CHAPTER VI.

_Invention of the telescope—Fracastoro—Porta—Reflecting

telescope—Roger Bacon—Digges—De

Dominis—Jansen—Lipperhey—Galileo constructs

telescopes—Microscopes—Re-elected Professor at Padua for life._

THE year 1609 was signalized by Galileo's discovery of the telescope,

which, in the minds of many, is the principal, if not the sole invention

associated with his name. It cannot be denied that his fame, as the

founder of the school of experimental philosophy, has been in an

unmerited degree cast into the shade by the splendour of his

astronomical discoveries; yet Lagrange[32] surely errs in the opposite

extreme, when he almost denies that these form any real or solid part of

the glory of this great man; and Montucla[33] omits an important

ingredient in his merit, when he (in other respects very justly)

remarks, that it required far less genius to point a telescope towards

the heavens than to trace the unheeded, because daily recurring,

phenomena of motion up to its simple and primary laws. We are to

remember that in the days of Galileo a telescope could scarcely be

pointed to the heavens with impunity, and that a courageous mind was

required to contradict, and a strong one to bear down, a party, who,

when invited to look on any object in the heavens which Aristotle had

never suspected, immediately refused all credit to those senses, to

which, on other occasions, they so confidently appealed. It surely is a

real and solid part of Galileo's glory that he consumed his life in

laborious and indefatigable observations, and that he persevered in

announcing his discoveries undisgusted by the invectives, and undismayed

by the persecutions, to which they subjected him. Plagiarist! liar!

impostor! heretic! were among the expressions of malignant hatred

lavished upon him, and although he also was not without some violent and

foul-mouthed partisans, yet it must be told to his credit that he

himself seldom condescended to notice these torrents of abuse, otherwise

than by good-humoured retorts, and by prosecuting his observations with

renewed assiduity and zeal.

The use of single lenses in aid of the sight had been long known.

Spectacles were in common use at the beginning of the fourteenth

century, and there are several hints, more or less obscure, in many

early writers, of the effects which might be expected from a combination

of glasses; but it does not appear with certainty that any of these

authors had attempted to reduce their ideas to practice. After the

discovery of the telescope, almost every country endeavoured to find in

the writings of its early philosophers traces of the knowledge of such

an instrument, but in general with success very inadequate to the zeal

of their national prepossessions. There are two authors especially to

whom the attention of Kepler and others was turned, immediately upon the

promulgation of the discovery, as containing the germ of it in their

works. These are Baptista Porta, and Gerolamo Fracastoro. We have

already had occasion to quote the Homocentrica of Fracastoro, who died

in 1553; the following expressions, though they seem to refer to actual

experiment, yet fall short of the meaning with which it has been

attempted to invest them. After explaining and commenting on some

phenomena of refraction through different media, to which he was led by

the necessity of reconciling his theory with the variable magnitudes of

the planets, he goes on to say—"For which reason, those things which

are seen at the bottom of water, appear greater than those which are at

the top; and if any one look through two eyeglasses, _one placed upon

the other_, he will see every thing much larger and nearer."[34] It

should seem that this passage (as Delambre has already remarked) rather

refers to the close application of one glass upon another, and it may

fairly be doubted whether anything analogous to the composition of the

telescope was in the writer's thoughts. Baptista Porta writes on the

same subject more fully;—"Concave lenses show distant objects most

clearly, convex those which are nearer, whence they may be used to

assist the sight. With a concave glass distant objects will be seen,

small, but distinct; with a convex one those near at hand, larger, but

confused; _if you know rightly how to combine one of each sort, you

will see both far and near objects larger and clearer_."[35] These words

show, if Porta really was then unacquainted with the telescope, how

close it is possible to pass by an invention without lighting on it, for

of precisely such a combination of a convex and concave lens, fitted to

the ends of an organ pipe by way of tube, did the whole of Galileo's

telescope consist. If Porta had stopped here he might more securely have

enjoyed the reputation of the invention, but he then professes to

describe the construction of his instrument, which has no relation

whatever to his previous remarks. "I shall now endeavour to show in what

manner we may contrive to recognize our friends at the distance of

several miles, and how those of weak sight may read the most minute

letters from a distance. It is an invention of great utility, and

grounded on optical principles, nor is it at all difficult of execution;

but it must be so divulged as not to be understood by the vulgar, and

yet be clear to the sharpsighted." The description which follows seems

far enough removed from the apprehended danger of being too clear, and

indeed every writer who has hitherto quoted it has merely given the

passage in its original Latin, apparently despairing of an intelligible

translation. With some alterations in the punctuation, which appear

necessary to bring it into any grammatical construction,[36] it may be

supposed to bear something like the following meaning:—"Let a view be

contrived in the centre of a mirror, where it is most effective. All the

solar rays are exceedingly dispersed, and do not in the least come

together (in the true centre); but there is a concourse of all the rays

in the central part of the said mirror, half way towards the other

centre, where the cross diameters meet. This view is contrived in the

following manner. A concave cylindrical mirror placed directly in front,

but with its axis inclined, must be adapted to that focus: and let

obtuse angled or right angled triangles be cut out with two cross lines

on each side drawn from the centre, and a glass (_specillum_) will be

completed fit for the purposes we mentioned." If it were not for the

word "_specillum_," which, in the passage immediately preceding this,

Porta[37] contrasts with "_speculum_," and which he afterwards explains

to mean a glass lens, it would be very clear that the foregoing passage

(supposing it to have any meaning) must be referred to a reflecting

telescope, and it is a little singular that while this obscure passage

has attracted universal attention, no one, so far as we are aware, has

taken any notice of the following unequivocal description of the

principal part of Newton's construction of the same instrument. It is in

the 5th chapter of the 17th book, where Porta explains by what device

exceedingly minute letters may be read without difficulty. "Place a

concave mirror so that the back of it may lie against your breast;

opposite to it, and within the burning point, place the writing; put a

plane mirror behind it, that may be under your eyes. Then the images of

the letters which are in the concave mirror, and which the concave has

magnified, will be reflected in the plane mirror, so that you may read

without difficulty."

We have not been able to meet with the Italian translation of Porta's

Natural Magic, which was published in 1611, under his own

superintendence; but the English translator of 1658 would probably have

known if any intelligible interpretation were there given of the

mysterious passage above quoted, and his translation is so devoid of

meaning as strongly to militate against this idea. Porta, indeed,

claimed the invention as his own, and is believed to have hastened his

death, (which happened in 1615, he being then 80 years old,) by the

fatigue of composing a Treatise on the Telescope, in which he had

promised to exhaust the subject. We do not know whether this is the same

work which was published after his death by Stelliola,[38] but which

contains no allusion to Porta's claim, and possibly Stelliola may have

thought it most for his friend's reputation to suppress it. Schott[39]

says, a friend of his had seen Porta's book in manuscript, and that it

did at that time contain the assertion of Porta's title to the

invention. After all it is not improbable that he may have derived his

notions of magnifying distant objects from our celebrated countryman

Roger Bacon, who died about the year 1300. He has been supposed, not

without good grounds, to have been one of the first who recognised the

use of single lenses in producing distinct vision, and he has some

expressions with respect to their combination which promise effects

analogous to those held out by Porta. In "The Admirable Force of Art and

Nature," he says, "Physical figurations are far more strange, for in

such manner may we frame perspects and looking-glasses that one thing

shall appear to be many, as one man shall seeme a whole armie; and

divers sunnes and moones, yea, as many as we please, shall appeare at

one time, &c. And so may the perspects be framed, that things most farre

off may seeme most nigh unto us, and clean contrarie, soe that we may

reade very small letters an incredible distance from us, and behold

things how little soever they be, and make stars to appeare wheresoever

we will, &c. And, besides all these, we may so frame perspects that any

man entering into a house he shall indeed see gold, and silver, and

precious stones, and what else he will, but when he maketh haste to the

place he shall find just nothing." It seems plain, that the author is

here speaking solely of mirrors, and we must not too hastily draw the

conclusion, because in the first and last of these assertions he is, to

a certain extent, borne out by facts, that he therefore was in

possession of a method of accomplishing the middle problem also. In the

previous chapter, he gives a long list of notable things, (much in the

style of the Marquis of Worcester's Century of Inventions) which if we

can really persuade ourselves that he was capable of accomplishing, we

must allow the present age to be still immeasurably inferior to him in

science.

Thomas Digges, in the preface to his Pantometria, (published in 1591)

declares, "My father, by his continuall painfull practises, assisted

with demonstrations mathematicall, was able, and sundry times hath by

proportionall glasses, duely situate in convenient angles, not only

discouered things farre off, read letters, numbered peeces of money,

with the verye coyne and superscription thereof, cast by some of his

freends of purpose, upon downes in open fields; but also, seuen miles

off, declared what hath beene doone at that instant in priuate places.

He hath also sundrie times, by the sunne beames, fired powder and

dischargde ordnance halfe a mile and more distante; which things I am

the boulder to report, for that there are yet living diverse (of these

his dooings) occulati testes, (eye witnesses) and many other matters

farre more strange and rare, which I omit as impertinent to this place."

We find another pretender to the honour of the discovery of the

telescope in the celebrated Antonio de Dominis, Archbishop of Spalatro,

famous in the annals of optics for being one of the first to explain the

theory of the rainbow. Montucla, following P. Boscovich, has scarcely

done justice to De Dominis, whom he treats as a mere pretender and

ignorant person. The indisposition of Boscovich towards him is

sufficiently accounted for by the circumstance of his being a Catholic

prelate who had embraced the cause of Protestantism. His nominal

reconciliation with the Church of Rome would probably not have saved him

from the stake, had not a natural death released him when imprisoned on

that account at Rome. Judgment was pronounced upon him notwithstanding,

and his body and books were publicly burnt in the Campo de Fiori, in

1624. His treatise, De Radiis, (which is very rarely to be met with) was

published by Bartolo after the acknowledged invention of the telescope

by Galileo; but Bartolo tells us, in the preface, that the manuscript

was communicated to him from a collection of papers written 20 years

before, on his inquiring the Archbishop's opinion with respect to the

newly discovered instrument, and that he got leave to publish it, "with

the addition of one or two chapters." The treatise contains a complete

description of a telescope, which, however, is professed merely to be an

improvement on spectacles, and if the author's intention had been to

interpolate an afterwritten account, in order to secure to himself the

undeserved honour of the invention, it seems improbable that he would

have suffered an acknowledgment of additions, previous to publication,

to be inserted in the preface. Besides, the whole tone of the work is

that of a candid and truth-seeking philosopher, very far indeed removed

from being, as Montucla calls him, conspicuous for ignorance even among

the ignorant men of his age. He gives a drawing of a convex and concave

lens, and traces the passage of the rays through them; to which he

subjoins, that he has not satisfied himself with any determination of

the precise distance to which the glasses should be separated, according

to their convexity and concavity, but recommends the proper distance to

be found by actual experiment, and tells us, that the effect of the

instrument will be to prevent the confusion arising from the

interference of the direct and refracted rays, and to magnify the object

by increasing the visible angle under which it is viewed. These, among

the many claimants, are certainly the authors who approached the most

nearly to the discovery: and the reader may judge, from the passages

cited, whether the knowledge of the telescope can with probability be

referred to a period earlier than the commencement of the 17th century.

At all events, we can find no earlier trace of its being applied to any

practical use; the knowledge, if it existed, remained speculative and

barren.

In 1609, Galileo, then being on a visit to a friend at Venice, heard a

rumour of the recent invention, by a Dutch spectacle-maker, of an

instrument which was said to represent distant objects nearer than they

usually appeared. According to his own account, this general rumour,

which was confirmed to him by letters from Paris, was all that he

learned on the subject; and returning to Padua, he immediately applied

himself to consider the means by which such an effect could be produced.

Fuccarius, in an abusive letter which he wrote on the subject, asserts

that one of the Dutch telescopes had been at that time actually brought

to Venice, and that he (Fuccarius) had seen it; which, even if true, is

perfectly consistent with Galileo's statement; and in fact the question,

whether or not Galileo saw the original instrument, becomes important

only from his expressly asserting the contrary, and professing to give

the train of reasoning by which he discovered its principle; so that any

insinuation that he had actually seen the Dutch glass, becomes a direct

impeachment of his veracity. It is certain, from the following extract

of a letter from Lorenzo Pignoria to Paolo Gualdo, that one at least of

the Dutch glasses had been sent to Italy. It is dated Padua, 31st

August, 1609.[40] "We have no news, except the return of His Serene

Highness, and the re-election of the lecturers, among whom Sign. Galileo

has contrived to get 1000 florins for life; and it is said to be on

account of an eyeglass, _like the one which was sent from Flanders to

Cardinal Borghese_. We have seen some here, and truly they succeed

well."

It is allowed by every one that the Dutchman, or rather Zealander, made

his discovery by mere accident, which greatly derogates from any honour

attached to it; but even this diminished degree of credit has been

fiercely disputed. According to one account, which appears consistent

and probable, it had been made for sometime before its importance was in

the slightest degree understood or appreciated, but was set up in the

optician's shop as a curious philosophical toy, showing a large and

inverted image of a weathercock, towards which it was directed. The

Marquis Spinola, chancing to see it, was struck with the phenomenon,

purchased the instrument, and presented it either to the Archduke Albert

of Austria, or to Prince Maurice of Nassau, whose name appears in every

version of the story, and who first entertained the idea of employing it

in military reconnoissances.

Zacharias Jansen, and Henry Lipperhey, two spectacle-makers, living

close to each other, near the church of Middleburg, have both had

strenuous supporters of their title to the invention. A third pretender

appeared afterwards in the person of James Metius of Alkmaer, who is

mentioned by Huyghens and Des Cartes, but his claims rest upon no

authority whatever comparable to that which supports the other two.

About half a century afterwards, Borelli was at the pains to collect and

publish a number of letters and depositions which he procured, as well

on one side as on the other.[41] It seems that the truth lies between

them, and that one, probably Jansen, was the inventor of the

_microscope_, which application of the principle was unquestionably of

an earlier date, perhaps as far back as 1590. Jansen gave one of his

microscopes to the Archduke, who gave it to Cornelius Drebbel, a

salaried mathematician at the court of our James the first, where

William Borelli (not the author above mentioned) saw it many years

afterwards, when ambassador from the United Provinces to England, and

got from Drebbel this account of the quarter whence it came. Lipperhey

afterwards, in 1609, accidentally hit upon the _telescope_, and on the

fame of this discovery it would not be difficult for Jansen, already in

possession of an instrument so much resembling it, to perceive the

slight difference between them, and to construct a telescope

independently of Lipperhey, so that each, with some show of reason,

might claim the priority of the invention. A notion of this kind

reconciles the testimony of many conflicting witnesses on the subject,

some of whom do not seem to distinguish very accurately whether the

telescope or microscope is the instrument to which their evidence

refers. Borelli arrives at the conclusion, that Jansen was the inventor;

but not satisfied with this, he endeavours, with a glaring partiality

which makes his former determination suspicious, to secure for him and

his son the more solid reputation of having anticipated Galileo in the

useful employment of the invention. He has however inserted in his

collections a letter from John the son of Zacharias, in which John,

omitting all mention of his father, speaks of his own observation of the

satellites of Jupiter, evidently seeking to insinuate that they were

earlier than Galileo's; and in this sense the letter has since been

quoted,[42] although it appears from John's own deposition, preserved in

the same collection, that at the time of their discovery he could not

have been more than six years old. An oversight of this sort throws

doubt on the whole of the pretended observations, and indeed the letter

has much the air of being the production of a person imperfectly

informed on the subject on which he writes, and probably was compiled to

suit Borelli's purposes, which were to make Galileo's share in the

invention appear as small as possible.

Galileo himself gives a very intelligible account of the process of

reasoning, by which he detected the secret.—"I argued in the following

manner. The contrivance consists either of one glass or of more—one is

not sufficient, since it must be either convex, concave, or plane; the

last does not produce any sensible alteration in objects, the concave

diminishes them: it is true that the convex magnifies, but it renders

them confused and indistinct; consequently, one glass is insufficient to

produce the desired effect. Proceeding to consider two glasses, and

bearing in mind that the plane glass causes no change, I determined that

the instrument could not consist of the combination of a plane glass

with either of the other two. I therefore applied myself to make

experiments on combinations of the two other kinds, and thus obtained

that of which I was in search." It has been urged against Galileo that,

if he really invented the telescope on theoretical principles, the same

theory ought at once to have conducted him to a more perfect instrument

than that which he at first constructed;[43] but it is plain, from this

statement, that he does not profess to have theorized beyond the

determination of the species of glass which he should employ in his

experiments, and the rest of his operations he avows to have been purely

empirical. Besides, we must take into account the difficulty of grinding

the glasses, particularly when fit tools were yet to be made, and

something must be attributed to Galileo's eagerness to bring his results

to the test of actual experiment, without waiting for that improvement

which a longer delay might and did suggest. Galileo's language bears a

resemblance to the first passage which we quoted from Baptista Porta,

sufficiently close to make it not improbable that he might be assisted

in his inquiries by some recollection of it, and the same passage seems,

in like manner, to have recurred to the mind of Kepler, as soon as he

heard of the invention. Galileo's telescope consisted of a plano-convex

and plano-concave lens, the latter nearest the eye, distant from each

other by the difference of their focal lengths, being, in principle,

exactly the same with the modern opera-glass. He seems to have thought

that the Dutch glass was the same, but this could not be the case, if

the above quoted particular of the _inverted_ weathercock, which belongs

to most traditions of the story, be correct; because it is the

peculiarity of this kind of telescope not to invert objects, and we

should be thus furnished with a demonstrative proof of the falsehood of

Fuccarius's insinuation: in that case the Dutch glass must have been

similar to what was afterwards called the astronomical telescope,

consisting of two convex glasses distant from each other by the sum of

their focal lengths. This supposition is not controverted by the fact,

that this sort of telescope was never employed by astronomers till long

afterwards; for the fame of Galileo's observations, and the superior

excellence of the instruments constructed under his superintendence,

induced every one in the first instance to imitate his constructions as

closely as possible. The astronomical telescope was however eventually

found to possess superior advantages over that which Galileo imagined,

and it is on this latter principle that all modern refracting telescopes

are constructed; the inversion being counteracted in those which are

intended for terrestrial observations, by the introduction of a second

pair of similar glasses, which restore the inverted image to its

original position. For further details on the improvements which have

been subsequently introduced, and on the reflecting telescope, which was

not brought into use till the latter part of the century, the reader is

referred to the Treatise on OPTICAL INSTRUMENTS.

Galileo, about the same time, constructed microscopes on the same

principle, for we find that, in 1612, he presented one to Sigismund,

King of Poland; but his attention being principally devoted to the

employment and perfection of his telescope, the microscope remained a

long time imperfect in his hands: twelve years later, in 1624, he wrote

to P. Federigo Cesi, that he had delayed to send the microscope, the use

of which he there describes, because he had only just brought it to

perfection, having experienced some difficulty in working the glasses.

Schott tells an amusing story, in his "Magic of Nature," of a Bavarian

philosopher, who, travelling in the Tyrol with one of the newly invented

microscopes about him, was taken ill on the road and died. The

authorities of the village took possession of his baggage, and were

proceeding to perform the last duties to his body, when, on examining

the little glass instrument in his pocket, which chanced to contain a

flea, they were struck with the greatest astonishment and terror, and

the poor Bavarian, condemned by acclamation as a sorcerer who was in the

habit of using a portable familiar, was declared unworthy of Christian

burial. Fortunately for his character, some bold sceptic ventured to

open the instrument, and discovered the true nature of the imprisoned

fiend.

As soon as Galileo's first telescope was completed, he returned with it

to Venice, and the extraordinary sensation which it excited tends also

strongly to refute Fuccarius's assertion that the Dutch glass was

already known there. During more than a month Galileo's whole time was

employed in exhibiting his instrument to the principal inhabitants of

Venice, who thronged to his house to satisfy themselves of the truth of

the wonderful stories in circulation; and at the end of that time the

Doge, Leonardo Donati, caused it to be intimated to him that such a

present would not be deemed unacceptable by the senate. Galileo took the

hint, and his complaisance was rewarded by a mandate confirming him for

life in his professorship at Padua, at the same time doubling his yearly

salary, which was thus made to amount to 1000 florins.

It was long before the phrenzy of public curiosity abated. Sirturi

describes a ludicrous violence which was done to himself, when, with the

first telescope which he had succeeded in making, he went up into the

tower of St. Mark, at Venice, in the vain hope of being there entirely

unmolested. Unluckily he was seen by some idlers in the street: a crowd

soon collected round him, who insisted on taking possession of his

instrument, and, handing it one to the other, detained him there for

several hours till their curiosity was satiated, when he was allowed to

return home. Hearing them also inquire eagerly at what inn he lodged, he

thought it better to quit Venice early the next morning, and prosecute

his observations in a less inquisitive neighbourhood.[44] Instruments of

an inferior description were soon manufactured, and vended every where

as philosophical playthings, much in the way in which, in our own time,

the kaleidoscope spread over Europe as fast as travellers could carry

them. But the fabrication of a better sort was long confined, almost

solely, to Galileo and those whom he immediately instructed; and so late

as the year 1637, we find Gaertner, or as he chose to call himself,

Hortensius, assuring Galileo that none could be met with in Holland

sufficiently good to show Jupiter's disc well defined; and in 1634

Gassendi begs for a telescope from Galileo, informing him that he was

unable to procure a good one either in Venice, Paris, or Amsterdam.

The instrument, on its first invention, was generally known by the names

of Galileo's tube, the perspective, the double eye-glass: the names of

telescope and microscope were suggested by Demisiano, as we are told by

Lagalla in his treatise on the Moon.[45]

FOOTNOTES:

[32] Mecanique Analytique.

[33] Histoire des Mathématiques, tom. ii.

[34] "Per duo specilla ocularia si quis perspiciat, altero alteri

superposito, majora multo et propinquiora videbit omnia."—Fracast.

Homocentrica, § 2, c. 8.

[35] Si utrumque recte componere noveris, et longinqua et proxima majora

et clara videbis.—Mag. Nat. lib. 17.

[36] The passage in the original, which is printed alike in the editions

of 1598, 1607, 1619, and 1650, is as follows: Visus constituatur centro

valentissimus speculi, ubi fiet, et valentissimè universales solares

radii disperguntur, et coeunt minimè, sed centro prædicti speculi in

illius medio, ubi diametri transversales, omnium ibi concursus.

Constituitur hoc modo speculum concavum columnare æquidistantibus

lateribus, sed lateri uno obliquo sectionibus illis accomodetur,

trianguli vero obtusianguli, vel orthogonii secentur, hinc inde duobus

transversalibus lineis, ex-centro eductis. Et confectum erit specillum,

ad id, quod diximus utile.

[37] Diximus de Ptolemæi _speculo_, sive _specillo_ potius, quo per

sexcentena millia pervenientes naves conspiciebat.

[38] Il Telescopio, 1627.

[39] Magia Naturæ et Artis Herbipoli, 1657.

[40] Lettère d'Uomini illustri. Venezia, 1744.

[41] Borelli. De vero Telescopii inventore, 1655.

[42] Encyclopædia Britannica. Art. TELESCOPE.

[43] Ibid.

[44] Telescopium, Venetiis, 1619.

[45] De phænomenis in orbe Lunæ. Venetiis, 1612.

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