Matches in DBpedia 2016-04 for { ?s ?p "3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days."@en }
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- 3_Camelopardalis abstract "3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days.".
- Q3281140 abstract "3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days.".
- 3_Camelopardalis comment "3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days.".
- Q3281140 comment "3 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 496 light years from Earth.The primary component, 3 Camelopardalis A, is an orange K-type giant with a mean apparent magnitude of +5.07. It is a Cepheid variable star and its brightness varies from magnitude +5.05 to +5.10. The binary star revolves around its common centre of mass once every 121 days.".