As only one side of an object can be viewed at a time, it is sufficient,

in general, to know how much the surface thereof is magnified: but when

it is necessary to know how many minute objects are contained in a

larger, as for instance, how many given animalculæ are contained in the

bulk of a grain of sand, then we must cube the first number, by which

means we shall obtain the solidity or magnified bulk.

The foregoing rule has been also applied to estimate the magnifying

power of the compound microscope. To this application, Mr. Magny, in the

“Journal d’Economie pour le mois d’Aout 1753,” has made several

objections: one or two of these I shall just mention; the first is the

difficulty of ascertaining with accuracy the precise focus of a small

lens; the second is the want of a fixed or known measure, with which to

compare the focus when ascertained. These considerations, though

apparently trifling, will be found of importance in the calculations

which are relative to deep magnifiers. To this it may be further added,

that the same standard or fixed measure cannot be assumed for a

short-sighted, that is used for a well-constituted eye. To obviate these

difficulties, and some errors in the methods which were recommended by

Mess. Baker and Needham, Mr. Magny offers the following

PROPOSITION. All convex lenses of whatsoever foci, double the apparent

diameter of an object, provided that the object be at the focus of the

glass on one side, and the eye be at the same distance, or on the focus

of the glass, at the opposite side.

EXPERIMENT. Take a double convex lens, of six or eight inches focus, and

fix it as at A, Fig. 1, Plate II. A, into the piece A, which is fixed

perpendicular to the rule F G, and may be slid along it by means of its

socket: the rule is divided into inches and parts. Paste a piece of

white paper, two or three tenths of an inch broad, and three inches

long, on the board D; draw three lines with ink on this piece of paper,

so as to divide it into four equal parts, taking care that the middle of

the paper corresponds with the center of the lens. There is also a

sliding eye-piece, which is represented at e.

Take this apparatus into the darkest part of the room, but opposite to

the window; direct the glass towards any remarkable and distant object

which is out of doors, and move the sliding piece B, until the image of

the object on the paper be sharp and clear. The distance between the

face of the paper and the lens (which is shewn on the side of the rule

by the divisions thereon) is the focus of the glass; now set the

eye-piece e E to the same distance on the other side of the glass, then

with one eye close to the sight at e, look at the magnified image of the

lines, and with the other eye at the lines themselves: the image, seen

by means of the glass, and expressed in the figure by the dotted lines,

will be double the breadth of the same object seen by the natural eye.

This will be found to be true, whatsoever is the focus of the lens with

which the experiment is made.

This experiment is rendered more simple to those who are not accustomed

to observe with both eyes at the same time, by making use of half a

lens, and placing the diameter perpendicular to the rule, as they may

then readily view the magnified image and real object with the same

glance of the eye, and thus compare them together with ease and

accuracy.

Let the angle A F B, Fig. 3. Plate II. A, represent that which is formed

at the naked eye, by the rays of light which pass from the extremities

of the object, and unite at the eye in the point F. The angle D F E is

formed of the two rays, which at first proceeded parallel to each other

from the extremities of the object, but that were afterwards so

refracted, or bent, by passing through the glass, as to unite at its

focal point F. C O is equal to the focal distance of the lens on the

side next the object, C F equal thereto on the side next the eye, F O

the distance of the eye.

From the allowed principles of optics, it is evident, that the object

would appear double the size to the eye at C, than it would to the eye

when placed at F; because the distance F O is double the distance C O.

We have only to prove then, that the angle A C B is equal to the angle I

F K, in order to establish the proposition.

The optical axis is perpendicular to the glass and the surface of the

object. The rays A I, B K, which flow from the points A B are parallel

to each other, and perpendicular to the glass, till they arrive at it;

they are then refracted and proceed to F, where they form the triangle I

F K, resting on the base I K: now as C F is equal to C O, and I K is

equal to A B, the two triangles A C B, I F K are similar, and

consequently the angle at C is equal to the angle F. If the visual rays

are continued to the surface of the object, they will form the triangle

D F E, equiangled to the triangle A B C; and therefore, as C O is to A

B, so is F D to D E; and consequently, the apparent diameter of the

object seen through the lens is double the size that it is when viewed

by the naked eye. No notice is here taken of the double refraction of

the rays, as it does not affect the demonstration.

If you advance towards M, half the focal distance, the apparent diameter

will be only increased one-third. If, on the contrary, the point of

sight is lengthened to double the distance of its focus, then the

magnified diameter will appear to be three times that of the real

object. Mr. Magny concludes from hence, that there is an impropriety in

estimating the magnifying power of the eye glass of compound

microscopes, by seeing how often its focus is contained in eight or ten

inches; and to obviate these defects, he recommends two methods to be

used, which reciprocally confirm each other.

The first and most simple method to find how much any compound

microscope magnifies an object, is the same which is described by Dr.

Hooke in his Micrographia, and is as follows: place an accurate scale,

which is divided into very minute parts of an inch, on the stage of your

microscope; adjust the microscope, till these divisions appear distinct;

then observe with the other eye how many divisions of a rule, similarly

divided and held at the stage, are included in one of the magnified

divisions: for if one division, as seen with one eye through the

microscope, extend to thirty divisions on the rule, which is seen by the

naked eye, it is evident, that the diameter of the object is increased

or magnified thirty times.

For this purpose, we often use a small black ebony rule, (see Fig. 4.

Plate II. A,) three or four tenths of an inch broad, and about seven

inches long; at each inch is fixed a piece of ivory, the first inch is

entirely of ivory, and subdivided into ten equal parts.

2. A piece of glass, Fig. 2, fixed in a brass or ivory slider; on the

diameter of this are drawn two parallel lines, about three-tenths of an

inch long; each tenth being divided, one into three, the second into

four, the third into five parts. To use this, place the glass, Fig. 2,

on the middle of the stage, and the rule, Fig. 4, on one side, but

parallel to it; then look into the microscope with one eye, keeping the

other open, and observe how many parts one-tenth of a line in the

microscope takes in upon the parts of the rule seen by the naked eye.

For instance, suppose with a fourth magnifier that one-tenth of an inch

magnified answers in length to forty-tenths or parts on the rule, when

seen by the naked eye, then this magnifier increases the diameter of the

object forty times.

This mode of actual admeasurement is, without doubt, the most simple

that can be used; by it we comprehend, as it were, at one glance, the

different effects of combined glasses; it saves the trouble, and avoids

the obscurity that attends the usual modes of calculation; but many

persons find it exceedingly difficult to adopt this method, because they

have not been accustomed to observe with both eyes at once. We shall

therefore proceed to describe another method, which has not this

inconvenience.

OF THE NEEDLE MICROMETER.

Fig. 8. Plate II. A, represents this micrometer. The first of this kind

was made by my father, and was described by him in his Micrographia

Illustrata. It consists of a screw, which has fifty threads to an inch;

this screw carries an index, which points to the divisions on a circular

plate, which is fixed at right angles to the axis of the screw. The

revolutions of the screw are counted on a scale, which is an inch

divided into fifty parts; the index to these divisions is a flower de

luce marked upon the slider, which carries the needle point across the

field of the microscope. Every revolution of the micrometer screw

measures ¹⁄₅₀ part of an inch, which is again subdivided by means of the

divisions on the circular plate, as this is divided into twenty equal

parts, over which the index passes at every revolution of the screw; by

which means, we obtain with ease the measure of one-thousandth part of

an inch; for 50, the number of threads on the screw in one inch, being

multiplied by 20, the divisions on the circular plate, are equal to

1000; so that each division on the circular plate shews that the needle

has either advanced or receded one-thousandth part of an inch.

To place this micrometer on the body of the microscope, open the

circular part F K H, Fig. 8. Plate II. A, by taking out the screw G,

throw back the semicircle F K which moves upon a joint at K, then turn

the sliding tube of the body of the microscope, so that the small holes

which are in both tubes may exactly coincide, and let the needle g of

the micrometer have a free passage through them; after this, screw it

fast upon the body by the screw G.

The needle will now traverse the field of the microscope, and measure

the length and breadth of the image of any object that is applied to it.

But further assistance must be had, in order to measure the object

itself, which is a subject of real importance; for though we have

ascertained the power of the microscope, and know that it is so many

thousand times, yet this will be of little assistance towards

ascertaining an accurate idea of its real size; for our ideas of bulk

being formed by the comparison of one object with another, we can only

judge of that of any particular body, by comparing it with another

whose size is known: the same thing is necessary, in order to form an

estimate by the microscope; therefore, to ascertain the real measure of

the object, we must make the point of the needle pass over the image of

a known part of an inch placed on the stage, and write down the

revolutions made by the screw, while the needle passed over the image of

this known measure; by which means we ascertain the number of

revolutions on the screw, which are adequate to a real and known measure

on the stage. As it requires an attentive eye to watch the motion of the

needle point, as it passes over the image of a known part of an inch on

the stage, we ought not to trust to one single measurement of the image,

but ought to repeat it at least six times; then add the six measures

thus obtained together, and divide their sum by six, or the number of

trials; the quotient will be the mean of all the trials. This result is

to be placed in a column of a table, next to that which contains the

number of the magnifiers.

By the assistance of the sectoral scale, we obtain with ease a small

part of an inch. This scale is shewn at Fig. 5, 6, 7. Plate II. A, in

which the two lines c a c b, with the side a b, form an isosceles

triangle; each of the sides is two inches long, and the base one-tenth

of an inch. The longer sides may be of any given length, and the base

still only of one-tenth of an inch. The longer lines may be considered

as the line of lines upon a sector opened to one-tenth of an inch.

Hence, whatever number of equal parts ca cb are divided into, their

transverse measure will be such a part of one-tenth as is expressed by

their divisions. Thus, if it be divided into ten equal parts, this will

divide the inch into one-hundred equal parts; the first division next c

will be equal to one-hundredth part of an inch, because it is the tenth

part of one-tenth of an inch. If these lines be divided into twenty

equal parts, the inch will be by those means divided into two hundred

equal parts. Lastly, if a b c a be made three inches long, and divided

into one-hundred equal parts, we obtain with ease the one-thousandth

part. The scale is represented as solid at Fig. 6, but as perforated at

Fig. 5 and 7; so that the light passes through the aperture, when the

sectoral part is placed on the stage.

To use this scale, first fix the micrometer, Fig. 8. Plate II. A, to the

body of the microscope; then fit the sectoral scale, Fig. 7, in the

stage, and adjust the microscope to its proper focus or distance from

the scale, which is to be moved till the base appears in the middle of

the field of view; then bring the needle point g, Fig. 8, by turning the

screw L, to touch one of the lines c a exactly at the point answering to

20 on the sectoral scale. The index a of the micrometer, Fig. 8, is to

be set to the first division, and that on the dial plate to 20, which is

both the beginning and end of its divisions; we are then prepared to

find the magnifying power of every magnifier in the compound microscope

which we are using.

EXAMPLE. Every thing being prepared agreeable to the foregoing

directions, suppose you are desirous of ascertaining the magnifying

power of the lens marked No. 4; turn the micrometer screw, until the

point of the needle has passed over the magnified image of the tenth

part of one inch; then the division, where the two indices remain, will

shew how many revolutions, and parts of a revolution, the screw has

made, while the needle point traversed the magnified image of the

one-tenth of an inch; suppose the result to be twenty-six revolutions of

the screw, and fourteen parts of another revolution, this is equal to 26

multiplied by 20, added to 14; that is, 534 thousandth parts of an

inch.

The twenty-six divisions found on the strait scale of the micrometer,

while the point of the needle passed over the magnified image of

one-tenth part of an inch, were multiplied by 20, because the circular

plate C D, Fig. 8, is divided into twenty equal parts; this produced

520; then adding the fourteen parts of the next revolution, we obtain

534 thousandth parts of an inch, or 5-tenths and 34-hundredth parts of

another tenth, which is the measure of the magnified image of 1-tenth of

an inch, at the aperture of the eye glasses, or at their foci. Now if we

suppose the focus of the two eye-glasses to be one inch, the double

thereof is two inches; or if we reckon in the thousandth part of an

inch, we have two thousand parts for the distance of the eye from the

needle point of the micrometer. Again, if we take the distance of the

image from the object at the stage at six inches, or six thousandths,

and add thereto two thousand, double the distance of the focus of the

eye glass, we shall have eight thousand parts of an inch for the

distance of the eye from the object; and as from the proposition, page

51, we gather that the glasses double the image, we must double the

number 534 found upon the micrometer, which then makes 1068: then, by

the following analogy, we shall obtain the number of times the

microscope magnifies the diameter of the object; say, as 240, the

distance of the eye from the image of the object, is to 800, the

distance of the eye from the object, so is 1068, double the measure

found on the micrometer, to 3563, or the number of times the microscope

magnifies the diameter of the object. By working in this manner, the

magnifying power of each lens used with the compound microscope may be

easily found, though the result will be different in different compound

microscopes, varying, according to the combination of the lenses, their

distance from the object, and one another, &c.

Having discovered the magnifying power of the microscope, with the

different object lenses that are used therewith, our next subject is to

find out the real size of the objects themselves, and their different

parts; this is easily effected, by finding how many revolutions of the

micrometer-screw answer to a known measure on the sectoral scale, or

other object placed on the stage; from the number thus found, a table

should be constructed, expressing the value of the different revolutions

of the micrometer with that object lens, by which the primary number was

obtained. Similar tables must be constructed for each object lens. By a

set of tables of this kind, the observer may readily find the measure of

any object he is examining; for he has only to make the needle point

traverse over this object, and observe the number of revolutions the

screw has made in its passage, and then look into his table for the real

measure which corresponds to this number of revolutions, which is the

measure required.

ACCOUNT OF GLASS, PEARL, &c. MICROMETERS, BY THE EDITOR.

Having seen some glass, &c. micrometers with exquisite fine divisions,

for the purposes of applying to microscopes and telescopes; and in

accuracy, being equivalent to the micrometer just described by our

author, I judge, some account of their application and uses here will be

very acceptable to the curious and inquisitive reader. A particular

description of these as made by the ingenious Mr. Coventry, has been

already given in the Encyclopædia Britannica, Vol. XI. p. 708.

The singular dexterity which Mr. Coventry and others now possess, of

cutting by an engine fine parallel lines upon glass, pearl, ivory, and

brass, at such minute distances as, by means of a microscope, are proved

to be from the 100th to the 5000dth part of an inch, render this sort of

micrometer the easiest and most accurate means of obtaining the exact

natural size of the object to be magnified, and how many times that

object is magnified. Mr. B. Martin, and other opticians, many years ago

applied divided slips of glass, ivory, and horn to the body, in the

focus of the eye glass of microscopes; but the thickness of the whole

medium of the glass was found to diminish the distinct view of the

object: ivory and horn, from their variable texture, were found to

expand and contract too readily to be commodious. It is therefore to Mr.

Cavallo that we are indebted for the happy thought of adapting slips of

divided pearl to telescopes, to ascertain their power, &c. which

substance the opticians now find to be the best for microscopical

micrometers. It possesses a sufficient degree of transparency, when made

about the thickness of writing paper; is a steady substance; admits very

easily of the finest graduations, and is generally made in breadth about

the 20th part of an inch.

Fig. 9. Plate II. A, is a representation of this scale, with divisions

of the 200ths of an inch, every fifth and tenth division being left

longer than the others, which only go to about the middle. If the eye

glass of the microscope or telescope, to which this micrometer is to be

applied, magnify very much, its divisions may be proportionably minute.

To measure by this micrometer the size of an object in a single

microscope, nothing more is required than to lay it on the micrometer,

and adjust it to the focus of the magnifier, noticing how many

divisions it covers or coincides with. Supposing the parallel lines to

be the 1000dths of an inch, and the object covers two divisions, its

real size is the 500th of an inch; if five, 200th of an inch, &c.

To find how much the object is magnified, is not so easily done by the

single, as by the compound microscope, as has been before explained. The

following simple method has been adopted by Mr. Coventry, and which may

be considered tolerably accurate. Adjust a micrometer under the

microscope, suppose 100th of an inch of divisions, with a small object

on it, if square, the better; notice how many divisions one side of the

object covers, suppose ten; then cut a piece of white paper something

larger than the magnified appearance of the object; fix one eye on the

object through the microscope, and the other at the same time on the

paper, lowering it down till the object and the paper appear level and

distinct: then cut the paper till it appear exactly the size of the

magnified object; the paper being then measured, suppose an inch square:

now, as the object under the magnifier, which appeared to be one inch

square, was in reality only ten hundredths, or the tenth of an inch, the

experiment proves that it is magnified ten times in length, one hundred

times in superficies, and one thousand times in cube, which is the

magnifying power of the glass; and in the same manner a table may be

made of the power of all the other glasses.

In using the compound microscope, the real size of the object is found

by the same method as in the single; but to demonstrate the magnifying

power to greater certainty, adopt the following method. Lay a two-feet

rule on the stage, and a micrometer level with its surface, (an inch

suppose, divided into 100 parts:) with one eye see how many of those

parts are contained in the field of the microscope, suppose 50; and with

the other, at the same time, look for the circle of light in the field

of the microscope, which with a little practice will soon appear

distinct; mark how much of the rule, from the center of the stage, is

intersected by the circle of light, which will be half the diameter of

the field. Suppose eight inches; consequently the whole diameter will be

sixteen. Now, as the real size of the field by the micrometers appeared

to be only 50 hundredths, or half an inch, and as half an inch is only

one 32d part of 16 inches, it shews the magnifying power to be 32 times

in length, 1024 superficies, and 32768 in cube or bulk. For accuracy, as

well as for comparative observations, the rule should always be a

certain distance from the eye; eight inches in general is a proper

distance.

Another way, and the most easy for finding the magnifying power of

compound microscopes, is by using two micrometers of the same divisions;

one adjusted under the magnifier, the other fixed in the body of the

microscope in the focus of the eye glass. Notice how many divisions of

the micrometer in the body are seen in one division of the micrometer

under the magnifier, which again must be multiplied by the power of the

eye glass. Example: Ten divisions of the micrometer in the body are

contained in one division under the magnifier; so far the power is

increased ten times: now, if the eye glass be one inch focus, such glass

will of itself magnify about eight times in length, which, with the ten

times magnified before, will be eight times ten, or 80 times in length,

6400 superficies, and 512000 cube.

Fig. 10. Plate II. A, represents the field of view of the compound

microscope, with the pearl micrometer, as applied to the aperture in the

body, called the eye stop; and a magnified micrometer that is laid on

the stage, shewing that one of the latter contains ten of the former.

A set of ivory and glass micrometers, about six in number, besides one

or two pearl ones for the eye stops, are generally packed up with the

best sort of microscopes made by Messrs. W. and S. Jones, Opticians,

Holborn. They are divided into lines and squares, from the 100th to the

1000dth parts of an inch; and, besides measuring the magnifying powers

of microscopes, are generally found useful in measuring the diameters,

proportions, &c. of opake and transparent objects, even of the minutest

kind. The smallest divisions of the glass micrometer to be useful, are

those divided into the 4000dth part of an inch; and as these may be

crossed again with an equal number of lines in the same manner, they

form squares of the SIXTEEN MILLIONTH part of an inch surface, each

square of which appearing under the microscope true and distinct. And,

even small as this is, animalculæ are found so minute as to be contained

in one of these squares!

Glass micrometers with squares, applied to the solar microscope, divide

the objects into squares on the screen in such a manner, as to render a

drawing from it very easy; and are employed with great advantage in the

lucernal microscope.

The micrometers are constructed with moveable frames or tubes, so as to

be either applied or taken away in the readiest manner.

For the uses of the pearl micrometer as applied to the telescope, see

Mr. Cavallo’s pamphlet descriptive of its use, 8vo. 1793, and the

Philosophical Transactions for 1791.

CHAP. III.

Essays on the Microscope Containing a Practical Description of the Most Improved Microscopes, a General History of Insects, etc., etc. · 第 5 / 56 段