Mira, designation Omicron Ceti, is a red-giant star estimated to be 200–300 light-years from the Sun in the constellation Cetus.
Mira at two different times
Mira as seen from the Earth
Mira in UV and visible light
Mira as seen by the Hubble Space Telescope in August 1997
A red giant is a luminous giant star of low or intermediate mass in a late phase of stellar evolution. The outer atmosphere is inflated and tenuous, making the radius large and the surface temperature around 5,000 K or lower. The appearance of the red giant is from yellow-white to reddish-orange, including the spectral types K and M, sometimes G, but also class S stars and most carbon stars.
An illustration of the structure of the Sun and its possible future as a red giant, comparing their structure and size.
This image tracks the life of a Sun-like star, from its birth on the left side of the frame to its evolution into a red giant on the right after billions of years
Mira A is an old star, already shedding its outer layers into space