( -87 )
r —=z but is the two Convexities be os the fame Sphere, so as r = &
rf {
then will the Distance be = p r, that is, is the Lens be Glaß — z r, so that ifan Object be placed at the Diameter os the Sphere distant, in this case theFocus will be as far within as the Object is without, and the Species repre-sented thereby will be as big as the Life; but if it were a Plano-Convex,the fame distance will be = if r, or in Glaß, to four times the Radius osthe Convexity.
A second Use is to find what Convexity or Concavity is required, to makea västly distant Object be represented at a given Focus, aster the one Sursaceos the Lens is formed - } which is but a Corollary of our Theorem for finding f,having />, d, r, and f, given ; for d being Infinite, that Rule becomes
rf
— x, that is in Glaß
rf
— ?, whence if / be greater than 2. > ,
pr-f " *r-f
r' f
f becomes Negative, and — - -is the Radius of the Concave sought.
But to return to our first Theorem , which accounting for the thicknefi ofthe Lens, we will here again resume, vi%. 'mpdr% — nd%t -p- nprft
m dr -+■ mdf — mp i r — m — hdt -+■ nrt
And let it be requir’d to find the Focus where a whole Sphere will col-
lecb the Beams procecding from an Object at the distance d. Here t is equal
to zr , and r — x; And aster due Reduction, the Theorem will stand thus,
mpdr — zndr ■+ Znprr r ,-s J . 7C - •• n.j
£ ---— f: but u d be lnhmte, it is contracted to
i sj + i»r — mp rZ n — m
r = fy wherefore a Sphere of Glaß collects the Sun's
tnp r
z n Zm — Z n
Beams at half the Semidiameter of the Sphere without it, and a Sphere ofA Vater at a whole Semidiameter. But if the Ratio of Refraction m to » beas z to 1, the Focus falis on the opposite Sursace of the Sphere, but if it beof greater Inequality it falis within.
Another Example shall be when a Hemisphere is exposed to Parallel Rays,that is, d and x being Infinite, and t = r, and aster due Reduction, the The-
orem
resolts
n n
m m
-r — f \ that is, in Glaß it is at -f r, in Water
at | r, but if the Hemilphere were Diamant, it would collect the Beams
at r? of the Radius beyond the Center.
Bb i
Lastly,