But this is not all; soon a new use was found for the spectroscope. We
found that we could measure with it the most difficult of all speeds
to measure, speed in the line of sight. Movement at right angles to the
direction in which one is looking is, if there is sufficient of it, easy
to detect, and, if the distance of the moving body is known, easy to
measure. But movement in the line of vision is both difficult to detect
and difficult to measure. Yet, even at the enormous distances with which
astronomers have to deal, the spectroscope can detect such movement and
furnish data for its measurement. If a luminous body containing, say,
sodium is moving rapidly towards the spectroscope, it will be found that
the sodium lines in the spectrum have moved slightly from their usual
definite positions towards the violet end of the spectrum, the amount of
the change of position increasing with the speed of the luminous body.
If the body is moving away from the spectroscope the shifting of the
spectral lines will be in the opposite direction, towards the red end of
the spectrum. In this way we have discovered and measured movements that
otherwise would probably not have revealed themselves unmistakably to us
for thousands of years. In the same way we have watched, and measured
the speed of, tremendous movements on the sun, and so gained proof that
the vast disturbances we should expect there actually do occur.
[Illustration: THE SPECTROSCOPE IS AN INSTRUMENT FOR ANALYSING LIGHT; IT
PROVIDES THE MEANS FOR IDENTIFYING DIFFERENT SUBSTANCES
This pictorial diagram illustrates the principal of Spectrum Analysis,
showing how sunlight is decomposed into its primary colours. What we
call white light is composed of seven different colours. The diagram is
relieved of all detail which would unduly obscure the simple process by
which a ray of light is broken up by a prism into different
wave-lengths. The spectrum rays have been greatly magnified.]