Philosophical Transactions of the Royal Society - Vol 1 - 1666: Giving some Accompt of the present Undertakings, Studies, and Labours of the Ingenious in many considerable parts of the WorldVarious
History
Philosophical Transactions of the Royal Society - Vol 1 - 1666: Giving some Accompt of the present Undertakings, Studies, and Labours of the Ingenious in many considerable parts of the World
Various
Science -- Periodicals
Yet this I must add, (that I be not mistaken) that whereas I cast the time
of the daily Tydes to be at all places, when the Moon is there in the
_Meridian_; it must be understood of _open_ Seas, where the water hath such
free scope for its motions, as if the whole Globe of Earth were equally
covered with water: Well knowing, that in _Bayes_ and _In land-Channels_,
the position of the Banks and other like causes must needs make the times
to be much different from what we suppose in the open Seas: And likewise,
that even in the Open Seas, _Islands_, and _Currents_, _Gulfs_ and
_Shallows_, may have some influence, though not comparable to that of
_Bays_ and _Channels_. And moreover, though I think, that Seamen do
commonly reckon the time of High-water in the _Open Seas_, to be then, when
the Moon is there in the _Meridian_ (as this Hypothesis would cast it:) Yet
I do not take my self to be so well furnished with a _History of Tides_, as
to assure my self of it; much less to accommodate it to particular places
and cases.
Having thus dispatched the main of what I had to say {280} concerning the
Seas Ebbing and Flowing: Had I not been already too tedious, I should now
proceed to give a further reason, why I do introduce this consideration of
the _Common Center of Gravity_ in reference to _Astronomical Accounts_. For
indeed, that which may possibly seem at first to be an Objection _against_
it, is with me one reason _for_ it.
It may be thought perhaps, that if the Earth should thus describe an
_Epicycle_ about the Common Center of Gravity, it would (by this its change
of place) disturbe the _Caelestial_ motions; and make the _apparent_ places
of the Planets, especially some of them, different from what they would
otherwise be. For though so small a removal of the Earth, as the _Epicycle_
would cause (especially if its _Semidiameter_ should not be above 1-1/3 of
the Earths Semidiameter) would scarce be sensible (if at all) to the
remoter Planets; yet as to the nearer it might.
Public-domain text, read in full here on John Shaqi.
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