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
206. That a greater number of rays fall on the same place, when they
come perpendicularly, than when they come obliquely on it, will appear
by the Figure. For, let _AB_ be a certain number of the Sun’s rays
falling on _CD_ (which, let us suppose to be _London_) on the 22d of
_June_: but, on the 22d of _December_, the line _CD_, or _London_; has
the oblique position _Cd_ to the same rays; and therefore scarce a third
part of them falls upon it, or only those between _A_ and _e_; all the
rest _eB_ being expended on the space _dP_, which is more than double
the length of _CD_ or _Cd_. Besides, those parts which are once heated,
retain the heat for some time; which, with the additional heat daily
imparted, makes it continue to increase, though the Sun declines toward
the south: and this is the reason why _July_ is hotter than _June_,
although the Sun has withdrawn from the summer Tropic; as we find it is
generally hotter at three in the afternoon, when the Sun has gone toward
the west, than at noon when he is on the Meridian. Likewise, those
places which are well cooled require time to be heated again; for the
Sun’s rays do not heat even the surface of any body till they have been
some time upon it. And therefore we find _January_ for the most part
colder than _December_, although the Sun has withdrawn from the winter
Tropic, and begins to dart his beams more perpendicularly upon us, when
we have the position _CF_. An iron bar is not heated immediately upon
being put into the fire, nor grows cold till some time after it has been
taken out.
CHAP. XI.
_The Method of finding the Longitude by the Eclipses of Jupiter’s
Satellites: The amazing Velocity of Light demonstrated by these
Eclipses._
[Sidenote: First Meridian, and Longitude of places, what.]
207. Geographers arbitrarily choose to call the Meridian of some
remarkable place _the first Meridian_. There they begin their reckoning;
and just so many degrees and minutes as any other place is to the
eastward or westward of that Meridian, so much east or west Longitude
they say it has. A degree is the 360th part of a Circle, be it great or
small; and a minute the 60th part of a degree. The _English_ Geographers
reckon the Longitude from the Meridian of the Royal Observatory at
_Greenwich_, and the _French_ from the Meridian of _Paris_.
[Sidenote: PLATE V.
Fig. II.
Hour Circles.
An hour of time equal to 15 degrees of motion.]
Public-domain text, read in full here on John Shaqi.
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