PERSPECTIVE.

If you transmit the rays of the sun through a hole in the shape of a

star you will see a beautiful effect of perspective in the spot

where the sun's rays fall.

[Footnote: In this and the following chapters of MS. C the order of

the original paging has been adhered to, and is shown in

parenthesis. Leonardo himself has but rarely worked out the subject

of these propositions. The space left for the purpose has

occasionally been made use of for quite different matter. Even the

numerous diagrams, most of them very delicately sketched, lettered

and numbered, which occur on these pages, are hardly ever explained,

with the exception of those few which are here given.]

214.

No small hole can so modify the convergence of rays of light as to

prevent, at a long distance, the transmission of the true form of

the luminous body causing them. It is impossible that rays of light

passing through a parallel [slit], should not display the form of

the body causing them, since all the effects produced by a luminous

body are [in fact] the reflection of that body: The moon, shaped

like a boat, if transmitted through a hole is figured in the surface

[it falls on] as a boatshaped object. [Footnote 8: In the MS. a

blank space is left after this question.] Why the eye sees bodies at

a distance, larger than they measure on the vertical plane?.

[Footnote: This chapter, taken from another MS. may, as an

exception, be placed here, as it refers to the same subject as the

preceding section.]

On gradation of shadows (215. 216).

215.

Although the breadth and length of lights and shadow will be

narrower and shorter in foreshortening, the quality and quantity of

the light and shade is not increased nor diminished.

[3]The function of shade and light when diminished by

foreshortening, will be to give shadow and to illuminate an object

opposite, according to the quality and quantity in which they fall

on the body.

[5]In proportion as a derived shadow is nearer to its penultimate

extremities the deeper it will appear, _g z_ beyond the intersection

faces only the part of the shadow [marked] _y z_; this by

intersection takes the shadow from _m n_ but by direct line it takes

the shadow _a m_ hence it is twice as deep as _g z_. _Y x_, by

intersection takes the shadow _n o_, but by direct line the shadow

_n m a_, therefore _x y_ is three times as dark as _z g_; _x f_, by

intersection faces _o b_ and by direct line _o n m a_, therefore we

must say that the shadow between _f x_ will be four times as dark as

the shadow _z g_, because it faces four times as much shadow.

Let _a b_ be the side where the primary shadow is, and _b c_ the

primary light, _d_ will be the spot where it is intercepted,_f g_

the derived shadow and _f e_ the derived light.

And this must be at the beginning of the explanation.

[Footnote: In the original MS. the text of No. 252 precedes the one

given here. In the text of No. 215 there is a blank space of about

four lines between the lines 2 and 3. The diagram given on Pl. VI,

No. 2 is placed between lines 4 and 5. Between lines 5 and 6 there

is another space of about three lines and one line left blank

between lines 8 and 9. The reader will find the meaning of the whole

passage much clearer if he first reads the final lines 11--13.

Compare also line 4 of No. 270.]

On relative proportion of light and shadows (216--221).

216.

That part of the surface of a body on which the images [reflection]

from other bodies placed opposite fall at the largest angle will

assume their hue most strongly. In the diagram below, 8 is a larger

angle than 4, since its base _a n_ is larger than _e n_ the base of

4. This diagram below should end at _a n_ 4 8. [4]That portion of

the illuminated surface on which a shadow is cast will be brightest

which lies contiguous to the cast shadow. Just as an object which is

lighted up by a greater quantity of luminous rays becomes brighter,

so one on which a greater quantity of shadow falls, will be darker.

Let 4 be the side of an illuminated surface 4 8, surrounding the

cast shadow _g e_ 4. And this spot 4 will be lighter than 8, because

less shadow falls on it than on 8. Since 4 faces only the shadow _i

n_; and 8 faces and receives the shadow _a e_ as well as _i n_ which

makes it twice as dark. And the same thing happens when you put the

atmosphere and the sun in the place of shade and light.

[12] The distribution of shadow, originating in, and limited by,

plane surfaces placed near to each other, equal in tone and directly

opposite, will be darker at the ends than at the beginning, which

will be determined by the incidence of the luminous rays. You will

find the same proportion in the depth of the derived shadows _a n_

as in the nearness of the luminous bodies _m b_, which cause them;

and if the luminous bodies were of equal size you would still

farther find the same proportion in the light cast by the luminous

circles and their shadows as in the distance of the said luminous

bodies.

[Footnote: The diagram originally placed between lines 3 and 4 is on

Pl. VI, No. 3. In the diagram given above line 14 of the original,

and here printed in the text, the words _corpo luminoso_ [luminous

body] are written in the circle _m_, _luminoso_ in the circle _b_

and _ombroso_ [body in shadow] in the circle _o_.]

217.

THAT PART OF THE REFLECTION WILL BE BRIGHTEST WHERE THE REFLECTED

RAYS ARE SHORTEST.

[2] The darkness occasioned by the casting of combined shadows will

be in conformity with its cause, which will originate and terminate

between two plane surfaces near together, alike in tone and directly

opposite each other.

[4] In proportion as the source of light is larger, the luminous and

shadow rays will be more mixed together. This result is produced

because wherever there is a larger quantity of luminous rays, there

is most light, but where there are fewer there is least light,

consequently the shadow rays come in and mingle with them.

[Footnote: Diagrams are inserted before lines 2 and 4.]

218.

In all the proportions I lay down it must be understood that the

medium between the bodies is always the same. [2] The smaller the

luminous body the more distinct will the transmission of the shadows

be.

[3] When of two opposite shadows, produced by the same body, one is

twice as dark as the other though similar in form, one of the two

lights causing them must have twice the diameter that the other has

and be at twice the distance from the opaque body. If the object is

lowly moved across the luminous body, and the shadow is intercepted

at some distance from the object, there will be the same relative

proportion between the motion of the derived shadow and the motion

of the primary shadow, as between the distance from the object to

the light, and that from the object to the spot where the shadow is

intercepted; so that though the object is moved slowly the shadow

moves fast.

[Footnote: There are diagrams inserted before lines 2 and 3 but they

are not reproduced here. The diagram above line 6 is written upon as

follows: at _A lume_ (light), at _B obbietto_ (body), at _C ombra

d'obbietto_ (shadow of the object).]

219.

A luminous body will appear less brilliant when surrounded by a

bright background.

[2] I have found that the stars which are nearest to the horizon

look larger than the others because light falls upon them from a

larger proportion of the solar body than when they are above us; and

having more light from the sun they give more light, and the bodies

which are most luminous appear the largest. As may be seen by the

sun through a mist, and overhead; it appears larger where there is

no mist and diminished through mist. No portion of the luminous body

is ever visible from any spot within the pyramid of pure derived

shadow.

[Footnote: Between lines 1 and 2 there is in the original a large

diagram which does not refer to this text. ]

220.

A body on which the solar rays fall between the thin branches of

trees far apart will cast but a single shadow.

[2] If an opaque body and a luminous one are (both) spherical the

base of the pyramid of rays will bear the same proportion to the

luminous body as the base of the pyramid of shade to the opaque

body.

[4] When the transmitted shadow is intercepted by a plane surface

placed opposite to it and farther away from the luminous body than

from the object [which casts it] it will appear proportionately

darker and the edges more distinct.

[Footnote: The diagram which, in the original, is placed above line

2, is similar to the one, here given on page 73 (section 120).--The

diagram here given in the margin stands, in the original, between

lines 3 and 4.]

221.

A body illuminated by the solar rays passing between the thick

branches of trees will produce as many shadows as there are branches

between the sun and itself.

Where the shadow-rays from an opaque pyramidal body are intercepted

they will cast a shadow of bifurcate outline and various depth at

the points. A light which is broader than the apex but narrower than

the base of an opaque pyramidal body placed in front of it, will

cause that pyramid to cast a shadow of bifurcate form and various

degrees of depth.

If an opaque body, smaller than the light, casts two shadows and if

it is the same size or larger, casts but one, it follows that a

pyramidal body, of which part is smaller, part equal to, and part

larger than, the luminous body, will cast a bifurcate shadow.

[Footnote: Between lines 2 and 3 there are in the original two large

diagrams.]

_IV._

_Perspective of Disappearance._

_The theory of the_ "Prospettiva de' perdimenti" _would, in many

important details, be quite unintelligible if it had not been led up

by the principles of light and shade on which it is based. The word_

"Prospettiva" _in the language of the time included the principles

of optics; what Leonardo understood by_ "Perdimenti" _will be

clearly seen in the early chapters, Nos._ 222--224. _It is in the

very nature of the case that the farther explanations given in the

subsequent chapters must be limited to general rules. The sections

given as_ 227--231 _"On indistinctness at short distances" have, it

is true, only an indirect bearing on the subject; but on the other

hand, the following chapters,_ 232--234, _"On indistinctness at

great distances," go fully into the matter, and in chapters_

235--239, _which treat "Of the importance of light and shade in the

Perspective of Disappearance", the practical issues are distinctly

insisted on in their relation to the theory. This is naturally

followed by the statements as to "the effect of light or dark

backgrounds on the apparent size of bodies"_ (_Nos._ 240--250). _At

the end I have placed, in the order of the original, those sections

from the MS._ C _which treat of the "Perspective of Disappearance"

and serve to some extent to complete the treatment of the subject_

(251--262).

Definition (222. 223).

222.

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