The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomyDick, Thomas
Science
The Practical Astronomer: Comprising illustrations of light and colours--practical descriptions of all kinds of telescopes--the use of the equatorial-transit--circular, and other astronomical instruments, a particular account of the Earl of Rosse's large telescopes, and other topics connected with astronomy
Dick, Thomas
Astronomical instruments; Astronomy; Telescopes
It was originally remarked by Newton, and the fact has since
been confirmed by the experiments of Sir W. Herschel, that _the
different-coloured rays have not the same illuminating power_. The
violet rays appear to have the least illuminating effect; the indigo
more, and the effect increases in the order of the colours,--the
_green_ being very great; between the green and the yellow the greatest
of all; the yellow the same as the green; but the red less than the
yellow. Herschel also endeavoured to determine whether the power of the
differently-coloured rays to _heat_ bodies, varied with their power
to illuminate them. He introduced a beam of light into a dark room,
which was decomposed by a prism, and then exposed a very sensible
thermometer to all the rays in succession, and observed the heights
to which it rose in a given time. He found that their heating power
increased from the violet to the red. The mercury in the thermometer
rose higher when its bulb was placed in the Indigo than when it was
placed in the violet, still higher in blue, and highest of all at red.
Upon placing the bulb of the thermometer below the red, quite out of
the spectrum, he was surprised to find that the mercury rose highest
of all; and concluded that _rays proceed from the sun, which have the
power of_ HEATING, _but not of illuminating bodies_. These
rays have been called _invisible_ solar rays. They were about half an
inch from the commencement of the red rays; at a greater distance from
this point the heat began to diminish, but was very perceptible even
at the distance of 1-1/2 inch. He determined that the heating power of
the _red_ to that of the _green_ rays, was 2-3/4 to 1, and 3-1/2 to 1,
in red to _violet_. He afterwards made experiments to collect those
invisible calorific rays, and caused them to act independently of the
light, from which he concluded that they are sufficient to account
for all the effects produced by the solar rays in exciting heat; that
they are capable of passing through glass, and of being refracted and
reflected, after they have been finally detached from the solar beam.
Public-domain text, read in full here on John Shaqi.
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