The English works of Thomas Hobbes of Malmesbury, Volume 01 (of 11) — Thomas Hobbes — John Shaqi
The English works of Thomas Hobbes of Malmesbury, Volume 01 (of 11)
Thomas Hobbes · en
point _m_; and consequently, as soon as ever it begins to be moved, it
will lose its parallelism with the strait line ♑ ♋; so that _m n_
produced will at last cut the strait line _g l_ produced. And
contrarily, as soon as _m n_ is past ♈, the earth making its way in the
internal elliptical line ♈ _l_ ♎, the same _m n_ produced towards _m_,
will cut _l g_ produced. And when the earth hath almost finished its
whole circumference, the same _m n_ shall again make a right angle with
a line drawn from the centre _i_, a little short of the point from which
the earth began its motion. And there the next year shall be one of the
equinoctial points, namely, near the end of ♍; the other shall be
opposite to it near the end of ♓. And thus the points in which the days
and nights are made equal do every year fall back; but with so slow a
motion, that, in a whole year, it makes but 51 first minutes. And this
relapse being contrary to the order of the signs, is commonly called the
_precession of the equinoxes_. Of which I have from my former
suppositions deduced a possible cause; which was to be done.
According to what I have said concerning the cause of the eccentricity
of the earth; and according to Kepler, who for the cause thereof
supposeth one part of the earth to be affected to the sun, the other
part to be disaffected; the apogæum and perigæum of the sun should be
moved every year in the same order, and with the same velocity, with
which the equinoctial points are moved; and their distance from them
should always be the quadrant of a circle; which seems to be otherwise.
For astronomers say, that the equinoxes are now, the one about 28
degrees gone back from the first star of Aries, the other as much from
the beginning of Libra; so that the apogæum of the sun or the aphelium
of the earth ought to be about the 28th degree of Cancer. But it is
reckoned to be in the 7th degree. Seeing, therefore, we have not
sufficient evidence of the ὁτί (that so it is,) it is in vain to seek
for the διότι (why it is so.) Wherefore, as long as the motion of the
apogæum is not observable by reason of the slowness thereof, and as long
as it remains doubtful whether their distance from the equinoctial
points be more or less than a quadrant precisely; so long it may be
lawful for me to think they proceed both of them with equal velocity.
Also, I do not at all meddle with the causes of the eccentricities of
Saturn, Jupiter, Mars, and Mercury. Nevertheless, seeing the
eccentricity of the earth may, as I have shewn, be caused by the unlike
constitution of the several parts of the earth which are alternately
turned towards the sun, it is credible also, that like effects may be
produced in these other planets from their having their superficies of
unlike parts.