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  4. <TITLE>Galileo -- Reading Revolutions -- Intellectual History</TITLE>
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  18. <font face="Verdana,Arial,Helvetica" size="-1"><b><a href="lectures.html">INDEX</a></b><br><br><font size="+1"><center><i>Reading Revolutions: Intellectual History</i><br><br>
  19. What We Have Here is a Failure to Communicate: Galileo and
  20. the Church<br><br><font size="+0">Christopher Magri</font></center>
  21. &nbsp;<p><font face="Verdana,Arial,Helvetica" size="-1">
  22. The following is a summary of a lecture given by Chris Magri based on his slides.</font></p>
  23. <p align="center">
  24. <img border="0" src="pictures/Galileo/S1.jpg" title="Galileo" width="450" height="337"></p>
  25. <font face="Verdana,Arial,Helvetica" size="-1">
  26. <p>As the story goes, Copernicus proposed a heliocentric solar system in <i>
  27. De Revolutionibus Orbium Coelestium</i>&nbsp; which was published after his
  28. death.&nbsp; The Church is outraged and threatened by the new science.&nbsp;
  29. Galileo is persecuted for defending the Copernican model, defiantly
  30. publishes <i>Dialogue on the Two Chief World Systems</i> and ends his life
  31. under house arrest.&nbsp; The history is more complicated and much more
  32. ambiguous.</p>
  33. <p>In the 1500's the understanding of the heavens were based on the writings
  34. of Aristotle and the model created by Ptolemy in the second century.&nbsp;
  35. Using observations of gravity and motion, the Aristotelian model proposes a
  36. geocentric universe.&nbsp; </p>
  37. <p align="center">
  38. <img border="0" src="pictures/Galileo/DSC00090.jpg" width="450" height="338"></p>
  39. <p align="left">The model fits most observations.&nbsp; Without modern
  40. measurement it is difficult to prove otherwise.&nbsp; It also fits nicely
  41. with personal egocentrism and the theology of the Church.&nbsp; There are
  42. anomalies.&nbsp; </p>
  43. <p align="center"><font face="Verdana,Arial,Helvetica" size="-1">
  44. <img border="0" src="pictures/Galileo/S3.jpg" width="450" height="340"></p>
  45. <p>The predictable but rather arbitrary motion of the planet Mars is
  46. illustrated by a chart created by Chris Magri.&nbsp; Of course, it is only
  47. arbitrary if you assume Mars is revolving around the earth.</p>
  48. <p align="center">
  49. <img border="0" src="pictures/Galileo/S4.jpg" title="Galileo" width="450" height="339"></p>
  50. </font>
  51. <p>Ptolemy explained the phenomenon of retrograde motion by proposing
  52. epicycles.</p>
  53. <p align="center">
  54. <img border="0" src="pictures/Galileo/S5.jpg" width="450" height="340"></p>
  55. <p>In addition, the earth would be off-center in relation to the path to
  56. account for changes in distance.</p>
  57. <div align="center">
  58. <table border="0" width="50%" id="table2">
  59. <tr>
  60. <td>
  61. <p align="center">
  62. <font size="+1" face="Verdana,Arial,Helvetica">
  63. <img border="0" src="pictures/Galileo/PTOLEMY2.jpg" width="450" height="353"></td>
  64. </tr>
  65. </table>
  66. </div>
  67. <p>Over time, the epicycle would be displaced.</p>
  68. <div align="center">
  69. <table border="0" width="50%" id="table3">
  70. <tr>
  71. <td>
  72. <p align="center">
  73. <font size="-1" face="Verdana,Arial,Helvetica">
  74. <img border="0" src="pictures/Galileo/PTOLEMY3.jpg" title="Ptolemy's System"width="450" height="356"></font></p>
  75. <p align="center"><font size="-2"><i>Anonymous author.&nbsp; See
  76. model in motion at:</i></font><font size="-2"><br>
  77. <a target="_blank" href="http://webpages.charter.net/middents/Ptolemy's%20Model.htm">
  78. http://webpages.charter.net/middents/Ptolemy's Model.htm</a></font></td>
  79. </tr>
  80. </table>
  81. </div>
  82. <p>When you add in the other four planets, you have what appear to be
  83. spinning rings on orbits.&nbsp; You can see the effect in this computer
  84. model from Paul Stoddard.&nbsp; Click on the link below, choose months, and
  85. change the speed on the slider in the upper right hand corner to observe
  86. both what we see from earth and what the motion would look like if seen from
  87. above.</p>
  88. <div align="center">
  89. <table border="0" width="50%" id="table1" cellpadding="7">
  90. <tr>
  91. <td>
  92. <p align="center">
  93. <font size="+1" face="Verdana,Arial,Helvetica">
  94. <img border="0" src="pictures/Galileo/PTOLEMYM.jpg" width="500" height="542"></font><i><font size="-2">
  95. <br>By permission of Paul Stoddard:&nbsp; See model in motion at<br>
  96. </font></i><font size="-2">
  97. <a class="fixed" target="_blank" href="https://mail1.maine.edu/horde-3.0.4/services/go.php?url=http://jove.geol.niu.edu/faculty/stoddard/JAVA/ptolemy.html">
  98. http://jove.geol.niu.edu/faculty/stoddard/JAVA/ptolemy.html </a>
  99. </font></td>
  100. </tr>
  101. </table>
  102. </div>
  103. <p align="center">
  104. <img border="0" src="pictures/Galileo/S6.jpg" width="450" height="339"></p>
  105. <p>When Copernicus proposed that the sun is central he did not simplify the
  106. mathematics.&nbsp; The model still requires epicycles.</p>
  107. <p align="center">
  108. <img border="0" src="pictures/Galileo/S7.jpg" width="450" height="339"></p>
  109. <p>Notice that the orbits are perfect circles.&nbsp; Copernicus felt that
  110. this was consistent with the ideal of harmony in the universe but it made
  111. his model difficult to describe.</p>
  112. <div align="center">
  113. <table border="0" width="50%" id="table4" cellspacing="0">
  114. <tr>
  115. <td>
  116. <p align="center">
  117. <font size="-1" face="Verdana,Arial,Helvetica">
  118. <img border="0" src="pictures/Galileo/COPERNIC.jpg" width="500" height="570"><i><font size="-2">
  119. <br>By permission of Paul Stoddard:&nbsp; See model in motion at
  120. </font></i><br>
  121. <font size="-2">
  122. <a class="fixed" target="_blank" href="https://mail1.maine.edu/horde-3.0.4/services/go.php?url=http://jove.geol.niu.edu/faculty/stoddard/JAVA/ptolemy.html">
  123. http://jove.geol.niu.edu/faculty/stoddard/JAVA/ptolemy.html </a>
  124. </font></td>
  125. </tr>
  126. </table>
  127. </div>
  128. <p>&nbsp;</p>
  129. <p align="center">
  130. <img border="0" src="pictures/Galileo/S8.jpg" width="450" height="342"></p>
  131. <font face="Verdana,Arial,Helvetica" size="-1">
  132. <p>For the Church, the main purpose of astronomy was to predict the position
  133. of the planets and thus set the time for the moveable feast days.&nbsp;
  134. Thus, the forward suggests that the Copernican model may be a convenient
  135. fiction, acceptable if it works.&nbsp; (Take a look at the
  136. <a target="_blank" href="http://en.wikipedia.org/wiki/Computus">calculations
  137. for Easter</a>).</p></font>
  138. <p><font face="Verdana,Arial,Helvetica" size="-1">
  139. Copernicus did not make many observations of his own, instead he relied on
  140. the observations of the ancients and his interpretation of Plato.&nbsp;
  141. Tycho Brahe, on the other hand, spent his life making extensive and exacting
  142. observations of planetary, solar, and stellar positions.</font></p>
  143. <p align="center">
  144. <img border="0" src="pictures/Galileo/S9.jpg" width="450" height="339"></p>
  145. <p align="left"><font face="Verdana,Arial,Helvetica" size="-1">
  146. Brahe, concluded that the earth doesn't move because if it did, if you
  147. measured the stars when the earth was on one side of the sun and contrasted
  148. those measurements to measurements made when the earth moved to the other
  149. side of the sun, closer stars would change their position relative to
  150. farther stars.&nbsp; This is called stellar parallax.&nbsp;
  151. </font></p>
  152. <p align="left"><font face="Verdana,Arial,Helvetica" size="-1">
  153. It is similar to binocular parallax.&nbsp; Hold your finger out in front of
  154. you, close one eye and then the other and look at your finger.&nbsp; The
  155. finger moves in relation to the objects behind it because your eyes are
  156. inches apart.&nbsp; Brahe was unable to find any evidence that parallax
  157. occurred in any of his extensive records.&nbsp; While the distance between
  158. the positions of the earth are great, the stars are so far away that the
  159. parallax effect is extremely small.&nbsp; Measurements of stellar parallax
  160. were not successfully made until 1838 by Friedrich Bessel.</font></p>
  161. <div align="center">
  162. <table border="0" width="50%" id="table5" cellspacing="0">
  163. <tr>
  164. <td>
  165. <p align="center">
  166. <img border="0" src="pictures/Galileo/BRAHEM3.jpg" width="500" height="477"><font face="Verdana,Arial,Helvetica"><i><font size="-2">
  167. <br>
  168. By permission of Paul Stoddard:&nbsp; See model in motion at
  169. </font></i><br>
  170. <font size="-2">
  171. <a class="fixed" target="_blank" href="https://mail1.maine.edu/horde-3.0.4/services/go.php?url=http%3A%2F%2Fjove.geol.niu.edu%2Ffaculty%2Fstoddard%2FJAVA%2Fptolemy.html">
  172. http://jove.geol.niu.edu/faculty/stoddard/JAVA/ptolemy.html</a>
  173. </font></td>
  174. </tr>
  175. </table>
  176. </div>
  177. <p>Galileo ignored Brahe's model and chose to support Copernicus.</p>
  178. <p align="center">
  179. <img border="0" src="pictures/Galileo/S10.jpg" width="450" height="340"></p>
  180. </font>
  181. <p><font face="Verdana,Arial,Helvetica" size="-1">Galileo
  182. was not the only scientist in the 1600's.&nbsp; There was a network of
  183. individuals across Europe who both corresponded and shared publications.&nbsp;
  184. Galileo was one of the first to use the telescope and in 1611 used one to
  185. show sunspots to a
  186. number of people in Rome.&nbsp; In October of 1611, a
  187. Jesuit, Scheiner, began to make observations of sunspots and published his
  188. findings in January 1612.&nbsp; He interpreted the sunspots as small
  189. planetoids revolving around the sun.&nbsp;
  190. </font></p>
  191. <p align="center">
  192. <img border="0" src="pictures/Galileo/S11.jpg" width="450" height="339"></p>
  193. </font>
  194. <p>After that, Galileo began a serious study of sunspots and carried out a series of
  195. debates with Scheiner, a member of the Jesuit order, in published letters.&nbsp; Galileo challenged
  196. Scheiner's interpretation and provided measurements and observations to
  197. prove that the spots were blemishes on the sun and that they showed that the
  198. sun rotates.&nbsp; Scheiner lost the debate and in subsequent publications
  199. changed his interpretation to agree with Galileo.&nbsp; Years later, Galileo
  200. complained that other scientists were trying to claim primacy in the
  201. discovery of sunspots -- credit for which Galileo felt belonged to him.&nbsp; Scheiner assumed that Galileo was talking about him and was outraged.&nbsp;
  202. Galileo had a new enemy.&nbsp; </p>
  203. <p>He was able to go on to alienate <i>all</i> of the Jesuits when he
  204. scathingly called their intelligence and integrity into question over the
  205. nature of comets.&nbsp; Jesuit observers had proposed that comets were
  206. short-lived planetary objects in orbit while Galileo claimed they were
  207. vapors in the earth's atmosphere.&nbsp; Galileo could not limit himself to
  208. proof and observations but felt compelled to vilify anyone who disagreed
  209. with him.</p>
  210. <p>Galileo's more reasoned style can be read in his letter to the
  211. <a target="_blank" href="http://www.fordham.edu/halsall/mod/galileo-tuscany.html">Grand Duchess Cristina</a>
  212. expressing his views on the relationship between science and Biblical
  213. interpretation:</p>
  214. <p align="center">
  215. <img border="0" src="pictures/Galileo/S12.jpg" width="450" height="337"></p>
  216. <p>Galileo posits that the denial of the Copernican theory has more to do
  217. with Galileo's defense of Copernicus since the Copernican theory had been
  218. read and discussed without problem for over 50 years.&nbsp; He calls on the
  219. writings of St. Augustine to show that enquiry and reason can be brought to
  220. bear on biblical issues and that literalism can be used in both directions.</p>
  221. <p>Magri goes on to give illustrations of places where it is absurd to take
  222. the Bible literally, even without touching on scientific matters:</p>
  223. <p align="center">
  224. <img border="0" src="pictures/Galileo/S13.jpg" width="450" height="339"></p>
  225. <p>Opposition against Galileo and by extension, his theories, grows.&nbsp;
  226. It is not limited to people within the Church but is found among academics
  227. who have been insulted, threatened, or refuted by Galileo in various
  228. publications on a vast array of topics.&nbsp; Cardinal Bellarmine is sent to
  229. warn Galileo not to promote the Copernican model but to treat it as an
  230. hypothesis.&nbsp; Caution is the word.</p>
  231. <p align="center">
  232. <img border="0" src="pictures/Galileo/S14.jpg" width="450" height="339"></p>
  233. <p>Pope Urban VIII suggests that Galileo consider that God might have made
  234. the world one way but allowed us to see it in another way.&nbsp; Galileo
  235. gets permission to publish a work about Copernican theory as long as it is
  236. clearly treated as unproven.</p>
  237. <p align="center">
  238. <img border="0" src="pictures/Galileo/S15.jpg" width="450" height="339"></p>
  239. <p>The use of a conversation to explore different sides to an issue allows Galileo
  240. to seem even-handed. The personalities and arguments he assigns his
  241. characters are anything but unbiased, in fact, they strengthen the insults
  242. directed at Aristotelian and Ptolemaic astronomy.&nbsp; He is even able to
  243. include a passing insult directed toward Scheiner.&nbsp; </p>
  244. <p align="center">
  245. <img border="0" src="pictures/Galileo/S16.jpg" width="450" height="339"></p>
  246. <p><br></font>To answer
  247. <font face="Verdana,Arial,Helvetica" size="-1">Cardinal Bellarmine's demand
  248. for evidence, Galileo has Salviati argue in the Dialogue that the
  249. presence of ocean tides
  250. proves that the earth moves.&nbsp;
  251. </p>
  252. <p align="center">
  253. <img border="0" src="pictures/Galileo/dialogue36.jpg" width="450" height="396"></p>
  254. <p>Pope Urban VIII is not amused and probably feels betrayed.&nbsp; He turns from supporter to judge.&nbsp; He orders that the
  255. Inquisition investigate.&nbsp; Where he had admired and sought to counsel
  256. Galileo on handling his enemies, now he joined them in seeing Galileo as
  257. totally out of control and a threat.</p>
  258. <p align="center">
  259. <img border="0" src="pictures/Galileo/S18B.jpg" width="450" height="339"></p>
  260. <p>The Catholic church continued to produce great scientists and removed
  261. itself from the controversies over stellar configurations.&nbsp; It was even
  262. able to absorb Darwin's evolution.&nbsp; The same cannot be said of all.&nbsp;
  263. Some still fear that knowledge may undermine belief.&nbsp;&nbsp;
  264. </p>
  265. <p align="center">
  266. <img border="0" src="pictures/Galileo/S19.jpg" width="450" height="339"></p>
  267. <p>Now they want belief to be disguised as science rather than science
  268. subsumed under belief.&nbsp; It leads to:</p>
  269. <p align="center">
  270. <img border="0" src="pictures/Galileo/S20.jpg" width="450" height="338"></p>
  271. </font><font face="Verdana,Arial,Helvetica" size="-1">
  272. <p>and also to:</p>
  273. <p align="center">
  274. <img border="0" src="pictures/Galileo/galileo57.jpg" width="450" height="338"></p>
  275. <p align="center">&nbsp;</p>
  276. <p align="center"><font face="Verdana,Arial,Helvetica" size="-1">
  277. <img border="0" src="pictures/Galileo/S22.jpg" width="450" height="340"></font><br>
  278. </p>
  279. <p>Kepler published <i>Epitome Astronomiae</i> in 1621 in which he provided
  280. extensive mathematical proofs of the Copernican heliocentric solar system as
  281. modified by Kepler to include elliptical orbits.&nbsp; Kepler's work did not attract the same kind of hysterical opposition.&nbsp; Earlier, Kepler attempted to share his findings with Galileo, but Galileo
  282. was on his own road.&nbsp;
  283. </p>
  284. <p align="center">
  285. <img border="0" src="pictures/Galileo/S23.jpg" width="450" height="337"></p>
  286. <p>Galileo's response to critics and to colleagues alike played an important
  287. part in the polarization of emotion and politics.&nbsp; Had he been able to
  288. restrain himself to his more reasoned arguments he may have been able to
  289. maintain the support of those both in the Church and in academia who had
  290. once defended and admired him.</p>
  291. <p align="center">
  292. <img border="0" src="pictures/Galileo/S24.jpg" width="450" height="339"></p>
  293. <p>As Galileo ended his <i>Dialogue </i>with the words of Sagredo:</p>
  294. <p align="center">
  295. <img border="0" src="pictures/Galileo/S25.jpg" width="450" height="338"></p>
  296. <p>so we must end.</p>
  297. <hr width="40%"><hr width="60%"><br>
  298. &nbsp;<div align="center">
  299. <table border="0" width="100%" id="table6">
  300. <tr>
  301. <td><a href="pictures/Galileo/1206cclosewl.jpg">
  302. <img border="0" src="pictures/Galileo/1206ws.jpg" width="350" height="271"></a></td>
  303. <td>
  304. <font face="Verdana,Arial,Helvetica" size="-1">
  305. <a href="pictures/Galileo/1218wl.jpg">
  306. <img border="0" src="pictures/Galileo/1218ws.jpg" width="361" height="271" align="right"></a></td>
  307. </tr>
  308. </table>
  309. </div>
  310. <p><font face="Verdana,Arial,Helvetica" size="-1">The 1710 Florence edition
  311. of <i>Dialogo di Galileo Galilei linceo matematico supremo dello studio di
  312. padova</i></font><font face="Verdana,Arial,Helvetica">.&nbsp; </font></font>
  313. </font>
  314. <font face="Verdana,Arial,Helvetica" size="-1">Click either picture for an
  315. enlargement.</p>
  316. <p>An English translation of the work can be found at
  317. <a target="_blank" href="http://webexhibits.org/calendars/year-text-Galileo.html">
  318. http://webexhibits.org/calendars/year-text-Galileo.html</a>.</p><hr width="60%"><hr width="40%">
  319. <p></font><br>
  320. </p>
  321. <center><table border="6" cellpadding="0" cellspacing="0" style="border-collapse: collapse" width="80%" id="decorative" bgcolor="#cccccc">
  322. <tr>
  323. <td width="100%"><center><table border="6" cellpadding="0" cellspacing="0" style="border-collapse: collapse" width="100%" id="credits" bordercolor="#111111" bgcolor="#cccccc">
  324. <tr>
  325. <td width="100%"><blockquote><font face="Verdana,Arial,Helvetica" size="-1"><br>Citation:<br><br>"What We Have Here is a Failure to Communicate:&nbsp; Galileo and the Church."&nbsp; Summary of a lecture by Christopher Magri.&nbsp; University of Maine at Farmington, September 14, 2005.&nbsp; Retrieved _______. &nbsp;
  326. &lt;http://hua.umf.maine.edu/Reading_Revolutions/Galileo.html&gt;.
  327. <br><br>URL: <a href="http://hua.umf.maine.edu/Reading_Revolutions/index.html">http://hua.umf.maine.edu/Reading_Revolutions/index.html</a> <br><br>Marilyn Shea, 2005<br><br>
  328. </blockquote></td></tr></table></center>
  329. </td></tr></table></center>
  330. </td>
  331. <td width="110" background="wrightcenter.jpg" height="456">&nbsp;</td>
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