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
7. _It is by light reflected from opake bodies that most of the objects
around us are rendered visible._ When a lighted candle is brought
into a dark room, not only the candle but all other bodies in the
room become visible. Rays of the sun passing into a dark room render
luminous a sheet of paper on which they fall, and this sheet in its
turn enlightens, to a certain extent, the whole apartment, and renders
objects in it visible, so long as it receives the rays of the sun. In
like manner, the moon and the planets are opake bodies, but the light
of the sun falling upon them, and being reflected from their surfaces,
renders them visible. Were no light to fall on them from the sun, or
were they not endued with a power of reflecting it, they would be
altogether invisible to our sight. When the moon comes between us and
the sun, as in a total eclipse of that luminary, as no solar light is
reflected from the surface next the earth, she is invisible--only the
curve or outline of her figure being distinguished by her shadow. In
this case, however, there is a certain portion of reflected light on
the lunar hemisphere next the earth, though not distinguishable during
a solar eclipse. The earth is enlightened by the sun, and a portion of
the rays which fall upon it is reflected upon the dark hemisphere of
the moon which is then towards the earth. This reflected light from the
earth is distinctly perceptible, when the moon appears as a slender
crescent, two or three days after new moon--when the earth reflects its
light back on the moon, in the same manner as the full moon reflects
her light on the earth. Hence, even at this period of the moon, her
whole face becomes visible to us, but its light is not uniform or of
equal intensity. The thin crescent on which the full blaze of the solar
light falls, is very brilliant and distinctly seen, while the other
part, on which falls only a comparatively feeble light from the earth,
appears very faint, and is little more than visible to the naked eye,
but with a telescope of moderate power,--if the atmosphere be very
clear--it appears beautifully distinct, so that the relative positions
of many of the lunar spots may be distinguished.
Public-domain text, read in full here on John Shaqi.
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