|
Hitherto the sidereal heavens have, not inadequately for the purpose designed, been represented by the concave surface of a sphere, in the center of which the eye of an observer might be supposed to be placed. It is true, the various magnitudes of the fixed stars even then plainly suggested to us, and would have better suited the idea of an expanded firmament of three dimensions; but the observations upon which I am now going to enter still farther illustrate and enforce the necessity of considering the heavens in this point of view. In
the future, therefore, we shall look upon those regions into which we
may now penetrate by means of such large telescopes, as a naturalist regards
a rich extent of ground or chain of mountains, containing strata variously
inclined and directed, as well as consisting of very different materials.
A surface of a globe or map, therefore, will but ill delineate the interior
parts of the heavens. |
|
Copyright ©. Brought to you by the Center for History of Physics, a Division of the American Institute of Physics |
|
|||||