Life in the Roman World of Nero and St. PaulTucker, T. G. (Thomas George)
History
Life in the Roman World of Nero and St. Paul
Tucker, T. G. (Thomas George)
Church history -- Primitive and early church, ca. 30-600; Rome -- Civilization; Rome -- Social conditions
Science, though its matter was attractive enough to the practical
Roman, was at a standstill. So far as it existed it was Greek. The
Greeks had done almost all that could be done by sheer brain-power and
acumen. They could hardly proceed further without those finer
instruments which we possess, but which they did not. Though they knew
of certain magnifying glasses, they had no real telescopes or
microscopes, no mariner's compass or chronometers, no very delicate
balances. They possessed a magnificent thinking apparatus and put it
to admirable use. The modern scientist has generally nothing but
admiration for their keen insight, and for the brilliant hypotheses
which they invented and which were frequently but unverified
anticipations or partial anticipations of theories now in vogue. Where
they stopped short was at experiment in test of hypothesis. Of all
exploits of pure thinking in the domain of science perhaps the
greatest has been the conception that the earth, instead of being a
flat disk, is a sphere. This theory was held before the age of Nero by
ancient astronomers and geographers, who had derived the notion partly
from the eclipses of the moon--of which they well understood the
cause--and partly from the rising of objects above the horizon. They
understood also that in a sphere there was gravitation to the centre,
and were able so to comprehend the level surface of water on the
globe. The geographer Strabo, more than a generation before our chosen
date, readily conceives that, if one sailed straight westward out of
the Mediterranean through the Straits of Gibraltar, he would
ultimately come back round the world by way of the East--that is to
say, by India. It was not left for Columbus to invent that doctrine.
It is true that in calculating the circumference of the earth they had
made it as much as one-seventh too large, but the wonder is that they
came so near as they did. In regard to the distance of the moon they
were not more than 1/12th from the modern estimate. The possibility of
error in dealing with the sun was much greater, and their 51,000,000
miles is little more than half of what it should have been. Exactly
how far this doctrine of the sphericity of the earth was popularly
entertained we cannot tell; it was probably almost confined to those
directly interested in the question. A theory, anticipating Galileo,
that it is the earth which moves round the sun, had been mooted, but
certainly had very little currency. Nor was speculation confined to
such astronomical conclusions. In the region of physical geography
rational attempts were made to account for various phenomena, such as
the existence of deltas or the risings of the Nile, or the appearance
of sea-shells high on dry land. Strabo, in dealing with the Black Sea,
has his theories of the elevation or subsidence of land. He also
suggests previous volcanic conditions of certain districts which had
been quiescent from before the memory or tradition of the inhabitants.
Public-domain text, read in full here on John Shaqi.
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