This HTML5 document contains 5 embedded RDF statements represented using HTML+Microdata notation.

The embedded RDF content will be recognized by any processor of HTML5 Microdata.

PrefixNamespace IRI
dbpedia-owlhttp://dbpedia.org/ontology/
foafhttp://xmlns.com/foaf/0.1/
rdfshttp://www.w3.org/2000/01/rdf-schema#
n4http://commons.wikimedia.org/wiki/Special:FilePath/Sun920607.
rdfhttp://www.w3.org/1999/02/22-rdf-syntax-ns#
n7http://commons.wikimedia.org/wiki/Special:FilePath/Sun920607.jpg?width=
xsdhhttp://www.w3.org/2001/XMLSchema#
dbpediahttp://dbpedia.org/resource/
Subject Item
dbpedia:Main_sequence
rdfs:comment
In astronomy, the main sequence is a continuous and distinctive band of stars that appears on plots of stellar color versus brightness. These color-magnitude plots are known as Hertzsprung–Russell diagrams after their co-developers, Ejnar Hertzsprung and Henry Norris Russell. Stars on this band are known as main-sequence stars or "dwarf" stars.After a star has formed, it generates thermal energy in the dense core region through the nuclear fusion of hydrogen atoms into helium.
rdfs:seeAlso
dbpedia:Stellar_nucleosynthesis dbpedia:Stellar_evolution
foaf:depiction
n4:jpg
dbpedia-owl:thumbnail
n7:300