The southern arm of the Andromeda galaxy, M31
AAO image reference INT 3.    « Previous || Next »
southern arm of M31
Top left is NE. Image width is about 38 arc min
© 1991-2002, Malin/IAC/RGO. Photograph from Isaac Newton Telescope plates by David Malin.

M31 is the finest and nearest large spiral galaxy in the sky, about 2 million light years away. Despite its distance it can be seen as an elongated streak with the unaided eye in northern skies and in a large telescope under good conditions it is clearly resolved into stars and star-forming regions. This picture shows less than half the galaxy but the spiral structure, star clouds and dust lanes are evident. Also here is one of M31's close companions, the compact elliptical galaxy M32 (NGC 221), at upper left (NE). M31 and its companions belong to the Local Group of about 30 galaxies that includes the Milky Way and M31 as its most massive members as well as the Magellanic Clouds.

This picture is about half a degree across and is of the same region as the frontispiece in Hubble's famous book "The Realm of the Nebulae" (Harvard UP, 1936). In his illustration Hubble points out a Cepheid variable star, a globular cluster, a star cloud and open cluster as typical ingredients of a spiral galaxy. The star cloud is so conspicuous that it has its own New General Catalogue number, NGC 206

Entry from NGC 2000.0 (R.W. Sinnott, Ed.) © Sky Publishing Corporation, 1988:
NGC  224  Gx 00 42.7  +41 16 s  And 178. 3.5  !!! eeB, eL, vmE (Andromeda); = M31
More data about this galaxy is accessible from the hotlinked NGC name and is reproduced
with permission from the NASA/IPAC Extragalactic Database (NED). Related images
INT 1.  The nucleus of M31, direct image
INT 2.  The nucleus of M31, unsharp mask
Caltech M31The Andromeda galaxy, M31 and its companions.

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