Omicron Serpentis (ο Ser / ο Serpentis) is a star in the constellation Serpens. Omicron Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +4.24. It is approximately 168 light years from Earth. It is classified as a Delta Scuti type variable star and its apparent magnitude varies by 0.01 with a period of 76 minutes.

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dbpprop:abstract
  • Omicron Serpentis (ο Ser / ο Serpentis) is a star in the constellation Serpens. Omicron Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +4.24. It is approximately 168 light years from Earth. It is classified as a Delta Scuti type variable star and its apparent magnitude varies by 0.01 with a period of 76 minutes.
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  • +4.24
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dbpprop:dec
  • -12° 52' 31"
dbpprop:distLy
  • 168 ± 9
dbpprop:distPc
  • 52 ± 3
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dbpprop:name
  • ο Serpentis
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  • 56 Serpentis, HR 6581,
    HD 160613, SAO 160747,
    HIP 86565
dbpprop:ra
  • 17h 41m 24.9s
dbpprop:spectral
  • A2Va
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rdfs:comment
  • Omicron Serpentis (ο Ser / ο Serpentis) is a star in the constellation Serpens. Omicron Serpentis is a white A-type main sequence dwarf with an apparent magnitude of +4.24. It is approximately 168 light years from Earth. It is classified as a Delta Scuti type variable star and its apparent magnitude varies by 0.01 with a period of 76 minutes.
rdfs:label
  • Omicron Serpentis
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