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GALILEO GALILEI
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- English
Galileo Galilei's
parents were Vincenzo Galilei and Guilia Ammannati. Vincenzo, who
was born in Florence in 1520, was a teacher of music and a fine lute
player. After studying music in Venice he carried out experiments on
strings to support his musical theories. Guilia, who was born in
Pescia, married Vincenzo in 1563 and they made their home in the
countryside near Pisa. Galileo was their first child and spent his
early years with his family in Pisa.
In 1572, when Galileo was eight
years old, his family returned to Florence, his father's home town.
However, Galileo remained in Pisa and lived for two years with Muzio
Tedaldi who was related to Galileo's mother by marriage. When he
reached the age of ten, Galileo left Pisa to join his family in
Florence and there he was tutored by Jacopo Borghini. Once he was
old enough to be educated in a monastery, his parents sent him to
the Camaldolese Monastery at Vallombrosa which is situated on a
magnificent forested hillside 33 km southeast of Florence. The
Camaldolese Order was independent of the Benedictine Order,
splitting from it in about 1012. The Order combined the solitary
life of the hermit with the strict life of the monk and soon the
young Galileo found this life an attractive one. He became a novice,
intending to join the Order, but this did not please his father who
had already decided that his eldest son should become a medical
doctor.
Vincenzo had Galileo return from
Vallombrosa to Florence and give up the idea of joining the
Camaldolese order. He did continue his schooling in Florence,
however, in a school run by the Camaldolese monks. In 1581 Vincenzo
sent Galileo back to Pisa to live again with Muzio Tedaldi and now
to enrol for a medical degree at the University of Pisa. Although
the idea of a medical career never seems to have appealed to
Galileo, his father's wish was a fairly natural one since there had
been a distinguished physician in his family in the previous century.
Galileo never seems to have taken medical studies seriously,
attending courses on his real interests which were in mathematics
and natural philosophy. His mathematics teacher at Pisa was Filippo
Fantoni, who held the chair of mathematics. Galileo returned to
Florence for the summer vacations and there continued to study
mathematics.
In the year 1582-83 Ostilio
Ricci, who was the mathematician of the Tuscan Court and
a former pupil of
Tartaglia, taught a course on
Euclid's Elements at the University of Pisa which
Galileo attended. During the summer of 1583 Galileo was
back in Florence with his family and Vincenzo encouraged
him to read Galen to further his medical studies. However
Galileo, still reluctant to study medicine, invited Ricci
(also in Florence where the Tuscan court spent the summer
and autumn) to his home to meet his father. Ricci tried
to persuade Vincenzo to allow his son to study mathematics
since this was where his interests lay. Certainly Vincenzo
did not like the idea and resisted strongly but eventually
he gave way a little and Galileo was able to study the works
of Euclid and
Archimedes from the Italian translations which
Tartaglia had made. Of course he was still officially
enrolled as a medical student at Pisa but eventually, by
1585, he gave up this course and left without completing
his degree.
Galileo began teaching mathematics,
first privately in Florence and then during 1585-86 at Siena where
he held a public appointment. During the summer of 1586 he taught at
Vallombrosa, and in this year he wrote his first scientific book
The little balance [La Balancitta] which described
Archimedes' method of finding the specific gravities (that is
the relative densities) of substances using a balance. In the
following year he travelled to Rome to visit
Clavius who was professor of mathematics at the Jesuit Collegio
Romano there. A topic which was very popular with the Jesuit
mathematicians at this time was centres of gravity and Galileo
brought with him some results which he had discovered on this topic.
Despite making a very favourable impression on
Clavius, Galileo failed to gain an appointment to teach
mathematics at the University of Bologna.
After leaving Rome Galileo
remained in contact with
Clavius by correspondence and Guidobaldo del
Monte was also a regular correspondent. Certainly the theorems
which Galileo had proved on the centres of gravity of solids, and
left in Rome, were discussed in this correspondence. It is also
likely that Galileo received lecture notes from courses which had
been given at the Collegio Romano, for he made copies of such
material which still survive today. The correspondence began around
1588 and continued for many years. Also in 1588 Galileo received a
prestigious invitation to lecture on the dimensions and location of
hell in Dante's Inferno at the Academy in Florence.
Fantoni left the chair of
mathematics at the University of Pisa in 1589 and Galileo was
appointed to fill the post (although this was only a nominal
position to provide financial support for Galileo). Not only did he
receive strong recommendations from
Clavius, but he also had acquired an excellent reputation
through his lectures at the Florence Academy in the previous year.
The young mathematician had rapidly acquired the reputation that was
necessary to gain such a position, but there were still higher
positions at which he might aim. Galileo spent three years holding
this post at the university of Pisa and during this time he wrote
De Motu a series of essays on the theory of motion which he
never published. It is likely that he never published this material
because he was less than satisfied with it, and this is fair for
despite containing some important steps forward, it also contained
some incorrect ideas. Perhaps the most important new ideas which
De Motu contains is that one can test theories by conducting
experiments. In particular the work contains his important idea that
one could test theories about falling bodies using an inclined plane
to slow down the rate of descent.
In 1591 Vincenzo Galilei, Galileo's
father, died and since Galileo was the eldest son he had
to provide financial support for the rest of the family
and in particular have the necessary financial means to
provide dowries for his two younger sisters. Being professor
of mathematics at Pisa was not well paid, so Galileo looked
for a more lucrative post. With strong recommendations from
Guidobaldo del Monte, Galileo was appointed professor
of mathematics at the University of Padua (the university
of the Republic of Venice) in 1592 at a salary of three
times what he had received at Pisa. On 7 December 1592 he
gave his inaugural lecture and began a period of eighteen
years at the university, years which he later described
as the happiest of his life. At Padua his duties were mainly
to teach Euclid's
geometry and standard (geocentric) astronomy to medical
students, who would need to know some astronomy in order
to make use of astrology in their medical practice. However,
Galileo argued against
Aristotle's view of astronomy and natural philosophy
in three public lectures he gave in connection with the
appearance of a New Star (now known as 'Kepler's
supernova') in 1604. The belief at this time was that of
Aristotle, namely that all changes in the heavens had
to occur in the lunar region close to the Earth, the realm
of the fixed stars being permanent. Galileo used parallax
arguments to prove that the New Star could not be close
to the Earth. In a personal letter written to
Kepler in 1598, Galileo had stated that he was a Copernican
(believer in the theories of
Copernicus). However, no public sign of this belief
was to appear until many years later.
At Padua, Galileo began a long
term relationship with Maria Gamba, who was from Venice, but they
did not marry perhaps because Galileo felt his financial situation
was not good enough. In 1600 their first child Virginia was born,
followed by a second daughter Livia in the following year. In 1606
their son Vincenzo was born.
We mentioned above an error in
Galileo's theory of motion as he set it out in De Motu around
1590. He was quite mistaken in his belief that the force acting on a
body was the relative difference between its specific gravity and
that of the substance through which it moved. Galileo wrote to his
friend Paolo Sarpi, a fine mathematician who was consultor to the
Venetian government, in 1604 and it is clear from his letter that by
this time he had realised his mistake. In fact he had returned to
work on the theory of motion in 1602 and over the following two
years, through his study of inclined planes and the pendulum, he had
formulated the correct law of falling bodies and had worked out that
a projectile follows a parabolic path. However, these famous results
would not be published for another 35 years.
In May 1609, Galileo received a
letter from Paolo Sarpi telling him about a spyglass that
a Dutchman had shown in Venice. Galileo wrote in the Sidereus
Nuncius (Starry
Messenger) in April 1610:-
About ten months ago a report
reached my ears that a certain Fleming had constructed a spyglass
by means of which visible objects, though very distant from the
eye of the observer, were distinctly seen as if nearby. Of this
truly remarkable effect several experiences were related, to which
some persons believed while other denied them. A few days later
the report was confirmed by a letter I received from a Frenchman
in Paris, Jacques Badovere, which caused me to apply myself
wholeheartedly to investigate means by which I might arrive at the
invention of a similar instrument. This I did soon afterwards, my
basis being the doctrine of refraction.
From these reports, and using his
own technical skills as a mathematician and as a craftsman,
Galileo began to make a series of telescopes whose optical
performance was much better than that of the Dutch instrument.
His first telescope was made from available lenses and gave
a magnification of about four times. To improve on this
Galileo learned how to grind and polish his own lenses and
by August 1609 he had an instrument with a magnification
of around eight or nine. Galileo immediately saw the commercial
and military applications of his telescope (which he called
a perspicillum) for ships at sea. He kept Sarpi informed
of his progress and Sarpi arranged a demonstration for the
Venetian Senate. They were very impressed and, in return
for a large increase in his salary, Galileo gave the sole
rights for the manufacture of telescopes to the Venetian
Senate. It seems a particularly good move on his part since
he must have known that such rights were meaningless, particularly
since he always acknowledged that the telescope was not
his invention!
By the end of 1609 Galileo had
turned his telescope on the night sky and began to make remarkable
discoveries. Swerdlow writes (see [16]):-
In about two months, December
and January, he made more discoveries that changed the world than
anyone has ever made before or since.
The astronomical discoveries he
made with his telescopes were described in a short book
called the Sidereus
Nuncious published in Venice in May 1610. This work
caused a sensation. Galileo claimed to have seen mountains
on the Moon, to have proved the
Milky
Way was made up of tiny stars, and to have seen
four small bodies orbiting Jupiter. These last, with an
eye to getting a position in Florence, he quickly named
'the Medicean stars'. He had also sent Cosimo de Medici,
the Grand Duke of Tuscany, an excellent telescope for himself.
The Venetian Senate, perhaps
realising that the rights to manufacture telescopes that Galileo had
given them were worthless, froze his salary. However he had
succeeded in impressing Cosimo and, in June 1610, only a month after
his famous little book was published, Galileo resigned his post at
Padua and became Chief Mathematician at the University of Pisa (without
any teaching duties) and 'Mathematician and Philosopher' to the
Grand Duke of Tuscany. In 1611 he visited Rome where he was treated
as a leading celebrity; the Collegio Romano put on a grand dinner
with speeches to honour Galileo's remarkable discoveries. He was
also made a member of the
Accademia dei Lincei (in fact the
sixth member) and this was an honour which was especially important
to Galileo who signed himself 'Galileo Galilei Linceo' from this
time on.
While in Rome, and after his return
to Florence, Galileo continued to make observations with
his telescope. Already in the Sidereus
Nuncious he had given rough periods of the four
moons of Jupiter, but more precise calculations were certainly
not easy since it was difficult to identify from an observation
which moon was I, which was II, which III, and which IV.
He made a long series of observations and was able to give
accurate periods by 1612. At one stage in the calculations
he became very puzzled since the data he had recorded seemed
inconsistent, but he had forgotten to take into account
the motion of the Earth round the sun.
Galileo first turned his telescope
on Saturn on 25 July 1610 and it appeared as three bodies (his
telescope was not good enough to show the rings but made them appear
as lobes on either side of the planet). Continued observations were
puzzling indeed to Galileo as the bodies on either side of Saturn
vanished when the ring system was edge on. Also in 1610 he
discovered that, when seen in the telescope, the planet Venus showed
phases like those of the Moon, and therefore must orbit the Sun not
the Earth. This did not enable one to decide between the Copernican
system, in which everything goes round the Sun, and that proposed by
Tycho
Brahe in which everything but the Earth (and Moon) goes round
the Sun which in turn goes round the Earth. Most astronomers of the
time in fact favoured
Brahe's system and indeed distinguishing between the two by
experiment was beyond the instruments of the day. However, Galileo
knew that all his discoveries were evidence for Copernicanism,
although not a proof. In fact it was his theory of falling bodies
which was the most significant in this respect, for opponents of a
moving Earth argued that if the Earth rotated and a body was dropped
from a tower it should fall behind the tower as the Earth rotated
while it fell. Since this was not observed in practice this was
taken as strong evidence that the Earth was stationary. However
Galileo already knew that a body would fall in the observed manner
on a rotating Earth.
Other observations made by Galileo
included the observation of sunspots. He reported these in
Discourse on floating bodies which he published in 1612 and more
fully in Letters on the sunspots which appeared in 1613. In
the following year his two daughters entered the Franciscan Convent
of St Matthew outside Florence, Virginia taking the name Sister
Maria Celeste and Livia the name Sister Arcangela. Since they had
been born outside of marriage, Galileo believed that they themselves
should never marry. Although Galileo put forward many revolutionary
correct theories, he was not correct in all cases. In particular
when three comets appeared in 1618 he became involved in a
controversy regarding the nature of comets. He argued that they were
close to the Earth and caused by optical refraction. A serious
consequence of this unfortunate argument was that the Jesuits began
to see Galileo as a dangerous opponent.
Despite his private support for
Copernicanism, Galileo tried to avoid controversy by not making
public statements on the issue. However he was drawn into the
controversy through Castelli who had been appointed to the chair of
mathematics in Pisa in 1613. Castelli had been a student of
Galileo's and he was also a supporter of
Copernicus. At a meeting in the Medici palace in Florence in
December 1613 with the Grand Duke Cosimo II and his mother the Grand
Duchess Christina of Lorraine, Castelli was asked to explain the
apparent contradictions between the Copernican theory and Holy
Scripture. Castelli defended the Copernican position vigorously and
wrote to Galileo afterwards telling him how successful he had been
in putting the arguments. Galileo, less convinced that Castelli had
won the argument, wrote Letter to Castelli to him arguing
that the Bible had to be interpreted in the light of what science
had shown to be true. Galileo had several opponents in Florence and
they made sure that a copy of the Letter to Castelli was sent
to the Inquisition in Rome. However, after examining its contents
they found little to which they could object.
The Catholic Church's most
important figure at this time in dealing with interpretations of the
Holy Scripture was Cardinal Robert Bellarmine. He seems at this time
to have seen little reason for the Church to be concerned regarding
the Copernican theory. The point at issue was whether
Copernicus had simply put forward a mathematical theory which
enabled the calculation of the positions of the heavenly bodies to
be made more simply or whether he was proposing a physical reality.
At this time Bellarmine viewed the theory as an elegant mathematical
one which did not threaten the established Christian belief
regarding the structure of the universe.
In 1616 Galileo wrote the
Letter to the Grand Duchess which vigorously attacked the
followers of
Aristotle. In this work, which he addressed to the Grand Duchess
Christina of Lorraine, he argued strongly for a non-literal
interpretation of Holy Scripture when the literal interpretation
would contradict facts about the physical world proved by
mathematical science. In this Galileo stated quite clearly that for
him the Copernican theory is not just a mathematical calculating
tool, but is a physical reality:-
I hold that the Sun is
located at the centre of the revolutions of the heavenly orbs and
does not change place, and that the Earth rotates on itself and
moves around it. Moreover ... I confirm this view not only by
refuting
Ptolemy's and
Aristotle's arguments, but also by producing many for the
other side, especially some pertaining to physical effects whose
causes perhaps cannot be determined in any other way, and other
astronomical discoveries; these discoveries clearly confute the
Ptolemaic system, and they agree admirably with this other
position and confirm it.
Pope Paul V ordered Bellarmine to
have the Sacred Congregation of the Index decide on the Copernican
theory. The cardinals of the Inquisition met on 24 February 1616 and
took evidence from theological experts. They condemned the teachings
of
Copernicus, and Bellarmine conveyed their decision to Galileo
who had not been personally involved in the trial. Galileo was
forbidden to hold Copernican views but later events made him less
concerned about this decision of the Inquisition. Most importantly
Maffeo Barberini, who was an admirer of Galileo, was elected as Pope
Urban VIII. This happened just as Galileo's book Il saggiatore
(The Assayer) was about to be published by the
Accademia dei Lincei in 1623 and
Galileo was quick to dedicate this work to the new Pope. The work
described Galileo's new scientific method and contains a famous
quote regarding mathematics:-
Philosophy is written in this
grand book, the universe, which stands continually open to our
gaze. But the book cannot be understood unless one first learns to
comprehend the language and read the characters in which it is
written. It is written in the language of mathematics, and its
characters are triangles, circles, and other geometric figures
without which it is humanly impossible to understand a single word
of it; without these one is wandering in a dark labyrinth.
Pope Urban VIII invited Galileo to
papal audiences on six occasions and led Galileo to believe that the
Catholic Church would not make an issue of the Copernican theory.
Galileo, therefore, decided to publish his views believing that he
could do so without serious consequences from the Church. However by
this stage in his life Galileo's health was poor with frequent bouts
of severe illness and so even though he began to write his famous
Dialogue in 1624 it took him six years to complete the work.
Galileo attempted to obtain
permission from Rome to publish the Dialogue in 1630 but this
did not prove easy. Eventually he received permission from Florence,
and not Rome. In February 1632 Galileo published Dialogue
Concerning the Two Chief Systems of the World - Ptolemaic and
Copernican. It takes the form of a dialogue between Salviati,
who argues for the Copernican system, and Simplicio who is an
Aristotelian philosopher. The climax of the book is an argument by
Salviati that the Earth moves which was based on Galileo's theory of
the tides. Galileo's theory of the tides was entirely false despite
being postulated after
Kepler had already put forward the correct explanation. It was
unfortunate, given the remarkable truths the Dialogue
supported, that the argument which Galileo thought to give the
strongest proof of
Copernicus's theory should be incorrect.
Shortly after publication of
Dialogue Concerning the Two Chief Systems of the World - Ptolemaic
and Copernican the Inquisition banned its sale and ordered
Galileo to appear in Rome before them. Illness prevented him from
travelling to Rome until 1633. Galileo's accusation at the trial
which followed was that he had breached the conditions laid down by
the Inquisition in 1616. However a different version of this
decision was produced at the trial rather than the one Galileo had
been given at the time. The truth of the Copernican theory was not
an issue therefore; it was taken as a fact at the trial that this
theory was false. This was logical, of course, since the judgement
of 1616 had declared it totally false.
Found guilty, Galileo was
condemned to lifelong imprisonment, but the sentence was carried out
somewhat sympathetically and it amounted to house arrest rather than
a prison sentence. He was able to live first with the Archbishop of
Siena, then later to return to his home in Arcetri, near Florence,
but had to spend the rest of his life watched over by officers from
the Inquisition. In 1634 he suffered a severe blow when his daughter
Virginia, Sister Maria Celeste, died. She had been a great support
to her father through his illnesses and Galileo was shattered and
could not work for many months. When he did manage to restart work,
he began to write Discourses and mathematical demonstrations
concerning the two new sciences.
After Galileo had completed work
on the Discourses it was smuggled out of Italy, and taken to
Leyden in Holland where it was published. It was his most rigorous
mathematical work which treated problems on impetus, moments, and
centres of gravity. Much of this work went back to the unpublished
ideas in De Motu from around 1590 and the improvements which
he had worked out during 1602-1604. In the Discourses he
developed his ideas of the inclined plane writing:-
I assume that the speed
acquired by the same movable object over different inclinations of
the plane are equal whenever the heights of those planes are equal.
He then described an experiment
using a pendulum to verify his property of inclined planes and used
these ideas to give a theorem on acceleration of bodies in free fall:-
The time in which a certain
distance is traversed by an object moving under uniform
acceleration from rest is equal to the time in which the same
distance would be traversed by the same movable object moving at a
uniform speed of one half the maximum and final speed of the
previous uniformly accelerated motion.
After giving further results of
this type he gives his famous result that the distance that a body
moves from rest under uniform acceleration is proportional to the
square of the time taken.
One would expect that Galileo's
understanding of the pendulum, which he had since he was a young man,
would have led him to design a pendulum clock. In fact he only seems
to have thought of this possibility near the end of his life and
around 1640 he did design the first pendulum clock. Galileo died in
early 1642 but the significance of his clock design was certainly
realised by his son Vincenzo who tried to make a clock to Galileo's
plan, but failed.
It was a sad end for so great a
man to die condemned of heresy. His will indicated that he wished to
be buried beside his father in the family tomb in the Basilica of
Santa Croce but his relatives feared, quite rightly, that this would
provoke opposition from the Church. His body was concealed and only
placed in a fine tomb in the church in 1737 by the civil authorities
against the wishes of many in the Church. On 31 October 1992, 350
years after Galileo's death, Pope John Paul II gave an address on
behalf of the Catholic Church in which he admitted that errors had
been made by the theological advisors in the case of Galileo. He
declared the Galileo case closed, but he did not admit that the
Church was wrong to convict Galileo on a charge of heresy because of
his belief that the Earth rotates round the sun.
In fieri.
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