KEPLER AND THE PATHWAYS OF THE PLANETS
1571–1635
[35] The invention of the telescope prepared all minds for new
wonders, and made astronomy the leading science of the
day. The heavenly bodies were observed with a new
interest, and their motions studied more intently; for,
while the Copernican system proved that the earth and
other planets moved around the sun as a centre, it left
many mysteries unexplained which could not be accounted
for by the fact of the daily rotation of the earth or
its annual revolution. And while Galileo was startling
the world by his magnificent discoveries in the
heavens, the German astronomer Kepler was revolving in
his mind a theory of the universe which would explain
some these mysteries, and was destined to make his name
as famous as that of his great contemporary.
[36] The motions and nature of the heavenly bodies were
questions that were puzzling the wisest heads, and many
strange theories were advanced to account for the
apparent irregularities in the movements of the planets
and their relation to the fixed stars.
Tycho Brahe, the Danish astronomer, from his
magnificent observatory, Uraniberg, had spent years in
studying the order of planetary motion, and at his
death left his observations recorded in a set of tables
which he intrusted to the care of Kepler, his friend
and pupil. Uraniberg, the city of the heavens, was
built on the Island of Huen, in the Baltic, and under
the patronage of the King of Denmark had become the
resort of many of the most earnest scientific students,
who gladly availed themselves of the teaching of Tycho
Brahe. The observatory was furnished with the most
complete set of astronomical instruments in the world,
and was famous for its facilities for studying the
heavens.
It was by means of these instruments, and by his great
knowledge of mathematics, that Tycho
[37] Brahe was able to make those accurate observations
which gave his tables a priceless value, and enabled
Kepler to work out calculations that it would have been
impossible to make without them.
Unlike many great scientists, Kepler had shown no
special liking for any particular study when a child,
and he was led to the study of astronomy only because
he was appointed professor of that science in the
university of Grätz. But while preparing his
lectures, he became so deeply interested in the subject
that before long it entirely occupied his mind, and
nothing else seemed of any importance as compared with
it.
Kepler possessed a very enthusiastic nature, and was
always ready to listen to new theories, no matter how
wild they might seem. He was among the first to rejoice
over the splendid discoveries of Galileo, and was an
ardent supporter of the Copernican system while it was
yet being reviled by the authority of the Church and
the disciples of Aristotle; and his originality and
enthusiam made him capable of turning the
[38] earnest work of Tycho Brahe to the very best account.
The Copernican theory had been steadily gaining ground
in the estimation of astronomers, and, as one after
another gave up the old system, they ceased to
speculate about the apparent movements of the sun and
stars around the earth, and began to study the planets
from a new point of view.
The path which a planet takes in revolving around the
sun is called its orbit, and astronomers now became
interested in the question of the size of the orbits
and the rate of motion.
The idea that there was always to be found a certain
harmony throughout all the works of nature, swayed the
minds of men as much in the sixteenth century as it had
done since the dawn of scientific thought, and no
sooner was a new theory advanced, or a new discovery
made, than the question arose as to how it would
harmonize with the truths already known, or how, by
following out some suggestion it contained, still other
discoveries might be made.
Kepler possessed more than any of his
con- [39] temporaries the gift of intuition, or the power of
grasping a truth that has not been demonstrated by any
known law of nature, and it is to this insight that he
owed his success. He believed that the entire universe
was governed by one great law or principle, and that
there was a subtle relation existing between things
that seemed to be utterly disconnected. All the great
discoveries of science, all the wonderful operations of
nature, every expression of beauty in the animal or
vegetable world, and every useful invention of man,
seemed alike to him to be controlled by some great
harmonious principles that might be applied with equal
appropriateness to the turning of a water-wheel, or the
rise of the tides, or the rushing of a comet through
illimitable space.
With this idea ruling his mind every new fact was at
once made a basis for calculations that might lead to
the discovery of the great secret law of the universe,
and no toil was considered irksome that could help him
on his way, for he believed that the relation existing
between the different forces of nature was so strong
that the
[40] discovery of the law of one would be the master-key
that would unlock the whole mystery of creation.
This belief, which had haunted the minds of
philosophers of all ages, seemed to Kepler of
infinitely more importance than anything else, and the
discovery of a new planet in the heavens meant to him
not only a new wonder to be admired and gazed at, but a
new instance of the harmonious working of the order of
creation.
Pythagoras had claimed, two thousand years before, that
he had discovered the world-secret, and that harmony,
or proportion, was the law of the universe. He taught
that the planets revolved around a central fire, moving
with an inconceivable swiftness that caused them to be
accompanied by mighty rushing sounds, but that the
different velocities were so beautifully proportioned
that the result was not mere noise, but the most
exquisite music, which excelled in sweetness and power
all earthly melodies. It was said that the reason that
these harmonies were not heard by man was because they
were unceasingly sounding in his ears from the
mo- [41] ment of the birth, and that they would therefore be
unnoticed by him. This notion was also held by many of
the philosophers of the Middle Ages, and even at a much
later day the astrologers and seers claimed that the
music of the spheres might be easily distinguished by
the initiated.
However absurd these theories may seem, it is
nevertheless a fact that the love and study of the
marvellous have in many cases led to the knowledge of
some great truth of nature, and had it not been for
Kepler's belief in the possibility of finding the
secret that had forever eluded mankind, he might never
have been led on to the discoveries that made him
famous.
Calculations whose length and intricacy would have
disheartened anyone else were cheerfully carried on him
for months and years, to be as cheerfully abandoned if
found incorrect, and the unwearied and painstaking
labor of a life-time would have been counted as nothing
in comparison to the discovery of some hitherto unknown
truth.
The possession of Tycho Brahe's tables aided
[42] him greatly in the work, for so accurate had been the
observations of the Danish astronomer, and so reliable
his deductions, that Kepler was able to depend upon
them almost absolutely, and to decide that in every
case his theories must be rejected if they did not
agree with the statements in the tables.
Having always in mind the discovery of the law of
harmony that governed the universe, Kepler bent the
whole energies of his mind to the study of the number
of the planets, their motions, and the sizes of their
orbits. It seemed to him that there must be some
proportion between the sizes of the orbits, and he made
many calculations to prove the truth of this
conjecture. There were at that time but five planets
known, and after having failed to prove any relation
existing between the sizes of their orbits, Kepler
imagined a new planet between Venus and Mercury, and
another between Mars and Jupiter, and then made a new
calculation to see if he could discover the proportion
he was looking for; but he failed also here, and, after
many months spent in fruitless toil, he was obliged
[43] to give up the the work without having proved that
there was any regular rate of increase between the
orbits of the planets nearest the sun and those
farthest from it.
In all his calculations Kepler started from the old
theories of the relations which were supposed to exist
between the different solid and plane figures, and when
he began the study of the planets' orbits he pursued
the same plan.
Up to this time the belief had always been that the
motions of the heavenly bodies were described in
circles. The circle, which was considered the most
beautiful of all curves, had always had a mystic
meaning for the old philosophers, and was always
associated in some manner with their religious belief.
It was the emblem of eternity, and was carved on the
tombs of kings, and inscribed in sacred books, and many
things in nature seemed to mark it with special
significance. The arch of the heavens stretching from
earth to earth again, the cycle of the seasons, the
expansion of the moon, which was worshipped as a deity,
from the crescent form to the perfectly rounded
fig- [44] ure, the circular disc of the sun, and many other
things all enveloped the circle with a sacred meaning
which had by no means losts its power when astronomy
was invested with new interest by the genius of
Copernicus.
And when it was conceded that the planets revolved
around the sun it was at once assumed that their orbits
were circular, for this shape alone would enable them
to harmonize with the popular belief in regard to the
mystic importance of the circle.
Kepler, starting with this idea, tried in vain to
account for the irregularities of the planets' motions
which had puzzled other astronomers. If the planets
moved in circles about the sun, each always taking the
same time for a revolution and moving at a perfectly,
regular rate, then, by knowing their positions at any
one time and the rate at which they were moving, it
would be easy for an astronomer to calculate where they
would be at any other time.
But this was found not to be the case. Mars was the
planet most convenient for making observations upon,
and Kepler made this planet
[45] the subject of careful study for years, in order to
determine the reason for its irregularity of motion.
Mars, travelling round the sun in a circular orbit
should reach a certain point on a certain date, and
because this did not happen the astronomers were sorely
puzzled and invented many ingenious reasons to account
for it.
Kepler made nineteen different theories to explain the
irregularity of the motion of the planets, but none of
them could be considered entirely satisfactory. Each
theory was made the subject of the most careful
calculation, but all failed, and planetary motion
remained as great a mystery as ever.
At last Kepler was forced to think that possibly the
planets did not move in circular orbits, although the
circle was the most beautiful of curves, and he began
to imagine the orbits to be of a different shape than
had hitherto been supposed. The careful study that he
had made the orbit of Mars seemed to show that it was
of an oval form, and as the ellipse was the simplest
form of oval, Kepler chose this curve as a basis for
new calculations.
[46] He had already become convinced, from his study of the
earth's motion, that the planets did not move in their
orbits at a regular rate of motion, but that the moved
faster when they were nearer the sun and slower when
farther from it; this in itself was a most important
discovery.
On applying this rule to calculate the motion of Mars,
Kepler found, to his surprise and delight, that when
its orbit was taken to be an ellipse the planet would
reach any point in its path just at the moment
calculated, but that this would not be so if any other
form of orbit were assumed. This was also found to be
the case with the other planets.
These two great discoveries startled the world by their
originality, and placed Kepler among the greatest
astronomers of the day. Hitherto his theories had been
regarded rather indifferently, as his contemporaries
thought him always too eager to run after new ideas,
and his method of starting a new hypothesis and making
one intricate calculation after another to test it, did
not correspond with their more sober way of proceeding.
[47] But Kepler kept on in his own manner of working, and
continued his study of the planets' orbits. He was
still desirous of proving his old theory of some
proportion existing between them, and after many months
of unremitting toil he was at length rewarded by the
discovery of a law which at once established a most
beautiful harmony in the solar system; for although he
had failed to find any relation existing between the
sizes of the orbits, he now found that there was a very
direct and beautiful proportion between the times of
the revolutions of the planets and their distances from
the sun, and that one, knowing the distance of any one
planet from the sun and the time it occupied in its
revolution, could calculate the distance of any other
planet whose period was given, or the period of any
planet whose distance was known.
These three great discoveries—the shape of the
planets' orbits, the rate of their motion, and the
relation existing between their distances and periods
of revolution—are called Kepler's Laws, and were
the basis for all astronomical calculations from that
time. Their discovery was of
[48] incalculable value to astronomers, and they contained,
besides, the first proof of the ancient belief in the
harmony that prevailed throughout the universe.
The thought of the old philosophers was found to be no
dream, but a reality as beautiful as the conception
that raised the walls of cities by the power of music
or changed the loved of the gods to
constellations, whose solemn motion through the heavens
possessed infinite power over the destinies of mankind;
and although the great discoverer of these laws lived a
life of the greatest hardship and died in extreme
poverty, he is yet to be envied as one who realized all
the hopes of his life and saw his greatest wish brought
to a satisfying completion.
|