Pi Cassiopeiae (π Cas / π Cassiopeiae) is a star in the constellation Cassiopeia. π Cassiopeiae is a white A-type main sequence dwarf with a mean apparent magnitude of +4.95. It is approximately 174.3 light years from Earth. It is classified as a rotating ellipsoidal variable star and its brightness varies by 0.02 magnitudes with a period of 23.57 hours.

PropertyValue
dbpedia-owl:thumbnail
dbpprop:absmagV
  • +1.31
dbpprop:abstract
  • Pi Cassiopeiae (π Cas / π Cassiopeiae) is a star in the constellation Cassiopeia. π Cassiopeiae is a white A-type main sequence dwarf with a mean apparent magnitude of +4.95. It is approximately 174.3 light years from Earth. It is classified as a rotating ellipsoidal variable star and its brightness varies by 0.02 magnitudes with a period of 23.57 hours.
dbpprop:appmagV
  • +4.95
dbpprop:bV
  • +0.18
dbpprop:class
  • A5V
dbpprop:constell
dbpprop:dec
  • +47°01′29″
dbpprop:distLy
  • 174.3 (xsd:double)
dbpprop:distPc
  • 53.4 (xsd:double)
dbpprop:epoch
dbpprop:hasPhotoCollection
dbpprop:name
  • π Cassiopeiae
dbpprop:pError
  • 0.73 (xsd:double)
dbpprop:parallax
  • 18.71 (xsd:double)
dbpprop:propMoDec
  • −37.16
dbpprop:propMoRa
  • −24.52
dbpprop:ra
  • 00h43m28.1s
dbpprop:radialV
  • 13 (xsd:integer)
dbpprop:uB
  • +0.09
dbpprop:variable
dbpprop:wikiPageUsesTemplate
rdf:type
rdfs:comment
  • Pi Cassiopeiae (π Cas / π Cassiopeiae) is a star in the constellation Cassiopeia. π Cassiopeiae is a white A-type main sequence dwarf with a mean apparent magnitude of +4.95. It is approximately 174.3 light years from Earth. It is classified as a rotating ellipsoidal variable star and its brightness varies by 0.02 magnitudes with a period of 23.57 hours.
rdfs:label
  • Pi Cassiopeiae
owl:sameAs
skos:subject
foaf:depiction
foaf:page
is owl:sameAs of