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.