| 词条 | 5012 Eurymedon |
| 释义 |
| minorplanet = yes | name = 5012 Eurymedon | background = #C2FFFF | image = | image_size = | caption = | discovery_ref = [1] | discoverer = C. J. van Houten I. van Houten-G. Tom Gehrels | discovery_site = Palomar Obs. | discovered = 17 October 1960 | mpc_name = (5012) Eurymedon | alt_names = 9507 P-L{{·}}{{mp|1984 SV|6}} {{mp|1988 AW|2}}{{·}}{{mp|1991 GD|3}} | pronounced = {{IPAc-en|j|uː|ˈ|r|ɪ|m|ᵻ|d|ən}} {{Respell|yoo|RIM|i|dən}} | named_after = Eurymedon [1] {{small|(Greek mythology)}} | mp_category = Jupiter trojan [1] {{nowrap|Greek [5]{{·}}background [6]}} | orbit_ref = | epoch = 23 March 2018 (JD 2458200.5) | uncertainty = 0 | observation_arc = 64.28 yr (23,478 d) | aphelion = 5.7231 AU | perihelion = 4.8142 AU | semimajor = 5.2686 AU | eccentricity = 0.0863 | period = 12.09 yr (4,417 d) | mean_anomaly = 276.30° | mean_motion = {{Deg2DMS|0.0815|sup=ms}} / day | inclination = 4.9948° | asc_node = 34.814° | arg_peri = 333.59° | jupiter_moid = 0.1348 AU | tisserand = 2.9850 | mean_diameter = {{val|36.96|0.36|ul=km}}[8] {{val|44.22|u=km}} {{small|(calculated)}}[9] | rotation = {{val|46|5|ul=h}}[10]{{efn|name=lightcurve-plots-CS3}} | albedo = {{val|0.057}} {{small|(assumed)}}[9] {{val|0.082|0.023}}[8] | spectral_type = C {{small|(Pan-STARRS)}}[9][14] C {{small|(SDSS-MOC)}}[15][16] | abs_magnitude = 10.50[1][8][9] {{val|10.72|0.22}}[14] }}5012 Eurymedon, provisional designation {{mp|9507 P-L}}, is a mid-sized Jupiter trojan from the Greek camp, approximately {{convert|37|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. It was discovered during the Palomar–Leiden survey at the Palomar Observatory in 1960.[1] The carbonaceous C-type asteroid has a tentative rotation period of 46 hours.[9] It was named from Greek mythology after Eurymedon.[1] DiscoveryEurymedon was discovered on 17 October 1960, by Dutch astronomers Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at the Palomar Observatory in California. The body's observation arc begins with a precovery taken at Palomar in February 1954, or more than 6 years prior to its official discovery observation.[1] Palomar–Leiden surveyThe survey designation "P-L" stands for "Palomar–Leiden", named after Palomar and Leiden observatories, which collaborated on the fruitful Palomar–Leiden survey in the 1960s. Gehrels used Palomar's Samuel Oschin telescope –also known as the 48-inch Schmidt Telescope – and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroids.[26] Orbit and classificationEurymedon is a carbonaceous Jupiter trojan in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's {{L4}} Lagrangian point, 60° ahead of its orbit {{cross reference|(see Trojans in astronomy)}}.[5] It is also a non-family asteroid in the Jovian background population.[6] This asteroid orbits the Sun at a distance of 4.8–5.7 AU once every 12 years and 1 month (4,417 days; semi-major axis of 5.27 AU). Its orbit has an eccentricity of 0.09 and an inclination of 5° with respect to the ecliptic.NamingThis minor planet was named after Eurymedon a servant to the Greek king Nestor during the Trojan War.[1] The official naming citation was published by the Minor Planet Center on 16 May 1992 ({{small|M.P.C. 20163}}).[31] Physical characteristicsIn the SDSS-based taxonomy, Eurymedon is a C-type asteroid.[15][16] It has also been characterized as a carbonaceous C-type by Pan-STARRS's survey,[9][14] while he dominant spectral type among the larger Jupiter trojans is that of D-types. Rotation periodIn April 2016, a rotational lightcurve of Eurymedon was obtained from only two nights of photometric observations by Linda French and Robert Stephens using the 4-meter Víctor M. Blanco Telescope at Cerro Tololo Inter-American Observatory in Chile. Lightcurve analysis gave a tentative rotation period of {{val|46|5}} hours with a brightness amplitude of 0.3 magnitude ({{small|U=1+}}).[9][10]{{efn|name=lightcurve-plots-CS3}} As of 2018, no refined period determination from follow-up observations has been published. Diameter and albedoAccording to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Eurymedon measures 36.96 kilometers in diameter and its surface has an albedo of 0.082,[8] while the Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 44.22 kilometers based on an absolute magnitude of 10.5.[9] In December 2011, an observed asteroid occultation event gave an cross section of {{val|26|x|26|u=km}} (no fit).[15] {{Largest Jupiter trojans}}Notes{{notelist|refs={{efn|name=lightcurve-plots-CS3|1=Lightcurve plots of (5012) Eurymedon from Apr 2016 by Linda French and Robert Stephens at the CTIO in Chile. Quality code is 2- (lightcurve rating at the CS3 website). Note: this plot shows an brightness amplitude of 0.49 rather than the published 0.30 magnitude. Summary figures at the LCDB and CS3.}}}} References1. ^1 2 3 4 5 6 7 8 {{cite web |title = 5012 Eurymedon (9507 P-L) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=5012 |accessdate = 28 June 2018}} [1][2][3][4][5][6][7][8][9][10][11]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 = 28 June 2018}} 3. ^1 {{cite web |title = Minor Planet Discoverers |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/lists/MPDiscsNum.html |date = 31 May 2018 |accessdate = 28 June 2018}} 4. ^1 {{cite web |title = MPC/MPO/MPS Archive |work = Minor Planet Center |url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |accessdate = 28 June 2018}} 5. ^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= 28 June 2018}} (online catalog) 6. ^1 2 {{cite web |title = Asteroid (5012) Eurymedon – Proper Elements |publisher = AstDyS-2, Asteroids – Dynamic Site |url = http://hamilton.dm.unipi.it/astdys/index.php?n=5012&pc=1.1.6 |access-date= 28 June 2018}} 7. ^1 2 3 {{cite web |title = Asteroid 5012 Eurymedon |work = Small Bodies Data Ferret |url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=5012+Eurymedon |accessdate = 28 June 2018}} 8. ^1 2 {{Cite journal |first1 = J. M. |last1 = Carvano |first2 = P. H. |last2 = Hasselmann |first3 = D. |last3 = Lazzaro |first4 = T. |last4 = Mothé-Diniz |date = February 2010 |title = SDSS-based taxonomic classification and orbital distribution of main belt asteroids |url = https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_I0035_5_SDSSTAX_V1_1/data/sdsstax_ast_table.tab |journal = Astronomy and Astrophysics |volume = 510 |page = 12 |bibcode = 2010A&A...510A..43C |doi = 10.1051/0004-6361/200913322 |access-date= 28 June 2018}} 9. ^1 2 3 4 5 6 7 8 {{cite web |title = LCDB Data for (5012) Eurymedon |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=5012%7CEurymedon |accessdate = 28 June 2018}} 10. ^1 2 {{Cite journal |first1 = Robert D. |last1 = Stephens |first2 = Daniel R. |last2 = Coley |first3 = Brian D. |last3 = Warner |first4 = Linda, M. |last4 = French |date = October 2016 |title = Lightcurves of Jovian Trojan Asteroids from the Center for Solar System Studies: L4 Greek Camp and Spies |url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016MPBu...43..323S |journal = The Minor Planet Bulletin |volume = 43 |issue = 4 |pages = 323–331 |issn = 1052-8091 |bibcode = 2016MPBu...43..323S |access-date= 28 June 2018}} 11. ^1 2 3 {{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 = https://arxiv.org/pdf/1506.00762.pdf |journal = Icarus |volume = 261 |pages = 34–47 |bibcode = 2015Icar..261...34V |doi = 10.1016/j.icarus.2015.08.007 |arxiv = 1506.00762 |access-date= 28 June 2018}} }} External links
8 : Jupiter trojans (Greek camp)|Discoveries by Cornelis Johannes van Houten|Discoveries by Ingrid van Houten-Groeneveld|Discoveries by Tom Gehrels|Discoveries by the Palomar–Leiden survey|Minor planets named from Greek mythology|Named minor planets|Astronomical objects discovered in 1960 |
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