The age following that of Copernicus
produced three outstanding figures associated with
the science of astronomy, then reaching the close of
what Professor Forbes so aptly styles the geometrical
period. These three Sir David Brewster has termed
“Martyrs of Science”; Galileo, the great
Italian philosopher, has his own place among the “Pioneers
of Science”; and invaluable though Tycho Brahe’s
work was, the latter can hardly be claimed as a pioneer
in the same sense as the other two. Nevertheless,
Kepler, the third member of the trio, could not have
made his most valuable discoveries without Tycho’s
observations.
Of noble family, born a twin on 14th
December, 1546, at Knudstrup in Scania (the southernmost
part of Sweden, then forming part of the kingdom of
Denmark), Tycho was kidnapped a year later by a childless
uncle. This uncle brought him up as his own son,
provided him at the age of seven with a tutor, and
sent him in 1559 to the University of Copenhagen,
to study for a political career by taking courses in
rhetoric and philosophy. On 21st August, 1560,
however, a solar eclipse took place, total in Portugal,
and therefore of small proportions in Denmark, and
Tycho’s keen interest was awakened, not so much
by the phenomenon, as by the fact that it had occurred
according to prediction. Soon afterwards he purchased
an edition of Ptolemy in order to read up the subject
of astronomy, to which, and to mathematics, he devoted
most of the remainder of his three years’ course
at Copenhagen. His uncle next sent him to Leipzig
to study law, but he managed to continue his astronomical
researches. He obtained the Alphonsine and the
new Prutenic Tables, but soon found that the latter,
though more accurate than the former, failed to represent
the true positions of the planets, and grasped the
fact that continuous observation was essential in order
to determine the true motions. He began by observing
a conjunction of Jupiter and Saturn in August, 1563,
and found the Prutenic Tables several days in error,
and the Alphonsine a whole month. He provided
himself with a cross-staff for determining the angular
distance between stars or other objects, and, finding
the divisions of the scale inaccurate, constructed
a table of corrections, an improvement that seems
to have been a decided innovation, the previous practice
having been to use the best available instrument and
ignore its errors. About this time war broke
out between Denmark and Sweden, and Tycho returned
to his uncle, who was vice-admiral and attached to
the king’s suite. The uncle died in the
following month, and early in the next year Tycho went
abroad again, this time to Wittenberg. After five
months, however, an outbreak of plague drove him away,
and he matriculated at Rostock, where he found little
astronomy but a good deal of astrology. While
there he fought a duel in the dark and lost part of
his nose, which he replaced by a composition of gold
and silver. He carried on regular observations
with his cross-staff and persevered with his astronomical
studies in spite of the objections and want of sympathy
of his fellow-countrymen. The King of Denmark,
however, having a higher opinion of the value of science,
promised Tycho the first canonry that should fall vacant
in the cathedral chapter of Roskilde, so that he might
be assured of an income while devoting himself to
financially unproductive work. In 1568 Tycho
left Rostock, and matriculated at Basle, but soon moved
on to Augsburg, where he found more enthusiasm for
astronomy, and induced one of his new friends to order
the construction of a large 19-foot quadrant of heavy
oak beams. This was the first of the series of
great instruments associated with Tycho’s name,
and it remained in use for five years, being destroyed
by a great storm in 1574. Tycho meanwhile had
left Augsburg in 1570 and returned to live with his
father, now governor of Helsingborg Castle, until
the latter’s death in the following year.
Tycho then joined his mother’s brother, Steen
Bille, the only one of his relatives who showed any
sympathy with his desire for a scientific career.
On 11th November, 1572, Tycho noticed
an unfamiliar bright star in the constellation of
Cassiopeia, and continued to observe it with a sextant.
It was a very brilliant object, equal to Venus at its
brightest for the rest of November, not falling below
the first magnitude for another four months, and remaining
visible for more than a year afterwards. Tycho
wrote a little book on the new star, maintaining that
it had practically no parallax, and therefore could
not be, as some supposed, a comet. Deeming authorship
beneath the dignity of a noble he was very reluctant
to publish, but he was convinced of the importance
of increasing the number and accuracy of observations,
though he was by no means free from all the erroneous
ideas of his time. The little book contained a
certain amount of astrology, but Tycho evidently did
not regard this as of very great importance.
He adopted the view that the very rarity of the phenomenon
of a new star must prevent the formulation and adoption
of definite rules for determining its significance.
We gather from lectures which he was persuaded to
deliver at the University of Copenhagen that, though
in agreement with the accepted canons of astrology
as to the influence of planetary conjunctions and
such phenomena on the course of human events, he did
not consider the fate predicted by anyone’s
horoscope to be unavoidable, but thought the great
value of astrology lay in the warnings derived from
such computations, which should enable the believer
to avoid threatened calamities. In 1575 he left
Denmark once more and made his way to Cassel, where
he found a kindred spirit in the studious Landgrave,
William IV. of Hesse, whose astronomical pursuits
had been interrupted by his accession to the government
of Hesse, in 1567. Tycho observed with him for
some time, the two forming a firm friendship, and
then visited successively Frankfort, Basle, and Venice,
returning by way of Augsburg, Ratisbon, and Saalfeld
to Wittenberg; on the way he acquired various astronomical
manuscripts, made friends among practical astronomers,
and examined new instruments. He seemed to have
considered the advantages of the several places thus
visited and decided on Basle, but on his return to
Denmark to fetch his family with the object of transferring
them to Basle, he found that his friend the Landgrave
had written to King Frederick on his behalf, urging
him to provide the means to enable Tycho to pursue
his astronomical work, promising that not only should
credit result for the king and for Denmark but that
science itself would be greatly advanced. The
ultimate result of this letter was that after refusing
various offers, Tycho accepted from the king a grant
of the small island of Hveen, in the Sound, with a
guaranteed income, in addition to a large sum from
the treasury for building an observatory on the island,
far removed from the distractions of court life.
Here Tycho built his celebrated observatory of Uraniborg
and began observations in December, 1576, using the
large instruments then found necessary in order to
attain the accuracy of observation which within the
next half-century was to be so greatly facilitated
by the invention of the telescope. Here also
he built several smaller observing rooms, so that his
pupils should be able to observe independently.
For more than twenty years he continued his observations
at Uraniborg, surrounded by his family, and attracting
numerous pupils. His constant aim was to accumulate
a large store of observations of a high order of accuracy,
and thus to provide data for the complete reform of
astronomy. As we have seen, few of the Danish
nobles had any sympathy with Tycho’s pursuits,
and most of them strongly resented the continual expense
borne by the King’s treasury. Tycho moreover
was so absorbed in his scientific pursuits that he
would not take the trouble to be a good landlord,
nor to carry out all the duties laid upon him in return
for certain of his grants of income. His buildings
included a chemical laboratory, and he was in the habit
of making up élixirs for various medical purposes;
these were quite popular, particularly as he made
no charge for them. He seems to have been something
of a homoeopathist, for he recommends sulphur to cure
infectious diseases “brought on by the sulphurous
vapours of the Aurora Borealis”!
King Frederick, in consideration of
various grants to Tycho, relied upon his assistance
in scientific matters, and especially in astrological
calculations; such as the horoscope of the heir apparent,
Prince Christian, born in 1577, which has been preserved
among Tycho’s writings. There is, however,
no known copy in existence of any of the series of
annual almanacs with predictions which he prepared
for the King. In November, 1577, appeared a bright
comet, which Tycho carefully observed with his sextant,
proving that it had no perceptible parallax, and must
therefore be further off than the moon. He thus
definitely overthrew the common belief in the atmospheric
origin of comets, which he had himself hitherto shared.
With increasing accuracy he observed several other
comets, notably one in 1585, when he had a full equipment
of instruments and a large staff of assistants.
The year 1588, which saw the death of his royal benefactor,
saw also the publication of a volume of Tycho’s
great work “Introduction to the New Astronomy”.
The first volume, devoted to the new star of 1572,
was not ready, because the reduction of the observations
involved so much research to correct the star places
for refraction, precession, etc.; it was not completed
in fact until Tycho’s death, but the second
volume, dealing with the comet of 1577, was printed
at Uraniborg and some copies were issued in 1588.
Besides the comet observations it included an account
of Tycho’s system of the world. He would
not accept the Copernican system, as he considered
the earth too heavy and sluggish to move, and also
that the authority of Scripture was against such an
hypothesis. He therefore assumed that the other
planets revolved about the sun, while the sun, moon,
and stars revolved about the earth as a centre.
Geometrically this is much the same as the Copernican
system, but physically it involves the grotesque demand
that the whole system of stars revolves round our
insignificant little earth every twenty-four hours.
Since his previous small book on the comet, Tycho
had evidently considered more fully its possible astrological
significance, for he foretold a religious war, giving
the date of its commencement, and also the rising of
a great Protestant champion. These predictions
were apparently fulfilled almost to the letter by
the great religious wars that broke out towards the
end of the sixteenth century, and in the person of
Gustavus Adolphus.
King Frederick’s death did not
at first affect Tycho’s position, for the new
king, Christian, was only eleven years old, and for
some years the council of regents included two of
his supporters. After their deaths, however,
his emoluments began to be cut down on the plea of
economy, and as he took very little trouble to carry
out any other than scientific duties it was easy enough
for his enemies to find fault. One after another
source of income was cut off, but he persevered with
his scientific work, including a catalogue of stars.
He had obtained plenty of good observations of 777
stars, but thought his catalogue should contain 1000
stars, so he hastily observed as many more as he could
up to the time of his leaving Hveen, though even then
he had not completed his programme. About the
time that King Christian reached the age of eighteen,
Tycho began to look about for a new patron, and to
consider the prospects offered by transferring himself
with his instruments and activities to the patronage
of the Emperor Rudolph II. In 1597, when even
his pension from the Royal treasury was cut off, he
hurriedly packed up his instruments and library, and
after a few weeks’ sojourn at Copenhagen, proceeded
to Rostock, in Mecklenburg, whence he sent an appeal
to King Christian. It is possible that had he
done this before leaving Hveen it might have had more
effect, but it can be readily seen from the tone of
the king’s unfavourable reply that his departure
was regarded as an aggravation of previous shortcomings.
Driven from Rostock by the plague, Tycho settled temporarily
at Wandsbeck, in Holstein, but towards the end of
1598 set out to meet the Emperor at Prague. Once
more plague intervened and he spent some time at Dresden,
afterwards going to Wittenberg for the winter.
He ultimately reached Prague in June, 1599. Rudolph
granted him a salary of at least 3000 florins,
promising also to settle on him the first hereditary
estate that should lapse to the Crown. He offered,
moreover, the choice between three castles outside
Prague, of which Tycho chose Benatek. There he
set about altering the buildings in readiness for
his instruments, for which he sent to Uraniborg.
Before they reached him, after many vexatious delays,
he had given up waiting for the funds promised for
his building expenses, and removed from Benatek to
Prague. It was during this interval that after
considerable negotiation, Kepler, who had been in
correspondence with Tycho, consented to join him as
an assistant. Another assistant, Longomontanus,
who had been with Tycho at Uraniborg, was finding
difficulty with the long series of Mars observations,
and it was arranged that he should transfer his energies
to the lunar observations, leaving those of Mars for
Kepler. Before very much could be done with them,
however, Tycho died at the end of October, 1601.
He may have regretted the peaceful island of Hveen,
considering the troubles in which Bohemia was rapidly
becoming involved, but there is little doubt that
had it not been for his self-imposed exile, his observations
would not have come into Kepler’s hands, and
their great value might have been lost. In any
case it was at Uraniborg that the mass of observations
was produced upon which the fame of Tycho Brahe rests.
His own discoveries, though in themselves the most
important made in astronomy for many centuries, are
far less valuable than those for which his observations
furnished the material. He discovered the third
and fourth inequalities of the moon in longitude, called
respectively the variation and the annual equation,
also the variability of the motion of the moon’s
nodes and the inclination of its orbit to the ecliptic.
He obtained an improved value of the constant of precession,
and did good service by rejecting the idea that it
was variable, an idea which, under the name of trepidation,
had for many centuries been accepted. He discovered
the effect of refraction, though only approximately
its amount, and determined improved values of many
other astronomical constants, but singularly enough
made no determination of the distance of the sun,
adopting instead the ancient and erroneous value given
by Hipparchus.
His magnificent Observatory of Uraniborg,
the finest building for astronomical purposes that
the world had hitherto seen, was allowed to fall into
decay, and scarcely more than mere indications of the
site may now be seen.