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TWILIGHT , formerly known as Crepusculum (a Latin word meaning dusky or obscure), properly the See also: interval during which the atmosphere is illuminated after the setting of the See also: sun
.
The analogous phenomenon in the See also: morning, i.e. the interval between the first appearance of See also: light and the rising of the sun, is known as the dawn
.
These phenomena are due to the light of the sun after refraction by the atmosphere being reflected to the observer by the clouds, dust, and other adventitious See also: matter See also: present in the atmosphere
.
Even in the early See also: infancy of astronomy, the duration of twilight was associated with the position of the sun below the See also: horizon, and measurements were made to determine the maximum vertical depression of the sun which admitted the phenomena
.
This was found by Alhazen, Tycho Brahe and others, to be about 18°, and although other observers obtained somewhat different values, yet this value is now generally admitted
.
The duration of twilight is therefore measured by the See also: time in which the sun traverses an arc of r8° of vertical depression, and primarily depends on the latitude of the observer and the declination of the sun
.
It is subject to several minor variations, occasioned by the variable amount of dust, clouds, &c. suspended in the air; and also on the temperature, which alters the altitude of the reflecting particles; thus at the same place and on the same See also: day, the morning twilight or dawn is generally shorter than the evening twilight
.
The duration and possibility of twilight may be geometrically exhibited as follows : Let 0 be the position of the observer (fig
.
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