19 Canum Venaticorum is a binary star in the constellation Canes Venatici. It is approximately 245 light years from Earth. The primary component, 19 Canum Venaticorum A, is a white A-type main sequence dwarf with an apparent magnitude of +5.77. It's companion, 19 Canum Venaticorum B, is a tenth magnitude star located only 0.37 arcseconds from the primary.

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  • 19 Canum Venaticorum is a binary star in the constellation Canes Venatici. It is approximately 245 light years from Earth. The primary component, 19 Canum Venaticorum A, is a white A-type main sequence dwarf with an apparent magnitude of +5.77. It's companion, 19 Canum Venaticorum B, is a tenth magnitude star located only 0.37 arcseconds from the primary.
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  • +5.77
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  • +40°51′19″
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  • 245 ± 14
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  • 75 ± 4
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  • 19 Canum Venaticorum
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  • HR 5004, HD 115271, BD+41°2374, HIP 64692, SAO 44531, GC 17953, CCDM 13155+4051
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  • 13h15m32.0s
dbpprop:spectral
  • A7V
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  • 19 Canum Venaticorum is a binary star in the constellation Canes Venatici. It is approximately 245 light years from Earth. The primary component, 19 Canum Venaticorum A, is a white A-type main sequence dwarf with an apparent magnitude of +5.77. It's companion, 19 Canum Venaticorum B, is a tenth magnitude star located only 0.37 arcseconds from the primary.
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  • 19 Canum Venaticorum
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