词条 | (32496) 2000 WX182 |
释义 |
| minorplanet = yes | name = (32496) {{mp|2000 WX|182}} | background = #C2FFFF | image = | image_size = | caption = | discovery_ref = [1] | discoverer = LINEAR | discovery_site = Lincoln Lab's ETS | discovered = 18 November 2000 | mpc_name = (32496) {{mp|2000 WX|182}} | alt_names = {{mp|2000 WX|182}} | pronounced = | named_after = | mp_category = Jupiter trojan [1] {{nowrap|Trojan [5]{{·}}background [6]}} | orbit_ref = | epoch = 23 March 2018 (JD 2458200.5) | uncertainty = 0 | observation_arc = 63.36 yr (23,141 d) | aphelion = 5.6821 AU | perihelion = 4.8579 AU | semimajor = 5.2700 AU | eccentricity = 0.0782 | period = 12.10 yr (4,419 d) | mean_anomaly = 198.44° | mean_motion = {{Deg2DMS|0.0815|sup=ms}} / day | inclination = 30.465° | asc_node = 65.861° | arg_peri = 275.57° | jupiter_moid = 0.0682 AU | tisserand = 2.7170 | mean_diameter = {{val|48.02|0.903|ul=km}}[8] {{val|51.63|3.99|u=km}}[9] | rotation = {{val|23.34|0.01|ul=h}}[10]{{efn|name=lightcurve-plots-CS3}} | albedo = {{val|0.070|0.016}}[8] {{val|0.080|0.013}}[9] | spectral_type = C {{small|(assumed)}}[13] B–V {{=}} {{val|0.760|0.060}}[14] V–R {{=}} {{val|0.460|0.040}}[14] V–I {{=}} {{val|0.950|0.027}}[13] BR {{=}} {{val|1.230|0.039}}[13] | abs_magnitude = 9.80[9] 10.10[8] 10.2[1][13] }}{{mp|(32496) 2000 WX|182}}, provisional designation {{mp|2000 WX|182}}, is a Jupiter trojan from the Trojan camp, approximately {{convert|50|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. It was discovered on 18 November 2000, by astronomers with the LINEAR program at the Lincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States.[1] The dark Jovian asteroid belongs the 100 largest Jupiter trojans and has a rotation period of 23.3 hours. It has not been named since its numbering in November 2001.[24] Orbit and classification{{mp|2000 WX|182}} is a Jupiter trojan in a 1:1 orbital resonance with Jupiter. It is located in the trailering Trojan camp at the Gas Giant's {{L5}} Lagrangian point, 60° behind its orbit {{cross reference|(see Trojans in astronomy)}}.[5] It is also a non-family asteroid of the Jovian background population.[6] It orbits the Sun at a distance of 4.9–5.7 AU once every 12 years and 1 month (4,419 days; semi-major axis of 5.27 AU). Its orbit has an eccentricity of 0.08 and an inclination of 30° with respect to the ecliptic.The body's observation arc begins with a precovery published by the Digitized Sky Survey and taken at Palomar Observatory in January 1955, more than 45 years prior to its official discovery observation at Socorro.[1] Numbering and namingThis minor planet was numbered by the Minor Planet Center on 30 November 2001 ({{small|M.P.C. 44050}}).[24] As of 2018, it has not been named.[1] Physical characteristics{{mp|2000 WX|182}} is an assumed, carbonaceous C-type asteroid.[13] Most Jupiter trojans are D-types, with the reminder being mostly C and P-type asteroids. It has a typical V–I color index of 0.95 and a BR color of 1.23 (also see table below).[13]Rotation periodIn November 2013, a rotational lightcurve of {{mp|2000 WX|182}} was obtained from eleven nights of photometric observations by Robert Stephens at the Center for Solar System Studies in Landers, California. Lightcurve analysis gave a rotation period of {{val|23.34|0.01}} hours with a brightness amplitude of 0.19 magnitude ({{small|U=3-}}).[10][13]{{efn|name=lightcurve-plots-CS3}} Diameter and albedoAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and the Japanese Akari satellite, {{mp|2000 WX|182}} measures 48.02 and 51.63 kilometers in diameter and its surface has an albedo of 0.070 and 0.080, respectively.[8][9] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 50.77 kilometers based on an absolute magnitude of 10.2.[13] {{Largest Jupiter trojans}}Notes{{notelist|refs={{efn|name=lightcurve-plots-CS3|1=Lightcurve plots of (32496) 2000 WX182 from Nov 2013 by Robert Stephens at the Center for Solar System Studies {{Obscode|U81}}. Quality code is not available(lightcurve rating at CS3). Summary figures at the LCDB and CS3.}}}} References1. ^1 2 3 4 5 6 7 {{cite web |title = 32496 (2000 WX182) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=32496 |accessdate = 27 June 2018}} [1][2][3][4][5][6][7][8][9]2. ^1 2 {{cite web |title = List of Jupiter Trojans |work = Minor Planet Center |first3 = V. |last3 = Carruba |date = 1 June 2018 |url = https://www.minorplanetcenter.net/iau/lists/JupiterTrojans.html |accessdate = 27 June 2018}} 3. ^1 2 {{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 27 June 2018}} 4. ^1 2 3 4 {{cite journal |first1 = T. |last1 = Grav |first2 = A. K. |last2 = Mainzer |first3 = J. M. |last3 = Bauer |first4 = J. R. |last4 = Masiero |first5 = C. R. |last5 = Nugent |date = November 2012 |title = WISE/NEOWISE Observations of the Jovian Trojan Population: Taxonomy |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759...49G |journal = The Astrophysical Journal |volume = 759 |issue = 1 |page = 10 |bibcode = 2012ApJ...759...49G |doi = 10.1088/0004-637X/759/1/49 |arxiv = 1209.1549 |access-date= 27 June 2018}} (online catalog) 5. ^1 2 {{cite web |title = Asteroid (32496) 2000 WX182 – Proper Elements |publisher = AstDyS-2, Asteroids – Dynamic Site |url = http://hamilton.dm.unipi.it/astdys/index.php?n=32496&pc=1.1.6 |access-date= 27 June 2018}} 6. ^1 2 3 4 5 6 7 8 {{cite web |title = LCDB Data for (32496) |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=32496%7C |accessdate = 27 June 2018}} 7. ^1 2 {{Cite journal |first1 = Robert D. |last1 = Stephens |first2 = Linda M. |last2 = French |first3 = Chelsea |last3 = Davitt |first4 = Daniel R. |last4 = Coley |date = April 2014 |title = At the Scaean Gates: Observations Jovian Trojan Asteroids, July- December 2013 |url = http://articles.adsabs.harvard.edu/cgi-bin/nph-iarticle_query?2014MPBu...41...95S?data_type=PDF_HIGH |journal = The Minor Planet Bulletin |volume = 41 |issue = 2 |pages = 95–100 |issn = 1052-8091 |bibcode = 2014MPBu...41...95S |access-date= 27 June 2018}} 8. ^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= 27 June 2018}} (online, [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153]) 9. ^1 2 {{Cite journal |first1 = Joseph P. |last1 = Chatelain |first2 = Todd J. |last2 = Henry |first3 = Linda M. |last3 = French |first4 = Jennifer G. |last4 = Winters |first5 = David E. |last5 = Trilling |date = June 2016 |title = Photometric colors of the brightest members of the Jupiter L5 Trojan cloud |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016Icar..271..158C |journal = Icarus |volume = 271 |pages = 158–169 |bibcode = 2016Icar..271..158C |doi = 10.1016/j.icarus.2016.01.026 |access-date= 13 June 2016}} }} External links
5 : Jupiter trojans (Trojan camp)|Discoveries by LINEAR|Minor planets named from Greek mythology|Named minor planets|Astronomical objects discovered in 2000 |
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