词条 | 3596 Meriones |
释义 |
| minorplanet = yes | name = 3596 Meriones | background = #C2FFFF | image = | image_size = | caption = | discovery_ref = [1] | discoverer = P. Jensen K. Augustesen | discovery_site = Brorfelde Obs. | discovered = 14 November 1985 | mpc_name = (3596) Meriones | alt_names = 1985 VO{{·}}{{mp|1950 TR|4}} {{mp|1973 SS|5}} | pronounced = {{IPAc-en|m|ə|ˈ|r|aɪ|oʊ-|n|iː|z}} {{Respell|mə|RY|o|neez}} | named_after = Meriones [1] {{small|(Greek mythology)}} | mp_category = Jupiter trojan [1][5] {{nowrap|Greek [6][7]{{·}}background [7]}} | orbit_ref = | epoch = 23 March 2018 (JD 2458200.5) | uncertainty = 0 | observation_arc = 67.61 yr (24,694 d) | aphelion = 5.5464 AU | perihelion = 4.7927 AU | semimajor = 5.1695 AU | eccentricity = 0.0729 | period = 11.75 yr (4,293 d) | mean_anomaly = 240.42° | mean_motion = {{Deg2DMS|0.0839|sup=ms}} / day | inclination = 23.530° | asc_node = 356.68° | arg_peri = 66.541° | jupiter_moid = 0.0446 AU | tisserand = 2.8290 | mean_diameter = {{val|73.28|1.91|ul=km}}[10] {{val|87.38|1.09|u=km}}[11] | rotation = {{val|12.96|ul=h}}[12] | albedo = {{val|0.048|0.008}}[11] {{val|0.064|0.004}}[10] | spectral_type = C {{small|(assumed)}}[5] V–I {{=}} {{val|0.830|0.057}}[5] | abs_magnitude = 9.2[1][11] 9.30[10] 9.35[5][12] }}3596 Meriones ({{IPAc-en|m|ə|ˈ|r|aɪ|oʊ-|n|iː|z}} {{Respell|mə|RY|o|neez}}), provisional designation {{mp|1985 VO}}, is a large Jupiter trojan from the Greek camp, approximately {{convert|80|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. It was discovered on 14 November 1985, by Danish astronomers Poul Jensen and Karl Augustesen at the Brorfelde Observatory near Holbæk, Denmark.[1] The assumed C-type asteroid belongs to the 50 largest Jupiter trojans and has a rotation period of 12.96 hours.[5] It was named after the Cretan leader Meriones from Greek mythology.[1] Orbit and classificationMeriones is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's {{L4}} Lagrangian point, 60° ahead of the Gas Giant's orbit in a 1:1 resonance (see Trojans in astronomy). It is also a non-family asteroid in the Jovian background population.[7]It orbits the Sun at a distance of 4.8–5.5 AU once every 11 years and 9 months (4,293 days; semi-major axis of 5.17 AU). Its orbit has an eccentricity of 0.07 and an inclination of 24° with respect to the ecliptic. The body's observation arc begins with a precovery taken at Uccle Observatory in October 1950, or 35 years prior to its official discovery observation at Brorfelde.[1] NamingThis minor planet was named from Greek mythology after Meriones, who co-commanded together with the Greek hero Idomeneus the Cretan contingent in the Trojan War, where they slew many Trojans, especially in the Battle of the Ships.[1] The official naming citation was published by the Minor Planet Center on 7 September 1987 ({{small|M.P.C. 12211}}).[30] Physical characteristicsMeriones is an assumed, carbonaceous C-type asteroid.[5]Rotation periodIn 1991, a rotational lightcurve of Meriones was published by German and Italian astronomers. Lightcurve analysis of the photometric observations gave a rotation period of 12.96 hours with a brightness amplitude of 0.15 magnitude ({{small|U=2}}).[5][12] Diameter and albedoAccording to the surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Meriones measures 73.28 and 87.38 kilometers in diameter and its surface has an albedo of 0.064 and 0.048, respectively.[10][11] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057, and derives a diameter of 75.09 kilometers based on an absolute magnitude of 9.35.[5] {{Largest Jupiter trojans}}References1. ^1 2 3 4 5 6 7 8 {{cite web |title = 3596 Meriones (1985 VO) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=3596 |accessdate = 6 June 2018}} [1][2][3][4][5][6][7][8]2. ^1 {{cite web |title = List of Jupiter Trojans |work = Minor Planet Center |date = 30 May 2018 |url = https://www.minorplanetcenter.net/iau/lists/JupiterTrojans.html |accessdate = 6 June 2018}} 3. ^1 {{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 6 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 = https://arxiv.org/pdf/1209.1549.pdf |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= 9 June 2018}} (online catalog) 5. ^1 2 3 {{cite web |title = Asteroid (3596) Meriones – Proper elements |publisher = AstDyS-2, Asteroids – Dynamic Site |url = http://hamilton.dm.unipi.it/astdys/index.php?n=3596&pc=1.1.6 |accessdate = 6 June 2018}} 6. ^1 2 3 4 5 6 7 8 {{cite web |title = LCDB Data for (3596) Meriones |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=3596%7CMeriones |accessdate = 6 June 2018}} 7. ^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= 15 June 2018}} (online, [https://core.ac.uk/download/pdf/43545172.pdf AcuA catalog p. 153]) 8. ^1 2 3 {{Cite journal |first1 = M. |last1 = Gonano |first2 = M. |last2 = di Martino |first3 = S. |last3 = Mottola |first4 = G. |last4 = Neukum |date = December 1990 |title = Physical study of outer belt asteroids |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1991AdSpR..11..197G |journal = Space dust and debris; Proceedings of the Topical Meeting of the Interdisciplinary Scientific Commission B /Meetings B2 |pages = 197–200 |issn = 0273-1177 |bibcode = 1991AdSpR..11..197G |doi = 10.1016/0273-1177(91)90563-Y |access-date= 6 June 2018}} }} External links
6 : Jupiter trojans (Greek camp)|Discoveries by Poul Jensen|Discoveries by Karl Augustesen|Minor planets named from Greek mythology|Named minor planets|Astronomical objects discovered in 1985 |
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