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The Death March of Betelgeuse

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A Cloudy Precursor to a Violent Stellar End

You can’t see it in the evening skies right now, but the bright, old star Betelgeuse that makes up one of the shoulders of Orion, the Hunter (visible beginning late in the year), is giving up more of its secrets even as it continues down the road of old age and eventual disruption by a supernova explosion. Betelgeuse is a red supergiant star.  It’s so big that if you placed it in our solar system in place of the Sun, its “surface” would be out at the orbit of Jupiter.  But, Betelgeuse’s influences stretches far out beyond that.  Why?  You have to understand something about this big old star. It’s big. It’s old. And when big, old stars get older, they shed much of their material out to space in an intense stellar wind. In the final step of aging, such stars can lose as much as one solar mass (that is, the amount of mass it takes to make the Sun) in just about 10,000 years.

For Betelgeuse, scientists describe this mass loss as two processes:  the first occurred when huge plumes of gas began to snake their way out from the star into nearby space; the second one involves giant bubbles in the star’s atmosphere. Those bubbles move up and down through the atmosphere quite vigorously, similar to boiling water in a pan.

This picture of the dramatic nebula around the bright red supergiant star Betelgeuse was created from images taken with the VISIR infrared camera on ESO’s Very Large Telescope (VLT). This structure, resembling flames emanating from the star, forms because the behemoth is shedding its material into space. The earlier NACO observations of the plumes are reproduced in the central disc. The small red circle in the middle has a diameter about four and half times that of the Earth’s orbit and represents the location of Betelgeuse’s visible surface. The black disc corresponds to a very bright part of the image that was masked to allow the fainter nebula to be seen. Courtesy ESO/P. Kervella.

How do we know that this is what Betelgeuse is doing?  For one thing, astronomers have been able to image the plumes of material blowing away from the star. They used an instrument called VISIR (an infrared-sensitive camera) attached to the European Southern Observatory’s Very Large Telescope in Chile to measure the extent of the clouds of material coming off Betelgeuse. They found an interesting structure to the clouds (see picture at left). It almost looks like flames licking out from the star.  They’re not fire, but warm streams of  “star stuff” blowing away from Betelgeuse.

The astronomers’ observations show the plumes that are close to the star are probably connected to structures in the outer nebula now imaged in the infrared with VISIR. The nebula cannot be seen in visible light, as the very bright Betelgeuse completely outshines it.

Notice that the clouds of material are irregularly shaped, not symmetrical. This also tells astronomers that Betelgeuse hasn’t been losing its material at the same rate in all directions. In other words, the loss is not symmetrical.  This is indirect evidence that the bubbles in the atmosphere and their plumes are responsible for the nebula’s appearance.

So, what is this material that’s flowing away from Betelgeuse?

Based on the observations, it’s most likely that this stellar stuff is composed of silicate and alumina dust. This is the same material that forms most of the crust of the Earth and other rocky planets.

This is kind of interesting. Think about it.  It means that at some time in the distant past, the silicates that make up Earth were formed by a massive (and now extinct) star similar to Betelgeuse. It’s interesting to see evidence for that now, but in a star that is at least several hundred light-years away from us (possibly farther).

Now, you’re probably wondering when Betelgeuse will finally go supernova.  A good question. In cosmic timekeeping, it could be anytime, meaning anytime in the next million years. Stars die on lengthy timelines.  And, its distance will keep us from knowing that it happened until a few hundred years after the initial explosion. So, if Betelgeuse is, oh, say 500 light-years away (and we don’t know for sure how far away it is, so I’m using that number as an example), and it blows up tomorrow, we won’t see that flash in our skies until the year 2511.  We’ll probably see an influx of neutrinos before that, emanating from the direction of Betelgeuse. Eventually, sky observers will see it start to get very large and bright in the sky, and once the initial flash dies out, they’d start to see a colorful, glowing nebula where Betelgeuse used to be.  It would be a bright source in radio and x-rays, a new “thing” to study in the annals of violent star death.

For now, however, astronomers are marking the progression of Betelgeuse’s “change of life” events by observing it as much as they can, in as many regimes of light as they can. Those continue to tell the story of this star’s inevitable death march.

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From Starbirth to Stardeath…

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… and Back Again

This picture of the star formation region NGC 3582 was taken using the Wide Field Imager at ESO's La Silla Observatory in Chile. The image reveals giant loops of gas ejected by dying stars that bear a striking resemblance to solar prominences. Courtesy ESO, Digitized Sky Survey 2 and Joe DePasquale

The process of stardeath is one of those events that is not just the end of a star’s life, but possibly the beginning of another one’s existence.  In some regions of our galaxy (and in many other galaxies), the explosion of a massive star in an event called a supernova, not only ejects material from the star that will eventually be recycled into other stars. It also sends shock waves through space that can compress nearby nebulae (clouds of gas and dust). That “ripple effect” starts the nebula down the path to star formation as the material begins to coalesce, heat up, and eventually “turn on” in the process of star birth. If the birth cloud has enough heavy elements to form planets, and the conditions are right, the stellar babies could also be born with worlds of their own.  This is what happened to create our Sun and planets, more than 4.5 billion years ago.

The image above is a scene of violent stellar destruction, lit up by strong ionizing radiation (UV light) from nearby newborn stars. It’s a star-forming region in the Milky Way called RCW 57, and the nebula itself (the glowing, loop-filled cloud of gas and dust) is called NGC 3582.  Some of the stars forming in regions like NGC 3582 are much heavier than the Sun. These monster stars emit energy at prodigious rates and have very short lives that end in supernova explosions. The material ejected from these dramatic events creates bubbles in the surrounding gas and dust. This is the probable cause of the loops visible in this picture. When the stellar beacons that are heating up this cloud start to die they will also send out clouds of gas and dust like these, and the forces of their deaths may well send the clouds back through a cycle of star birth, creating new stars that will light up the death-clouds of their forebears.

The image was processed by the European Southern Observatory (ESO),  using observational data identified by Joe DePasquale, from the United States, who participated in ESO’s Hidden Treasures 2010 astrophotography competition. The activity was organised by ESO in October–November 2010, for everyone who enjoys making beautiful images of the night sky using astronomical data obtained using professional telescopes.