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- Q2527492 subject Q6271579.
- Q2527492 subject Q7216027.
- Q2527492 subject Q7217188.
- Q2527492 subject Q7724320.
- Q2527492 subject Q8216920.
- Q2527492 subject Q8236110.
- Q2527492 subject Q8293947.
- Q2527492 subject Q8790837.
- Q2527492 abstract "Iota Cassiopeiae (ι Cas, ι Cassiopeiae) is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth.The primary component, ι Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an α² Canum Venaticorum type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days. Component A is a spectroscopic binary. Its unresolved companion has an orbital period of 52.4 years and is separated from the primary by 0.113 arcseconds, or at least 5 AU.The second astrometric component, ι Cassiopeiae B, is a yellow-white F-type main sequence dwarf with an apparent magnitude of +6.89. It is 2.27 arcseconds, or at least 100 AU, from the primary. It has an orbital period of 840 years. The third astrometric component, ι Cassiopeiae C, is a yellow G-type dwarf, with an apparent magnitude of +8.40. It is 7.3 arcseconds (at least 300 AU) from the primary.Template:Multi-star-stub".
- Q2527492 thumbnail Iota_cassiopeiae_diagram.jpg?width=300.
- Q2527492 wikiPageWikiLink Q10464.
- Q2527492 wikiPageWikiLink Q111130.
- Q2527492 wikiPageWikiLink Q1141942.
- Q2527492 wikiPageWikiLink Q124313.
- Q2527492 wikiPageWikiLink Q13424908.
- Q2527492 wikiPageWikiLink Q179600.
- Q2527492 wikiPageWikiLink Q1811.
- Q2527492 wikiPageWikiLink Q2.
- Q2527492 wikiPageWikiLink Q22066400.
- Q2527492 wikiPageWikiLink Q2703.
- Q2527492 wikiPageWikiLink Q3450.
- Q2527492 wikiPageWikiLink Q37640.
- Q2527492 wikiPageWikiLink Q499138.
- Q2527492 wikiPageWikiLink Q50053.
- Q2527492 wikiPageWikiLink Q531.
- Q2527492 wikiPageWikiLink Q555846.
- Q2527492 wikiPageWikiLink Q595871.
- Q2527492 wikiPageWikiLink Q6243.
- Q2527492 wikiPageWikiLink Q6271579.
- Q2527492 wikiPageWikiLink Q7216027.
- Q2527492 wikiPageWikiLink Q7217188.
- Q2527492 wikiPageWikiLink Q7724320.
- Q2527492 wikiPageWikiLink Q8216920.
- Q2527492 wikiPageWikiLink Q8236110.
- Q2527492 wikiPageWikiLink Q8293947.
- Q2527492 wikiPageWikiLink Q845735.
- Q2527492 wikiPageWikiLink Q8790837.
- Q2527492 wikiPageWikiLink Q8928.
- Q2527492 wikiPageWikiLink Q984158.
- Q2527492 comment "Iota Cassiopeiae (ι Cas, ι Cassiopeiae) is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth.The primary component, ι Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an α² Canum Venaticorum type variable star and the brightness of the system varies from magnitude +4.45 to +4.53 with a period of 1.74 days. Component A is a spectroscopic binary.".
- Q2527492 label "Iota Cassiopeiae".
- Q2527492 depiction Iota_cassiopeiae_diagram.jpg.