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
The large speculum is enclosed in a strong iron ring, braced across
with bars of iron, and an enclosure of iron and ten sheets makes a case
for it. It is lifted by three handles of iron attached to the sides of
the ring, and is put into and taken out of its proper place in the tube
by the help of a moveable crane, running on a carriage, which operation
requires great care. The speculum is made of a metallic composition,
and is 49-1/2 inches in diameter; but the concave polished surface is
only 48 inches, or 4 feet in diameter. Its thickness is 31 inches; and
when it came from the cast its weight was 2118 pounds. The metals for
its formation were procured at a warehouse in Thames Street, London,
where they kept ingots of two kinds ready made, one of white, and the
other of bell-metal; and it was composed of two ingots of bell-metal
for one of white. It was not to be expected that a speculum of such
large dimensions, could have a perfect figure imparted to its surface,
nor that the curve, whatever it might be, would remain identically the
same in changes of temperature; therefore we are not surprised when we
are told, that the magnifying powers used with this telescope seldom
exceeded 200; the quantity of light collected by so large a surface
being the principal aim of the maker. The raising of the balcony, on
which the observer stands, and the sliding of the lower end of the
tube, in which the speculum rests, are effected by separate tackles,
and require only occasional motions; but the elevation of the telescope
requires the main tackle to be employed, and the motion usually given
in altitude at once was two degrees; the breadth of the zone in which
the observations were made, as the motion of the sphere in right
ascension brought the objects into view. A star, however, could be
followed for about a quarter of an hour. Three persons were employed
in using this telescope, one to work the tackle, another to observe,
and a third to mark down the observations. The elevation was pointed
out by a small quadrant fixed to the main tube, near the lower end, but
the polar distance was indicated by a piece of machinery, worked by a
string, which continually indicated the degree and minute on a dial in
the small house adjoining, while the time was shown by a clock in the
same place, Miss Herschel performing the office of Registrar.
Public-domain text, read in full here on John Shaqi.
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