Limits of Eclipses.]

317. If the Moon’s Orbit were coincident with the Plane of the Ecliptic,

in which the Earth always moves and the Sun appears to move, the Moon’s

shadow would fall upon the Earth at every Change, and eclipse the Sun to

some parts of the Earth. In like manner the Moon would go through the

middle of the Earth’s shadow, and be eclipsed at every Full; but with

this difference, that she would be totally darkened for above an hour

and half; whereas the Sun never was above four minutes totally eclipsed

by the interposition of the Moon. But one half of the Moon’s Orbit, is

elevated 5-1/3 degrees above the Ecliptic, and the other half as much

depressed below it: consequently, the Moon’s Orbit intersects the

Ecliptic in two opposite points called _the Moon’s Nodes_, as has been

already taken notice of § 288. When these points are in a right line

with the center of the Sun at New or Full Moon, the Sun, Moon, and Earth

are all in a right line; and if the Moon be then New, her shadow falls

upon the Earth; if Full the Earth’s shadow falls upon her. When the Sun

and Moon are more than 17 degrees from either of the Nodes at the time

of Conjunction, the Moon is then too high or too low in her Orbit to

cast any part of her shadow upon the Earth. And when the Sun is more

than 12 degrees from either of the Nodes at the time of Full Moon, the

Moon is too high or too low in her Orbit to go through any part of the

Earth’s shadow: and in both these cases there will be no Eclipse. But

when the Moon is less than 17 degrees from either Node at the time of

Conjunction, her shadow or Penumbra falls more or less upon the Earth,

as she is more or less within this limit. And when she is less than 12

degrees from either Node at the time of opposition, she goes through a

greater or less portion of the Earth’s shadow, as she is more or less

within this limit. Her Orbit contains 360 degrees; of which 17, the

limit of solar Eclipses on either side of the Nodes, and 12 the limit of

lunar Eclipses, are but small portions: and as the Sun commonly passes

by the Nodes but twice in a year, it is no wonder that we have so many

New and Full Moons without Eclipses.

[Sidenote: Fig. I.

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