Observing the night sky,
in 1744, a teenaged boy from Badonviller, France - Charles Messier - saw something unusual. It wasn’t the first time this keenly observant lad had studied the heavens. But on this night, he saw
a comet which had developed six tails.
A contemporary artist
recorded how
the comet appeared when its
head was below the horizon. By March 8, 1744, the comet was visible in the predawn sky, its tails resembling a Japanese fan.
Messier, for years thereafter, continued to search the sky hoping to see (or discover) more comets.
The Frenchman thus grew up with a profound love of astronomy. Observing, and
recording, what he saw in the heavens became a career for him. Astronomers still use
“M” designations, based on a catalog
he created, to identify deep-sky objects with fixed positions.
His list includes such things as “fuzzy” non-comets known as nebulae. M1 (or, Messier 1), for example, is another name for the Crab Nebula.
Observed by
Chinese astronomers in 1054 AD - when it was an
exploding
supernova
- and discovered in 1731 by
John Bevis (a British physician and amateur astronomer), the
Crab Nebula is still one of the
most studied of all objects in the sky. It takes its name from an 1844 (or thereabouts)
drawing by
William Parsons, the Third Earl of Rosse, who observed it with a
36-inch reflector at his home,
Birr Castle, near Parsonstown,
County Offaly, Ireland. Thanks to the Hubble telescope, we can
examine it in much
greater detail than Lord Rosse could have ever imagined - even with his later
72-inch
telescope which, for nearly a century, was the
biggest in the world.
Hubble’s image of the Crab - assembled from twenty-four separate exposures - provides astronomers with
incredible detail of
the nebula. And, because of
the space telescopes (Hubble,
Spitzer and
Chandra), scientists have learned how the
Crab moves (don’t miss this animation) through space: It is
propelled by a dynamic
pulsar [PULSating stAR] at
its core.
As we continue our virtual
visit to space, let’s examine a few more notable nebulae.