Mira Ceti


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Related to Mira Ceti: Omicron Ceti

Mira Ceti

(ˈmaɪrə ˈsiːtaɪ)
n
(Celestial Objects) a binary star one component of which, a red supergiant, is a long-period variable with an average period of 332 days
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They contain valuable observations of Mira Ceti in the years 1751-1782....
This origin is thought to be the Milky Way, the nebulas or stars of the Mira Ceti type.
Mira Ceti remained unique until 1686, when a second Mira-type variable was found: Chi ([Chi]) Cygni.