| Torricelli received a mathematical education
in Rome. He was profoundly affected when in 1638 he first read Galile's works.
A book he himself wrote on mechanics in turn impressed Galileo, who invited him to
Florence. Torricelli went gladly to meet the blind old man and served as his
secretary and companion for the last three months of his life. He then succeeded him
as court mathematician to Grand Duke Ferdinand II of Tuscany. Galileo suggested the
problem through which Torricelli was to gain fame. The ability to pump water upward was attributed to the proposed fact that
"Nature abhors a vacuum." When a piston was raised, a vacuum would be
produced unless the water within the cylinder rose with the piston. Since a vacuum
could not occur in nature, it was thought, the water had to rise. In that case, it
ought to have risen upward indefinitely as long as the Piston rose. Water, however,
could only be raised about thirty-three feet above its natural level.
Galileo, who accepted the vacuum-abhorrence of nature
(despite his many revolutionary deeds he was surprisingly conservative in many ways),
could only suppose that this "abhorrence" was limited and not absolute. He
suggested that Torricelli look into the matter.
It occurred to Torricelli that this was no matter of
vacuum-abhorrence, but a simple mechanical effect. If the air had weight
(according to Aristotle it didn't but tended rather to have "levity" and to
rise) but Galileo had shown that a full balloon weight would push against the water
outside the pump. When the piston was raised, that push would force the water up
with the piston. However, suppose that the total weight for the air would only
balance thirty-three feet of water. In that case, further pumping would have no
effect. The weight of the air would push water no higher.
In 1643, to check this theory, Torricelli made use of
mercury, whose density is nearly thirteen-and-a-half-times that of water. He filled
a four-foot length of glass tubing, closed at one end, put his thumb over the opening and
upended it (open and down) into a large dish of mercury. The mercury began to empty
out of the tube as one might expect, but it did not do so altogether. Thirty inches
of mercury remained in the tube, supported by the weight of the air pressing down on the
mercury in the dish. The weight of the air could easily be used to account for the
mercury column's remaining in place in defiance of gravity.
Above the mercury in the upended tube was a vacuum (except
for a small quantity of mercury vapor). It was the first man-made vacuum, and,
thanks to the publicity given the experiment by Meraenne, is called a Torricellian vacuum
to this day (Seven years later Guericke produced a vacuum on a far larger scale by pumping
and did dramatic things as a result).
Torricelli noticed that the height of the mercury in the
tube varied slightly from day to day and this he correctly attributed to the fact that the
atmosphere positioned a slightly different weight at different times. He had
invented the first barometer.
(The weight of the stratosphere is equivalent to that of a
column of mercury 760 millimeters high. The pressure exerted by one millimeter of
mercury is sometimes defined as one Torricelli, in honor of the physicist.)
The fact that air had a finite weight meant it could only
have a finite height, a view confirmed by Pascal a few years later. This was the
first definite indication (aside from philosophical speculation) that the atmosphere does
not extend indefinitely outward and that the depths of space must be a vacuum.
Thus, far from a vacuum being an impossibility, it is undoubtedly the natural state of
most of the universe.
Questions concerning the existence of a vacuum may have
seemed mystical and philosophical, but the proof of its existence led by a chain of event
and reassuring to the development of the steam engine, the advent of the Industrial
Revolution, and the making of our own technological society. All resulted from the
upending of a tube of mercury. Similarly, the proof for massive space-time will create a
new paradigm of thinking and technology that will start a space-industry revolution.

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