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
In viewing the _Nebulæ_, and the very small and immensely distant
fixed stars, which require much light to render them visible, a large
aperture of the object-glass or speculum, which admits of a great
quantity of light, is of more importance than high magnifying powers.
It is light chiefly, accompanied with a moderate magnifying power,
that enables us to _penetrate_ into the distant regions of space. Sir
W. Herschel, when sweeping the profundities of the Milky way, and the
Hand and Club of Orion, used a telescope of the Newtonian form, 20-feet
focal length, and 18-7/10 inches diameter, with a power of only 157.
On applying this telescope and power to a part of the _Via Lactea_, he
found that it completely resolved the whole whitish appearance into
stars, which his former telescopes had not light enough to effect; and
which smaller instruments with much higher magnifying powers would
not have effected. He tells us, that with this power, ‘the glorious
multitude of stars,’ in the vicinity of Orion, ‘of all possible sizes,
that presented themselves to view, was truly astonishing, and that
he had fields which contained 70, 90 and 110 stars, so that a belt
of 15 degrees long, and 2 degrees broad, which passed through the
field of the telescope in an hour, could not contain less than fifty
thousand stars that were large enough to be distinctly numbered.’ In
viewing the Milky way, the Nebulæ, and small clusters of stars, such
as _Præsepe_ in Cancer, I generally use a power of 55 times, on an
achromatic telescope 6 feet 6 inches in focal length, and 4 inches
diameter. The eye-piece, which produces this power--which I formed
for the purpose--consists of two convex lenses, the one next the eye
3 inches focal length, and 1-2/10 inch diameter, and that next the
object 3-1/2 inches focus, and 1-4/10 inch diameter, the deepest convex
surfaces being next each other, and their distance 1/4 inch. With this
eye-piece a very large and brilliant field of view is obtained; and I
find it preferable to any higher powers in viewing the nebulosities,
and clusters of stars. In certain spaces of the heavens, it sometimes
presents in one field, nearly a hundred stars. It likewise serves to
exhibit a very clear and interesting view of the full moon.
Public-domain text, read in full here on John Shaqi.
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