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
One of the means used by M. _Auzout_ to enlighten an Object, in what
proportion one pleaseth, is by some great _Object-Glass_, by him called a
_Planetary_ one, because that by it he shews the difference of Light, which
all the _Planets_ receive from the _Sun_, by making use of several
_Apertures_, proportionate to their distance from the _Sun_, provided that
for every 9 foot draught, or thereabout, one inch of _Aperture_ be given
for the _Earth_. Doing this, one sees (_saith he_) that the Light which
_Mercury_ receives, is far enough from being able to burn Bodies, and yet
that the same Light is great enough in _Saturn_ to see cleer there, seeing
that (to him) it appears greater in _Saturn_, than it doth upon our
_Earth_, when it is overcast with Clouds: Which (he adds) would scarce be
believed, if by means of this Glass it did not sensibly appear so; Whereof
he promises to discourse more fully in his {70} _Treatise of the usefulness
of great Optick-Glasses_, where he also intends to deliver several
Experiments, by him made, 1. Touching the quantity of Light, which a Body,
that is 10, 15 and 20 times, &c. remoter than _Saturn_, would yet receive
from the _Sun_. 2. Touching the quantity of Light, by which the _Earth_ is
illuminated even in the _Eclipses_ of the _Sun_, in proportion of their
bigness. 3. Touching the quantity of Light, which is necessary to burn
Bodies: he having found, that not abating the Light, which is reflected by
the Surfaces of the Glass (whereof he confesseth, he doth not yet exactly
know the quantity) there would be necessary about 50 times as much Light,
as we have here, for the burning of _Black_ Bodies; and neer 9 times more
for the burning of _White_ Bodies, than for the burning of _Black_ ones:
and so observing the immediate proportions between these two, for burning
bodies of _other_ Colors. Whence (he tells us) he hath drawn some
consequences, touching the distance, at which we may hope, to burn Bodies
here, by the means of _great Glasses_ and great _Looking-glasses_. So that
(_saith he_) we must yet be seven times neerer the _Sun_, than we are, to
be in danger of being burned by it. Where he mentions, that having given
_Instructions_ to certain persons, gon to travel in _Hot Countries_, he
hath among other particulars recommended to them, to try by means of great
_Burning-glasses_, with how much less _Aperture_ they will burn _there_,
than _here_, to know from thence, whether there by more Light _there_ than
_here_, and how much; since this perhaps may be the only means of trying
it, supposing, the same matters be used: although the difference of the Air
already heated, both in _hot Countries_, and in the _Planets_, that are
neerer than we, may alter, if not the quantity of Light, at least that of
the Heat, found there.
* * * * *
_A further Account, touching Signor _Campani_'s Book and Performances about
_Optick-glasses_._
Public-domain text, read in full here on John Shaqi.
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