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
Sir William Herschel has observed, in reference to this point, ‘In
beautiful nights, when the outside of our telescopes is dropping with
moisture, discharged from the atmosphere, there are now and then
favourable _hours_ in which it is hardly possible to put a limit to
the magnifying powers. But such valuable opportunities are extremely
scarce, and with large instruments it will always be lost labour to
observe at other times. In order therefore, to calculate how long a
time it must take to sweep the heavens, as far as they are within
the reach of my forty-feet telescope, charged with a magnifying
power of 1000, I have had recourse to my journals to find how many
favourable hours we may annually hope for in this climate. And, under
all favourable circumstances, it appears, that a year which will
afford ninety, or at most, one hundred _hours_ is to be called very
productive.’ ‘In the equator, with my twenty feet telescope, I have
swept over zones of two degrees with a power of 157, but an allowance
of ten minutes in Polar distance must be made for lapping the sweeps
over one another where they join. As the breadth of the zones may be
increased towards the poles, the northern hemisphere may be swept in
about 40 zones; to these we must add 19 southern zones; then 59 zones
which, on account of the sweeps lapping over one another, about 5
minutes of time in right ascension, we must reckon of 25 hours each,
will give 1475 hours. And allowing 100 hours per year, we find that
with the 20 feet telescope, the heavens may be swept in about 14 years
and three quarters. Now the time of sweeping with different magnifying
powers will be as the squares of the powers; and putting _p_ and _t_
for the power and time in the 20 feet telescope, and P = 1000 for
the power in the 40 feet instrument, we shall have p^2 : t :: P^2 :
^{tP2}/_{p^2} = 59840. Then making the same allowance for 100 hours per
year, it appears that it will require not less than 598 years, to look
with the 40 feet reflector, charged with the above-mentioned power,
only one single moment into each point of space; and even then, so much
of the southern hemisphere will remain unexplored, as will take up 213
years more to examine.’[28]
Public-domain text, read in full here on John Shaqi.
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