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Statements

Subject Item
dbr:(184212)_2004_PB112
rdf:type
yago:Whole100003553 yago:Object100002684 dbo:Planet yago:Planet109394007 yago:PhysicalEntity100001930 yago:NaturalObject100019128 owl:Thing schema:Place yago:CelestialBody109239740 yago:WikicatTrans-NeptunianObjects wikidata:Q634 dbo:CelestialBody dbo:Place yago:WikicatAstronomicalObjectsDiscoveredIn2004 dbo:Location
rdfs:label
(184212) 2004 PB112 (184212) 2004 PB112 2004 PB112 (184212) 2004 PB112 (184212) 2004 PB112
rdfs:comment
(184212) 2004 PB112, prov. designation: 2004 PB112, is a trans-Neptunian object from the scattered disc, approximately 154 kilometers (96 miles) in diameter, and in a rare high-order orbital resonance ratio (4:27) with Neptune. It was discovered on 13 August 2004, by American astronomer Marc Buie at the Cerro Tololo Inter-American Observatory in Chile. (182926) 2002 FU6, também escrito como (184212) 2004 PB112, é um objeto transnetuniano (TNO) que está localizado no cinturão de Kuiper, uma região do Sistema Solar. Este objeto é classificado como um cubewano. O mesmo possui uma magnitude absoluta (H) de 7,2 e, tem um diâmetro com cerca de 160 km, por isso existem poucas chances que possa ser classificado como um planeta anão, devido ao seu tamanho relativamente pequeno. 2004 PB112, eller (184212) 2004 PB112, är en småplanet i en långsträckt omloppsbana utanför Neptunus omloppsbana. Den upptäcktes 13 augusti 2004 av Marc W. Buie vid . Det finns ett par alternativa klassificeringar av den omloppsbana 2004 PB112 uppvisar, båda faller dock tillbaka på den som ett Transneptunskt objekt. Minor Planet Center listar den bland Scattered disc objects och Centaurer. Johnstonsarchive.net listar dem som Scattered disc medan Brett Gladman listar den som 4:27-banresonant med Neptunus. Småplaneten befinner sig därmed i en stabil omloppbana där den gör fyra varv runt solen medan Neptunus gör 27. 2004 بي بي 112 (ويعرف أيضًا باسم (184212) 2004 بي بي 112 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2004 PB112)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 184212 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة مارك ويليام بوي في 13 أغسطس 2004. (184212) 2004 PB112 est un objet transneptunien qui mesurerait entre 100 et 220 km de diamètre. Son aphélie est de 184,6 UA et son périhélie de 35,3 UA, il possède donc une orbite excentrique. À son périhélie, il se situe parfois plus près du Soleil que Pluton. Il est passé au périhélie le 25 octobre 2011.
foaf:name
(184212)
dct:subject
dbc:Discoveries_by_Marc_Buie dbc:Scattered_disc_and_detached_objects dbc:Astronomical_objects_discovered_in_2004
dbo:wikiPageID
33614959
dbo:wikiPageRevisionID
1035194169
dbo:wikiPageWikiLink
dbr:Minor_Planet_Center dbr:Minor_Planet_Circulars dbc:Discoveries_by_Marc_Buie dbr:Cerro_Tololo_Inter-American_Observatory dbr:Trans-Neptunian_object dbr:List_of_named_minor_planets_(alphabetical) dbr:Astronomical_unit dbr:Scattered_disc_object dbr:Minor_planet dbr:Orbital_resonance dbr:Geometric_albedo dbr:Orbital_eccentricity dbr:Observation_arc dbr:Deep_Ecliptic_Survey dbr:Absolute_magnitude dbr:Semi-major_axis dbr:Perihelion dbc:Scattered_disc_and_detached_objects dbr:Precovery dbr:Marc_Buie dbr:Astronomical_albedo dbr:Minor_planet_designation dbr:Minor_planet_provisional_designation dbr:Scattered_disc dbc:Astronomical_objects_discovered_in_2004 dbr:Ecliptic dbr:Julian_year_(astronomy) dbr:Orbital_inclination dbr:Degree_(angle) dbr:Julian_day dbr:Neptune dbr:Resonant_trans-Neptunian_object
dbo:wikiPageExternalLink
n18:t_centaurs.html n18:NumberedMPs180001.html n26:OneAsteroidInfo.php
owl:sameAs
dbpedia-fr:(184212)_2004_PB112 dbpedia-ar:(184212)_2004_PB112 wikidata:Q4542010 yago-res:(184212)_2004_PB112 n19:4CXqh freebase:m.0hgnqqp dbpedia-sv:2004_PB112 dbpedia-pt:(184212)_2004_PB112 n27:(184212)_2004_PB112_(كويكب)
dbp:wikiPageUsesTemplate
dbt:Mp dbt:Asof dbt:JPL_small_body dbt:Small dbt:Small_Solar_System_bodies dbt:Use_dmy_dates dbt:Rp dbt:Infobox_planet dbt:Val dbt:Minor_planets_navigator dbt:Deg2DMS dbt:Reflist dbt:Convert dbt:·
dbp:absMagnitude
7.3
dbp:aphelion
184.6
dbp:argPeri
3.6578
dbp:ascNode
356.73
dbp:background
#C2E0FF
dbp:discovered
2004-08-13
dbp:discoverer
dbr:Marc_Buie
dbp:discoverySite
dbr:Cerro_Tololo_Inter-American_Observatory
dbp:eccentricity
0.6787
dbp:epoch
2021-07-01
dbp:inclination
15.403
dbp:meanAnomaly
3.0647
dbp:meanDiameter
dbp:meanMotion
/ day
dbp:minorplanet
yes
dbp:mpCategory
267.0 TNOSDO
dbp:observationArc
5.38688232E8
dbp:perihelion
35.333
dbp:period
1153.2
dbp:semimajor
109.97
dbp:uncertainty
30
dbo:abstract
(184212) 2004 PB112, prov. designation: 2004 PB112, is a trans-Neptunian object from the scattered disc, approximately 154 kilometers (96 miles) in diameter, and in a rare high-order orbital resonance ratio (4:27) with Neptune. It was discovered on 13 August 2004, by American astronomer Marc Buie at the Cerro Tololo Inter-American Observatory in Chile. 2004 بي بي 112 (ويعرف أيضًا باسم (184212) 2004 بي بي 112 وفق تسمية الكوكب الصغير) (بالإنجليزية: 2004 PB112)‏ هو كويكب ضمن حزام الكويكبات؛ وترتيبه 184212 من حيث الاكتشاف.اكتُشف هذا الجُرم الفلكي بواسطة مارك ويليام بوي في 13 أغسطس 2004. (182926) 2002 FU6, também escrito como (184212) 2004 PB112, é um objeto transnetuniano (TNO) que está localizado no cinturão de Kuiper, uma região do Sistema Solar. Este objeto é classificado como um cubewano. O mesmo possui uma magnitude absoluta (H) de 7,2 e, tem um diâmetro com cerca de 160 km, por isso existem poucas chances que possa ser classificado como um planeta anão, devido ao seu tamanho relativamente pequeno. (184212) 2004 PB112 est un objet transneptunien qui mesurerait entre 100 et 220 km de diamètre. Son aphélie est de 184,6 UA et son périhélie de 35,3 UA, il possède donc une orbite excentrique. À son périhélie, il se situe parfois plus près du Soleil que Pluton. Il est passé au périhélie le 25 octobre 2011. 2004 PB112, eller (184212) 2004 PB112, är en småplanet i en långsträckt omloppsbana utanför Neptunus omloppsbana. Den upptäcktes 13 augusti 2004 av Marc W. Buie vid . Det finns ett par alternativa klassificeringar av den omloppsbana 2004 PB112 uppvisar, båda faller dock tillbaka på den som ett Transneptunskt objekt. Minor Planet Center listar den bland Scattered disc objects och Centaurer. Johnstonsarchive.net listar dem som Scattered disc medan Brett Gladman listar den som 4:27-banresonant med Neptunus. Småplaneten befinner sig därmed i en stabil omloppbana där den gör fyra varv runt solen medan Neptunus gör 27.
gold:hypernym
dbr:Object
prov:wasDerivedFrom
wikipedia-en:(184212)_2004_PB112?oldid=1035194169&ns=0
n5:apoapsis
2.761576693122E10
n5:orbitalPeriod
1153.2
n5:periapsis
5.2857415654431E9
dbo:wikiPageLength
6757
dbo:absoluteMagnitude
7.3
dbo:apoapsis
27615766931220.0
dbo:discovered
2004-08-13
dbo:epoch
1 July 2021 (JD2459396.5)
dbo:formerName
dbo:orbitalPeriod
99636480.0
dbo:periapsis
5285741565443.1
dbo:discoverer
dbr:Marc_Buie
foaf:isPrimaryTopicOf
wikipedia-en:(184212)_2004_PB112