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
Let _a_, _b_, _c_, _d_, _e_, _f_, _g_, _h_ be the Earth in eight
different parts of it’s Orbit, equidistant from one another; _Ns_ it’s
Axis, _N_ the north Pole, _s_ the south Pole, and _S_ the Sun nearly in
the center of the Earth’s Orbit § 18. As the Earth goes round the Sun
according to the order of the letters _abcd_, &c. it’s Axis _Ns_ keeps
the same obliquity, and is still parallel to the line _MNs_. When the
Earth is at _a_, it’s north Pole inclines toward the Sun, and brings all
the northern places more into the light than at any other time of the
year. But when the Earth is at _e_ in the opposite time of the year, the
north Pole declines from the Sun, which occasions the northern places to
be more in the dark than in the light; and the reverse at the southern
places, as is evident by the Figure, which I have taken from Dr. LONG’s
Astronomy. When the Earth is either at _c_ or _g_, it’s Axis inclines
not either to or from the Sun, but lies sidewise to him; and then the
Poles are in the boundary of light and darkness; and the Sun, being
directly over the Equator, makes equal day and night at all places. When
the Earth is at _b_ it is half way between the Summer Solstice and
Harvest Equinox; when it is at _d_ it is half way from the Harvest
Equinox to the Winter Solstice; at _f_ half way from the Winter Solstice
to the Spring Equinox: and at _h_ half way from the Spring Equinox to
the Summer Solstice.
[Sidenote: Fig. II.
PLATE V.
The Ecliptic.
The seasons shewn in another view of the Earth, and it’s Orbit.]
203. From this oblique view of the Earth’s Orbit, let us suppose
ourselves to be raised far above it, and placed just over it’s center
_S_, looking down upon it from it’s north pole; and as the Earth’s Orbit
differs but very little from a Circle, we shall have it’s figure in such
a view represented by the Circle _ABCDEFGH_. Let us suppose this Circle
to be divided into 12 equal parts called _Signs_, having their names
affixed to them; and each Sign into 30 equal parts called _Degrees_,
numbered 10, 20, 30, as in the outermost Circle of the Figure, which
represents the great Ecliptic in the Heavens. The Earth is shewn in
eight different positions in this Circle, and in each position _Æ_ is
the Equator, _T_ the Tropic of Cancer, the _dotted Circle_ the parallel
of _London_, _U_ the arctic or north polar Circle, and _P_ the north
Pole where all the Meridians or hour Circles meet § 198. As the Earth
goes round the Sun the north Pole keeps constantly towards one part of
the Heavens, as it keeps in the Figure towards the right hand side of
the Plate.
[Sidenote: Vernal Equinox.]
Public-domain text, read in full here on John Shaqi.
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