Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematicsFerguson, James
Science
Astronomy Explained Upon Sir Isaac Newton's Principles: And made easy to those who have not studied mathematics
Ferguson, James
Astronomy -- Early works to 1800
225. The Tables of the Equation of natural days, at the end of the next
Chapter, shew the time that ought to be pointed out by a well regulated
clock or watch every day of the year at the precise moment of solar
noon; that is, when the Sun’s centre is on the Meridian, or when a true
Sun-dial shews it to be precisely Twelve. Thus, on the 5th of _January_
in Leap-year, when the Sun is on the Meridian, it ought to be 5 minutes
51 seconds past twelve by the clock; and on the 15th of _May_, when the
Sun is on the Meridian, the time by the clock should be but 55 minutes
57 seconds past eleven; in the former case, the clock is 5 minutes 51
seconds beforehand with the Sun; and in the latter case, the Sun is 4
minutes 3 seconds faster than the clock. The column at the right hand of
each month shews the daily difference of this equation, as it increases
or decreases. But without a Meridian Line, or a Transit-Instrument fixed
in the plane of the Meridian, we cannot set a Sun-dial true.
[Sidenote: How to draw a Meridian Line.]
226. The easiest and most expeditious way of drawing a Meridian Line is
this: Make four or five concentric Circles, about a quarter of an inch
from one another, on a flat board about a foot in breadth; and let the
outmost Circle be but little less than the board will contain. Fix a pin
perpendicularly in the center, and of such a length that it’s whole
shadow may fall within the innermost Circle for at least four hours in
the middle of the day. The pin ought to be about an eighth part of an
inch thick, with a round blunt point. The board being set exactly level
in a place where the Sun shines, suppose from eight in the morning till
four in the afternoon, about which hours the end of the shadow should
fall without all the Circles; watch the times in the forenoon, when the
extremity of the shortening shadow just touches the several Circles, and
_there_ make marks. Then, in the afternoon of the same day, watch the
lengthening shadow, and where it’s end touches the several Circles in
going over them, make marks also. Lastly, with a pair of compasses, find
exactly the middle point between the two marks on any Circle, and draw a
straight line from the center to that point; which Line will be covered
at noon by the shadow of a small upright wire, which should be put in
the place of the pin. The reason for drawing several Circles is, that in
case one part of the day should prove clear, and the other part somewhat
cloudy, if you miss the time when the point of the shadow should touch
one Circle, you may perhaps catch it in touching another. The best time
for drawing a Meridian Line in this manner is about the middle of
summer; because the Sun changes his Declination slowest and his Altitude
fastest in the longest days.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account