Aquarius and Capricornus
Andromeda is one of the most prominent constellations in the evening
sky in autumn and early winter. It is also quite easy to find, with its three brightest
stars almost in a straight line immediately east of the Great Square of Pegasus. All
three of these stars are second magnitude and one of them, Alpheratz, although deemed
to belong to Andromeda is actually one of the corner stars of the Great Square of Pegasus.
M31, The Andromeda galaxy
The middle
star of the three, Mirach, leads us to Andromeda’s showpiece, the
Great Andromeda Nebula, M31. This is close to the second of two fainter
stars in a line north of Mirach, more or less at right angles to the line
of the three bright stars. On a dark night with a clear sky it can be
seen quite easily with the naked eye, being about magnitude 3.5. M31 is
the nearest major galaxy to our own Milky Way and the largest galaxy in
the so-called “Local Group”. It contains some 200 million
stars – about twice as many as the Milky Way. This means that, despite
its immense distance – over 2 million light years, M31 is such a
large object that the best views of it are in fact through good binoculars
rather than a telescope. Under good conditions, binoculars might also
pick up the two eighth magnitude satellite galaxies M32 & M110 and
these two are certainly well seen in even a small telescope.
The last
of Andromeda’s three main stars, Almach, is one of the finest doubles
in the sky, consisting of a golden second magnitude primary and a bluish
fifth magnitude secondary. The separation (10 seconds of arc) means that
they can be comfortably split even by quite small telescopes. The companion
star is double again but the separation of this pair is too small for
amateur instruments. The brightest member of the close pair is itself
a spectroscopic binary, so that Almach is in fact a quadruple system.
Fairly
close to Almach is the open cluster NGC 752, a large cluster of fairly
bright stars, which like M31 is better observed in binoculars than telescopes.
A different proposition altogether is the edge-on spiral galaxy NGC 891,
about ten times further away than M31. Due to its low surface brightness
an aperture of at least 6”, a dark sky and excellent conditions
are required to be able to see it. Finally in Andromeda the “Blue
Snowball” planetary nebula (NGC 7662) is worth tracking down if
you have a telescope. It is an excellent example of an object which is
far more conspicuous with averted vision than when viewed directly.
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