The last of Bentley’s works which we shall notice is his unfortunate

edition of Milton’s Paradise Lost, given to the public in 1732. It is a

sad instance of utter perversion of judgment in a man of extraordinary

talent. Fenton first suggested, that the spots in that sun-like

performance might be owing to the misapprehension of the amanuensis, and

the ignorant blunders of a poverty-stricken printer. On this foundation

Bentley, neither himself a poet, nor possessing much taste or feeling

for the higher effusions of even his own favourite authors, the Greek

and Latin poets, undertook to revise the language, remedy the blemishes,

and reject the supposed interpolations of our national epic. He was

peculiarly disqualified for such a task, not only by prosaic temperament

and the chill of advanced years, but by his entire ignorance of the

Italian poets and romance writers, from whose fables and imagery Milton

borrowed his illustrations as freely as from the more familiar stories

and modes of expression of the classical authorities. As usual with him,

his notes were written hastily, and sent immediately to the press. The

public disapprobation was unanimous and just: but even in this

performance many acute pieces of criticism are scattered up and down,

for which the world, disgusted by his audacity and flippancy, allows him

no credit.

We must pass quickly over the ten remaining years of Bentley’s life.

They were embittered by a fresh contest for character and station before

the supreme tribunal of the kingdom. The case between the Bishop of Ely

and Dr. Bentley, respecting the visitatorial jurisdiction over Trinity

College in general, and over the Master in particular, was argued first

in the Court of King’s Bench, and then carried by appeal to the House of

Lords, where it was finally affirmed that the Bishop of Ely was visitor.

In his seventy-second year Bentley underwent a second trial at Ely

House, and was sentenced to be deprived of his mastership; but he eluded

the execution of the sentence, and continued to perform the duties of

the office which he held. At length a compromise was effected between

him and some of his most active prosecutors, many of whom, as well as

himself, were septuagenarians. On his proposed edition of Homer,

distinguished by the restoration of the Digamma, we need not enlarge. It

appears to have been broken off by a paralytic attack, in the course of

1739. In the following year he sustained the severest loss, by the death

of his wife in the fortieth year of their union. His own death took

place July 14, 1742, when he had completed his eightieth year. He was

buried in the chapel; to which he had been a benefactor by giving £200

towards its repairs, soon after he was appointed to the mastership.

Bentley’s literary character is known in all parts of Europe where

learning is known. In his private character he was what Johnson liked, a

good hater: there was much of arrogance, and no little obstinacy in his

composition; but it must be admitted on the other hand, that he had many

high and amiable qualities. Though too prone to encounter hostility by

oppression, he was warm and sincere in friendship, an affectionate

husband, and a good father. In the exercise of hospitality at his lodge

he maintained the dignity of the college, and rivalled the munificence

even of the papal priesthood. His benefactions to the college were also

liberal: but he exacted from it far more than it was willing to pay, or

than any former master had received; and his name would stand fairer if

his generosity had been less distinguished, provided that, at the same

time, his conduct had been less grasping. We shall only add that the

severity of his temper as a critic and controversial writer was

exchanged in conversation for a strain of vivacity and pleasantry

peculiar to himself.

Bentley had three children: a son called by his own name, and two

daughters. The son was bred under his own tuition at Trinity College,

where he obtained a fellowship. His contemporaries acknowledge his

genius, but lament that his pursuits were so desultory and various as to

exclude him from that substantial fame which his talents might have

ensured. Dr. Bentley’s eldest daughter, Elizabeth, married Mr. Humphry

Ridge, a gentleman of good family in Hampshire, but was left a widow in

less than a year, and returned to reside with her father. The youngest,

Joanna, married Mr. Denison Cumberland, grandson to the learned Bishop

of Peterborough. The first issue of this marriage was the late Richard

Cumberland, well known in the republic of letters, and especially as a

dramatic writer. In his memoir of his own life Mr. Cumberland gives some

amusing anecdotes of his grandfather in his old age. His object seems to

have been to paint the domestic character of Bentley in a pleasing

light, and to counteract the prevalent opinion of his stern and

overbearing manners. The old man’s personal kindness towards himself

seems to have produced a deep and well merited feeling of gratitude. His

communications however are of little value, for he neglected his

opportunities of obtaining accurate and more important information from

his mother and other relatives of the great critic.

[Illustration:

_Engraved by F. Mackenzie._

KEPPLER.

_From a Picture in the Collection of

Godefroy Kraenner, Merchant at Ratisbon._

Under the Superintendance of the Society for the Diffusion of Useful

Knowledge.

_London, Published by Charles Knight, Ludgate Street, & Pall Mall

East._

]

[Illustration]

KEPLER.

The matter contained in this sketch of Kepler’s history, is exclusively

derived from the Life published in the Library of Useful Knowledge. To

that work we refer all readers who wish to make themselves acquainted

with the contents of Kepler’s writings, and with the singular methods by

which he was led to his great discoveries: it will be evident, on

inspection, that it would be useless to attempt farther compression of

the scientific matter therein contained. Our object therefore will be to

select such portions as may best illustrate his singular and

enthusiastic mind, and to give a short account of his not uneventful

life.

John Kepler was born December 21, 1571, Long. 29° 7´, Lat. 48° 54´, as

we are carefully informed by his earliest biographer Hantsch. It is well

to add that on the spot thus astronomically designated as our

astronomer’s birth-place, stands the city of Weil, in the Duchy of

Wirtemberg. Kepler was first sent to school at Elmendingen, where his

father, a soldier of honourable family, but indigent circumstances, kept

a tavern: his education was completed at the monastic school of

Maulbronn, and the college of Tubingen, where he took his Master’s

degree in 1591. About the same time he was offered the astronomical

lectureship at Gratz, in Styria: and he accepted the post by advice, and

almost by compulsion, of his tutors, “better furnished,” he says, “with

talent than knowledge, and with many protestations that I was not

abandoning my claim to be provided for in some other more brilliant

profession.” Though well skilled in mathematics, and devoted to the

study of philosophy, he had felt hitherto no especial vocation to

astronomy, although he had become strongly impressed with the truth of

the Copernican system, and had defended it publicly in the schools of

Tubingen. He was much engrossed by inquiries of a very different

character: and it is fortunate for his fame that circumstances withdrew

him from the mystical pursuits to which through life he was more or less

addicted; from such profitless toil as the “examination of the nature of

heaven, of souls, of genii, of the elements, of the essence of fire, of

the cause of fountains, of the ebb and flow of the tide, the shape of

the continents and inland seas, and things of this sort,” to which, he

says, he had devoted much time. The sort of spirit in which he was

likely to enter on the more occult of these inquiries, and the sort of

agency to which he was likely to ascribe the natural phenomena of which

he speaks, may be estimated from an opinion which he gravely advanced in

mature years and established fame, that the earth is an enormous living

animal, with passions and affections analogous to those of the creatures

which live on its surface. “The earth is not an animal like a dog, ready

at every nod; but more like a bull or an elephant, slow to become angry,

and so much the more furious when incensed.” “If any one who has climbed

the peaks of the highest mountains throw a stone down their very deep

clefts, a sound is heard from them; or if he throw it into one of the

mountain lakes, which beyond doubt are bottomless, a storm will

immediately arise, just as when you thrust a straw into the ear or nose

of a ticklish animal, it shakes its head, and runs shuddering away. What

so like breathing, especially of those fish who draw water into their

mouths, and spout it out again through their gills, as that wonderful

tide! For although it is so regulated according to the course of the

moon, that in the preface to my ‘Commentaries on Mars’ I have mentioned

it as probable that the waters are attracted by the moon, as iron is by

the loadstone, yet if any one uphold that the earth regulates its

breathing according to the motion of the sun and moon, as animals have

daily and nightly alternations of sleep and waking, I shall not think

his philosophy unworthy of being listened to; especially if any flexible

parts should be discovered in the depths of the earth to supply the

functions of lungs or gills.”

The first fruit of Kepler’s astronomical researches was entitled

‘Prodromus Dissertationis Cosmographicæ,’ the first part of a work to be

called ‘Mysterium Cosmographicum,’ of which, however, the sequel was

never written. The most remarkable part of the book is a fanciful

attempt to show that the orbits of the planets may be represented by

spheres circumscribed and inscribed in the five regular solids. Kepler

lived to be convinced of the total baselessness of this supposed

discovery, in which, however, at the time, he expressed high exultation.

In the same work are contained his first inquiries into the proportion

between the distances of the planets from the sun and their periods of

revolution. He also attempted to account for the motion of the planets,

by supposing a moving influence emitted like light from the sun, which

swept round those bodies, as the sails of a windmill would carry any

thing attached to them: of a genuine central force he had no knowledge,

though he had speculated on the existence of an attractive force in the

centre of motion, and rejected it on account of difficulties which he

could not explain. The ‘Prodromus’ was published in 1596, and the genius

and industry displayed in it gained praise from the best astronomers of

the age.

In the following year Kepler withdrew from Gratz into Hungary,

apprehending danger from the unadvised promulgation of some, apparently

religious, opinions. During this retirement he became acquainted with

the celebrated Tycho Brahe, at that time retained by the Emperor Rodolph

II. as an astrologer and mathematician, and residing at the castle of

Benach, near Prague. Kepler, harassed throughout life by poverty, was

received by his more fortunate fellow-labourer with cordial kindness. No

trace of jealousy is to be found in their intercourse. Tycho placed the

observations which he had made with unremitted industry during many

years in the hands of Kepler, and used his interest with the Emperor to

obtain permission for his brother astronomer to remain at Benach as

assistant observer, retaining his salary and professorship at Gratz.

Before all was settled, however, Kepler finally threw up that office,

and remained, it should seem, entirely dependent on Tycho’s bounty. The

Dane was then employed in constructing a new set of astronomical tables,

to be called the Rudolphine, intended to supersede those calculated on

the Ptolemaic and Copernican systems. He was interrupted in this labour

by death, in 1601; and the task of finishing it was intrusted to Kepler,

who succeeded him as principal mathematician to the Emperor. A large

salary was attached to this office, but to extract any portion of it

from a treasury deranged and almost exhausted by a succession of wars,

proved next to impossible. He remained for several years, as he himself

expresses it, begging his bread from the Emperor at Prague, during which

the Rudolphine Tables remained neglected, for want of funds to defray

the expenses of continuing them. He published, however, several smaller

works; a treatise on Optics, entitled a Supplement to Vitellion, in

which he made an unsuccessful attempt to determine the cause and the

laws of refraction; a small work on a new star which appeared in

Cassiopeia in 1604, and shone for a time with great splendour; another

on comets, in which he suggests the possibility of their being planets

moving in straight lines. Meanwhile he was continuing his labours on the

observations of Tycho, and especially on those relating to the planet

Mars: and the result of them appeared in 1609, in his work entitled

‘Astronomia Nova;’ or Commentaries on the motions of Mars. He engaged in

these extensive calculations from dissatisfaction with the existing

theories, by none of which could the observed and calculated motions of

the planets be made to coincide; but without any notion whither the task

was about to lead him, or of rejecting the complicated machinery of

former astronomers—

the sphere

With centric and eccentric scribbled o’er,

Cycle and epicycle, orb in orb.

His inquiries are remarkable for the patience with which he continued to

devise hypotheses, one after another, and the scrupulous fidelity with

which he rejected them in succession, as they proved irreconcileable

with the unerring test of observation. Not less remarkable is the

singular good fortune by which, while groping in the dark among

erroneous principles and erroneous assumptions, he was led, by careful

observation of Mars, to discover the true form of its orbit, and the

true law of its motion, and the motion of all planets, round the sun.

These are enunciated in two of the three celebrated theorems known by

the name of Kepler’s Laws, beyond comparison the most important

discoveries made in astronomy from the time of Copernicus to that of

Newton, of which the first is, that the planets move in ellipses, in one

of the foci of which the sun is placed the second, that the time of

describing any arc is proportional, in the same orbit, to the area

comprised by the arc itself, and lines drawn from the sun to the

beginning and end of it.

About the year 1613 Kepler quitted Prague, after a residence of eleven

years, to assume a professorship in the University of Linz. The year

preceding his departure saw him involved in great domestic distress.

Want of money, sickness, the occupation of the city by a turbulent army,

the death of his wife and of the son whom he best loved, these, he says

to a correspondent, “were reasons enough why I should have overlooked

not only your letter, but even astronomy itself.” His first marriage,

contracted early in life, had not been a happy one: but he resolved on a

second venture, and no less than eleven ladies were successively the

objects of his thoughts. After rejecting, or being rejected, by the

whole number, he at last settled on her who stood fifth in the list; a

woman of humble station, but, according to his own account, possessed of

qualities likely to wear well in a poor man’s house. He employed the

judgment and the mediation of his friends largely in this delicate

matter: and in a letter to the Baron Strahlendorf, he has given a full

and amusing account of the process of his courtships, and the

qualifications of the ladies among whom his judgment wavered. He

proposed to one lady whom he had not seen for six years, and was

rejected: on paying her a visit soon after, he found, to his great

relief, that she had not a single pleasing point about her. Another was

too proud of her birth; another too old; another married a more ardent

lover, while Kepler was speculating whether he would take her or not;

and a fifth punished the indecision which he had shown towards others by

alternations of consent and denial, until after a three months’

courtship, the longest in the list, he gave her up in despair.

Kepler did not long hold his professorship at Linz. Some religious

opinions relative to the doctrine of transubstantiation gave offence to

the Roman Catholic party, and he was excommunicated. In 1617 he received

an invitation to fill the chair of mathematics at Bologna: this however

he declined, pleading his German origin and predilections, and his

German habits of freedom in speech and manners, which he thought likely

to expose him to persecution or reproach in Italy. In 1618 he published

his Epitome of the Copernican system, a summary of his philosophical

opinions, drawn up in the form of question and answer. In 1619 appeared

his celebrated work ‘Harmonice Mundi,’ dedicated to King James I. of

England; a book strongly illustrative of the peculiarities of Kepler’s

mind, combining the accuracy of geometric science with the wildest

metaphysical doctrines, and visionary theories of celestial influences.

The two first books are almost strictly geometrical; the third treats of

music; for the fourth and fifth, we take refuge from explaining their

subjects in transcribing the author’s exposition of their contents. “The

fourth, metaphysical, psychological, and astrological, on the mental

essence of harmonies, and of their kinds in the world, especially on the

harmony of rays emanating on the earth from the heavenly bodies, and on

their effect in nature, and on the sublunary and human soul; the fifth,

astronomical and metaphysical, on the very exquisite harmonies of the

celestial motions, and the origin of the eccentricities in harmonious

proportions.” This work, however, is remarkable for containing amid the

varied extravagances of its two last books, the third of Kepler’s Laws,

namely, that the squares of the periods of the planets’ revolution vary

as the cubes of their distances from the sun; a discovery in which he

exulted with no measured joy. “It is now eighteen months since I got the

first glimpse of light, three months since the dawn, very few days since

the unveiled sun, most admirable to gaze upon, burst out upon me.

Nothing holds me; I will indulge in my sacred fury; I will triumph over

mankind by the honest confession that I have stolen the golden vases of

the Egyptians, to build up a tabernacle for my God far away from the

confines of Egypt. If you forgive me, I rejoice; if you are angry, I can

bear it: the die is cast, the book is written; to be read either now or

by posterity, I care not which: it may well wait a century for a reader,

as God has waited six thousand years for an observer.”

The substance of Kepler’s astrological opinions is contained in this

work. It is remarkable that one whose candour and good faith are so

conspicuous, one so intent on correcting his various theories by

observation and experience, should have given in to this now generally

rejected system of imposture and credulity; nay should profess to have

been forced to adopt it from direct and positive observations. “A most

unfailing experience (as far as can be hoped in natural phenomena), of

the excitement of sublunary nature by the conjunctions and aspects of

the planets, has instructed and compelled my unwilling belief.” At the

same time he professed through life a supreme contempt for the common

herd of nativity casters, and claimed to be the creator of a “new and

most true philosophy, a tender plant which, like all other novelties,

ought to be carefully nursed and cherished.” His plant was rooted in the

sand, and it has perished; nor is it important to explain the fine-spun

differences by which his own astrological belief was separated from

another not more baseless. Poor through life, he relieved his ever

recurring wants by astrological calculations: and he enjoyed

considerable reputation in this line, and received ample remuneration

for his predictions. It was principally as astrologers that both Tycho

Brahe and Kepler were valued by the Emperor Rudolph: and it was in the

same capacity that the latter was afterwards entertained by Wallenstein.

One circumstance may suggest a doubt whether his predictions were always

scrupulously honest. From the year 1617 to 1620, he published an annual

Ephemeris, concerning which he writes thus: “In order to pay the expense

of the Ephemeris for these two years, I have also written a _vile

prophesying almanac_, which is hardly more respectable than begging;

unless it be because it saves the Emperor’s credit, who abandons me

entirely, and, with all his frequent and recent orders in council, would

suffer me to perish with hunger.” Poverty is a hard task-master; yet

Kepler should not have condescended to become the Francis Moore of his

day.

In 1620, Kepler was strongly urged by Sir Henry Wotton, then ambassador

to Venice, to take refuge in England from the difficulties which beset

him. This invitation was not open to the objections which had deterred

him from accepting an appointment in Italy: but love of his native land

prevailed to make him decline it also. He continued to weary the

Imperial Government with solicitations for money to defray the expense

of the Rudolphine Tables, which were not printed until 1627. These were

the first calculated on the supposition of elliptic orbits, and contain,

besides tables of the sun and planets, logarithmic and other tables to

facilitate calculation, the places of one thousand stars as determined

by Tycho, and a table of refractions. Similar tables of the planetary

motions had been constructed by Ptolemy, and reproduced with alterations

in the thirteenth century under the direction of Alphonso, King of

Castile. Others, called the Prussian Tables, had been calculated after

the discoveries of Copernicus, by two of that great astronomer’s pupils.

All these, however, were superseded in consequence of the observations

of Tycho Brahe, observations far more accurate than had ever before been

made: and for the publication of the Rudolphine Tables alone, which for

a long time continued unsurpassed in exactness, the name of Kepler would

deserve honourable remembrance.

Kepler was the first of the Germans to appreciate and use Napier’s

invention of logarithms: and he himself calculated and published a

series, under the title ‘Chilias Logarithmorum,’ in 1624. Not long after

the Rudolphine Tables were printed, he received permission from the

Emperor Ferdinand to attach himself to the celebrated Wallenstein, a

firm believer in the science of divination by the stars. In him Kepler

found a more munificent patron than he had yet enjoyed; and by his

influence he was appointed to a professorship at the University of

Rostock, in the Duchy of Mecklenburgh. But the niggardliness of the

Imperial Court, which kept him starving through life, was in some sense

the cause of his death. He had claims on it to the amount of eight

thousand crowns, which he took a journey to Ratisbon to enforce, but

without success. Fatigue or disappointment brought on a fever which put

an end to his life in November, 1630, in his 59th year. A plain stone,

with a simple inscription, marked his grave in St. Peter’s church-yard,

in that city. Within seventy paces of it, a marble monument has been

erected to him in the Botanic Garden, by a late Bishop of Constance. He

left a wife and numerous family ill provided for. His voluminous

manuscripts are now deposited in the Imperial Library of St. Petersburg.

Only one volume of letters, in folio, has been published from them; and

out of these the chief materials for his biography have been extracted.

[Illustration]

SIR MATTHEW HALE.

Matthew Hale was born on the 1st of November, 1609, at Alderley, a small

village situated in Gloucestershire, about two miles from

Wotton-under-Edge. His father, Robert Hale, was a barrister of Lincoln’s

Inn, and his mother, whose maiden name was Poyntz, belonged to an

ancient and respectable family which had resided for several generations

at Iron Acton. Hale’s father is represented to have been a man of such

scrupulous delicacy of conscience, that he abandoned his profession,

because he thought that some things, of ordinary practice in the law,

were inconsistent with that literal and precise observance of truth

which he conceived to be the duty of a Christian. “He gave over his

practice,” says Burnet, in his Life of Hale, “because he could not

understand the reason of giving colour in pleadings, which, as he

thought, was to tell a lie.”

[Illustration:

_Engraved by J. W. Cook._

HALE.

_From an original Picture in the Library

of Lincolns Inn._

Under the Superintendance of the Society for the Diffusion of Useful

Knowledge.

_London, Published by Charles Knight, Ludgate Street, & Pall Mall

East._

]

The Gallery of Portraits: with Memoirs. Volume 3 (of 7) · 第 6 / 20 段