Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schoolsServiss, Garrett Putman
Science
Astronomy in a nutshell : $b The chief facts and principles explained in popular language for the general reader and for schools
Serviss, Garrett Putman
Astronomy -- Juvenile literature
The most useful constellations for the beginner are those surrounding
the north celestial pole, and we give a little circular chart showing
their characteristic stars. The names of the months running round the
circle indicate the times of the year when these constellations are to
be seen on or near the meridian in the north. Turn the chart so that the
particular month is at the bottom, and suppose yourself to be facing
northward. The hour when the observation is supposed to be made is, in
every case, about 9 o'clock in the evening, and the date is about the
first of the month. The top of the chart represents the sky a little
below the zenith in the north, and the bottom represents the horizon in
the north.
[Illustration:
_Fig. 18. The North Circumpolar Stars._
]
The apparent yearly revolution of the heavens, resulting from the motion
of the earth in its orbit, causes the constellations to move westward in
a circle round the pole, at the rate of about 30° per month. But the
daily rotation of the earth on its axis causes a similar westward motion
of the heavens, at the rate of about 30° for every two hours. From this
it results that on the same night, after an interval of two hours, you
will see the constellations occupying the place that they will have, at
the original hour of observation, one month later. Thus, if you observe
their positions at 9 P.M. on the first of January, and then turn the
chart so as to bring February at the bottom, you will see the
constellations around the north pole of the heavens placed as they will
be at 11 P.M. on the first of January.
[Illustration:
_Fig. 19. Key to North Circumpolar Stars._
]
Only the conspicuous stars have been represented in the chart, just
enough being included to enable the learner to recognise the
constellations by their characteristic star groups, from which they have
received their names. The chart extends to a distance of 40° from the
pole, so that, for observers situated in the mean latitude of the United
States, none of the constellations represented ever descends below the
horizon, those that are at the border of the chart just skimming the
horizon when they are below the pole.
Public-domain text, read in full here on John Shaqi.
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