词条 | 1704 Wachmann |
释义 |
| minorplanet = yes | name = 1704 Wachmann | background = #D6D6D6 | image = 1704Wachmann (Lightcurve Inversion).png | image_size = 265px | caption = {{longitem|Light curve based 3D-model of Wachmann|style=padding: 5px 0;}} | discovery_ref = | discovered = 7 March 1924 | discoverer = K. Reinmuth | discovery_site = Heidelberg Obs. | mpc_name = (1704) Wachmann | alt_names = A924 EE{{·}}1947 CE 1957 BJ | pronounced = | named_after = Arno Wachmann {{small|(German astronomer)}}[2] | mp_category = main-belt{{·}}{{small|(inner)}} [3] | orbit_ref = | epoch = 4 September 2017 (JD 2458000.5) | uncertainty = 0 | observation_arc = 93.16 yr (34,026 days) | aphelion = 2.4163 AU | perihelion = 2.0292 AU | semimajor = 2.2228 AU | eccentricity = 0.0871 | period = 3.31 yr (1,210 days) | mean_anomaly = 67.047° | mean_motion = {{Deg2DMS|0.2974|sup=ms}} / day | inclination = 0.9715° | asc_node = 259.47° | arg_peri = 280.77° | dimensions = {{val|6.618|0.070}}[5] {{val|6.934|0.070}} km[6] 7.82 km {{small|(calculated)}}[3] | rotation = {{val|3.314|0.001}} h[8] | albedo = {{val|0.1767|0.0133}}[6] {{val|0.193|0.036}}[5] 0.20 {{small|(assumed)}}[3] | spectral_type = S [3] | abs_magnitude = 12.9[3]{{·}}{{val|12.97|0.13}}[15]{{·}}13.3[6] }}1704 Wachmann, provisional designation {{mp|A924 EE}}, is a stony asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered by German astronomer Karl Reinmuth at Heidelberg Observatory on 7 March 1924. It was later named after astronomer Arno Wachmann.[2][18] Classification and orbitThe S-type asteroid orbits the Sun in the inner main-belt at a distance of 2.0–2.4 AU once every 3 years and 4 months (1,210 days). Its orbit has an eccentricity of 0.09 and an inclination of 1° with respect to the ecliptic. No precoveries were taken. The asteroid's observation arc begins 3 days after its official discovery observation.[18] Physical characteristicsLightcurvesIn April 2007, a rotational lightcurve Wachmann was obtained at the U.S. Sandia View Observatory in New Mexico ({{small|H03}}). Lightcurve analysis gave a well-defined rotation period of {{val|3.314|0.001}} hours with a brightness variation of 0.40 magnitude ({{small|U=3}}).[8] Diameter and albedoAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Wachmann measures 6.6 and 6.9 kilometers in diameter, and its surface has an albedo of 0.177 and 0.193, respectively,[5][6] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 7.8 kilometers, based on an absolute magnitude of 12.9.[3] NamingThis minor planet was named for Arno Wachmann (1902–1990), long-time astronomer at the Bergedorf Observatory in Hamburg, discoverer of minor planets and comets, and observer of variable and binary stars. He is best known for the co-discovery of the three "Schwassmann–Wachmann" comets, 29P, 31P and 73P.[2] The official naming citation was published by the Minor Planet Center before November 1977 ({{small|M.P.C. 3933}}).[26] References1. ^1 2 3 {{cite book |title = Dictionary of Minor Planet Names – (1704) Wachmann |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |pages = 135–136 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1705 |chapter = (1704) Wachmann }} [1][2][3][4][5][6][7][8]2. ^1 2 {{cite web |title = 1704 Wachmann (A924 EE) |work = Minor Planet Center |url = http://www.minorplanetcenter.net/db_search/show_object?object_id=1704 |accessdate = 20 July 2016}} 3. ^1 {{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = http://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 20 July 2016}} 4. ^1 2 3 4 5 6 {{cite web |title = LCDB Data for (1704) Wachmann |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1704%7CWachmann |accessdate = 20 July 2016}} 5. ^1 2 3 4 {{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 }} 6. ^1 2 {{Cite journal |last = Julian, II |first = William M. |date = March 2008 |title = Period Determination for 1704 Wachmann |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2008MPBu...35....4J |journal = The Minor Planet Bulletin |volume = 35 |issue = 1 |page = 4 |issn = 1052-8091 |bibcode = 2008MPBu...35....4J |access-date= 20 July 2016}} 7. ^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= 20 July 2016}} 8. ^1 2 3 {{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 |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...791..121M |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 |access-date= 8 December 2016}} }} External links
5 : Background asteroids|Discoveries by Karl Wilhelm Reinmuth|Minor planets named for people|Named minor planets|Astronomical objects discovered in 1924 |
随便看 |
|
开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。