The discovery of a world in the moone : $b or, A discovrse tending to prove that 'tis probable there may be another habitable world in that planetWilkins, John
Philosophy
The discovery of a world in the moone : $b or, A discovrse tending to prove that 'tis probable there may be another habitable world in that planet
Wilkins, John
Astronomy -- Early works to 1800; Moon -- Early works to 1800
1. ’Tis observed, that so much of the Moone as is enlightened, is
alwaies part of a bigger circle then that which is darker. Their
frequent experience hath proved this, and an easie observation may
quickely confirme it. But now this cannot proceede from any other cause
so probable, as from this orbe of aire, especially when we consider how
that planet shining with a borrowed light, doth not send forth any such
rayes as may make her appearance bigger then her body.
2. ’Tis observed in the Solary eclipses, that there is a great
trepidation about the body of the Moone, from which we may likewise
argue an Atmo-sphæra, since we cannot well conceive what so probable a
cause there should be of such an appearance as this,
_Quod radii Solares à vaporibus Lunam ambientibus fuerint
intercisi_,[1]
that the Sun beames were broken and refracted by the vapours that
encompassed the Moone.
[Sidenote 1: _Scheiner. Ros. Vrs. l. 4. pars 2. c. 27._]
3. I may adde the like argument taken from another observation which
will be easily tried and granted. When the Sunne is eclipsed, wee
discerne the Moone as shee is in her owne naturall bignesse, but then
she appeares somewhat lesse then when shee is in the full, though she be
in the same place of her supposed excentrick and epicycle, and therefore
_Tycho_ hath calculated a Table for the Diameter of the divers new
Moones. But now there is no reason so probable to salve this appearance,
as to place an orbe of thicker aire, neere the body of that Planet,
which may be enlightened by the reflected beames, and through which the
direct raies may easily penetrate.
But some may object that this will not consist with that which was
before delivered, where I said, that the thinnest parts had least light.
If this were true, how comes it to passe then, that this aire should be
as bright as any of the other parts, when as tis the thinnest of all?
I answer, if the light be received by reflection, then the thickest body
hath most because it is best able to beare backe the raies, but if the
light be received by illumination[1] (especially if there be an opacous
body behinde, which may double the beames by reflexion) as it is here,
then I deny not but a thinne body may retaine much light, and perhaps,
some of those appearances which wee take for fiery comets, are nothing
else but a bright cloud enlightened, so that probable it is, there may
be such aire without the Moone, and hence it comes to passe, that the
greater spots are onely visible towards her middle parts, and none neere
the circumference, not but that there are some as well in those parts as
else where, but they are not there perceiveable, by reason of those
brighter vapours which hide them.
[Sidenote 1: _Hist. l. 1. c. 7. § 11._]
Proposition 11.
_That as their world is our Moone, so our world is their Moone._
Public-domain text, read in full here on John Shaqi.
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