Introduction to the Stars
H
ow many stars can you see with the naked eye on a
clear, dark night? Many people will say, ‘Millions’, but
this is quite wrong. There are roughly 5800 stars within
naked-eye range. Only half these will be above the horizon
at any one time, and faint stars which are low down will
probably not be seen. This means that if you can see a
grand total of 2500 stars, you are doing very well.
The ancients divided up the stars into groups of constel-
lations, which were named in various ways. The Egyptians
had one method, the Chinese another, and so on; the con-
stellations we use today are those of the Greeks (admittedly
with Latin names) and if we had used one of the other sys-
tems our sky-maps would look very different, though the
stars themselves would be exactly the same. In fact, a con-
stellation pattern has no real significance, because the stars
are at very different distances from us, and we are dealing
with nothing more than line of sight effects.
Ptolemy, last of the great astronomers of Classical
times, listed 48 constellations, all of which are still given
modern maps even though they have been modified in
places. Some of the groups were named after mythological
characters, such as Orion and Perseus; others after animals
or birds, such as Cygnus (the Swan) and Ursa Major (the
Great Bear), and there are a few inanimate objects, such as
Triangulum (the Triangle). Other constellations have been
added since, notably those in the far south of the sky
which never rose above the horizon in Egypt, where
Ptolemy seems to have spent the whole of his life.
Some of the new groups have modern-sounding
names, such as Telescopium (the Telescope) and Octans
(the Octant). During the 17th century various astronomers
compiled star catalogues, usually by stealing stars from
older groups. Some of the additions have survived (includ-
ing Crux Australis, the Southern Cross), while others
have been mercifully deleted; our maps no longer show
constellations such as Globus Aerostaticus (the Balloon),
Officina Typographica (the Printing Press) and Sceptrum
Brandenburgicum (the Sceptre of Brandenburg). Today
we recognize a total of 88 constellations. They are very
unequal in size and importance, and some of them are so
obscure that they seem to have little claim to separate
identity. One can sympathize with Sir John Herschel, who
once commented that the constellation patterns seemed to
have been drawn up so as to cause the maximum possible
inconvenience and confusion.
Very bright stars such as Sirius, Canopus, Betelgeux
and Rigel have individual names, most of which are
Arabic, but in other cases a different system is used. In
1603 Johann Bayer, a German amateur astronomer, drew
up a star catalogue in which he took each constellation and
gave its stars Greek letters, starting with Alpha for the
brightest star and working through to Omega. This proved
to be very satisfactory, and Bayer’s letters are still in use,
though in many cases the proper alphabetical sequence has
not been followed; thus in Sagittarius (the Archer), the
brightest stars are Epsilon, Sigma and Zeta, with Alpha and
Beta Sagittarii very much ‘also rans’. Later in the century
John Flamsteed, the first Astronomer Royal, gave numbers
to the stars, and these too are still in use; thus Sirius, in
Canis Major (the Great Dog) is not only Alpha Canis
Majoris but also 19 Canis Majoris.
The stars are divided into classes or magnitudes
depending upon their apparent brilliance. The scheme
works rather like a golfer’s handicap, with the more bril-
liant performers having the lower values; thus magnitude 1
is brighter than 2, 2 brighter than 3, and so on. The faintest
stars normally visible with the naked eye are of magnitude
6, though modern telescopes using electronic equipment
ATLAS OF THE UNIVERSE
THE GREEK
ALPHABET
· Alpha
‚ Beta
Á Gamma
‰ Delta
 Epsilon
̇ Zeta
Ë Eta
ı Theta
È Iota
Î Kappa
Ï Lambda
Ì Mu
Ó Nu
Í Xi
Ô Omicron
Pi
Ú Rho
Û Sigma
Ù Tau
̆ Upsilon
Ê Phi
̄ Chi
„ Psi
ˆ Omega
Ursa Major (The Great
Bear). This is the most
famous of all the northern
constellations. Seven main
stars make up the ‘Plough’
or ‘Dipper’ pattern. Six
of them are white; the
seventh, Dubhe, is orange.
Orion. This brilliant
constellation is crossed by
the celestial equator, and can
therefore be seen from every
inhabited country. Its pattern
is unmistakable; two of the
stars (Rigel and Betelgeux)
are of the first magnitude,
and the remainder between
11 ⁄ 2 and 2. Like Ursa Major,
Orion is a ‘guide’ to the
constellations, though it is
out of view for part of the
year when it is close to the
Sun and above the horizon
only during daylight.
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