
Mira Ceti
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Mira is a binary star system in the constellation Cetus. It has the Bayer designation Omicron Ceti, which is Latinized from ο Ceti, and abbreviated Omicron Cet or ο Cet. The system consists of a variable red giant along with a white dwarf companion. Mira A is a pulsating variable star and was the first non-supernova variable star discovered, with the possible exception of Algol. It is the prototype of the Mira variables. The system lies at a distance of 300 light-years.
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Zulaye
Himest Mesi
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Uriat
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Esker mila
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Lesole
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Ani Kuni
Ani Kuni
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Kakhuri nana
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Balulu
Ament
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Nonooni
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Sudrabina
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