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    35
    Western civilization. It was a gift of the civilization whose cen-
    ter was the Catholic Church.
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    Chapter Five
    The Church and Science
    as it just a coincidence that modern science devel-
    oped in a largely Catholic milieu, or was there some-
    Wthing about Catholicism itself that enabled the
    success of science? Even to raise the question is to transgress the
    boundaries of fashionable opinion. Yet more and more scholars
    have begun to ask it, and their answers may come as a surprise.
    This is no small matter. The Catholic Church s alleged hostil-
    ity toward science may be her greatest debit in the popular mind.
    The one-sided version of the Galileo affair with which most peo-
    ple are familiar is very largely to blame for the widespread belief
    that the Church has obstructed the advance of scientific inquiry.
    But even if the Galileo incident had been every bit as bad as peo-
    ple think it was, John Henry Cardinal Newman, the celebrated
    nineteenth-century convert from Anglicanism, found it reveal-
    ing that this is practically the only example that ever comes to
    mind.
    The controversy centered around the work of Polish
    astronomer Nicholas Copernicus (1473 1543). Some modern
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    68 How the Catholic Church Built Western Civilization
    treatments of Copernicus have gone so far as to call him a priest,
    but although he was named a canon of the chapter of Frauenburg
    in the late 1490s, there is no direct evidence that he ever took
    higher orders. One indication that he may have received priestly
    ordination comes from the decision of Poland s King Sigismund
    in 1537 to name him one of four possible candidates to a vacant
    episcopal seat. Whatever his clerical status, Copernicus had come
    from a religious family, all of whom belonged to the Third Order
    of Saint Dominic, which extended to the laity the opportunity to
    1
    partake in Dominican spirituality and tradition.
    As a scientist, he was a figure of no small renown in ecclesias-
    tical circles. He was consulted by the Fifth Lateran Council
    (1512 1517) on the subject of calendar reform. In 1531, Coper-
    nicus prepared an outline of his astronomy for the benefit of his
    friends. It attracted considerable attention; Pope Clement VII
    even called on Johann Albert Widmanstadt to deliver a public
    lecture at the Vatican on the subject. The pope left very favorably
    2
    impressed by what he had heard.
    Meanwhile, churchmen and academic colleagues alike
    implored Copernicus to publish his work for general circulation.
    Thus at the urging of friends, including several prelates, Coperni-
    cus finally relented and published Six Books on the Revolutions
    of the Celestial Orbits, which he dedicated to Pope Paul III, in
    1543. Copernicus retained much of the conventional astronomy
    of his day, which was overwhelmingly indebted to Aristotle and
    above all to Ptolemy (87 150 A.D.), a brilliant Greek astronomer
    who posited a geocentric universe. Copernican astronomy shared
    with its Greek precursors such features as perfectly spherical
    heavenly bodies, circular orbits, and constant planetary speed.
    The significant difference that Copernicus introduced was that
    he placed the sun, rather than Earth, at the center of the system.
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    THE CHURCH AND SCIENCE 69
    This heliocentric model posited a moving Earth orbiting the sun
    just as the other planets did.
    Although viciously attacked by Protestants for its alleged
    opposition to Holy Scripture, the Copernican system was subject
    to no formal Catholic censure until the Galileo case. Galileo
    Galilei (1564 1642), in addition to his work in physics, made
    some important astronomical observations with his telescope that
    helped to undermine aspects of the Ptolemaic system. He saw
    mountains on the moon, thus undermining the ancient certainty
    that the heavenly bodies were perfect spheres. He discovered four
    moons orbiting Jupiter, demonstrating not only the presence of
    celestial phenomena of which Ptolemy and the ancients had been
    unaware, but also that a planet moving in its orbit would not leave
    its smaller satellites behind. (One of the arguments against the
    motion of the Earth had been that the moon would be left behind.)
    Galileo s discovery of the phases of Venus was yet another piece of
    evidence in favor of the Copernican system.
    Initially, Galileo and his work were welcomed and celebrated
    by prominent churchmen. In late 1610, Father Christopher
    Clavius wrote to tell Galileo that his fellow Jesuit astronomers
    had confirmed the discoveries he had made through his tele-
    scope. When Galileo went to Rome the following year he was
    greeted with enthusiasm by religious and secular figures alike.
    He wrote to a friend,  I have been received and shown favor by
    many illustrious cardinals, prelates, and princes of this city. He
    enjoyed a long audience with Pope Paul V, and the Jesuits of the
    Roman College held a day of activities in honor of his achieve-
    ments. Galileo was delighted: Before an audience of cardinals,
    scholars, and secular leaders, students of Father Christopher
    Grienberger and Father Clavius spoke about the great
    astronomer s discoveries.
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    70 How the Catholic Church Built Western Civilization
    These were scholars of considerable distinction. Father Grien-
    berger, who personally verified Galileo s discovery of Jupiter s
    moons, was an accomplished astronomer who had invented the
    equatorial mount, which rotated a telescope about an axis paral-
    lel to Earth s. He also contributed to the development of the
    3
    refracting telescope in use today.
    Father Clavius, one of the great mathematicians of his day, had
    headed the commission that yielded the Gregorian calendar
    (which went into effect in 1582), which resolved the inaccuracies
    that had plagued the old Julian calendar. His calculations regard-
    ing the length of the solar year and the number of days necessary
    to keep the calendar in line with the solar year ninety-seven leap
    days every four hundred years, he explained were so precise that
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