It remains to describe in greater detail the apparent movements of the sun
and the sun's effect upon the seasons. In Figure 3, the great circle MWM'E
represents the equinoctial and XVX'A the ecliptic. The point X represents
the farthest point south that the sun reaches in its apparent journey
around the earth, and this point is called the _winter solstice_, because,
for the northern hemisphere the sun reaches this point in mid-winter. When
the sun is south of the celestial equator its apparent daily path is the
same as it would be for a star so situated. Thus its daily path at the
time of the winter solstice, about December 21, can be represented by the
circle Xmn'. The arc gXh represents the part of the sun's path that would
be above the horizon, showing that night would last much longer than day
and the rays of the sun would strike the northern hemisphere of the earth
more indirectly than when the sun is north of the equator. As the sun
passes along the ecliptic from X toward V, the part of its daily path
that is above the horizon gradually increases until at V, the vernal
equinox, the sun's path would, roughly speaking, coincide with the
celestial equator so that half of it would be above the horizon and half
below and day and night would be of equal length. This explains why the
celestial equator was formerly called the equinoctial (Chaucer's term for
it). As the sun passes on toward X' its daily arc continues to increase
and the days to grow longer until at X' it reaches its greatest
declination north of the equator and we have the longest day, June 21, the
summer solstice. When the sun reaches this point, its rays strike the
northern hemisphere more directly than at any other time causing the hot
or summer season in this hemisphere. Next the sun's daily arc begins to
decrease, day and night to become more nearly equal, at A the autumnal
equinox[196] is reached and the sun again shapes its course towards the
point of maximum declination south of the equator. The two points of
maximum declination are called _solstices_.
The two small circles of the celestial sphere, parallel to the equator,
which pass through the two points where the sun's declination is greatest,
are called _Tropics_; the one in the northern hemisphere is called the
_Tropic of Cancer_, that in the southern hemisphere, the _Tropic of
Capricorn_. They correspond to circles on the earth's surface having the
same names.
II. By "artificial day" Chaucer means the time during which the sun is
above the horizon, the period from sunrise to sunset. The arc of the
artificial day may mean the extent or duration of it, as measured on the
rim of an astrolabe, or it may mean (as here), the arc extending from the
point of sunrise to that of sunset. See _Astrolabe_ ii.7.
Public-domain text, read in full here on John Shaqi.
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