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This is the fabulous Crab Nebula in the constellation Taurus (the Bull). What we see here are the remains of a star that went supernova (exploded violently). In 1050 A.D., Chinese astronomers noted a "guest star" in the skies in precisely this position. When stars go supernova, they can temporarily produce more light than the entire galaxy in which they are contained, and this star was no exception; for weeks it was visible in broad daylight.
What remains now are glowing tendrils of hydrogen gas that seem woven among a ghostly bluish glow. At the center of this cloud is the fading ember of the original star, an intriguing object with roughly the mass of our sun, but compressed to the size of a city: a neutron star. Highly magnetized, and spinning at a fantastic rate of 33 times per second, it sends out powerful radio pulses that can be picked up here on Earth. It is this same spinning motion that provides the energy that lights up the Crab Nebula.
Image and text copyright © Russell Croman. All rights reserved. |
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