伽利略指出,“只要下落的介质产生的阻力微不足道,或者在限定的真空条件下落下,落体将以均匀加速度下落。”[168]他也推导出均匀加速度正确的运动学规律,也就是说与所经历时间的平方成比例(d ∝ t2)。[169]在伽利略之前,尼科尔·奥雷姆[170]与14世纪推导出匀加速改变的时间平方规则,[171]多明戈·德索托(Domingo de Soto)于16世纪提出,“落体在均匀介质中将匀加速下落。”[172]通过几何结构和精确的数学语言,伽利略依据他所处时代的标准表达了时间平方规则。(这就为其他人也使用代数术语重新表达了这一规则留下余地)。伽利略还总结道“除非对物体施加一个力,常常是摩擦力,否则物体将一直保持匀速运动。这驳斥了当时为人们所普遍公认的亚里士多德假说---除非对物体施加外力,否则运动的物体将“自然”减速并停下来。正如让·布里丹[173]所说的那样,早在亚里斯多德提出这一假设几个世纪之前,约翰·菲洛波努斯[174]就已提出了有关惯性的哲学思想。据乔瑟芬·李约瑟[175]所述,“在他们之前,墨子早在几个世纪之前已经提出这一观点。但是,这是首次使用数学表达这一观点,并经过实验验证,并引入摩擦力的概念,这是验证惯性中所取得的一次突破。”伽利略的惯性原理提到,“除非受到外力的作用,否则运动在水平面上的物体就会按照其原来的方向,保持匀速运动。后来,这一原理纳入了牛顿运动定律(牛顿第一运动定律)。
O'Connor, J. J.; Robertson, E. F. Galileo Galilei. The MacTutor History of Mathematics archive. 苏格兰圣安德鲁大学. [2007-07-24]. (原始内容存档于2009-10-06). 引文使用过时参数coauthors (帮助)
O'Connor, J. J.; Robertson, E. F. "Galileo Galilei". The MacTutor History of Mathematics archive. University of St Andrews, Scotland. Retrieved 2007-07-24.
Sobel(2000, p. 5)Chapter 1. Retrieved on 26 August 2007. "But because he never married Virginia's mother, he deemed the girl herself unmarriageable. Soon after her 13th birthday, he placed her at the Convent of San Matteo in Arcetri."
Pedersen, O.(24–27 May 1984). "Galileo's Religion". Proceedings of the Cracow Conference, The Galileo affair: A meeting of faith and science. Cracow: Dordrecht, D. Reidel Publishing Co.. pp. 75–102. Bibcode 1985gamf.conf...75P.
Panofsky, Erwin (1956). "Galileo as a Critic of the Arts: Aesthetic Attitude and Scientific Thought". Isis 47 (1): 3–15. doi:10.1086/348450. JSTOR 227542.
Rutkin, H. Darrel. "Galileo, Astrology, and the Scientific Revolution: Another Look". Program in History & Philosophy of Science & Technology, Stanford University. Retrieved 2007-04-15.
Einstein(1954, p.271). "Propositions arrived at by purely logical means are completely empty as regards reality. Because Galileo realised this, and particularly because he drummed it into the scientific world, he is the father of modern physics—indeed, of modern science altogether."
United Nations Educational, Scientific and Cultural Organization (11 August 2005). "Proclamation of 2009 as International year of Astronomy"(PDF). UNESCO. Retrieved 2008-06-10.
Kusukawa, Sachiko. "Starry Messenger: The Telescope". Department of History and Philosophy of Science of the University of Cambridge. Retrieved 2007-03-10.
Drake(1978, p. 494), Favaro(1896, 6:111). The pseudonym was a slightly imperfect anagram of Oratio Grasio Savonensis, a latinised version of his name and home town.
Brodrick(1965, c1964, p. 95)quoting Cardinal Bellarmine's letter to Foscarini, dated 12 April 1615. Translated from Favaro(1902, 12:171–172) (Italian).
See Langford(1966, pp. 133–134), and Seeger(1966, p. 30), for example. Drake(1978, p. 355)asserts that Simplicio's character is modelled on the Aristotelian philosophers, Lodovico delle Colombe and Cesare Cremonini, rather than Urban. He also considers that the demand for Galileo to include the Pope's argument in the Dialogue left him with no option but to put it in the mouth of Simplicio(Drake, 1953, p. 491). Even Arthur Koestler, who is generally quite harsh on Galileo in The Sleepwalkers (1959), after noting that Urban suspected Galileo of having intended Simplicio to be a caricature of him, says "this of course is untrue"(1959, p. 483).
Fantoli(2005, p. 139), Finocchiaro(1989, pp. 288–293). Finocchiaro's translation of the Inquisition's judgement against Galileo is available on-line. "Vehemently suspect of heresy" was a technical term of canon law and did not necessarily imply that the Inquisition considered the opinions giving rise to the verdict to be heretical. The same verdict would have been possible even if the opinions had been subject only to the less serious censure of "erroneous in faith"(Fantoli, 2005, p. 140; Heilbron, 2005, pp. 282–284).
Drake(1978, p. 356). The phrase "Eppur si muove" does appear, however, in a painting of the 1640s by the Spanish painter Bartolomé Esteban Murillo or an artist of his school. The painting depicts an imprisoned Galileo apparently pointing to a copy of the phrase written on the wall of his dungeon(Drake, 1978, p. 357).
William Shea, M. A. The Galileo Affair 2006. Available online William Shea (January 2006). "The Galileo Affair". Grupo de Investigación sobre Ciencia, Razón y Fe (CRYF). Unpublished work. Retrieved 12 September 2010.
In Sidereus Nuncius(Favaro,1892, 3:81(Latin)) Galileo stated that he had reached this conclusion on 11 January. Drake(1978, p. 152), however, after studying unpublished manuscript records of Galileo's observations, concluded that he did not do so until 15 January.
In the Capellan model only Mercury and Venus orbit the Sun, whilst in its extended version such as expounded by Riccioli, Mars also orbits the Sun, but the orbits of Jupiter and Saturn are centred on the Earth
In Kepler's Thomist 'inertial' variant of Aristotelian dynamics as opposed to Galileo's impetus dynamics variant all bodies universally have an inherent resistance to all motion and tendency to rest, which he dubbed 'inertia'. This notion of inertia was originally introduced by Averroes in the 12th century just for the celestial spheres in order to explain why they do not rotate with infinite speed on Aristotelian dynamics, as they should if they had no resistance to their movers. And in his Astronomia Nova celestial mechanics the inertia of the planets is overcome in their solar orbital motion by their being pushed around by the sunspecks of the rotating sun acting like the spokes of a rotating cartwheel. And more generally it predicted all but only planets with orbiting satellites, such as Jupiter for example, also rotate to push them around, whereas the Moon, for example, does not rotate, thus always presenting the same face to the Earth, because it has no satellites to push around. These seem to have been the first successful novel predictions of Thomist 'inertial' Aristotelian dynamics as well as of post-spherist celestial physics. In his 1630 Epitome(See p514 on p896 of the Encyclopædia Britannica 1952 Great Books of the Western World edition)Kepler keenly stressed he had proved the Sun's axial rotation from planetary motions in his Commentaries on Mars Ch 34 long before it was telescopically established by sunspot motion.
Drake(1978, p. 209). Sizzi reported the observations he and his companions had made over the course of a year to Orazio Morandi in a letter dated 10 April 1613(Favaro,1901, 11:491 (Italian)). Morandi subsequently forwarded a copy to Galileo.
In geostatic systems the apparent annual variation in the motion of sunspots could only be explained as the result of an implausibly complicated precession of the Sun's axis of rotation(Linton, 2004, p. 212; Sharratt, 1994, p. 166; Drake, 1970, pp. 191–196). This did not apply, however, to the modified version of Tycho's system introduced by his protegé, Longomontanus, in which the Earth was assumed to rotate. Longomontanus's system could account for the apparent motions of sunspots just as well as the Copernican.
Drake(1978, pp. 19,20). At the time when Viviani asserts that the experiment took place, Galileo had not yet formulated the final version of his law of free fall. He had, however, formulated an earlier version which predicted that bodies of the same material falling through the same medium would fall at the same speed(Drake, 1978, p. 20).
Groleau, Rick. "Galileo's Battle for the Heavens. July 2002". Ball, Phil (2005-06-30). "Science history: setting the record straight. 30 June 2005". The Hindu(Chennai, India).
Lucretius, De rerum natura II, 225–229; Relevant passage appears in: Lane Cooper, Aristotle, Galileo, and the Tower of Pisa(Ithaca, N.Y.: Cornell University Press, 1935), p. 49.
Simon Stevin, De Beghinselen des Waterwichts, Anvang der Waterwichtdaet, en de Anhang komen na de Beghinselen der Weeghconst en de Weeghdaet [The Elements of Hydrostatics, Preamble to the Practice of Hydrostatics, and Appendix to The Elements of the Statics and The Practice of Weighing](Leiden, Netherlands: Christoffel Plantijn, 1586)reports an experiment by Stevin and Jan Cornets de Groot in which they dropped lead balls from a church tower in Delft; relevant passage is translated in: E. J. Dijksterhuis, ed., The Principal Works of Simon Stevin Amsterdam, Netherlands: C. V. Swets & Zeitlinger, 1955 vol. 1, pp. 509, 511.
Clagett(1968, p. 561). Oresme, however, regarded this discovery as a purely intellectual exercise having no relevance to the description of any natural phenomena, and consequently failed to recognise any connection with the motion of falling bodies(Grant, 1996, p.103).
Sharratt(1994, p. 198), Wallace(2004, pp.II 384, II 400, III 272)Soto, however, did not anticipate many of the qualifications and refinements contained in Galileo's theory of falling bodies. He did not, for instance, recognise, as Galileo did, that a body would only fall with a strictly uniform acceleration in a vacuum, and that it would otherwise eventually reach a uniform terminal velocity.
Two of his non-scientific works, the letters to Castelli and the Grand Duchess Christina, were explicitly not allowed to be included(Coyne 2005, p. 347).
Heilbron(2005, p. 307); Coyne(2005, p. 347)The practical effect of the ban in its later years seems to have been that clergy could publish discussions of heliocentric physics with a formal disclaimer assuring its hypothetical character and their obedience to the church decrees against motion of the earth: see for example the commented edition (1742) of Newton's 'Principia' by Fathers Le Seur and Jacquier, which contains such a disclaimer('Declaratio')before the third book (Propositions 25 onwards) dealing with the lunar theory.
Discourse of His Holiness Pope Pius XII given on 3 December 1939 at the Solemn Audience granted to the Plenary Session of the Academy, Discourses of the Popes from Pius XI to John Paul II to the Pontifical Academy of the Sciences 1939–1986, Vatican City, p. 34
An earlier version had been delivered on 16 December 1989, in Rieti, and a later version in Madrid on 24 February 1990(Ratzinger, 1994, p. 81). According to Feyerabend himself, Ratzinger had also mentioned him "in support of" his own views in a speech in Parma around the same time(Feyerabend, 1995, p. 178).
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