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 — John Shaqi
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
through a small hole not more than 1/100th of an inch in diameter, the
sky, the trees, houses, and nearly all the objects in an extensive
landscape, occupying nearly an entire hemisphere, the light of all
which may pass through this small aperture.
3. _Light is sent forth in all directions from every visible point
of luminous bodies._ If we hold a sheet of paper before a candle,
or the sun, or any other source of light, we shall find that the
paper is illuminated in whatever position we hold it, provided the
light is not obstructed by its edge or by any other body. Hence,
wherever a spectator is placed with regard to a luminous body,
every point of that part of its surface which is toward him will
be visible, when no intervening object intercepts the passage of
the light. Hence, likewise, it follows, that the sun illuminates,
not only an immense plane extending along the paths of the planets,
from the one side of the orbit of Uranus to the other, but the whole
of that sphere, or solid space, of which the distance of Uranus
is the radius. The diameter of this sphere is three thousand six
hundred _millions_ of miles, and it, consequently, contains about
24,000,000,000,000,000,000,000,000,000, or twenty-four thousand
_quartillions_ of cubical miles,--every point of which immense space
is filled with the solar beams. Not only so, but the whole cubical
space which intervenes between the sun and the nearest fixed stars
is more or less illuminated by his rays. For, at the distance of
Sirius, or any other of the nearest stars, the sun would be visible,
though only as a small twinkling orb; and consequently, his rays
must be diffused, however faint, throughout the most distant spaces
whence he is visible. The diameter of this immense sphere of light
cannot be less than _forty billions_ of miles, and its solid contents
33,500,000,000,000,000,000,000,000,000,000,000,000,000 or, thirty-three
thousand, five hundred _sextillions_ of cubical miles. All this
immense, and incomprehensible space is filled with the radiations of
the solar orb; for were an eye placed in any one point of it, where
no extraneous body interposed, the sun would be visible either as a
large luminous orb, or as a small twinkling star. But he can be visible
only by the rays he emits, and which enter the organs of vision. How
inconceivably immense, then, must be the quantity of rays which are
thrown off in all directions from that luminary which is the source of
our day! Every star must likewise be considered as emitting innumerable
streams of radiance over a space equally extensive, so that no point in
the universe can be conceived where absolute darkness prevails, unless
in the _interior_ regions of planetary bodies.
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