| 词条 | 806 Gyldénia |
| 释义 |
| minorplanet = yes | name = 806 Gyldénia | background = #D6D6D6 | image = | caption = | discovery_ref = | discovered = 18 April 1915 | discoverer = M. F. Wolf | discovery_site = Heidelberg Obs. | mpc_name = (806) Gyldénia | alt_names = 1915 WX{{·}}1950 LT | named_after = Hugo Gyldén {{small|(astronomer)}}[2] | mp_category = main-belt{{·}}{{small|(outer)}} | orbit_ref = | epoch = 16 February 2017 (JD 2457800.5) | uncertainty = 0 | observation_arc = 101.57 yr (37,097 days) | aphelion = 3.4506 AU | perihelion = 2.9678 AU | semimajor = 3.2092 AU | eccentricity = 0.0752 | period = 5.75 yr (2,100 days) | mean_anomaly = 280.53° | mean_motion = {{Deg2DMS|0.1714|sup=ms}} / day | inclination = 14.240° | asc_node = 43.987° | arg_peri = 119.50° | dimensions = {{val|62.63|1.3}} km {{small|(IRAS:14)}}[5] 62.78 km {{small|(derived)}}[6] {{val|67.79|0.89}} km[7] {{val|83.10|0.74}} km[8] | rotation = {{val|14.45|0.05}} h[9] {{val|14.452|0.001}} h[9] {{val|16.846|0.007}} h[11] {{val|16.852|0.006}} h[12] {{val|16.8537|0.0094}} h[13] | albedo = {{val|0.022|0.001}}[7] {{val|0.023|0.004}}[8] {{val|0.0259|0.001}} {{small|(IRAS:14)}}[5] 0.0373 {{small|(derived)}}[6] | spectral_type = C [6] | abs_magnitude = {{val|9.953|0.002}} {{small|(R)}}[13]{{·}}10.10[8]{{·}}10.2[6]{{·}}{{val|10.55|0.22}}[23]{{·}}10.6[5][7] }}806 Gyldénia, provisional designation {{mp|1915 WX}}, is a carbonaceous asteroid from the outer region of the asteroid belt, approximately 63 kilometers in diameter. It was discovered on 18 April 1915, by German astronomer Max Wolf at Heidelberg Observatory in southern Germany.[26] The discovery observation was ignored for orbital determination, with the first used observation made at Vienna Observatory on 1 May 2015, reducing the asteroid's observation arc by 2 weeks.[26] The dark C-type asteroid orbits the Sun at a distance of 3.0–3.5 AU once every 5 years and 9 months (2,100 days). Its orbit has an eccentricity of 0.08 and an inclination of 14° with respect to the ecliptic. Several photometric light-curve analysis rendered a rotation period of {{val|16.852|0.006}} hours (best result) with a brightness variation of 0.18 in magnitude ({{small|U=3}}).[12] According to the surveys carried out by the Infrared Astronomical Satellite, IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the asteroid's surface has a notably low albedo of less than 0.03, while the Collaborative Asteroid Lightcurve Link derived a somewhat higher value of 0.04.[5][7][8][6] The minor planet was named in honor of the Fenno-Swedish astronomer Hugo Gyldén (1841–1896), who was a director of the Stockholm Observatory. He developed a new technique to calculate the perturbations of planets and comets. The lunar crater Gyldén is also named after the astronomer ({{small|H 80}})[2] References1. ^1 2 {{cite book |title = Dictionary of Minor Planet Names – (806) Gyldénia |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 75 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_807 |chapter = (806) Gyldénia }} [1][2][3][4][5][6][7][8][9][10][11]2. ^1 2 {{cite web |title = 806 Gyldenia (1915 WX) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=806 |accessdate = 4 July 2016}} 3. ^1 2 {{cite web |title = Asteroids and comets rotation curves – (806) Gyldenia |last = Behrend |first = Raoul |publisher = Geneva Observatory |url = http://obswww.unige.ch/~behrend/page3cou.html#000806 |accessdate = 4 July 2016}} 4. ^1 2 3 4 5 {{cite web |title = LCDB Data for (806) Gyldenia |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=806%7CGyldenia |accessdate = 4 July 2016}} 5. ^1 2 3 4 {{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 = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2004PDSS...12.....T |journal = NASA Planetary Data System |volume = 12 |pages = IRAS-A-FPA-3-RDR-IMPS-V6.0 |bibcode = 2004PDSS...12.....T |access-date= 4 July 2016}} 6. ^1 2 3 4 {{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://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011PASJ...63.1117U |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= 4 July 2016}} 7. ^1 2 3 4 {{cite journal |display-authors = 6 |first1 = Joseph R. |last1 = Masiero |first2 = A. 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5 : Background asteroids|Discoveries by Max Wolf|Minor planets named for people|Named minor planets|Astronomical objects discovered in 1915 |
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