词条 | 1868 Thersites |
释义 |
| minorplanet = yes | name = 1868 Thersites | background = #C2FFFF | image = | image_size = | caption = | discovery_ref = [1] | discovered = 24 September 1960 | discoverer = C. J. van Houten I. van Houten G. T. Gehrels | discovery_site = Palomar Obs. | mpc_name = (1868) Thersites | alt_names = 2008 P-L{{·}}{{mp|1972 RB|2}} | pronounced = {{IPAc-en|θ|ər|ˈ|s|aɪ|t|iː|z}} {{respell|thər|SY|teez}} | named_after = Thersites [2] {{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 = 63.50 yr (23,195 d) | aphelion = 5.9015 AU | perihelion = 4.7316 AU | semimajor = 5.3166 AU | eccentricity = 0.1100 | period = 12.26 yr (4,478 d) | mean_anomaly = 277.51° | mean_motion = {{Deg2DMS|0.0804|sup=ms}} / day | inclination = 16.751° | asc_node = 197.82° | arg_peri = 169.76° | jupiter_moid = 0.2116 AU | tisserand = 2.9030 | mean_diameter = {{val|68.16|0.81|ul=km}}[10] {{val|70.08|u=km}} {{small|(calculated)}}[5] {{val|78.89|2.02|u=km}}[12] | rotation = {{val|10.412|0.003|ul=h}}{{efn|name=lcdb-Stephens-2017}} {{val|10.416|0.014|u=h}}[13] {{val|10.48|0.01|u=h}}[14]{{efn|name=lightcurve-plot-Stephens-2016}} | albedo = {{val|0.055|0.003}}[12] {{val|0.055|0.008}}[10] {{val|0.057}} {{small|(assumed)}}[5] | spectral_type = C {{small|(assumed)}}[5] V–I {{=}} {{val|0.960|0.034}}[5] | abs_magnitude = 9.30[12] 9.5[1][5] 9.6[10] }}1868 Thersites ({{IPAc-en|θ|ər|ˈ|s|aɪ|t|iː|z}} {{respell|thər|SY|teez}}), provisional designation {{mp|2008 P-L}}, is a large Jupiter trojan from the Greek camp, approximately {{convert|70|km|mi|abbr=off|sigfig=2|sp=us}} in diameter. Discovered during the Palomar–Leiden survey at Palomar in 1960, it was later named after the warrior Thersites from Greek mythology. The presumed carbonaceous C-type asteroid belongs to the 50 largest Jupiter trojans and has a rotation period of 10.48 hours.[5] DiscoveryThersites was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at the Palomar Observatory in California.[1] On the same day, the group discovered another Jupiter trojan, 1869 Philoctetes. The body's observation arc begins with a precovery taken at Palomar in March 1954, more than 6 years prior to its official discovery observation.[1] Palomar–Leiden surveyThe provisional survey designation "P-L" stands for Palomar–Leiden, named after the Palomar and Leiden observatories, which collaborated on the fruitful Palomar–Leiden survey in the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope, also known as the 48-inch Schmidt Telescope, and shipped the photographic plates to Cornelis and Ingrid van Houten at Leiden Observatory, where astrometry was carried out. The trio are credited with the discovery of several thousand minor planets.[28] Orbit and classificationThersites 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][30] It orbits the Sun at a distance of 4.7–5.9 AU once every 12 years and 3 months (4,478 days; semi-major axis of 5.32 AU). Its orbit has an eccentricity of 0.11 and an inclination of 17° with respect to the ecliptic.Physical characteristicsThe Trojan asteroid has been assumed to be a carbonaceous C-type asteroid.[5] Rotation periodIn July 1994, a first rotational lightcurve of Thersites was obtained from photometric observations by Italian astronomer Stefano Mottola using the former Dutch 0.9-metre Telescope at ESO's La Silla Observatory in northern Chile. Lightcurve analysis gave a rotation period of {{val|10.416|0.014}} hours with a brightness variation of {{val|0.14|0.01}} magnitude ({{small|U=2+}}).[5][13] The best-rated lightcurve by Robert Stephens at the Center for Solar System Studies from June 2016 gave a period of 10.48 hours and an amplitude of 0.27 magnitude ({{small|U=3-}}).[5][14]{{efn|name=lightcurve-plot-Stephens-2016}} Follow-up observation in 2017 gave a similar period of 10.412 hours ({{small|U=2}}).{{efn|name=lcdb-Stephens-2017}} Diameter and albedoAccording to the space-based surveys carried out by the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Thersites has a low albedo of 0.055 and measures 78.9 and 68.2 kilometers in diameter, respectively.[10][12] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057, and calculates an intermediate diameter of 70.08 kilometers with an absolute magnitude of 9.5.[5] {{Largest Jupiter trojans}}NamingThis minor planet was named from Greek mythology after Thersites, a Greek warrior who wanted to abandon Troy's siege during the Trojan War and head home. The given name also refers to the fact, that the asteroid was discovered farthest from the {{L4|nolink=yes}} Lagrangian point.[2] The official naming citation was published by the Minor Planet Center before November 1977 ({{small|M.P.C. 3826}}).[41] Notes{{notelist|30em|refs={{efn|name=lightcurve-plot-Stephens-2016|1=Lightcurve plot of (1868) Thersites (July 2016) Rotation period {{val|10.48|0.01}} hours with a brightness amplitude of {{val|0.27|0.02}} mag. Quality code is 3-. Summary figures for at the LCDB.}}{{efn|name=lcdb-Stephens-2017|1=Stephens (2017). Observations from July 2017. (lightcurve plot) Rotation period {{val|10.412|0.003}} hours with a brightness amplitude of {{val|0.18|0.01}} mag. Quality code of 2. Summary figures for (1868) Thersites at the LCDB.}}}} References1. ^1 2 {{cite book |title = Dictionary of Minor Planet Names – (1868) Thersites |last = Schmadel | first = Lutz D. |publisher = Springer Berlin Heidelberg |page = 150 |date = 2007 |isbn = 978-3-540-00238-3 |doi = 10.1007/978-3-540-29925-7_1869 |chapter = (1868) Thersites }} [1][2][3][4][5][6][7][8][9][10][11][12]2. ^1 2 3 4 5 {{cite web |title = 1868 Thersites (2008 P-L) |work = Minor Planet Center |url = https://www.minorplanetcenter.net/db_search/show_object?object_id=1868 |accessdate = 9 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 = 9 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 = 9 June 2018}} 5. ^1 {{cite web |title = List of Jupiter Trojans |work = Minor Planet Center |date = 31 May 2018 |url = https://www.minorplanetcenter.net/iau/lists/JupiterTrojans.html |accessdate = 9 June 2018}} 6. ^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 |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 }} (online catalog) 7. ^1 {{cite web |title = Asteroid 1868 Thersites |work = Small Bodies Data Ferret |url = https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1868+Thersites |accessdate = 9 June 2018}} 8. ^1 2 3 {{cite web |title = Asteroid (1868) Thersites |publisher = AstDyS-2, Asteroids – Dynamic Site |url = http://hamilton.dm.unipi.it/astdys/index.php?n=1868&pc=1.1.6 |accessdate = 9 June 2018}} 9. ^1 2 3 4 5 6 7 8 9 10 11 {{cite web |title = LCDB Data for (1868) Thersites |publisher = Asteroid Lightcurve Database (LCDB) |url = http://www.minorplanet.info/PHP/GenerateALCDEFPage_Local.php?AstInfo=1868%7CThersites |accessdate = 9 June 2018}} 10. ^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]) 11. ^1 2 {{cite journal |display-authors = 6 |first1 = Stefano |last1 = Mottola |first2 = Mario |last2 = Di Martino |first3 = Anders |last3 = Erikson |first4 = Maria |last4 = Gonano-Beurer |first5 = Albino |last5 = Carbognani |first6 = Uri |last6 = Carsenty |first7 = Gerhard |last7 = Hahn |first8 = Hans-Josef |last8 = Schober |first9 = Felix |last9 = Lahulla |first10 = Marco |last10 = Delbò |first11 = Claes-Ingvar |last11 = Lagerkvist |date = May 2011 |title = Rotational Properties of Jupiter Trojans. I. Light Curves of 80 Objects |journal = The Astronomical Journal |volume = 141 |issue = 5 |page = 32 |bibcode = 2011AJ....141..170M |doi = 10.1088/0004-6256/141/5/170 }} 12. ^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= 9 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|Minor planets named from Greek mythology|Discoveries by the Palomar–Leiden survey|Named minor planets|Astronomical objects discovered in 1960 |
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