Iota Cassiopeiae
Constellation, Cassiopeia (constellation), Star system, Light-year, Stellar classification, Main sequence
Herausgegeben: Bert, Adam Cornelius
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Iota Cassiopeiae is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth. The primary component, Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an ² 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 orbita...
Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Iota Cassiopeiae is a star system in the constellation Cassiopeia. It is approximately 141.6 light years from Earth. The primary component, Cassiopeiae A, is a white A-type main sequence dwarf with a mean apparent magnitude of +4.64. It is classified as an ² 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.
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