |first15 = Paul A. |last15 = Price |first16 = John L. |last16 = Tonry |first17 = Christopher |last17 = Waters |date = November 2015 |title = Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015Icar..261...34V |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 15 December 2017}}
[1][2][3][4][5][6][7][8][9][10][11][12][13][14][15]

}}

External links

  • (1309) Hyperborea at AstDyS-2
  • Asteroid Lightcurve Database (LCDB), query form (info)
  • [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • {{JPL small body}}
{{Minor planets navigator |1308 Halleria |number=1309 |1310 Villigera}}{{Small Solar System bodies}}{{DEFAULTSORT:Hyperborea}}

5 : Background asteroids|Discoveries by Grigory Neujmin|Minor planets named from Greek mythology|Named minor planets|Astronomical objects discovered in 1931

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