3288 Seleucus: Difference between revisions
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{{Infobox planet |
{{Infobox planet |
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| minorplanet = yes |
| minorplanet = yes |
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| name = 3288 Seleucus |
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| width = 25em |
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| |
| background = #FFC2E0 |
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| image = |
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| image_size = |
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| name = Seleucus |
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| |
| caption = |
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| discovery_ref =  <ref name="jpldata" /> |
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| image = |
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| discovered = 28 February 1982 |
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| caption = |
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| discoverer = [[Hans-Emil Schuster|H.-E. Schuster]] |
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| discovery = yes |
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| discovery_site = [[La Silla Observatory|La Silla Obs.]] |
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| discovery_ref = |
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| mpc_name = (3288) Seleucus |
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| discoverer = [[H.-E. Schuster]] |
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| alt_names = 1982 DV |
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| discovery_site = [[La Silla]] |
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| pronounced = {{IPAc-en|s|ᵻ|ˈ|l|uː|k|@|s}} |
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| discovered = February 28, 1982 |
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| named_after = [[Seleucus I Nicator]]<br />{{small|([[Seleucid Empire]])}}<ref name="springer" /> |
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| designations = yes |
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| mp_category = [[Amor asteroid|Amor]]{{·}}[[Near-Earth object|NEO]] <ref name="jpldata" /><ref name="MPC-Seleucus" /> |
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| mp_name = 3288 |
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| orbit_ref =  <ref name="jpldata" /> |
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| alt_names = 1982 DV |
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| epoch = 4 September 2017 ([[Julian day|JD]] 2458000.5) |
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| mp_category = |
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| |
| uncertainty = 0 |
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| observation_arc = 35.34 yr (12,907 days) |
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| epoch = May 14, 2008 |
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| aphelion = 2. |
| aphelion = 2.9605 [[Astronomical unit|AU]] |
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| perihelion = 1. |
| perihelion = 1.1053 AU |
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| semimajor = |
| semimajor = 2.0329 AU |
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| eccentricity = . |
| eccentricity = 0.4563 |
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| period = 2.90 [[Julian year (astronomy)|yr]] (1,059 days) |
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| period = 1058.612611490388 |
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| mean_anomaly = 77.175[[Degree (angle)|°]] |
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| avg_speed = |
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| mean_motion = {{Deg2DMS|0.3400|sup=ms}} / day |
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| inclination = 5.9311798788266 |
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| inclination = 5.9306° |
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| asc_node = 218.7441930794189 |
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| asc_node = 218.65° |
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| mean_anomaly = .8686030665866835 |
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| arg_peri = 349. |
| arg_peri = 349.29° |
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| moid = 0.1029 AU{{·}}40.1 [[Lunar distance (astronomy)|LD]] |
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| satellites = |
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| dimensions = {{val|2.2}} km<ref name="Harris-1998a" /><br />{{val|2.49|0.07}} km<ref name="Nugent-2015" /><br />2.8 km {{small|(Gehrels)}}<ref name="jpldata" /><br />{{val|2.832|1.100}} km<ref name="Mainzer-2012" /> |
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| physical_characteristics = yes |
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| rotation = {{val|16|}} [[Hour|h]] {{small|(dated)}}<ref name="Debehogne-1983" /><br />{{val|75|5}} h<ref name="Harris-1999a" /><br />{{val|75|}} h<ref name="Pravec-2005a" /> |
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| dimensions = |
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| albedo = {{val|0.139|0.127}}<ref name="Mainzer-2012" /><br />0.22 {{small|(Gehrels)}}<ref name="jpldata" /><br />{{val|0.23}}<ref name="Harris-1998a" /><br />{{val|0.24|0.04}}<ref name="Nugent-2015" /> |
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| mass = |
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| spectral_type = [[S-type asteroid|S]] {{small|([[Tholen classification|Tholen]])}} <ref name="jpldata" />{{·}}K {{small|([[SMASS classification|SMASS]])}} <ref name="jpldata" />{{·}}[[S-type asteroid|S]] <ref name="lcdb" /><br />[[Asteroid color indices|B–V]] = 0.910<ref name="jpldata" /><br />[[Asteroid color indices|U–B]] = 0.500<ref name="jpldata" /> |
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| density = |
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| abs_magnitude = 15.2<ref name="Nugent-2015" />{{·}}15.3<ref name="jpldata" />{{·}}15.5<ref name="Harris-1998a" /><ref name="lcdb" />{{·}}{{val|15.50|0.3}}<ref name="Mainzer-2012" />{{·}}{{val|15.6|0.3}}<ref name="Harris-1999a" /> |
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| surface_grav = |
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| escape_velocity = |
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| sidereal_day = |
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| axial_tilt = |
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| pole_ecliptic_lat = |
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| pole_ecliptic_lon = |
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| albedo = 0.22 |
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| temperatures= |
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| temp_name1 = |
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| mean_temp_1 = |
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| max_temp_1 = |
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| temp_name2 = |
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| max_temp_2 = |
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| spectral_type = |
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| abs_magnitude = 15.3 |
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}} |
}} |
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'''3288 Seleucus''' (1982 DV) is an [[Amor asteroid]] discovered on February 28, 1982 by [[H.-E. Schuster]] at [[La Silla]]. |
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== External links == |
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*[http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=3288+Seleucus JPL Small-Body Database Browser on 3288 Seleucus] |
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'''3288 Seleucus''', provisional designation {{mp|1982 DV}}, is a rare-type stony [[asteroid]], classified as [[near-Earth object]] of the [[Amor asteroid|Amor]] group of asteroids, approximately 2.5 kilometers in diameter. It was discovered on 28 February 1982, by German astronomer [[Hans-Emil Schuster]] at [[European Southern Observatory|ESO]]'s [[La Silla Observatory]] site in northern Chile.<ref name="MPC-Seleucus" /> It was named after the Hellenistic general and Seleucid ruler [[Seleucus I Nicator]].<ref name="springer" /> |
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{{Reflist}} |
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== Orbit == |
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{{Minor planets navigator|3287 Olmstead|3289 Mitani}} |
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{{Small Solar System bodies}} |
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''Seleucus'' orbits the Sun in the [[Kirkwood gap|inner]] main-belt at a distance of 1.1–3.0 [[Astronomical unit|AU]] once every 2 years and 11 months (1,059 days). Its orbit has an [[orbital eccentricity|eccentricity]] of 0.46 and an [[orbital inclination|inclination]] of 6[[Degree (angle)|°]] with respect to the [[ecliptic]].<ref name="jpldata" /> ''Seleucus'' has an ''Earth [[minimum orbital intersection distance]]'' of {{convert |0.1029 |AU |km |abbr=on |lk=off |sigfig=3}}, which corresponds to 40.1 [[Lunar distance (astronomy)|lunar distances]].<ref name="jpldata" /> As no [[precoveries]] were taken, and no prior identifications were made, the body's [[observation arc]] begins with its official discovery observation at La Silla.<ref name="MPC-Seleucus" /> |
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{{DEFAULTSORT:Seleucus}} |
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[[Category:Amor asteroids]] |
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[[Category:Asteroids named for people]] |
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[[Category:Astronomical objects discovered in 1982]] |
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== Physical parameters == |
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{{NE-asteroid-stub}} |
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=== Spectral type === |
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On the [[Tholen classification|Tholen]] and [[SMASS classification|SMASS]] taxonomic scheme, ''Seleucus'' is classified as a featureless [[S-type asteroid|S-type]] and rare [[K-type asteroid|K-type]] asteroid, respectively.<ref name="jpldata" /> |
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[[de:(3288) Seleucus]] |
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[[eo:3288 Seleŭko]] |
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=== Rotation period === |
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[[fa:سیارک ۳۲۸۸]] |
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[[it:3288 Seleucus]] |
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It has a relatively long [[rotation period]] of 75 hours with a brightness variation of 1.0 [[Magnitude (astronomy)|magnitude]], indicative of a non-spheroidal shape ({{small|[[LCDB quality code|U=3/3]]}}).<ref name="Harris-1999a" /><ref name="Pravec-2005a" /> While most [[minor planet]]s have spin rate between 2 and 20 hours, ''Seleucus'' still rotates faster than a typical [[List of slow rotators (minor planets)|slow rotator]], which have periods above 100 hours. |
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[[la:3288 Seleucus]] |
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[[hu:3288 Seleucus]] |
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=== Diameter and albedo === |
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[[ja:セレウコス (小惑星)]] |
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[[pl:3288 Seleucus]] |
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According to the survey carried out by NASA's [[Wide-field Infrared Survey Explorer]] with its subsequent [[NEOWISE]] mission, ''Seleucus'' measures 2.49 and 2.83 kilometers in diameter, and its surface has an [[astronomical albedo|albedo]] of 0.139 and 0.24, respectively.<ref name="Nugent-2015" /><ref name="Mainzer-2012" /> The ''Collaborative Asteroid Lightcurve Link'' adopts an albedo of 0.23 and a diameter of 2.2 kilometers, based on modeled data by Alan Harris.<ref name="Harris-1998a" /><ref name="lcdb" /> |
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[[sk:3288 Seleucus]] |
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[[sr:3288 Seleucus]] |
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== Naming == |
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[[vi:3288 Seleucus]] |
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This [[minor planet]] is named for [[Seleucus I Nicator]], a general in the army of [[Alexander the Great]], and, after the death of Alexander, founder and king of the [[Seleucid Empire]].<ref name="springer" /> The approved naming citation was published by the [[Minor Planet Center]] on 29 September 1985 ({{small|[[Minor Planet Circulars|M.P.C.]] 10046}}).<ref name="MPC-Circulars-Archive" /> |
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== See also == |
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* [[Seleucus (crater)]], a lunar crater |
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== References == |
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{{reflist|30em|refs= |
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<ref name="jpldata">{{cite web |
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|type = 2017-07-01 last obs. |
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|title = JPL Small-Body Database Browser: 3288 Seleucus (1982 DV) |
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|url = https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2003288 |
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|publisher = [[Jet Propulsion Laboratory]] |
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|access-date = 3 July 2017}}</ref> |
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<ref name="springer">{{cite book |
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|title = Dictionary of Minor Planet Names – (3288) Seleucus |
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|last = Schmadel | first = Lutz D. |
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|publisher = [[Springer Berlin Heidelberg]] |
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|page = 274 |
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|date = 2007 |
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|isbn = 978-3-540-00238-3 |
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|doi = 10.1007/978-3-540-29925-7_3289 |chapter = (3288) Seleucus }}</ref> |
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<ref name="MPC-Seleucus">{{cite web |
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|title = 3288 Seleucus (1982 DV) |
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|work = Minor Planet Center |
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|url = https://www.minorplanetcenter.net/db_search/show_object?object_id=3288 |
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|access-date = 9 January 2017}}</ref> |
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<ref name="MPC-Circulars-Archive">{{cite web |
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|title = MPC/MPO/MPS Archive |
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|work = Minor Planet Center |
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|url = https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html |
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|access-date = 9 January 2017}}</ref> |
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<ref name="lcdb">{{cite web |
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|title = LCDB Data for (3288) Seleucus |
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|publisher = Asteroid Lightcurve Database (LCDB) |
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|url = http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=3288%7CSeleucus |
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|access-date = 9 January 2017}}</ref> |
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<ref name="Harris-1998a">{{Cite journal |
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|author = Harris, Alan W. |
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|date = February 1998 |
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|title = A Thermal Model for Near-Earth Asteroids |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1998Icar..131..291H |
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|journal = Icarus |
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|volume = 131 |
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|issue = 2 |
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|pages = 291–301 |
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|bibcode = 1998Icar..131..291H |
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|doi = 10.1006/icar.1997.5865 |
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|access-date= 9 January 2017}}</ref> |
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<ref name="Mainzer-2012">{{Cite journal |
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|display-authors = 6 |
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|first1 = A. |last1 = Mainzer |
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|first2 = T. |last2 = Grav |
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|first3 = J. |last3 = Masiero |
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|first4 = J. |last4 = Bauer |
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|first5 = R. M. |last5 = Cutri |
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|first6 = R. S. |last6 = McMillan |
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|first7 = C. R. |last7 = Nugent |
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|first8 = D. |last8 = Tholen |
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|first9 = R. |last9 = Walker |
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|first10 = E. L. |last10 = Wright |
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|date = November 2012 |
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|title = Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...760L..12M |
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|journal = The Astrophysical Journal Letters |
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|volume = 760 |
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|issue = 1 |
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|page = 6 |
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|bibcode = 2012ApJ...760L..12M |
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|doi = 10.1088/2041-8205/760/1/L12 |
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|access-date= 9 January 2017|arxiv = 1210.0502 |s2cid = 41459166 }}</ref> |
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<ref name="Nugent-2015">{{cite journal |
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|display-authors = 6 |
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|first1 = C. R. |last1 = Nugent |
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|first2 = A. |last2 = Mainzer |
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|first3 = J. |last3 = Masiero |
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|first4 = J. |last4 = Bauer |
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|first5 = R. M. |last5 = Cutri |
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|first6 = T. |last6 = Grav |
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|first7 = E. |last7 = Kramer |
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|first8 = S. |last8 = Sonnett |
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|first9 = R. |last9 = Stevenson |
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|first10 = E. L. |last10 = Wright |
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|date = December 2015 |
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|title = NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N |
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|journal = The Astrophysical Journal |
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|volume = 814 |
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|issue = 2 |
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|page = 13 |
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|bibcode = 2015ApJ...814..117N |
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|doi = 10.1088/0004-637X/814/2/117 |
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|arxiv = 1509.02522 |
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|s2cid = 9341381 |access-date= 9 January 2017}}</ref> |
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<ref name="Debehogne-1983">{{Cite journal |
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|first1 = H. |last1 = Debehogne |
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|first2 = G. |last2 = de Sanctis |
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|first3 = V. |last3 = Zappala |
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|date = August 1983 |
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|title = Photoelectric photometry of asteroids 45, 120, 776, 804, 814, and 1982DV |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1983Icar...55..236D |
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|journal = Icarus |
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|volume = 55 |
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|issue = 2 |
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|pages = 236–244 |
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|issn = 0019-1035 |
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|bibcode = 1983Icar...55..236D |
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|doi = 10.1016/0019-1035(83)90078-7 |
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|access-date= 9 January 2017}}</ref> |
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<ref name="Harris-1999a">{{Cite journal |
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|first1 = A. W. |last1 = Harris |
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|first2 = J. W. |last2 = Young |
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|first3 = E. |last3 = Bowell |
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|first4 = D. J. |last4 = Tholen |
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|date = November 1999 |
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|title = Asteroid Lightcurve Observations from 1981 to 1983 |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1999Icar..142..173H |
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|journal = Icarus |
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|volume = 142 |
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|issue = 1 |
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|pages = 173 |
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|bibcode = 1999Icar..142..173H |
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|doi = 10.1006/icar.1999.6181 |
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|access-date= 9 January 2017}}</ref> |
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<ref name="Pravec-2005a">{{Cite journal |
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|display-authors = 6 |
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|first1 = P. |last1 = Pravec |
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|first2 = A. W. |last2 = Harris |
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|first3 = P. |last3 = Scheirich |
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|first4 = P. |last4 = Kusnirák |
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|first5 = L. |last5 = Sarounová |
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|first6 = C. W. |last6 = Hergenrother |
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|first7 = S. |last7 = Mottola |
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|first8 = M. D. |last8 = Hicks |
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|first9 = G. |last9 = Masi |
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|first10 = Yu. N. |last10 = Krugly |
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|first11 = V. G. |last11 = Shevchenko |
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|first12 = M. C. |last12 = Nolan |
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|first13 = E. S. |last13 = Howell |
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|first14 = M. |last14 = Kaasalainen |
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|first15 = A. |last15 = Galád |
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|first16 = P. |last16 = Brown |
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|first17 = D. R. |last17 = DeGraff |
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|first18 = J. V. |last18 = Lambert |
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|first19 = W. R. |last19 = Cooney |
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|first20 = S. |last20 = Foglia |
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|date = January 2005 |
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|title = Tumbling asteroids |
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|url = http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2005Icar..173..108P |
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|journal = Icarus |
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|volume = 173 |
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|issue = 1 |
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|pages = 108–131 |
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|bibcode = 2005Icar..173..108P |
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|doi = 10.1016/j.icarus.2004.07.021 |
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|access-date= 9 January 2017}}</ref> |
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}} <!-- end of reflist --> |
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== External links == |
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* [http://www.minorplanet.info/PHP/lcdbsummaryquery.php Asteroid Lightcurve Database (LCDB)], query form ([http://www.minorplanet.info/lightcurvedatabase.html info] {{Webarchive|url=https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html |date=2017-12-16 }}) |
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* [https://books.google.com/books?id=aeAg1X7afOoC&pg Dictionary of Minor Planet Names], Google books |
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* [http://obswww.unige.ch/~behrend/page_cou.html Asteroids and comets rotation curves, CdR] – Observatoire de Genève, Raoul Behrend |
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* {{NeoDys|3288}} |
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* {{ESA-SSA|3288|Seleucus}} |
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* {{JPL small body}} |
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{{Minor planets navigator|3287 Olmstead|number=3288|3289 Mitani}} |
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{{Small Solar System bodies}} |
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{{Authority control}} |
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{{DEFAULTSORT:Seleucus}} |
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[[Category:Amor asteroids|003288]] |
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[[Category:Discoveries by Hans-Emil Schuster]] |
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[[Category:Named minor planets]] |
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[[Category:S-type asteroids (Tholen)|003288]] |
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[[Category:K-type asteroids (SMASS)|003288]] |
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[[Category:Astronomical objects discovered in 1982|19820228]] |
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[[Category:Seleucus I Nicator]] |
Latest revision as of 22:41, 19 December 2023
Discovery [1] | |
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Discovered by | H.-E. Schuster |
Discovery site | La Silla Obs. |
Discovery date | 28 February 1982 |
Designations | |
(3288) Seleucus | |
Pronunciation | /sɪˈluːkəs/ |
Named after | Seleucus I Nicator (Seleucid Empire)[2] |
1982 DV | |
Amor · NEO [1][3] | |
Orbital characteristics [1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 35.34 yr (12,907 days) |
Aphelion | 2.9605 AU |
Perihelion | 1.1053 AU |
2.0329 AU | |
Eccentricity | 0.4563 |
2.90 yr (1,059 days) | |
77.175° | |
0° 20m 24s / day | |
Inclination | 5.9306° |
218.65° | |
349.29° | |
Earth MOID | 0.1029 AU · 40.1 LD |
Physical characteristics | |
Dimensions | 2.2 km[4] 2.49±0.07 km[5] 2.8 km (Gehrels)[1] 2.832±1.100 km[6] |
16 h (dated)[7] 75±5 h[8] 75 h[9] | |
0.139±0.127[6] 0.22 (Gehrels)[1] 0.23[4] 0.24±0.04[5] | |
S (Tholen) [1] · K (SMASS) [1] · S [10] B–V = 0.910[1] U–B = 0.500[1] | |
15.2[5] · 15.3[1] · 15.5[4][10] · 15.50±0.3[6] · 15.6±0.3[8] | |
3288 Seleucus, provisional designation 1982 DV, is a rare-type stony asteroid, classified as near-Earth object of the Amor group of asteroids, approximately 2.5 kilometers in diameter. It was discovered on 28 February 1982, by German astronomer Hans-Emil Schuster at ESO's La Silla Observatory site in northern Chile.[3] It was named after the Hellenistic general and Seleucid ruler Seleucus I Nicator.[2]
Orbit
[edit]Seleucus orbits the Sun in the inner main-belt at a distance of 1.1–3.0 AU once every 2 years and 11 months (1,059 days). Its orbit has an eccentricity of 0.46 and an inclination of 6° with respect to the ecliptic.[1] Seleucus has an Earth minimum orbital intersection distance of 0.1029 AU (15,400,000 km), which corresponds to 40.1 lunar distances.[1] As no precoveries were taken, and no prior identifications were made, the body's observation arc begins with its official discovery observation at La Silla.[3]
Physical parameters
[edit]Spectral type
[edit]On the Tholen and SMASS taxonomic scheme, Seleucus is classified as a featureless S-type and rare K-type asteroid, respectively.[1]
Rotation period
[edit]It has a relatively long rotation period of 75 hours with a brightness variation of 1.0 magnitude, indicative of a non-spheroidal shape (U=3/3).[8][9] While most minor planets have spin rate between 2 and 20 hours, Seleucus still rotates faster than a typical slow rotator, which have periods above 100 hours.
Diameter and albedo
[edit]According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Seleucus measures 2.49 and 2.83 kilometers in diameter, and its surface has an albedo of 0.139 and 0.24, respectively.[5][6] The Collaborative Asteroid Lightcurve Link adopts an albedo of 0.23 and a diameter of 2.2 kilometers, based on modeled data by Alan Harris.[4][10]
Naming
[edit]This minor planet is named for Seleucus I Nicator, a general in the army of Alexander the Great, and, after the death of Alexander, founder and king of the Seleucid Empire.[2] The approved naming citation was published by the Minor Planet Center on 29 September 1985 (M.P.C. 10046).[11]
See also
[edit]- Seleucus (crater), a lunar crater
References
[edit]- ^ a b c d e f g h i j k l m "JPL Small-Body Database Browser: 3288 Seleucus (1982 DV)" (2017-07-01 last obs.). Jet Propulsion Laboratory. Retrieved 3 July 2017.
- ^ a b c Schmadel, Lutz D. (2007). "(3288) Seleucus". Dictionary of Minor Planet Names – (3288) Seleucus. Springer Berlin Heidelberg. p. 274. doi:10.1007/978-3-540-29925-7_3289. ISBN 978-3-540-00238-3.
- ^ a b c "3288 Seleucus (1982 DV)". Minor Planet Center. Retrieved 9 January 2017.
- ^ a b c d Harris, Alan W. (February 1998). "A Thermal Model for Near-Earth Asteroids". Icarus. 131 (2): 291–301. Bibcode:1998Icar..131..291H. doi:10.1006/icar.1997.5865. Retrieved 9 January 2017.
- ^ a b c d Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv:1509.02522. Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID 9341381. Retrieved 9 January 2017.
- ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Cutri, R. M.; McMillan, R. S.; et al. (November 2012). "Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey". The Astrophysical Journal Letters. 760 (1): 6. arXiv:1210.0502. Bibcode:2012ApJ...760L..12M. doi:10.1088/2041-8205/760/1/L12. S2CID 41459166. Retrieved 9 January 2017.
- ^ Debehogne, H.; de Sanctis, G.; Zappala, V. (August 1983). "Photoelectric photometry of asteroids 45, 120, 776, 804, 814, and 1982DV". Icarus. 55 (2): 236–244. Bibcode:1983Icar...55..236D. doi:10.1016/0019-1035(83)90078-7. ISSN 0019-1035. Retrieved 9 January 2017.
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- ^ a b c "LCDB Data for (3288) Seleucus". Asteroid Lightcurve Database (LCDB). Retrieved 9 January 2017.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 9 January 2017.
External links
[edit]- Asteroid Lightcurve Database (LCDB), query form (info Archived 2017-12-16 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- 3288 Seleucus at NeoDyS-2, Near Earth Objects—Dynamic Site
- 3288 Seleucus at ESA–space situational awareness
- 3288 Seleucus at the JPL Small-Body Database