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    { "id" : "http://dbpedia.org/resource/Stellar_classification"
      "properties" : {
        "http://www.w3.org/2000/01/rdf-schema#comment" : [ "In astronomy, stellar classification is the classification of stars based on their spectral characteristics.  Light from the star is analyzed by splitting it with a prism or diffraction grating into a spectrum exhibiting the rainbow of colors interspersed with absorption lines.  Each line indicates an ion of a certain chemical element, with the line strength indicating the abundance of that ion.  The relative abundance of the different ions varies with the temperature of the photosphere." ] ,
        "http://www.w3.org/2000/01/rdf-schema#seeAlso" : [ "http://dbpedia.org/resource/K-type_main-sequence_star",
          "http://dbpedia.org/resource/O-type_main-sequence_star",
          "http://dbpedia.org/resource/F-type_main-sequence_star",
          "http://dbpedia.org/resource/G-type_main-sequence_star",
          "http://dbpedia.org/resource/Red_dwarf",
          "http://dbpedia.org/resource/A-type_main-sequence_star",
          "http://dbpedia.org/resource/B-type_main-sequence_star",
          "http://dbpedia.org/resource/Sub-brown_dwarf" ] ,
        "http://xmlns.com/foaf/0.1/depiction" : [ "http://commons.wikimedia.org/wiki/Special:FilePath/TernaryColorTmap.PNG" ] ,
        "http://dbpedia.org/ontology/thumbnail" : [ "http://commons.wikimedia.org/wiki/Special:FilePath/TernaryColorTmap.PNG?width=300"] } } }
