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Cavalieri in his "New method of Guaging," which is the earliest work with which we are acquainted, where principles of this sort are employed.*

CHAPTER VI.

Invention of the telescope-Fracastoro
-Porta - Reflecting telescope-Ro -
ger Bacon-Digges-De Dominis-
Galileo con-
Jansen-Lipperhey·
structs 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 prin-
cipal, 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 astro-
nomical discoveries; yet Lagranget
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 Montuclat omits an im -
portant 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 re-
curring, 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 con-
tradict, and a strong one to bear down,
a party, who, when invited to look on
any object in the heavens which Aris-
totle had never suspected, immediately
refused all credit to those senses, to
which, on other occasions, they so confi-
It surely is a real
dently appealed.
and solid part of Galileo's glory that he
consumed his life in laborious and inde-
fatigable observations, and that he per-
severed in announcing his discoveries
undisgusted by the invectives, and un-
dismayed by the persecutions, to which
they subjected him. Plagiarist ! liar !
impostor! heretic! were among the ex-
pressions 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-

* Nova Stereometria Doliorum-Lincii, 1615.
+ Mecanique Analytique.

7 Histoire des Mathématiques, tom. ii.

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 prac-
After the discovery of the tele-
tice.
scope, 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 inadeqnate to the zeal of
There
their national prepossessions.
are two authors especially to whom the
attention of Kepler and others was
turned, immediately upon the promulga-
tion of the discovery, as containing the
germ of it in their works. These are
Baptista Porta, and Gerolamo Fracas-
toro.

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."* 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 any thing 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

"Per duo specilla ocularia si quis perspiciat, altero alteri superposito, majora multo et propinquiora videbit omnia."-Fracast. Homocentrica, § 2, c. 8.

GALILEO.

know rightly how to combine one of
each sort, you will see both far and near
These
objects larger and clearer."*
words show, if Porta really was then
unacquainted with the telescope, how
close it is possible to pass by an inven-
tion without lighting on it, for of pre-
cisely 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 repu-
tation of the invention, but he then pro-
fesses 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 prin-
ciples, nor is it at all difficult of execu-
tion; but it must be so divulged as not
to be understood by the vulgar, and yet
The
be clear to the sharpsighted."
description which follows seems far
enough removed from the apprehended
danger of being too clear, and in-
deed every writer who has hitherto
quoted it has merely given the passage
in its original Latin, apparently despair-
With
ing of an intelligible translation.
some alterations in the punctuation,
which appear necessary to bring it into
any grammatical construction, 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
A concave cylindrical mirror

manner.

* Si utrumque recte componere noveris, et longin

qua et proxima majora et clara videbis-Mag. Nat.
lib. 17.

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 coeant minimè, sed centro præ-
dicti speculi in illius medio, ubi diametri transver
Constituitur hoc modo
sales, omnium ibi concursus.
speculum concavum columnare æquidistantibus late.
ribus, sed lateri uno obliquo sectionibus illis accomo-
detur, trianguli vero obtusianguli, vel orthogonii
secentur, hinc inde duobus transversalibus lineis, ex
centro eductis. Et confectum erit specillum, ad id,
quod diximus, utile.

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
aglass (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 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 in-
strument. It is in the 5th chapter
of the 17th book, where Porta explains
by what device exceedingly minute let-
ters 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
Then the images of the letters
eyes.
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, 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 says, a friend of his had

* Diximus de Ptolemæi speculo,sive specillo potius, quo per sexcentena millia pervenientes naves conspi+11 Telescopio, 1627. Magia Naturæ et Artis Herbipoli, 1657.

ciobat.

66

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 lookingglasses 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 eise 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

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scription 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 Mon

tucla 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 knowlege, 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.* "We have no news, except the return of His Serene Highness, and the reelection 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. 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

Lettère d'Uomini illustri Venezia, 1744.
Borelli. De vero Telescopii inventore, 1655.

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,* 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

• Encyclopædia Britannica. Art. TELESCOPE.

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; 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 as sisted 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

• Ibid.

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