NASA previews Eta Carinae supernova

At the turn of the 19th century, the binary star system Eta Carinae appeared faint and rather undistinguished to astronomers.

However, during the first decades of the century, the system became brighter and brighter, until, by April 1843, it was the second brightest star in the sky, outshone only by Sirius (which is almost a thousand times closer to Earth). 

In subsequent years, Eta Carinae gradually dimmed again and by the 20th century was totally invisible to the naked eye.

The star has continued to vary in brightness ever since, and while it is once again visible to the naked eye on a dark night, it has never again come close to its peak of 1843.

The larger of the two stars in the Eta Carinae system is a huge and unstable star nearing the end of its life.

As such, the event witnessed by 19th century astronomers is now known to be a stellar near-death experience. 

Scientists call these outbursts supernova impostor events, because they appear similar to supernovae – but stop just short of destroying their star.

Although 19th century astronomers did not have telescopes powerful enough to see the 1843 outburst in detail, its effects can be studied today. Indeed, NASA’s Hubble Telescope recently captured an image of Eta Carinae consisting of ultraviolet and visible light image.

The huge clouds of matter thrown out a century and a half ago, known as the Homunculus Nebula, have been a regular target for Hubble since its launch in 1990. The image, snapped with the Advanced Camera for Surveys High Resolution Channel, is the most detailed yet, and shows how the material from the star was not thrown out in a uniform manner, but rather, forms a huge dumbbell shape.

Eta Carinae is not only interesting because of its past, but also because of its future. To be sure, it is one of the closest stars to Earth that is likely to explode in a supernova in the relatively near future. Of course,  in astronomical timescales the “near future” could still be a million years away.