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Mira the Wonderful

This star in the constellation Cetus varies in brightness over about 11 months. Its next brightness maximum is due in early 2017.

Mira, from NASA's Galaxy Evolution Explorer

The star Mira has a comet-like tail, discovered in 2007. The tail stretches 13 light-years in space. Image via NASA’s Galaxy Evolution Explorer.

The star Omicron Ceti – proper name Mira and known to early astronomers as Mira the Wonderful – lies 420 light-years away in the constellation Cetus the Whale. It’s in an unremarkable patch of the night sky along the celestial equator, well to the west of the hard-to-miss constellation Orion the Hunter. Mira is visible to the unaided eye – except when it isn’t, which is most of the time. And that’s why it earned the name wonderful, in the sense of arousing wonder.

Today we know this star varies in brightness. Its changes happen on a regular schedule of about 11 months. Mira’s last brightness peak was in March of 2016. Its next brightness peak is scheduled for around February, 2017.

How bright Mira will become at its next peak also isn’t as predictable.

You should be able to spot Mira's constellation, Cetus, during the evening hours.  Mira won't be visible, though.  Its next brightness peak will come in May, 2015.

You should be able to spot Mira’s constellation, Cetus, during the evening hours. Will Mira be visible? Maybe. Look and see.

Here’s what we do know about Mira. This star varies in brightness on a fairly regular schedule. Its unusual fluctuations were known to modern astronomers as far back as at least the late 16th century. In 1662, German-Polish astronomer Johannes Hevelius named it Mira (meaning wonderful or astonishing in Latin).

Throughout the centuries, Mira has been as bright as 2nd magnitude (approaching the noticeability of the stars of the Big Dipper), but it usually peaks at about magnitude 3.5, putting it below the brightness of other stars in Cetus. At its dimmest, Mira falls to 10th magnitude, below the visibility limit of modest binoculars. That’s an overall factor of more than 1,500 times. Astonishing, indeed!

Mira varies because it’s past its prime. It has exhausted most of its hydrogen fuel and puffed up to become a red giant. The last gasps of its stellar furnace make the star pulsate and throw off its outer layers. Eventually, most of it will be gone, leaving behind a shell of gas called a planetary nebula that will surround the stellar cinder called a white dwarf.

As modern astronomers study the star, Mira continues to amaze. In 2007, observations by a satellite viewing in ultraviolet light discovered that Mira has a luminous tail of gas more than a dozen light-years long. This is the material that Mira has shed, leaving it behind as it speeds through the galaxy at some 80 miles per second (130 km per second) – very speedy for a star! The invisible tail spans about 2 degrees in the sky, about four times the diameter of a full moon. See the image at the top of this post.

Bottom line: The star Omicron Ceti – aka Mira – in the constellation Cetus varies in brightness regularly, over about 11 months. That’s why, for centuries, stargazers have called it Mira the Wonderful.

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