The Science of the StarsMaunder, E. Walter (Edward Walter)
History
The Science of the Stars
Maunder, E. Walter (Edward Walter)
Astronomy
The theory of Copernicus deprived the Earth of its special position as
the immovable centre of the universe, but raised it to the rank of a
planet. It is therefore a heavenly body, yet needs no telescope to
bring it within our ken; bad weather does not hide it from us, but
rather shows it to us under new conditions. We find it to be a globe
of land and water, covered by an atmosphere in which float changing
clouds; we have mapped it, and we find that the land and water are
always there, but their relations are not quite fixed; there is give
and take between them. We have found of what elements the land and
water consist, and how these elements combine with each other or
dissociate. In a word, the Earth is the heavenly body that we know the
best, and with it we must compare and contrast all the others.
Before the invention of the telescope there were but {55} two other
heavenly bodies--the Sun and the Moon--that appeared as orbs showing
visible discs, and even in their cases nothing could be satisfactorily
made out as to their conditions. Now each of the five planets known to
the ancients reveals to us in the telescope a measurable disc, and we
can detect significant details on their surfaces.
THE MOON is the one object in the heavens which does not disappoint a
novice when he first sees it in the telescope. Every detail is hard,
clear-cut, and sharp; it is manifest that we are looking at a globe, a
very rough globe, with hills and mountains, plains and valleys, the
whole in such distinct relief that it seems as if it might be touched.
No clouds ever conceal its details, no mist ever softens its outlines;
there are no half-lights, its shadows are dead black, its high lights
are molten silver. Certain changes of illumination go on with the
advancing age of the Moon, as the crescent broadens out to the half,
the half to the full, and the full, in its turn, wanes away; but the
lunar day is nearly thirty times as long as that of the Earth, and
these changes proceed but slowly.
The full Moon, as seen by the naked eye, shows several vague dark
spots, which most people agree to fancy as like the eyes, nose, and
mouth of a broad, sorrowful face. The ordinary astronomical telescope
inverts the image, so the "eyes" of the Moon are seen in the lower part
of the field of the telescope as a series of dusky plains stretching
right across the disc. But in the upper part, near the left-hand
corner of the underlip, there is a bright, round spot, from which a
number of bright streaks radiate--suggesting a peeled orange with its
stalk, and the lines marking the sections radiating from it. This
bright spot has been called after the great {56}
Public-domain text, read in full here on John Shaqi.
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