If the glacial epoch resulted from a high condition of eccentricity, we
have not only a means of determining the positive date of that epoch,
but we have also a means of determining geological time in absolute
measure. For if the glacial epochs of prior ages correspond to periods
of high eccentricity, then the intervals between those periods of high
eccentricity become the measure of the intervals between the glacial
epochs. The researches of Lagrange and Leverrier into the secular
variations of the elements of the orbits of the planets enable us
to determine with tolerable accuracy the values of the eccentricity
of the earth’s orbit for, at least, four millions of years past and
future. With the view of determining those values, I several years
ago computed from Leverrier’s formula the eccentricity of the earth’s
orbit and longitude of the perihelion, at intervals of ten thousand and
fifty thousand years during a period of three millions of years in the
past, and one million of years in the future. The tables containing
these values will be found in Chapter XIX. These tables not only give
us the date of the glacial epoch, but they afford, as will be seen
from Chapter XXI., evidence as to the probable date of the Eocene and
Miocene periods.
Ten years ago, when the theory was first advanced, it was beset by
a very formidable difficulty, arising from the opinions which then
prevailed in reference to geological time. One or two glacial epochs in
the course of a million of years was a conclusion which at that time
scarcely any geologist would admit, and most would have felt inclined
to have placed the last glacial epoch at least one million of years
back. But then if we assume that the glacial epoch was due to a high
state of eccentricity, we should be compelled to admit of at least two
glacial epochs during that lapse of time. It was the modern doctrine
that the great changes undergone by the earth’s crust were produced,
not by convulsions of nature, but by the slow and almost imperceptible
action, of rain, rivers, snow, frost, ice, &c., which impressed so
strongly on the mind of the geologist the vast duration of geological
periods. When it was considered that the rocky face of our globe had
been carved into hills and dales, and ultimately worn down to the
sea-level by means of those apparently trifling agents, not only once
or twice, but many times, during past ages, it was not surprising that
the views entertained by geologists regarding the immense antiquity of
our globe should not have harmonised with the deductions of physical
science on the subject. It had been shown by Sir William Thomson and
others, from physical considerations relating to the age of the sun’s
heat and the secular cooling of our globe, that the geological history
of our earth’s crust must be limited to a period of something like
one hundred millions of years. But these speculations had but little
weight when pitted against the stern and undeniable facts of subaërial
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