Crab Nebula: Awesome Beauty From Destruction

The Crab Nebula as seen through Chabot Space & Science Center’s 8-inch refracting telescope, Leah. Image: Conrad Jung, Chabot Space & Science CenterWhen asked what got me interested in astronomy, the stock answer I offer is my childhood experience going to Chabot Observatory and looking through the telescopes—and I'm sure that had a great deal to do with it. But, if I want to give an even shorter answer, I just say, "Crab Nebula!" and walk away….

What's the Crab Nebula? Astronomy enthusiasts are very familiar with this celestial object, or at least become so very quickly after entering the world of space. It's a supernova remnant—a torn and tortured cloud of gases expanding outward into space, the aftermath of a supernova explosion that happened almost a thousand years ago in the constellation Taurus. In fact, as I write this blog, the age of the Crab Nebula is exactly 955 years and 40 days.

How do we know with such precision when this former star went supernova? The answer, as always in science, is careful observation! The explosion of the star was witnessed by Chinese and Japanese astronomers—and possibly sky watchers of the American Southwest—who carefully observed and recorded the event. The explosion took place on July 4th, 1054 CE.

Seven hundred years later, a century after the invention of the telescope, the Crab Nebula was discovered in the same spot—first in 1731 by John Bevis, then again by Charles Messier in 1758 (August 28, in fact—the date of this blog posting!). Messier ran across it while searching for Halley's Comet, and at first mistook it for a comet. This was the reason that he began compiling his famous Messier catalog of "fuzzy" objects: a wall of mug shots of unusual suspects that resembled, but were imposters of, comets. He began his catalog with Messier 1 (M1), the Crab Nebula.

Messier 1 got its nickname of the Crab from a drawing made by observer Lord Rosse in 1844.
Today, the Crab Nebula is an expanding cloud of gas and some dust spanning 10 light years, or 60 trillion miles. The cloud is still expanding at a speed of about 1,800 kilometers per second—a speed that would get you to the Moon in just under 4 minutes! At its center is the collapsed remnant of the dead star's core, which has become the incredibly small and dense object known as a neutron star.

So why did the Crab Nebula spark my interest in astronomy? I have a specific memory of being at a summer camp and engaging in a craft activity where we cut out the pictures from a bunch of astronomy calendars and made frames and matting to display them in. I selected a few of my favorite images, which included the Dumbbell Nebula (a planetary nebula), the Veil Nebula (another supernova remnant), and, of course, the Crab. Of all these stunning astrophotos, it was the Crab that stuck the longest in my mind and on my bedroom wall, and impelled me to get my first subscription to Astronomy Magazine, and eventually my first telescope. Sometimes, our lives are guided by stars….

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  • john trenholme

    I happened to run across your blog on the crab nebula and couldn't help but notice that you identified the date of the supernova as the year 1054, the year the event was seen here on earth. The nebula is several thousand light years away, however, so the supernova actually occurred several millennia BCE. People so often seem to forget that the universe we see today is only an image of the universe as it existed thousands or millions of years ago, depending on what you're looking at. It's the closest thing we have to an ability to travel back in time.

  • http://www.chabotspace.org Ben Burress

    Point taken, John; thanks. I could have phrased that better, such as "the supernova was observed on July 4th, 1054 AD." But you are of course correct.