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Routledge History of Philosophy Volume IV

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112 SCIENCE AND MATHEMATICS UP TO DESCARTES<br />

in that language rather than the mutually accessible Latin, and the result <strong>of</strong><br />

Galileo’s side <strong>of</strong> the exchange was published in 1613 as Istoria e Dimostrazioni<br />

intorno allé Macchie Solari.<br />

Besides a rather fruitless dispute about priority, the authors disagreed about<br />

the nature <strong>of</strong> sunspots, with Galileo favouring the view that they were like clouds<br />

around the Sun, thus emphasizing the theme <strong>of</strong> mutability <strong>of</strong> the heavens. But<br />

other matters were discussed, the most important <strong>of</strong> which was undoubtedly the<br />

phases <strong>of</strong> Venus. It is a notable consequence <strong>of</strong> Ptolemaic theory that the two<br />

inner planets, Mercury and Venus, never deviate far from the Sun in celestial<br />

longitude—hence the position <strong>of</strong> Venus as both morning and evening star. Also,<br />

it was almost universally held that they were nearer to us than the Sun. There<br />

accordingly arose the question <strong>of</strong> how they received the light to make them<br />

visible, for on the common assumption that this came from the Sun they would<br />

be almost entirely illuminated from behind, and at most we should see a small<br />

sliver. One opinion had it that they were possessed <strong>of</strong> their own light and another<br />

that they were translucent, but basically the problem remained unresolved, or, to<br />

use T.S.Kuhn’s phraseology, was an anomaly within the Ptolemaic paradigm. On<br />

the Copernican hypothesis the predictions were different, for, if these planets<br />

were orbiting the Sun, they should display phases in the manner <strong>of</strong> the Moon.<br />

And this is what Galileo observed in the case <strong>of</strong> Venus, and triumphantly<br />

reported in the Letters on Sunspots.<br />

These things leave no room for doubt about the orbit <strong>of</strong> Venus. With<br />

absolute necessity we shall conclude, in agreement with the theories <strong>of</strong> the<br />

Pythagoreans and <strong>of</strong> Copernicus, that Venus revolves about the Sun just as<br />

do all the other planets. 29<br />

So far so good, but what Galileo fails to mention, and what remained a thorn in his<br />

flesh, was that these observations were also perfectly compatible with the<br />

Tychonic system <strong>of</strong> the world, which, as mentioned above, soon became a<br />

favourite with Jesuit astronomers.<br />

Until the 1610s the Copernican system had aroused little religious discussion,<br />

apart from a few casual references to scriptural passages that seemed to<br />

contradict it, such as the command to the Sun to stand still over Gibeon in order<br />

to lengthen the day, so that Joshua could have time to finish a battle. With the<br />

new popularity that Galileo had brought to the issue, the religious implications<br />

became <strong>of</strong> major concern, and opposition to the system was probably egged on<br />

by mere conservatism masquerading as high principle. Galileo was himself<br />

drawn into the controversy, and wrote a long letter on the relation <strong>of</strong><br />

Copernicanism to the Scriptures. This closely reasoned piece made relatively<br />

liberal use <strong>of</strong> the principle <strong>of</strong> accommodation in biblical interpretation. The Bible<br />

was addressed to ignorant people, and appealed to the common understanding <strong>of</strong><br />

the time; it was not intended as a textbook in astronomy. In the epigram <strong>of</strong> one<br />

Cardinal Baronius, which Galileo gleefully quoted, ‘The intention <strong>of</strong> the Holy

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