Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
Newton first published the doctrine of universal gravitation in the
'Principia,' in 1687. The name implies that the work contains the
fundamental principles of natural philosophy and astronomy. Being
founded upon the immutable basis of mathematics, its conclusions must of
course be true and unalterable, and thenceforth we may regard the great
laws of the universe as traced to their remotest principle. The greatest
astronomers and mathematicians have since occupied themselves in
following out the plan which Newton began, by applying the principles of
universal gravitation to all the subordinate as well as to the grand
movements of the spheres. This great labor has been especially achieved
by La Place, a French mathematician of the highest eminence, in his
profound work, the 'Mecanique Celeste.' Of this work, our distinguished
countryman, Dr. Bowditch, has given a magnificent translation, and
accompanied it with a commentary, which both illustrates the original,
and adds a great amount of matter hardly less profound than that.
[Illustration Fig. 31.]
We have thus far taken the earth's orbit around the sun as a great
circle, such being its projection on the sphere constituting the
celestial ecliptic. The real path of the earth around the sun is
learned, as I before explained to you, by the apparent path of the sun
around the earth once a year. Now, when a body revolves about the earth
at a great distance from us, as is the case with the sun and moon, we
cannot certainly infer that it moves in a circle because it appears to
describe a circle on the face of the sky, for such might be the
appearance of its orbit, were it ever so irregular a curve. Thus, if E,
Fig. 31, represents the earth, and ACB, the irregular path of a body
revolving about it, since we should refer the body continually to some
place on the celestial sphere, XYZ, determined by lines drawn from the
eye to the concave sphere through the body, the body, while moving from
A to B through C, would appear to move from X to Z, through Y. Hence, we
must determine from other circumstances than the actual appearance, what
is the true figure of the orbit.
[Illustration Fig. 32.]
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