{ "items" : [
    { "id" : "http://dbpedia.org/resource/(308193)_2005_CB79"
      "properties" : {
        "http://www.w3.org/2000/01/rdf-schema#comment" : [ "(308193) 2005 CB79 is a trans-Neptunian object that is a member of the Haumea family.As a member of the Haumea family, (308193) 2005 CB79 is suspected of being an icy mantle collisional fragment from dwarf planet Haumea.  With an absolute magnitude (H) of 4.7, and a Haumea-family albedo of 0.7, this object would have a diameter of 158 km.Observations by Mike Brown in 2012 using the W. M. Keck Observatory suggest that (308193) 2005 CB79 does not have a companion." ] ,
        "http://xmlns.com/foaf/0.1/depiction" : [ "http://commons.wikimedia.org/wiki/Special:FilePath/TheTransneptunians_Color_Distribution-2005RR43.png" ] ,
        "http://dbpedia.org/ontology/absoluteMagnitude" : [ 4.7 ] ,
        "http://dbpedia.org/ontology/albedo" : [ 0.7 ] ,
        "http://dbpedia.org/ontology/apoapsis" : [ 7356924085284.6 ] ,
        "http://dbpedia.org/ontology/apparentMagnitude" : [ 21.1 ] ,
        "http://dbpedia.org/ontology/discoverer" : [ "http://dbpedia.org/resource/David_L._Rabinowitz",
          "http://dbpedia.org/resource/Michael_E._Brown",
          "http://dbpedia.org/resource/Chad_Trujillo" ] ,
        "http://dbpedia.org/ontology/epoch" : [ "January 10, 2010 (2455200.5)" ] ,
        "http://dbpedia.org/ontology/orbitalPeriod" : [ 8946895175.999998 ] ,
        "http://dbpedia.org/ontology/periapsis" : [ 5555017732703.1 ] ,
        "http://dbpedia.org/ontology/thumbnail" : [ "http://commons.wikimedia.org/wiki/Special:FilePath/TheTransneptunians_Color_Distribution-2005RR43.png?width=300"] } } }
