Quantcast

Whirlpool Galaxy (M51)

Whirlpool Galaxy — Discovered 1773 by Charles Messier.

The famous Whirlpool galaxy M51 was one of Charles Messier’s original discoveries: He discovered it on October 13, 1773, when observing a comet, and described it as a “very faint nebula, without stars” which is difficult to see.

Its companion, NGC 5195, was discovered in 1781 by his friend, Pierre Mchain, so that it is mentioned in Messier’s 1784 catalog: `It is double, each has a bright center, which are separated 4’35″. The two “atmospheres” touch each other, the one is even fainter than the other.’ NGC 5195 was assigned an own number by William Herschel: H I.186.

Occasionally, there is some confusion what is meant with the designation M51: The pair (justified by Messier’s mention of both “nebulae”) or the larger galaxy, NGC 5194. If the pair is meant, NGC 5194 is sometimes called “M51A”, and NGC 5195 is then “M51B”.

M51 is the dominating member of a small group of galaxies. As it is about 37 million light years distant and so conspicuous, it is actually a big and luminous galaxy. The value of M51′s (and the whole group’s) distance is still not very well known.

Our value, of 37 Mly, is based on photometric methods and e.g. given by Kenneth Glyn Jones. Some authors give significantly lower values (less than 20 Mly), but a recent (2001) STScI Press Release gave 31 million light years.

This galaxy was the first one where the spiral structure was discovered, in spring 1845 by Lord Rosse, who made a very careful and acurate painting. Therefore, M51 is sometimes referenced as Rosse’s Galaxy or Lord Rosse’s “Question Mark” – he is cited with this name (see, e.g., NED).

According to our present understanding, the pronounced spiral structure is a result of M51′s current encounter with its neighbor, NGC 5195 (the fainter one in Messier’s description). Due to this interaction, the gas in the galaxy was disturbed and compressed in some regions, resulting in the formation of new young stars.

As is common in galactic encounters, spiral structure is preferably induced in the more massive galaxy. Halton Arp has included M51 as No. 85 in his Catalogue of Peculiar Galaxies as “Spiral with Large High-Surface-Brightness Companion”.

For the amateur, M51 is easy and a showpiece if the sky is dark, but is quite sensitive for light pollution which easily makes it fade in the background. Under very cood conditions, even suggestions of its spiral arms can be glanced with telescopes starting from 4-inch. Low magnification is best for viewing this pair.

The Hubble Space Telescope has investigated especially the central region of M51. Its compact nucleus is now classified as of Seyfert type 2.5. Newer HST investigations (published 2001) focus on investigation of the inner spiral arms and dust clouds, which are the birth sites of massive and luminous stars. ESA’s ISO (Infrared Space Observatory) satellite has investigated the Whirlpool Galaxy in the infrared light.

—–

NASA

Click here to learn more on this topic from eLibrary:

Whirlpool Galaxy M51


comments powered by Disqus