About: (342842) 2008 YB3

An Entity of Type: planet, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org

(342842) 2008 YB3, provisional designation: 2008 YB3, is a sizable centaur and retrograde damocloid from the outer Solar System, approximately 67 kilometers (42 miles) in diameter. It was discovered on 18 December 2008, by astronomers with the Siding Spring Survey at the Siding Spring Observatory in Australia. The minor planet was numbered in 2012 and has since not been named.

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dbo:Planet/orbitalPeriod	28797.155 (dbd:day)
dbo:Planet/periapsis	9.6749430917811E8 (dbd:kilometre)
dbo:absoluteMagnitude	9.300000 (xsd:double)
dbo:abstract	(342842) 2008 YB3, provisional designation: 2008 YB3, is a sizable centaur and retrograde damocloid from the outer Solar System, approximately 67 kilometers (42 miles) in diameter. It was discovered on 18 December 2008, by astronomers with the Siding Spring Survey at the Siding Spring Observatory in Australia. The minor planet was numbered in 2012 and has since not been named. (en) (342842) 2008 YB3 ist ein Planetoid, der am 18. Dezember 2008 im Rahmen des Projekts Siding Spring Survey entdeckt wurde und zur Gruppe der Zentauren gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in fast 40 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,44, wobei diese 105° gegen die Ekliptik geneigt ist, so dass er eine retrograde Umlaufbahn aufweist. Es wird vermutet, dass der große retrograde Zentaur (342842) 2008 YB3 ebenso wie die beiden Zentauren (468861) 2013 LU28 und 2011 MM4 ein Besucher aus der Oort’schen Wolke ist. (de)
dbo:albedo	0.062000 (xsd:double)
dbo:apoapsis	2497985244948.600098 (xsd:double)
dbo:discovered	2008-12-18 (xsd:date)
dbo:discoverer	dbr:Siding_Spring_Survey
dbo:epoch	1 July 2021 (JD2459396.5)
dbo:formerName	(en)
dbo:orbitalPeriod	2488074192.000000 (xsd:double)
dbo:periapsis	967494309178.109985 (xsd:double)
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dbp:absMagnitude	9.300000 (xsd:double)
dbp:albedo	0.062000 (xsd:double)
dbp:aphelion	16.698 (dbd:astronomicalUnit)
dbp:argPeri	330.440000 (xsd:double)
dbp:ascNode	112.640000 (xsd:double)
dbp:background	#C7FF8F (en)
dbp:discovered	2008-12-18 (xsd:date)
dbp:discoverer	dbr:Siding_Spring_Survey
dbp:discoverySite	dbr:Siding_Spring_Observatory
dbp:eccentricity	0.441700 (xsd:double)
dbp:epoch	2021-07-01 (xsd:date)
dbp:inclination	105.060000 (xsd:double)
dbp:meanAnomaly	94.371000 (xsd:double)
dbp:meanMotion	/ day (en)
dbp:minorplanet	yes (en)
dbp:mpCategory	dbr:Distant_minor_planet centaurdamocloid (en)
dbp:observationArc	3.71748528E8 (dbd:second)
dbp:perihelion	6.4673 (dbd:astronomicalUnit)
dbp:period	1.2440005920000002E9 (dbd:second)
dbp:rotation	n.a. (en)
dbp:semimajor	11.583 (dbd:astronomicalUnit)
dbp:spectralType	dbr:Distant_object_spectral_type B–I (en) B–R (en) R–I (en) V–R (en)
dbp:tisserand	-0.246000 (xsd:double)
dbp:uncertainty	1 (xsd:integer)
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rdfs:comment	(342842) 2008 YB3, provisional designation: 2008 YB3, is a sizable centaur and retrograde damocloid from the outer Solar System, approximately 67 kilometers (42 miles) in diameter. It was discovered on 18 December 2008, by astronomers with the Siding Spring Survey at the Siding Spring Observatory in Australia. The minor planet was numbered in 2012 and has since not been named. (en) (342842) 2008 YB3 ist ein Planetoid, der am 18. Dezember 2008 im Rahmen des Projekts Siding Spring Survey entdeckt wurde und zur Gruppe der Zentauren gehört. Der Asteroid läuft auf einer mäßig exzentrischen Bahn in fast 40 Jahren um die Sonne. Die Bahnexzentrizität seiner Bahn beträgt 0,44, wobei diese 105° gegen die Ekliptik geneigt ist, so dass er eine retrograde Umlaufbahn aufweist. Es wird vermutet, dass der große retrograde Zentaur (342842) 2008 YB3 ebenso wie die beiden Zentauren (468861) 2013 LU28 und 2011 MM4 ein Besucher aus der Oort’schen Wolke ist. (de)
rdfs:label	(342842) 2008 YB3 (de) (342842) 2008 YB3 (en)
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