• Mira, also called omicron Ceti, was the first pulsating variable star to be discovered. At first, it was thought to be a nova… a star that brightens then fade from view forever. But in the early 1600's, astronomers discovered it changed periodically every 11 months or so.
• Mira is the brightest long-period pulsating variable in the sky. It varies from magnitude 2.0 to 10.0, roughly. That's a factor of 1,500 in brightness… a huge change. But it's not always completely regular in its extremes. For a few months every year you see it, then you don't. Here's how to find it.
• Why does Mira pulsate? The short answer is that it's going through a phase of evolution where the pull of gravity and the unsteady burning of fuel in its core fight against each other. Each dominates for a few months before the other takes over. It's a little of like a weight on the end of a spring bobbing up and down in the Earth's gravitational field: the spring pulls up, the Earth pulls down, again and again.
• The Hubble Space telescope has imaged Mira and shown it to be not spherical but asymmetrical… very strange:

An image of irregularly-shaped variable star Mira
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