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
Whereas ’tis the common opinion and found true enough by observation,
that _Olympus_, _Atlas_, _Taurus_ and _Enius_, with many others are much
above this height. _Tenariffa_ in the Canary Ilands is proved by
computation to bee above 8 miles perpendicular, and about this height is
the mount _Perjacaca_ in _America_. Sr. _Walter Rawleigh_ seemes to
thinke, that the highest of these is neere 30 miles upright: nay
_Aristotle_[1] speaking of _Caucasus_ in _Asia_, affirmes it to bee
visible for 560 miles, as some interpreters finde by computation, from
which it will follow, that it was 78 miles perpendicularly high, as you
may see confirmed by _Jacobus Mazonius_,[2] and out of him in
_Blancanus_ the Jesuite.[3] But this deviates from the truth more in
excesse then the other doth in defect. However though these in the moone
are not so high as some amongst us, yet certaine it is they are of a
great height, and some of them at the least foure miles perpendicular.
This I shall prove from the observation of _Galilæus_, whose glasse can
shew this truth to the senses, a proofe beyond exception and certaine
that man must needs be of a most timerous faith who dares not believe
his owne eye.
[Sidenote 1: _Meteor. l. 1. c. 11._]
[Sidenote 2: _Comparatio Arist. cum Platone, Sect. 3. c. 5._]
[Sidenote 3: _Exposi. in loc. Math. Artis. loc. 148._]
By that perspective you may plainely discerne some enlightned parts
(which are the mountaines) to be distant from the other about the
twentieth part of the diameter. From whence it will follow, that those
mountaines must necessarily be at the least foure Italian miles in
height.
[Illustration]
For let BDEF be the body of the moone, ABC will be a ray or beame of the
Sunne, which enlightens a mountaine at A and _B_ is the point of
contingency, the distance betwixt A and B must bee supposed to be the
twentieth part of the diameter which is an 100 miles, for so far are
some enlightened parts severed from the common terme of illumination.
Now the aggregate of the quadrate from A _B_ a hundred, and _B_ _G_ a
1000 will bee 1010000, unto which the quadrate arising from A G must be
equall according to the 47th proposition in the first booke of elements.
Therefore the whole line _A_ _G_ is somewhat more than 104, and the
distance betwixt H A must be above 4 miles, which was the thing to be
proved.
But it may be againe objected, if there be such rugged parts, and so
high mountaines, why then cannot wee discerne them at this distance, why
doth the moone appeare unto us so exactly round, and not rather as a
wheele with teeth?
I answere, by reason of too great a distance, for if the whole body
appeare to our eye so little, then those parts which beare so small a
proportion to the whole will not at all be sensible.
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Elsewhere in the archive
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account