Curiosities of Science, Past and Present: A Book for Old and YoungTimbs, John
Science
Curiosities of Science, Past and Present: A Book for Old and Young
Timbs, John
Science
The first object to which Galileo directed his telescope was the
mountainous parts of the moon, when he showed how their summits
might be measured: he found in the moon some circular districts
surrounded on all sides by mountains similar to the form of
Bohemia. The measurements of the mountains were made by the method
of the tangents of the solar ray. Galileo, as Helvetius did still
later, measured the distance of the summit of the mountains from
the boundary of the illuminated portion at the moment when the
mountain summit was first struck by the solar ray. Humboldt found
no observations of the lengths of the shadows of the mountains:
the summits were “much higher than the mountains on our earth.”
The comparison is remarkable, since, according to Riccioli,
very exaggerated ideas of the height of our mountains were then
entertained. Galileo like all other observers up to the close of
the eighteenth century, believed in the existence of many seas and
of a lunar atmosphere.
THE MOON AND THE WEATHER.
The only influence of the Moon on the Weather of which we have any
decisive evidence is the tendency to disappearance of clouds under the
full moon, which Sir John Herschel refers to its heat being much more
readily absorbed in traversing transparent media than direct solar
heat, and being extinguished in the upper regions of our atmosphere,
never reaches the surface of the atmosphere at all.
THE MOON’S ATTRACTION.
Mr. G. P. Bond of Cambridge, by some investigations to ascertain
whether the Attraction of the Moon has any effect upon the motion of
a pendulum, and consequently upon the rate of a clock, has found the
last to be changed to the amount of 9/1000 of a second daily. At
the equator the moon’s attraction changes the weight of a body only
1/7000000 of the whole; yet this force is sufficient to produce the
vast phenomena of the tides!
It is no slight evidence of the importance of analysis, that Laplace’s
perfect theory of tides has enabled us in our astronomical ephemerides
to predict the height of spring-tides at the periods of new and full
moon, and thus put the inhabitants of the sea on their guard against
the increased danger attending the lunar revolutions.
MEASURING THE EARTH BY THE MOON.
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