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
From the above remarks of so eminent an observer, the reader will
perceive how difficult it is to explore the heavens with minuteness and
accuracy, and with how many disappointments, arising from the state
of the atmosphere, the astronomer must lay his account, when employed
in planetary or sidereal investigation. Besides the circumstances now
stated, it ought to be noticed that a star or a planet is only in
a situation for a high magnifying power, about half the time it is
above the horizon. The density of the atmosphere, and the quantity of
vapours with which it is charged near the horizon, prevent distinct
vision of celestial objects with high powers, till they have risen to
at least 15 or 20 degrees in altitude, and the highest magnifiers can
scarcely be applied with good effect, unless the object is near the
meridian, and at a considerable elevation above the horizon. If the
moon be viewed a little after her rising, and afterwards when she comes
to her highest elevation in autumn, the difference in her appearance
and distinctness will be strikingly perceptible. It is impossible to
guess whether a night be well adapted for celestial observations,
till we actually make the experiment, and instruments are frequently
condemned, when tried at improper seasons, when the atmosphere only is
in fault. A certain observer remarks,--‘I have never seen the face of
Saturn more distinctly than in a night when the air has been so hazy,
that with my naked eye, I could hardly discern a star of less than the
third magnitude.’ The degree of the transparency of the air is likewise
varying almost in the course of every minute, so that even in the
course of the same half hour, planets and stars will appear perfectly
defined, and the reverse. The vapours moving and undulating the
atmosphere, even when the sky appears clear to the naked eye, will in a
few instants destroy the distinctness of vision, and in a few seconds
more, the object will resume its clear and well-defined aspect.[29]
3. _On the magnifying powers requisite for observing the phenomena of
the different planets--comets--double stars, &c._
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