Matches in DBpedia 2016-04 for { ?s ?p "Iota Cancri (ι Cnc, ι Cancri) is a double star in the constellation Cancer. The brighter component is approximately 298 light years from Earth.The brighter star is a yellow G-type bright giant with an apparent magnitude of +4.02. The companion is a white A-type main sequence dwarf with an apparent magnitude of +6.57. The two stars are separated by 30.6 arcseconds on the sky, and are resolvable through a small telescope.Despite having different distances when measured by the HIPPARCOS satellite, the two stars share a common proper motion and appear to be a natural binary star system."@en }
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- Iota_Cancri abstract "Iota Cancri (ι Cnc, ι Cancri) is a double star in the constellation Cancer. The brighter component is approximately 298 light years from Earth.The brighter star is a yellow G-type bright giant with an apparent magnitude of +4.02. The companion is a white A-type main sequence dwarf with an apparent magnitude of +6.57. The two stars are separated by 30.6 arcseconds on the sky, and are resolvable through a small telescope.Despite having different distances when measured by the HIPPARCOS satellite, the two stars share a common proper motion and appear to be a natural binary star system.".
- Q2333595 abstract "Iota Cancri (ι Cnc, ι Cancri) is a double star in the constellation Cancer. The brighter component is approximately 298 light years from Earth.The brighter star is a yellow G-type bright giant with an apparent magnitude of +4.02. The companion is a white A-type main sequence dwarf with an apparent magnitude of +6.57. The two stars are separated by 30.6 arcseconds on the sky, and are resolvable through a small telescope.Despite having different distances when measured by the HIPPARCOS satellite, the two stars share a common proper motion and appear to be a natural binary star system.".