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The Andromeda Galaxy is most
visible in the northern sky towards the end of autumn and beginning of
winter. The constellation of Andromeda is simple to locate: an imaginary
line from the pole star through the "W" of Cassiopeia leads directly to
it, and the pale form of the Andromeda Galaxy is not hard to find in its
central regions.
Our local group of galaxies is relatively small in comparison to many others: it contains no more than about thirty galactic systems. Our own Galaxy and the Triangulum Galaxy are among the most prominent members, but easily the largest is the huge spiral of the Andromeda Galaxy with roughly twice the mass of our own Milky Way. Though the Andromeda Galaxy is considerably larger than our own, the two share many common features. Both have a clearly recognizable spiral structure, and both have various attendant dwarf galaxies associated with them. For the Milky Way, the most prominent of these are the Magellanic Clouds, while for the Andromeda Galaxy this role is fulfilled by several small galaxies, especially the two catalogued as M32 and NGC205 The distance to the Andromeda Galaxy is immense – some 2,300,000 light years, but nonetheless its vast size and luminosity mean that it is still visible to the naked eye. (In fact, it is the most distant object that can been seen without a telescope). Even so, much of the structure in its spiral arms is too faint to be seen, so that it appears smaller than it actually is. If we could see the entire galaxy, it would occupy an area of the sky nearly six times the size of the Moon’s disc. |
| *Source: eSky, "The Electronic Sky" |
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Andromeda Galaxy* 
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Andromeda Galaxy,
