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HORGEN
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Source
Encyclopaedia Britannica (1911) / britannica_1911
License
public_domain
Chunk ID
1911:horgen:7cf2d2f90c02
Section
Hash Algorithm
sha256
Stored Hash
f5f12a109461ee2cf7eed78e7176da6d105f94bc8c96efca3fc2ad501ae5e710
Computed Hash
f5f12a109461ee2cf7eed78e7176da6d105f94bc8c96efca3fc2ad501ae5e710
Normalizer
ggnorm 1.0
Observed
2026-02-08 18:43:05
Source URL
Verified Text
horgen, a small town in the swiss canton of zurich, situated on the left or west shore of the lake of zurich, and by rail 10(1/2) m. s.e. of the town of zurich. pop. (1900) 6883, mostly german-speaking and protestants. it possesses many industrial establishments of various kinds, and is a centre of the zurich silk manufacture. it came in 1406 into the possession of zurich, with which it communicates by means of steamers on the lake, as well as by rail. horizon (gr. [greek: horizon], dividing), the apparent circle around which the sky and earth seem to meet. at sea this circle is well defined, the line being called the sea horizon, which divides the visible surface of the ocean from the sky. in astronomy the horizon is that great circle of the sphere the plane of which is at right angles to the direction of the plumb line. sometimes a distinction is made between the rational and the apparent horizon, the former being the horizon as determined by a plane through the centre of the earth, parallel to that through the station of an observer. but on the celestial sphere the great circles of these two planes are coincident, so that this distinction is not necessary (see astronomy: _spherical_). the _dip_ of the horizon at sea is the angular depression of the apparent sea horizon, or circle bounding the visible ocean, below the apparent celestial horizon as above defined. it is due to the rotundity of the earth, and the height of the observer's eye above the water. the dip of the horizon and its distance in sea-miles when the height of the observer's eye above the sea-level is h feet, are approximately given by the formulae: dip = 0'.97 [root]h; distance = 1^m.17 [root]h. the difference between the coefficients 0.97 and 1.17 arises from the refraction of the ray, but for which they would be equal.