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Subject Item
dbpedia:Sub-brown_dwarf
rdfs:comment
A sub-brown dwarf or planetary-mass brown dwarf is an astronomical object formed in the same manner as stars and brown dwarfs (i.e. through the collapse of a gas cloud) but that has a mass below the limiting mass for thermonuclear fusion of deuterium (about 13 MJ).Some researchers call them free-floating planets whereas others call them planetary-mass brown dwarfs.
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