53 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 321 light years from Earth. The binary has an orbital period of 6.52 years. The primary component, 53 Camelopardalis A, is a white A-type main sequence dwarf with a mean apparent magnitude of +6.02. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +5.95 to +6.08 with a period of 8.03 days.

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dbpprop:abstract
  • 53 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 321 light years from Earth. The binary has an orbital period of 6.52 years. The primary component, 53 Camelopardalis A, is a white A-type main sequence dwarf with a mean apparent magnitude of +6.02. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +5.95 to +6.08 with a period of 8.03 days.
dbpprop:appmagV
  • +6.02
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dbpprop:dec
  • +60°19′28″
dbpprop:distLy
  • 321 ± 24
dbpprop:distPc
  • 98 ± 7
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dbpprop:name
  • 53 Camelopardalis
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  • AX Camelopardalis, HR 3109, HD 65339, BD+60°1105, FK5 302, HIP 39261, SAO 14402, GC 10822, CCDM 08017+6019
dbpprop:ra
  • 08h01m42.4s
dbpprop:spectral
  • A2pSrCrEu
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  • 53 Camelopardalis is a spectroscopic binary in the constellation Camelopardalis. It is approximately 321 light years from Earth. The binary has an orbital period of 6.52 years. The primary component, 53 Camelopardalis A, is a white A-type main sequence dwarf with a mean apparent magnitude of +6.02. It is classified as an Alpha2 Canum Venaticorum type variable star and its brightness varies from magnitude +5.95 to +6.08 with a period of 8.03 days.
rdfs:label
  • 53 Camelopardalis
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