Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
History
Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
Natural history; Science -- Early works to 1800; Voyages and travels -- Early works to 1800
Now suppose the _Earth_, being in _L_, towards the second Quadrature of
_Jupiter_, hath seen the first Satellit, at the time of its emersion, or
issuing out of the shadow at _D_, and that about 42½ Hours after
(_viz._ after one Revolution of this _Satellit_) the _Earth_ being in
_K_, do see it return'd in _D_: It is manifest, that if the Light
require time to traverse the Interval _LK_, the _Satellit_ will be seen
return'd later in _D_, than it would have been if the _Earth_ had
remained in _L_. So that the Revolution of the _Satellit_ being thus
observ'd by the Emersions, will be retarded by so much time, as the
Light shall have taken in passing from _L_ to _K_; and that on the
contrary, in the other Quadrature _FG_, where the _Earth_ by approaching
goes to meet the Light, the Revolutions of the Emersions will appear to
be shortned, by so much as those of the Emersions had appear'd to be
lengthned. And because 42½ Hours, which this _Satellit_ very near
takes to make one Revolution, the distance between the _Earth_ and
_Jupiter_, in both the Quadratures, varies at least 210 Diameters of the
_Earth_: It follows, that if for the Account of every Diameter of the
_Earth_ there were required a Second of Time, the Light would take 3½
Minutes for each of the Intervals _GF_, _KL_; which would cause near
half a quarter of an Hour between two Revolutions of the first
_Satellit_, one observ'd in _FG_, and the other in _KL_, whereas there
is not observed any sensible difference.
Yet doth it not follow hence, that Light demands no time. For after M.
_Romer_ had examin'd the thing more nearly, he found that what was not
sensible in two Revolutions, became very considerable in many being
taken together; and that, for Example, forty Revolutions observed on the
side _F_, might be sensibly shorter, than forty others observ'd in any
place of the _Zodiack_ where _Jupiter_ may be met with; and that in
proportion of Twenty two for the whole Interval of _HE_, which is the
double of the Interval that is from hence to the Sun.
The necessity of this new Equation of the Retardment of Light, is
establish'd by all the Observations that have been made in the _Royal
Academy_, and in the _Observatory_, for the space of eight Years; and it
hath been lately confirmed by the Emersion of the first _Satellit_
observ'd at _Paris_, the _9th_ of _November_ last, at 5 a-clock 35' 45"
at Night, 10 Minutes later than it was to be expected, by deducting it
from those that had been observ'd in the Month of _August_, when the
_Earth_ was much nearer to _Jupiter_; which M. _Romer_ had predicted to
the said Academy from the beginning of _September_.
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