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
But enough of this. I have now sufficiently shewed what at the first I
promised, that this light is not proper to the Moone. It remaines in the
next place, that I tell you the true reason of it. And here, I thinke
’tis probable that the light which appeares in the Moone at the eclipses
is nothing else but the second species of the Sunnes rayes which passe
through the shadow unto her body: and from a mixture of this second
light with the shadow, arises that rednesse which at such times appeares
unto us. I may call it _Lumen crepusculum_, the _Aurora_ of the Moone,
or such a kinde of blushing light, that the Sunne causes when he is
neere his rising, when he bestowes some small light upon the thicker
vapours. Thus wee see commonly the Sunne being in the Horizon, and the
reflexion growing weake, how his beames make the waters appeare very
red.
The Moabites in _Iehorams_ time when they rose early in the morning, and
beheld the waters a farre off, mistooke them for blood.[1]
_Et causa hujus est, quia radius solaris in aurora contrahit quandam
rubedinem, propter vapores combustos manentes circa superficiem
terræ, per quos radii transeunt, & ideo cum repercutiantur in aqua
ad oculos nostros, trahunt secum eundem ruborem, & faciunt apparere
locum aquarum, in quo est repercussio esse rubrum_,
saith _Tostatus_.[2] The reason is, because of his rayes, which being in
the lower vapours, those doe convey an imperfect mixed light upon the
waters. Thus the Moone being in the earths shadow, and the Sunne beames
which are round about it, not being able to come directly unto her body,
yet some second raies there are, which passing through the shadow, make
her appeare in that ruddy colour: So that she must appeare brightest,
when shee is eclipsed, being in her Apoge, of greatest distance from us,
because then the cone of the earths shadow is lesse, and the refraction
is made through a narrower medium. So on the contrary, she must be
represented under a more darke and obscure forme when she is eclipsed,
being in her Perige, or neerest to the earth, because then she is
involved in a greater shadow, or bigger part of the cone, and so the
refraction passing through a greater medium, the light must needes be
weaker which doth proceed from it. If you aske now what the reason may
be of that light which we discerne in the darker part of the new Moone:
I answer, ’tis reflected from our earth which returnes as great a
brightnesse to that Planet, as it receives from it. This I shall have
occasion to prove afterward.
[Sidenote 1: 2 King. 3. 22.]
[Sidenote 2: _2ª. Quæst. in hoc cap._]
I have now done with these propositions which were set downe to cleare
the passage, and confirme the suppositions implied in the opinion, I
shall in the next place proceed to a more direct treating of the chiefe
matter in hand.
Proposition 6.
Public-domain text, read in full here on John Shaqi.
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