词条 | 1014 Semphyra |
释义 |
| minorplanet = yes | name = 1014 Semphyra | background = #D6D6D6 | image = | image_size = | caption = | discovery_ref = | discoverer = K. Reinmuth | discovery_site = Heidelberg Obs. | discovered = 29 January 1924 | mpc_name = (1014) Semphyra | alt_names = 1924 PW{{·}}1932 WH {{mp|1984 YP|6}} | pronounced = | named_after = figure in poem by Aleksandr Pushkin [2] | mp_category = main-belt{{·}}{{small|(middle)}} [3] | orbit_ref = | epoch = 4 September 2017 (JD 2458000.5) | uncertainty = 0 | observation_arc = 93.02 yr (33,975 days) | aphelion = 3.3624 AU | perihelion = 2.2443 AU | semimajor = 2.8034 AU | eccentricity = 0.1994 | period = 4.69 yr (1,714 days) | mean_anomaly = 332.39° | mean_motion = {{Deg2DMS|0.2100|sup=ms}} / day | inclination = 2.2681° | asc_node = 251.71° | arg_peri = 233.24° | dimensions = {{val|14.89|3.58}} km[5] {{val|17.17|0.88}} km[6] {{val|17.487|0.250}} km[7][8] 23.21 km {{small|(calculated)}}[3] | rotation = {{val|5.636|0.002}} h[10] | albedo = 0.057 {{small|(assumed)}}[3] {{val|0.083|0.013}}[7] {{val|0.0835|0.0130}}[8] {{val|0.087|0.009}}[6] {{val|0.12|0.06}}[5] | spectral_type = SMASS {{=}} Xe {{·}}P [8]{{·}}X [3] | abs_magnitude = 11.90[3][5]{{·}}{{val|12.04|0.15}}[22]{{·}}12.10[6][8] }}1014 Semphyra, provisional designation {{mp|1924 PW}}, is a background asteroid from the central regions of the asteroid belt, approximately 17 kilometers in diameter. It was discovered on 29 January 1924, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany.[25] The asteroid was named after the character "Semphyra" in a poem by Aleksandr Pushkin.[2] Orbit and classificationSemphyra has not been associated with any known asteroid family. It orbits the Sun in the central main belt at a distance of 2.2–3.4 AU once every 4 years and 8 months (1,714 days). Its orbit has an eccentricity of 0.20 and an inclination of 2° with respect to the ecliptic.The body's observation arc begins with its official discovery observation at Heidelberg.[25] Physical characteristicsin the SMASS classification, Semphyra is an Xe-subtype that transitions from the X-type to the bright E-type asteroids, while the Wide-field Infrared Survey Explorer characterizes it as a dark P-type.[3][8] Rotation periodIn February 2004, a rotational lightcurve of Semphyra was obtained from photometric observations by American astronomer Donald Pray at the Carbuncle Hill Observatory, Rhode Island ({{small|I00}}). The observations were made at a low phase angle of 1.6–2.9°. Lightcurve analysis gave a well-defined rotation period of 5.636 hours with a brightness amplitude of 0.12 magnitude ({{small|U=3}}), indicating that the body has a rather spheroidal shape.[10] Diameter and albedoAccording to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's WISE, Semphyra measures between 14.89 and 17.487 kilometers in diameter and its surface has an albedo between 0.083 and 0.12.[5][6][7][8] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 23.21 kilometers based on an absolute magnitude of 11.9.[3] NamingThis minor planet was named after the character "Semphyra" in a poem by Russian Aleksandr Pushkin (1799–1837), who was directly honored with the naming of {{MoMP|2208|(2208)}}. The asteroid's official name was proposed by N. Komendantov ({{small|RI 740}}) and mentioned in The Names of the Minor Planets by Paul Herget in 1955 ({{small|H 97}}).[2] References1. ^1 2 3 {{cite book |title = Dictionary of Minor Planet Names – (1014) Semphyra |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 87 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1015 |chapter = (1014) Semphyra }} [1][2][3][4][5][6][7][8][9]2. ^1 2 {{cite web |title = 1014 Semphyra (1924 PW) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1014 |accessdate = 29 August 2017}} 3. ^1 2 3 {{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 = J. |last6 = Dailey |first7 = P. R. M. |last7 = Eisenhardt |first8 = R. S. |last8 = McMillan |first9 = T. B. |last9 = Spahr |first10 = M. F. |last10 = Skrutskie |first11 = D. |last11 = Tholen |first12 = R. G. |last12 = Walker |first13 = E. L. |last13 = Wright |first14 = E. |last14 = DeBaun |first15 = D. |last15 = Elsbury |first16 = T., IV |last16 = Gautier |first17 = S. |last17 = Gomillion |first18 = A. |last18 = Wilkins |date = November 2011 |title = Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M |journal = The Astrophysical Journal |volume = 741 |issue = 2 |page = 20 |bibcode = 2011ApJ...741...68M |doi = 10.1088/0004-637X/741/2/68 |arxiv = 1109.4096 |access-date= 29 August 2017}} 4. ^1 2 3 4 5 6 7 {{cite web |title = LCDB Data for (1014) Semphyra |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1014%7CSemphyra |accessdate = 29 August 2017}} 5. ^1 2 3 4 {{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= 29 August 2017}} 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://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= 29 August 2017}} 7. ^1 2 3 4 5 6 {{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 }} 8. ^1 2 {{Cite journal |author = Pray, Donald P. |date = March 2005 |title = Lightcurve analysis of asteroids 276, 539, 1014, 1067, 3693 and 4774 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005MPBu...32....8P |journal = The Minor Planet Bulletin |volume = 32 |issue = 1 |pages = 8–9 |issn = 1052-8091 |bibcode = 2005MPBu...32....8P |access-date= 29 August 2017}} 9. ^1 {{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= 29 August 2017}} }} External links
8 : Background asteroids|Discoveries by Karl Wilhelm Reinmuth|Astronomical objects discovered in 1924|Minor planets named for fictional characters|Minor planets named from literature|Named minor planets|Alexander Pushkin|Xe-type asteroids (SMASS) |
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