Yet they had received a shock: as by a breath of fresh salt breeze and a

dash of spray in their faces, they had been awakened out of their

comfortable lethargy. They felt the approach of a new era. Yes, it was a

shock, and they hated the young Galileo for giving it them--hated him

with the sullen hatred of men who fight for a lost and dying cause.

We need scarcely blame these men; at least we need not blame them

overmuch. To say that they acted as they did is to say that they were

human, were narrow-minded, and were the apostles of a lost cause. But

_they_ could not know this; _they_ had no experience of the past to

guide them; the conditions under which they found themselves were novel,

and had to be met for the first time. Conduct which was excusable then

would be unpardonable now, in the light of all this experience to guide

us. Are there any now who practically repeat their error, and resist new

truth? who cling to any old anchorage of dogma, and refuse to rise with

the tide of advancing knowledge? There may be some even now.

Well, the unpopularity of Galileo smouldered for a time, until, by

another noble imprudence, he managed to offend a semiroyal personage,

Giovanni de' Medici, by giving his real opinion, when consulted, about a

machine which De' Medici had invented for cleaning out the harbor of

Leghorn. He said it was as useless as it in fact turned out to be.

Through the influence of the mortified inventor he lost favor at court;

and his enemies took advantage of the fact to render his chair

untenable. He resigned before his three years were up, and retired to

Florence.

His father at this time died, and the family were left in narrow

circumstances. He had a brother and three sisters to provide for. He was

offered a professorship at Padua for six years by the Senate of Venice,

and willingly accepted it. Now began a very successful career. His

introductory address was marked by brilliant eloquence, and his lectures

soon acquired fame. He wrote for his pupils on the laws of motion, on

fortifications, on sun-dials, on mechanics, and on the celestial globe:

some of these papers are now lost, others have been printed during the

present century.

Kepler sent him a copy of his new book, _Mysterium Cosmographicum_, and

Galileo, in thanking him for it, writes him the following letter:

"I count myself happy, in the search after truth, to have so great an

ally as yourself, and one who is so great a friend of the truth itself.

It is really pitiful that there are so few who seek truth, and who do

not pursue a perverse method of philosophizing. But this is not the

place to mourn over the miseries of our times, but to congratulate you

on your splendid discoveries in confirmation of truth. I shall read your

book to the end, sure of finding much that is excellent in it. I shall

do so with the more pleasure, because _I have been for many years an

adherent of the Copernican system_, and it explains to me the causes of

many of the appearances of nature which are quite unintelligible on the

commonly accepted hypothesis. _I have collected many arguments for the

purpose of refuting the latter_; but I do not venture to bring them to

the light of publicity, for fear of sharing the fate of our master,

Copernicus, who, although he has earned immortal fame with some, yet

with very many (so great is the number of fools) has become an object of

ridicule and scorn. I should certainly venture to publish my

speculations if there were more people like you. But this not being the

case, I refrain from such an undertaking."

Kepler urged him to publish his arguments in favor of the Copernican

theory, but he hesitated for the present, knowing that his declaration

would be received with ridicule and opposition, and thinking it wiser to

get rather more firmly seated in his chair before encountering the storm

of controversy. The six years passed away, and the Venetian Senate,

anxious not to lose so bright an ornament, renewed his appointment for

another six years at a largely increased salary.

Soon after this appeared a new star--the _stella nova_ of 1604--not the

one Tycho had seen--that was in 1572--but the same that Kepler was so

much interested in. Galileo gave a course of three lectures upon it to a

great audience. At the first the theatre was overcrowded, so he had to

adjourn to a hall holding one thousand persons. At the next he had to

lecture in the open air. He took occasion to rebuke his hearers for

thronging to hear about an ephemeral novelty, while for the much more

wonderful and important truths about the permanent stars and facts of

nature they had but deaf ears.

But the main point he brought out concerning the new star was that it

upset the received Aristotelian doctrine of the immutability of the

heavens. According to that doctrine the heavens were unchangeable,

perfect, subject neither to growth nor to decay. Here was a body, not a

meteor but a real distant star, which had not been visible and which

would shortly fade away again, but which meanwhile was brighter than

Jupiter.

The staff of petrified professorial wisdom were annoyed at the

appearance of the star, still more at Galileo's calling public attention

to it; and controversy began at Padua. However, he accepted it, and now

boldly threw down the gauntlet in favor of the Copernican theory,

utterly repudiating the old Ptolemaic system, which up to that time he

had taught in the schools according to established custom.

The earth no longer the only world to which all else in the firmament

were obsequious attendants, but a mere insignificant speck among the

host of heaven! Man no longer the centre and cynosure of creation, but,

as it were, an insect crawling on the surface of this little speck! All

this not set down in crabbed Latin in dry folios for a few learned

monks, as in Copernicus' time, but promulgated and argued in rich

Italian, illustrated by analogy, by experiment, and with cultured wit;

taught not to a few scholars here and there in musty libraries, but

proclaimed in the vernacular to the whole populace with all the energy

and enthusiasm of a recent convert and a master of language! Had a

bombshell been exploded among the fossilized professors it had been less

disturbing.

But there was worse in store for them. A Dutch optician, Hans Lippershey

by name, of Middleburg, had in his shop a curious toy, rigged up, it is

said, by an apprentice, and made out of a couple of spectacle lenses,

whereby, if one looked through it, the weather-cock of a neighboring

church spire was seen nearer and upside down. The tale goes that the

Marquis Spinola, happening to call at the shop, was struck with the toy

and bought it. He showed it to Prince Maurice of Nassau, who thought of

using it for military reconnoitring. All this is trivial. What is

important is that some faint and inaccurate echo of this news found its

way to Padua and into the ears of Galileo.

The seed fell on good soil. All that night he sat up and pondered. He

knew about lenses and magnifying-glasses. He had read Kepler's theory of

the eye, and had himself lectured on optics. Could he not hit on the

device and make an instrument capable of bringing the heavenly bodies

nearer? Who knew what marvels he might not so perceive! By morning he

had some schemes ready to try, and one of them was successful.

Singularly enough it was not the same plan as the Dutch optician's: it

was another mode of achieving the same end. He took an old small

organ-pipe, jammed a suitably chosen spectacle glass into either end,

one convex, the other concave, and, behold! he had the half of a

wretchedly bad opera-glass capable of magnifying three times. It was

better than the Dutchman's, however: it did not invert.

Such a thing as Galileo made may now be bought at a toy-shop for I

suppose half a crown, and yet what a potentiality lay in that "glazed

optic tube," as Milton called it. Away he went with it to Venice and

showed it to the Seigniory, to their great astonishment. "Many noblemen

and senators," says Galileo, "though of advanced age, mounted to the

top of one of the highest towers to watch the ships, which were visible

through my glass two hours before they were seen entering the harbor,

for it makes a thing fifty miles off as near and clear as if it were

only five." Among the people, too, the instrument excited the greatest

astonishment and interest, so that he was nearly mobbed. The Senate

hinted to him that a present of the instrument would not be

unacceptable, so Galileo took the hint and made another for them. They

immediately doubled his salary at Padua, making it one thousand florins,

and confirmed him in the enjoyment of it for life.

He now eagerly began the construction of a larger and better instrument.

Grinding the lenses with his own hands with consummate skill, he

succeeded in making a telescope magnifying thirty times. Thus equipped

he was ready to begin a survey of the heavens. The first object he

carefully examined was naturally the moon. He found there everything at

first sight very like the earth, mountains and valleys, craters and

plains, rocks, and apparently seas. You may imagine the hostility

excited among the Aristotelian philosophers, especially, no doubt, those

he had left behind at Pisa, on the ground of his spoiling the pure,

smooth, crystalline, celestial face of the moon as they had thought it,

and making it harsh and rugged, and like so vile and ignoble a body as

the earth.

He went further, however, into heterodoxy than this: he not only made

the moon like the earth, but he made the earth shine like the moon. The

visibility of "the old moon in the new moon's arms" he explained by

earth-shine. Leonardo had given the same explanation a century before.

Now, one of the many stock arguments against Copernican theory of the

earth being a planet like the rest was that the earth was dull and dark

and did not shine. Galileo argued that it shone just as much as the moon

does, and in fact rather more--especially if it be covered with clouds.

One reason of the peculiar brilliancy of Venus is that she is a very

cloudy planet.[29] Seen from the moon the earth would look exactly as

the moon does to us, only a little brighter and sixteen times as

big--four times the diameter.

Wherever Galileo turned his telescope new stars appeared. The Milky Way,

which had so puzzled the ancients, was found to be composed of stars.

Stars that appeared single to the eye were some of them found to be

double; and at intervals were found hazy nebulous wisps, some of which

seemed to be star clusters, while others seemed only a fleecy cloud.

Now we come to his most brilliant, at least his most sensational,

discovery. Examining Jupiter minutely on January 7, 1610, he noticed

three little stars near it, which he noted down as fixing its then

position. On the following night Jupiter had moved to the other side of

the three stars. This was natural enough, but was it moving the right

way? On examination it appeared not. Was it possible the tables were

wrong? The next evening was cloudy, and he had to curb his feverish

impatience. On the 10th there were only two, and those on the other

side. On the 11th two again, but one bigger than the other. On the 12th

the three reappeared, and on the 13th there were four. No more appeared.

Jupiter, then, had moons like the earth--four of them in fact!--and they

revolved round him in periods which were soon determined.

The news of the discovery soon spread and excited the greatest interest

and astonishment. Many of course refused to believe it. Some there were

who, having been shown them, refused to believe their eyes, and asserted

that although the telescope acted well enough for terrestrial objects,

it was altogether false and illusory when applied to the heavens. Others

took the safer ground of refusing to look through the glass. One of

these who would not look at the satellites happened to die soon

afterward. "I hope," says Galileo, "that he saw them on his way to

heaven."

The way in which Kepler received the news is characteristic, though by

adding four to the supposed number of planets it might have seemed to

upset his notions about the five regular solids.

He says: "I was sitting idle at home thinking of you, most excellent

Galileo, and your letters, when the news was brought me of the discovery

of four planets by the help of the double eye-glass. Wachenfels stopped

his carriage at my door to tell me, when such a fit of wonder seized me

at a report which seemed so very absurd, and I was thrown into such

agitation at seeing an old dispute between us decided in this way, that

between his joy, my coloring, and the laughter of us both, confounded as

we were by such a novelty, we were hardly capable, he of speaking, or I

of listening.

"On our separating, I immediately fell to thinking how there could be

any addition to the number of planets without overturning my _Mysterium

Cosmographicon_, published thirteen years ago, according to which

Euclid's five regular solids do not allow more than six planets round

the sun. But I am so far from disbelieving the existence of the four

circumjovial planets that I long for a telescope to anticipate you if

possible in discovering two round Mars--as the proportion seems to me to

require--six or eight round Saturn, and one each round Mercury and

Venus."

As an illustration of the opposite school I will take the following

extract from Francesco Sizzi, a Florentine astronomer, who argues

against the discovery thus:

"There are seven windows in the head--two nostrils, two eyes, two ears,

and a mouth; so in the heavens there are two favorable stars, two

unpropitious, two luminaries, and Mercury alone undecided and

indifferent. From which and many other similar phenomena of nature, such

as the seven metals, etc., which it were tedious to enumerate, we gather

that the number of planets is necessarily seven.

"Moreover, the satellites are invisible to the naked eye, and therefore

can have no influence on the earth, and therefore would be useless, and

therefore do not exist.

"Besides, the Jews and other ancient nations as well as modern Europeans

have adopted the division of the week into seven days, and have named

them from the seven planets: now if we increase the number of the

planets this whole system falls to the ground."

To these arguments Galileo replied that whatever their force might be as

a reason for believing beforehand that no more than seven planets would

be discovered, they hardly seemed of sufficient weight to destroy the

new ones when actually seen. Writing to Kepler at this time, Galileo

ejaculates:

"Oh, my dear Kepler, how I wish that we could have one hearty laugh

together! Here, at Padua, is the principal professor of philosophy whom

I have repeatedly and urgently requested to look at the moon and planets

through my glass, which he pertinaciously refuses to do. Why are you not

here? What shouts of laughter we should have at this glorious folly! And

to hear the professor of philosophy at Pisa laboring before the Grand

Duke with logical arguments, as if with magical incantations, to charm

the new planets out of the sky."

A young German _protégé_ of Kepler, Martin Horkey, was travelling in

Italy, and meeting Galileo at Bologna was favored with a view through

his telescope. But supposing that Kepler must necessarily be jealous of

such great discoveries, and thinking to please him, he writes: "I cannot

tell what to think about these observations. They are stupendous, they

are wonderful, but whether they are true or false I cannot tell." He

concludes, "I will never concede his four new planets to that Italian

from Padua, though I die for it." So he published a pamphlet asserting

that reflected rays and optical illusions were the sole cause of the

appearance, and that the only use of the imaginary planets was to

gratify Galileo's thirst for gold and notoriety.

When after this performance he paid a visit to his old instructor Kepler

he got a reception which astonished him. However, he pleaded so hard to

be forgiven that Kepler restored him to partial favor, on this

condition, that he was to look again at the satellites, and this time to

see them and own that they were there.

By degrees the enemies of Galileo were compelled to confess to the truth

of the discovery, and the next step was to outdo him. Scheiner counted

five, Rheiter nine, and others went as high as twelve. Some of these

were imaginary, some were fixed stars, and four satellites only are

known to this day.[30]

Here, close to the summit of his greatness, we must leave him for a

time. A few steps more and he will be on the brow of the hill; a short

piece of table-land, and then the descent begins.

In dealing with these historic events will you allow me to repudiate

once for all the slightest sectarian bias or meaning? I have nothing to

do with Catholic or Protestant as such. I have nothing to do with the

Church of Rome as such. I am dealing with the history of science. But

historically at one period science and the Church came into conflict. It

was not specially one church rather than another--it was the Church in

general, the only one that then existed in those countries.

Historically, I say, they came into conflict, and historically the

Church was the conqueror. It got its way; and science, in the persons of

Bruno, Galileo, and several others, was vanquished. Such being the

facts, there is no help but to mention them in dealing with the history

of science. Doubtless _now_ the Church regards it as an unhappy victory,

and gladly would ignore this painful struggle. This, however, is

impossible. With their creed the churchmen of that day could act in no

other way. They were bound to prosecute heresy, and they were bound to

conquer in the struggle or be themselves shattered.

But let me insist on the fact that no one accuses the ecclesiastical

courts of crime or evil motives. They attacked heresy after their

manner, as the civil courts attacked witchcraft after _their_ manner.

Both erred grievously, but both acted with the best intentions.

We must remember, moreover, that his doctrines were scientifically

heterodox, and the university professors of that day were probably quite

as ready to condemn them as the Church was. To realize the position we

must think of some subjects which _to-day_ are scientifically heterodox,

and of the customary attitude adopted toward them by persons of widely

differing creeds.

If it be contended now, as it is, that the ecclesiastics treated Galileo

well, I admit it freely: they treated him as well as they possibly

could. They overcame him, and he recanted; but if he had not recanted,

if he had persisted in his heresy, they would--well, they would still

have treated his soul well, but they would have set fire to his body.

Their mistake consisted not in cruelty, but in supposing themselves the

arbiters of eternal truth; and by no amount of slurring and glossing

over facts can they evade the responsibility assumed by them on account

of this mistaken attitude.

We left Galileo standing at his telescope and beginning his survey of

the heavens. We followed him indeed through a few of his first great

discoveries--the discovery of the mountains and other variety of

surface in the moon, of the nebulæ and a multitude of faint stars, and

lastly of the four satellites of Jupiter.

This latter discovery made an immense sensation, and contributed its

share to his removal from Padua, which quickly followed it. Before the

end of the year 1610 Galileo had made another discovery--this time on

Saturn. But to guard against the host of plagiarists and impostors he

published it in the form of an anagram, which, at the request of the

Emperor Rudolph--a request probably inspired by Kepler--he interpreted;

it ran thus: The farthest planet is triple.

Very soon after he found that Venus was changing from a full-moon to a

half-moon appearance. He announced this also by an anagram, and waited

till it should become a crescent, which it did. This was a dreadful blow

to the anti-Copernicans, for it removed the last lingering difficulty to

the reception of the Copernican doctrine. Copernicus had predicted,

indeed, a hundred years before, that, if ever our powers of sight were

sufficiently enhanced, Venus and Mercury would be seen to have phases

like the moon. And now Galileo with his telescope verifies the

prediction to the letter.

Here was a triumph for the grand old monk, and a bitter morsel for his

opponents.

Castelli writes, "This must now convince the most obstinate." But

Galileo, with more experience, replies: "You almost make me laugh by

saying that these clear observations are sufficient to convince the most

obstinate; it seems you have yet to learn that long ago the observations

were enough to convince those who are capable of reasoning and those who

wish to learn the truth; but that to convince the obstinate and those

who care for nothing beyond the vain applause of the senseless vulgar,

not even the testimony of the stars would suffice, were they to descend

on earth to speak for themselves. Let us, then, endeavor to procure some

knowledge for ourselves, and rest contented with this sole satisfaction;

but of advancing in popular opinion, or of gaining the assent of the

book-philosophers, let us abandon both the hope and the desire."

What a year's work it had been! In twelve months observational astronomy

had made such a bound as it has never made before or since.[31] Why did

not others make any of these observations? Because no one could make

telescopes like Galileo. He gathered pupils round him, however, and

taught them how to work the lenses, so that gradually these instruments

penetrated Europe, and astronomers everywhere verified his splendid

discoveries.

FOOTNOTES:

[29] It is of course the "silver lining" of clouds that outside

observers see.

[30] A fifth satellite of Jupiter has been recently discovered; and

Kepler's guess at two moons for Mars has also been justified.

[31] The next year Galileo discovered also the spots upon the sun

and estimated roughly its time of rotation.

BEGINNING OF BRITISH POWER IN INDIA

A.D. 1612

BECKLES WILLSON

By chartering the original English East India Company, Queen

Elizabeth took the first step toward establishing that empire

in the Orient which has since become such an important appanage

of the British crown. This oldest English company in India is

also called the "Mother Company" and the "John Company." It

began English trade with India, and its operations prepared the

way for British government in that vast country.

After the Portuguese discovery of the passage round Africa,

toward the end of the fifteenth century, other European nations

for some time appeared to recognize Portugal's exclusive claim

to the navigation of that route. In 1510 the Portuguese made a

permanent settlement in India at Goa. But during this century

the Dutch obtained a foothold in the country, and in 1580

Portugal was conquered by Spain.

Dutch enterprise and the Spanish absorption of Portugal's

Indian establishments aroused the commercial spirit of England.

In 1599 an English association was formed, with a large fund,

"for trade to the East Indies." In December, 1600, Queen

Elizabeth granted this association a charter, incorporating the

"Adventurers" under the title of "the Governor and Company of

Merchants of London trading into the East Indies." The company

was allowed unlimited rights of purchasing lands, and a fifteen

years' monopoly of trade. In 1609 the charter was renewed and

made perpetual by James I; but at first the company appears to

have done no very extensive business. The beginning of its more

active career, in the midst of grave difficulties and

conflicts, is well described by Willson, whose history thus

covers an important period in the development of India and in

the expansion of British power.

When the East India Company had been in existence eleven years it

possessed hardly more than the rudiments of factories in the Indies,

while the Dutch boasted fully a dozen regularly established

trading-settlements, from most of which they had ejected the Spaniards

and Portuguese.

The Great Events by Famous Historians, Volume 11 · 第 3 / 37 段