Intellectual
Heritage
Galileo, The Starry Messenger, ed. Stillman Drake
STUDY GUIDE
This short essay changed
the way we look at the world, winning instant (and initially positive)
attention from the astronomers of the Roman College and other Church officials.
In this class, we will
concentrate on Galileo's discoveries. Please read from page 32 on
with special care. Please also consult the very useful short essay by
Professor Dieter Forster of Temple's Department of Physics, Galileo's Starry
Messenger.
This publication
inaugurated the series of events that culminated in the epochal
confrontation between Galileo and the Roman Catholic Church. Although his
discoveries were acknowleged, the way in which he presented them led to serious
criticism, since he openly insisted that he'd found not just a better theory
but better facts -- and these facts contradicted holy scripture, which placed
the earth at the center of the universe. (It was not only Catholics who
were upset: Martin Luther had condemned this sort of thinking in even
stronger terms.) Our task with this text is to focus on the particular
discoveries that Galileo's method and his equipment (the telescope, which he had not
"invented" but had constructed) made possible. In many ways,
Galileo was the first modern scientist: he insisted on acquiring detailed
knowledge of the phenomena under consideration, and, to some degree, he
worked empirically, moving from the "facts" to a
theory. (Or, so it seems: there is dispute about this.)
Title page (21)
Note the date: March
1610 , Galileo's first major publication at age 46. Leads to his appointment as
"Chief Mathematician and Philosopher" to the Medici court in Florence
& his visit to Rome, spring 1611, where he was welcomed by the scientific
academy, the pope, & the Jesuit Roman College, noted for its own famous
astronomers. "When the head of the College, the Lord Cardinal Bellarmine,
asked for their official opinion on the new discoveries, they unanimously
confirmed them": i.e. the initial response of the Church is positive.
(Koestler 4 -7, cf. Cohen 84) "The book became known throughout Europe
immediately, and made a special impression in England."
Dedication (23-26)
Written in the tradition
of ancient and renaissance prefaces. Nice illustration of attitudes to
kingship, and of use of analogy so common in Shakespeare. "Just as these
stars, like children worthy of their sire, never leave the side of Jupiter ...,
so ...clemency, kindness..., gentleness..., splendor..., nobility... have all
fixed their abode and habitation in Your Highness."
Galileo is addressing
one of the Medici family, prominent or dominant in Florence, Italy, from the
14th century. Machiavelli in The Prince also addresses a Medici
ruler. Both of these revolutionary thinkers sought governmental
protection and support: only Galileo got it, winning a very well-paying
professorship for the publication of this book.
Introductory comments (27-30)
How many achievements
does G. catalogue here? What are they?
The Telescope (30-31)
You
needn't master the details of this section.
Surface of moon (32-45)
This section is very
important, because it reveals how much Galileo's telescope permitted him to
see. Copernicus in 1542 had suggested that the sun was the center of the
solar system--as a theory, at least. Kepler, Galileo's near-contemporary,
had also come to this theory. Galileo was the first to provide hard new
data that the universe was not as everyone had thought. Revealing that
the moon had peaks and valleys was an important start.
Large vs. smaller spots.
Attack on "philosophers": who are these? Spots signify mountains
& valleys. Darker region = water. Large spots. Explanations of the
smoothness of the moon's edges. Greater number of irregularities on lunar
sutface than on earth's.
Estimated height of
lunar mountains. "It is characteristic cf Galileo as a scientist of the
modern school that as soon as he found any kind of phenomenon he wanted to
measure it." (Cohen 73)
Cohen 74 remarks that
Dante, writing in the 14th century, described the moon as an "eternal
pearl . . . a perfect entity without blemish," the marks on which are not
really there, despite the testimony of the senses and "reason." Be
prepared to comment on the difference between Dante and Galileo as revealed by
this passage.
Secondary light of moon
(42-45): "earthshine" (Cohen 75-6); Gegenschein in German
physics. Can you explain this in your own words? Now, note that the
planets, too, including the moon, "shine." What conclusions can you
draw from this?
Fixed Stars (45-50)
Telescope fails to enlarge
these much, since it reduces their radiance.
Stars differ in form
from planets, which "look like little Moons" 154, see Toulmin 192f.,
Cohen 76-78). And more stars exist than we'd thought. Fainter stars likely mre
distant, though there is as yet no noticeable parallax. (Toulmin 194).
Discussion of Orion 155-156), etc.: many new stars.
Medicean stars 50-58
"The last of G's
observations was the most exciting" (Toulmin 194-6): 4 largest satellites
of Jupiter. "Most of [this] book is...devoted to...methodological
observations of Jupiter and the 'stars' near it." (Cohen 79) Is
"stars" the correct word to use? How did this discovery affect
people's understandinq of the heavens?
Cohen 80 remarks that
"Galileo,...could not explain why ... Jupiter could move in its orbit
without losing its four encircling companions, any more than...how the earth
could move through space and not lose its one encircling moon." It
is worthwhile to ask why Galileo would have trouble with these questions.
Cohen, 83 summarizes
three other discoveries made by Galileo with his telescope that don't appear in
Starry Messenger: 1) the phases of Venus (proof that Venus shines only
by reflected light), and Venus' orbit around the sun & varying distance
from earth; 2) rings or "ears" of Saturn; 3) sunspots, which show
that sun is not perfect, and that it rotates at a known speed.
Words worth knowing:
parallax
References:
Koestler = Arthur
Koestler, The Sleepwalkers (N.Y.: MacMillan, 1959); Cohen = I. Bernard
Cohen, The Birth of a New Physics (Garden City, N.Y.: Doubleday, 1960);
Butterfield = Herbert Butterfield, The Origins of Modern Science 1300-1800,
rev. ed. N.Y.: The Free Press, 1957); Drake = Stillman Drake, Galileo at
Work. A Scientific Biography (Chicago: Chicago UP, 1978); Morphet = Clive
Morphet, Galileo and Copernican Astronomy: A Scientific World View Defined
(London: Butterworths, 1977); Kuhn = Thomas S. Kuhn, The Copernican
Revolution (Cambridge: Harvard UP, 1957); Toulmin= Stephen Toulmin and June
Goodfield, The Fabric of the Heavens (N.Y.: Harper, 1961)
Useful web pages:
http://csep10.phys.utk.edu/astr161/lect/history/galileo.html