AR Aurigae (AR Aur) is an eclipsing binary in the constellation Auriga. It is approximately 398 light-years from Earth. Both components are blue-white B-type or main sequence dwarfs which do not fill their Roche lobes. The system has a with a mean apparent magnitude of +6.15 but because of the eclipses, AR Aurigae is a variable star and its brightness varies from magnitude +6.15 to +6.82 with a period of 4.13 days.

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dbpprop:abstract
  • AR Aurigae (AR Aur) is an eclipsing binary in the constellation Auriga. It is approximately 398 light-years from Earth. Both components are blue-white B-type or main sequence dwarfs which do not fill their Roche lobes. The system has a with a mean apparent magnitude of +6.15 but because of the eclipses, AR Aurigae is a variable star and its brightness varies from magnitude +6.15 to +6.82 with a period of 4.13 days.
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  • 6.143 (xsd:double)
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  • -0.06 (xsd:double)
dbpprop:caption
  • AR Aurigae
dbpprop:class
  • B9.5V
dbpprop:constell
dbpprop:dec
  • +33° 46′ 02.454″
dbpprop:epoch
  • J2000
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  • 20000 (xsd:integer)
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  • 18 (xsd:integer)
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  • 0.78 (xsd:double)
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  • 8.2 (xsd:double)
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  • -29.06 (xsd:double)
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  • 15.09 (xsd:double)
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  • 05h 18m 18.8994s
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  • 7 (xsd:integer)
dbpprop:reference
dbpprop:rotation
  • 58 Km/s
    0,0167514 Year
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  • HD+34364
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  • CCDM
  • HIP
  • HR
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  • 10,000–30,000
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  • -0.18 (xsd:double)
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  • AR Aurigae (AR Aur) is an eclipsing binary in the constellation Auriga. It is approximately 398 light-years from Earth. Both components are blue-white B-type or main sequence dwarfs which do not fill their Roche lobes. The system has a with a mean apparent magnitude of +6.15 but because of the eclipses, AR Aurigae is a variable star and its brightness varies from magnitude +6.15 to +6.82 with a period of 4.13 days.
rdfs:label
  • AR Aurigae
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