THE OPTICIAN.

1. The word optician is applicable to persons who are particularly

skilled in the science of vision, but especially to those who devote

their attention to the manufacture of optical instruments, such as the

spectacles, the camera obscura, the magic lantern, the telescope, the

microscope, and the quadrant.

2. Light is an emanation from the sun and other luminous bodies, and

is that substance which renders opaque bodies visible to the eye. It

diverges in a direct line, unless interrupted by some obstacle, and

its motion has been estimated at _two hundred thousand miles_ in a

second.

3. A _ray of light_ is the motion of a single particle: and a parcel

of rays passing from a single point, is called _a pencil of rays_.

_Parallel rays_ are such as always move at the same distance from each

other. Rays which continually approach each other, are said to

_converge_; and when they continually recede from each other, they are

said to _diverge_. The point at which converging rays meet is called

the _focus_.

4. Any pellucid or transparent body, as air, water, and glass, which

admits the free passage of light, is called a _medium_. When rays,

after having passed through one medium, are bent out of their original

course by entering another of different density, they are said to be

_refracted_; and when they strike against a surface, and are sent back

from it, they are said to be _reflected_.

5. A _lens_ is glass ground in such a form as to collect or disperse

the rays of light which pass through it. These are of different

shapes; and they have, therefore, received different appellations. A

_plano-convex_ lens has one side flat, and the other convex; a

_plano-concave_ lens is flat on one side, and concave on the other; a

_double convex_ lens is convex on both sides; a _double concave_ lens

is concave on both sides; a _meniscus_ is convex on one side, and

concave on the other. By the following cut, the lenses are exhibited

in the order in which they have been mentioned.

[Illustration]

6. An _incident ray_ is that which comes from any luminous body to a

reflecting surface; and that which is sent back from a reflecting

surface, is called a _reflected ray_. The _angle of incidence_ is the

angle which is formed by the incident ray with a perpendicular to the

reflecting surface; and the _angle of reflection_ is the angle formed

by the same perpendicular and the reflected ray.

7. When the light proceeding from every point of an object placed

before a lens is collected in corresponding points behind it, a

perfect image of the object is there produced. The following cut is

given by way of illustration.

[Illustration]

8. The lens, _a_, may be supposed to be placed in the hole of a

window-shutter of a darkened room, and the arrow at the right to be

standing at some distance without. All the light reflected from the

latter object towards the lens, passes through it, and concentrates,

within the room, in a focal point, at which, if a sheet of paper, or

any other plane of a similar color, is placed, the image of the object

will be seen upon it.

9. This phenomenon is called the _camera obscura_, or dark chamber,

because it is necessary to darken the room to exhibit it. The image at

the focal point within the room is in an inverted position. The reason

why it is thrown in this manner will be readily understood by

observing the direction of the reflected rays, as they pass from the

object through the lens. In the camera obscura, it is customary to

place a small mirror immediately behind the lens, so as to throw all

the light which enters, downwards upon a whitened table, where the

picture may be conveniently contemplated.

10. From the preceding explanation of the camera obscura, the theory

of vision may be readily comprehended, since the eye itself is a

perfect instrument of this kind. A careful examination of the

following representation of the eye will render the similarity

obvious. The eye is supposed to be cut through the middle, from above

downwards.

[Illustration: _a a_, the _sclerotica_; _b b_, the _choroides_; _c c_,

the _retina_; _d d_, the _cornea_; _e_, the _pupil_; _f f_, the

_iris_; _g_, the _aqueous humor_; _h_, the _crystalline humor_; _i i_,

the _vitreous humor_.]

11. The _sclerotica_ is a membranous coat, to which the muscles are

attached which move the eye. The _cornea_ is united to the sclerotica

around the circular opening of the latter, and is that convex part of

the eye, which projects in advance of the rest of the organ. The space

between this and the crystalline lens is occupied by the aqueous humor

and the iris. The _iris_ is united to the choroides, and it possesses

the power of expanding and contracting, to admit a greater or less

number of rays.

12. The _crystalline lens_ is a small body of a crystalline appearance

and lenticular shape, whence its name. It is situated between the

aqueous and vitreous humors, and consists of a membranous sack filled

with a humor of a crystalline appearance. The _vitreous humor_ has

been thus denominated on account of its resemblance to glass in a

state of fusion. The _retina_ is a membrane which lines the whole

cavity of the eye, and is formed chiefly, if not entirely, by the

expansion of the optic nerve.

13. The rays of light which proceed from objects pass through the

cornea, aqueous humor, crystalline lens, and vitreous humor, and fall

upon the retina in a focal point, to which it is brought, chiefly by

the influence of the cornea and the crystalline lens. The image, in

an inverted position, is painted or thrown on the cornea, which

perceives its presence, and conveys an impression of it to the brain,

by means of the optic nerve.

14. _Optical instruments._--The art of constructing optical

instruments is founded upon the anatomical structure, and

physiological action of the eye, and on the laws of light. They are

designed to increase the powers of the eye, or to remedy some defect

in its structure. In the cursory view which we may give of a few of

the many optical instruments which have been invented, we will begin

with the _spectacles_, since they are the best known, and withal the

most simple.

15. The _visual point_, or the distance at which small objects can be

distinctly seen, varies in different individuals. As an average, it may

be assumed at eight or nine inches from the eye. In some persons, it is

much nearer, and in others, considerably more distant. The extreme, in

the former case, constitutes _myopy_, or _short-sightedness_, and, in

the latter case, _presbyopy_, or _long-sightedness_.

16. _Myopy_ is chiefly caused by too great a convexity of the cornea

and the crystalline lens, which causes the rays to converge to a

focus, before they reach the retina. Objects are, therefore,

indistinctly seen by myoptic persons, unless held very near the eye to

throw the focus farther back. This defect may be palliated by the use

of concave glasses, which render the rays proceeding from objects more

divergent.

17. _Presbyopy_ is principally caused by too little convexity of the

cornea and crystalline lens, which throws the focal point of rays

reflected from near objects, beyond the retina. This defect is

experienced by most people, to a greater or less degree, after they

have advanced beyond the fortieth year, and occasionally even by

youth. A remedy, or, at least, a palliation, is found in the use of

convex glasses, which render the rays more convergent, and enable the

eye to refract them to a focus farther forward, at the proper point.

18. The opticians have their spectacles numbered, to suit different

periods of life; but, as the short-sighted and long-sighted conditions

exist in a thousand different degrees, each person should select for

himself such as will enable him to read without effort at the usual

distance.

19. The great obstacle to viewing small objects at the usual distance,

arises from too great a divergence of the light reflected from them,

which causes the rays to reach the retina before they have converged

to a focus. This defect is remedied by convex lenses, which bring the

visual point nearer to the eye, and consequently cause the rays to

concentrate in a large focus upon the retina. The most powerful

microscopic lenses are small globules of glass, which permit the eye

to be brought very near to the object.

20. _Microscopes_ are either _single_ or _double_. In the former case,

but one lens is used, and through this the object is viewed directly;

but, in the latter case, two or more glasses are employed, through one

of which a magnified image is thrown upon a reflecting surface, and

this is viewed through the other glass, or glasses, as the real object

is seen through a single microscope.

21. The _solar microscope_, on account of its great magnifying powers,

is the most wonderful instrument of this kind. The principles of its

construction are the same with those of the camera obscura. The

difference consists chiefly in the minor circumstance of placing the

object very near the lens, by which a magnified image is thrown at the

focal point within the room.

22. In the case of the camera obscura, the objects are at a far

greater distance from the glass on the outside than the images, at the

focal point, on the inside. The comparatively great distance of the

object, in this case, causes the image to be proportionably smaller.

In the solar microscope, a small mirror is used to receive the rays,

and to reflect them directly upon the object.

23. The _magic lantern_ is an instrument used for magnifying paintings

on glass, and for throwing their images upon a white surface in a

darkened room. Its general construction is the same with that of the

solar microscope; but, in the application, the light of a lamp is

employed instead of that from the sun.

24. _Telescopes_ are employed for viewing objects which from their

distances appear small, or are invisible to the naked eye. They are of

two kinds, _refracting_ and _reflecting_. The former kind is a

compound of the camera obscura and the single microscope. It consists

of a tube, having at the further end a double convex lens, which

concentrates the rays at a focal point within, where the image is

viewed through a microscopic lens, placed at the other end.

25. In the construction of reflecting telescopes, concave mirrors, or

specula, are combined with a double convex lens. A large mirror of

this kind is so placed in the tube, that it receives the rays of light

from objects, and reflects them upon another of a smaller size. From

this they are thrown to a focal point, where the image is viewed

through a double convex lens. The specula are made of speculum metal,

which is a composition of certain proportions of copper and tin.

26. Many optical appearances are of such frequent recurrence, that

they could not have escaped the earliest observers; nevertheless, ages

appear to have elapsed, before any progress was made towards an

explanation of them. Empedocles, a Greek philosopher, born at

Agrigentum in Sicily, 460 years before Christ, is the first person on

record who attempted to write systematically on light.

27. The subject was successively treated by several other

philosophers; but the ancients never attained to a high degree of

information upon it. We have reason to believe, however, that convex

lenses were, in some cases, used as magnifiers, and as burning

glasses, although the theory of their refractive power was not

understood.

28. The magnifying power of glasses, and some other optical phenomena,

were largely treated by Al Hazen, an Arabian philosopher, who

flourished about the year 1100 of our era; and, in 1270, Vitellio, a

Polander, published a treatise on optics, containing all that was

valuable in Al Hazen's work, digested in a better manner, and with

more lucid explanations of various phenomena.

29. Roger Bacon, an English monk, who was born in 1214, and who lived

to the age of seventy-eight, described very accurately the effects of

convex and concave lenses, and demonstrated, by actual experiment,

that a small segment of a glass globe would greatly assist the sight

of old persons. Concerning the actual inventor of spectacles, however,

we have no certain information; we only know that these useful

instruments were generally known in Europe, about the beginning of the

fourteenth century.

30. In the year 1575, Maurolicus, a teacher of mathematics, at

Messina, published a treatise on optics, in which he demonstrated that

the crystalline humor of the eye is a lens, which collects the rays of

light from external objects, and throws them upon the retina. Having

arrived at a knowledge of these facts, he was enabled to assign the

reasons why some people were short-sighted, and others long-sighted.

31. John Baptista Porta, of Naples, was contemporary with Maurolicus.

He invented the camera obscura, and his experiments with this

instrument convinced him, that light was a substance, and that its

reception into the eye produced vision. These discoveries corresponded

very nearly with those by Maurolicus, although neither of these

philosophers had any knowledge of what the other had done. The

importance of Porta's discoveries will be evident, when it is

observed, that, before his time, vision was supposed to be dependent

on what were termed _visual rays_, proceeding from the eye.

32. The telescope was invented towards the latter end of the sixteenth

century. Of this, as of many other valuable inventions, accident

furnished the first hint. It is said, that the children of Zacharias

Jansen, a spectacle-maker, of Middleburg in Holland, while playing

with spectacle-glasses in their father's shop, perceived that, when

the glasses were held at a certain distance from each other, the dial

of the clock appeared greatly magnified, but in an inverted position.

33. This incident suggested to their father the idea of adjusting two

of these glasses on a board, so as to move them at pleasure. Two such

glasses inclosed in a tube completed the invention of the simplest

kind of the refracting telescope. Galileo greatly improved the

telescope, and constructed one that magnified thirty-three times, and

with this he made the astronomical discoveries which have immortalized

his name.

34. John Kepler, a great mathematician and astronomer, who was born at

Weir, in Wurtemburg, in the year 1571, paid great attention to the

phenomena of light and vision. He was the first who demonstrated that

the degree of refraction suffered by light in passing through lenses,

corresponds with the diameter of the circle of which the concavity or

convexity is the portion of an arch. He very successfully pursued the

discoveries of Maurolicus and Porta, and asserted that the images of

external objects were formed upon the optic nerve by the concentration

of rays which proceed from them.

35. In 1625, the curious discovery of Scheiner was published, at Rome,

which placed beyond doubt the fact, that vision depends upon the

formation of the image of objects upon the retina. The fact was

demonstrated by cutting away, at the back part, the two outside coats

of the eye of an animal, and by presenting different objects before

it. The images were distinctly seen painted on the naked retina.

36. Near the middle of the seventeenth century, the velocity of light

was discovered by Roemer; and, in 1663, James Gregory, a celebrated

Scotch mathematician, published the first proposal for a reflecting

telescope. But, as he possessed no mechanical dexterity himself, and

as he could find no workman capable of executing his designs, he never

succeeded in carrying his conceptions into effect. This was reserved

for Sir Isaac Newton; who, being remarkable for manual skill, executed

two instruments of this kind, in the year 1672, on a plan, however,

somewhat different from that proposed by Gregory.

37. In the course of the year 1666, the attention of Sir Isaac Newton

was drawn to the phenomena of the refraction of light through the

prism; and, having observed a certain surprising fact, he instituted a

variety of experiments, by which he was brought to the conclusion,

that light was not a homogeneous substance, but that it is composed of

particles, which are capable of different degrees of refrangibility.

38. By the same experiments, he also proved, that the rays or

particles of light differ from each other in exhibiting different

colors, some producing the color red, others that of yellow, blue, &c.

He applied his principles to the explanation of most of the phenomena

of nature, where light and color are concerned; and almost every thing

which we know upon these subjects, was laid open by his experiments.

39. The splendor of Sir Isaac Newton's discoveries obscures, in some

measure, the merits of earlier and subsequent philosophers; yet

several interesting discoveries in regard to light and color, as well

as many important improvements of optical instruments, have been made

since his time, although the light by which these have been achieved,

was derived principally from his labors.

[Illustration: GOLDBEATER.]

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