Ecliptic

Definition and stakes

George F. Chambers,  The Story of Eclipses

“ Fig. 5.—PARTIAL ECLIPSE OF THE SUN.
Now we must advance one stage in our conceptions of the movements of the Earth and the Moon, so far as regards the bearing of those [18] movements on the question of eclipses. The Earth moves in a plane which is called the “Plane of the Ecliptic,” and correspondingly, the Sun has an apparent annual motion in the same plane. The Moon moving in a different plane, inclined to the first mentioned one to the extent of rather more than 5°, the Moon’s orbit will evidently intersect the ecliptic in two places.
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Source: Gutenberg

Portrait of Denison Olmsted Denison Olmsted,  Letters on Astronomy

“ We must keep in mind, that the celestial equator and celestial ecliptic are here understood, and we may imagine them to be two great circles delineated on the face of the sky. On comparing observations made at different periods, for more than two thousand years, it is found, that the obliquity of the ecliptic is not constant, but that it undergoes a slight diminution, from age to age, amounting to fifty-two seconds in a century, or about half a second annually. ”
Source: Gutenberg

C. E. Brame,  Popular Science Monthly (1877)

“ It appears to best advantage when the ecliptic makes its highest angle with the spectator's horizon, at which time, in moderate latitudes, it reaches to the zenith or beyond it, having near the horizon a striking brilliancy, and thence fading upward, mostly by imperceptible degrees, till at its vertex it can be made out only by a careful and experienced eye. ”
Source: Wikisource

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