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Kepler's Philosophy and the New Astronomy

Princeton University Press (2000)

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  1. “To Measure by a Known Measure”: Kepler’s Geometrical Epistemology in the Harmonices Mundi Libri V.Domenica Romagni - 2024 - Hopos: The Journal of the International Society for the History of Philosophy of Science 14 (1):103-133.
    In this article, I address the epistemological role that geometry plays in Kepler’s Harmonices Mundi Libri V and argue that the framework he develops there is meant to address concerns regarding the confirmation of astronomical hypotheses, which are supported by comments in earlier works regarding empirical underdetermination. The geometrical epistemology that he constructs to combat these concerns in the Harmonices Mundi is introduced in Book I and then is extended to his theory of harmonic proportion in Book III, finally providing (...)
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  • Dynamic Oppositional Symmetries for Color, Jungian and Kantian Categories.Julio Michael Stern - manuscript
    This paper investigates some classical oppositional categories, like synthetic vs. analytic, posterior vs. prior, imagination vs. grammar, metaphor vs. hermeneutics, metaphysics vs. observation, innovation vs. routine, and image vs. sound, and the role they play in epistemology and philosophy of science. The epistemological framework of objective cognitive constructivism is of special interest in these investigations. Oppositional relations are formally represented using algebraic lattice structures like the cube and the hexagon of opposition, with applications in the contexts of modern color theory, (...)
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  • O método da astronomia segundo Kepler.Claudemir Roque Tossato & Pablo Rubén Mariconda - 2010 - Scientiae Studia 8 (3):339-366.
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  • Discussão cosmológica e renovação metodológica na carta de 9 de dezembro de 1599 de Brahe a Kepler.Claudemir Roque Tossato - 2004 - Scientiae Studia 2 (4):537-565.
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  • Early Numerical Analysis in Kepler's New Astronomy.Steinar Thorvaldsen - 2010 - Science in Context 23 (1):39-63.
    ArgumentJohannes Kepler published hisAstronomia novain 1609, based upon a huge amount of computations. The aim of this paper is to show that Kepler's new astronomy was grounded on methods from numerical analysis. In his research he applied and improved methods that required iterative calculations, and he developed precompiled mathematical tables to solve the problems, including a transcendental equation. Kepler was aware of the shortcomings of his novel methods, and called for a new Apollonius to offer a formal mathematical deduction. He (...)
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  • A sharper image: the quest of science and recursive production of objective realities.Julio Michael Stern - 2020 - Principia: An International Journal of Epistemology 24 (2):255-297.
    This article explores the metaphor of Science as provider of sharp images of our environment, using the epistemological framework of Objective Cognitive Constructivism. These sharp images are conveyed by precise scientific hypotheses that, in turn, are encoded by mathematical equations. Furthermore, this article describes how such knowledge is pro-duced by a cyclic and recursive development, perfection and reinforcement process, leading to the emergence of eigen-solutions characterized by the four essential properties of precision, stability, separability and composability. Finally, this article discusses (...)
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  • Colloquium 3: Why Beauty is Truth in All We Know: Aesthetics and Mimesis in Neoplatonic Science1.Marije Martijn - 2010 - Proceedings of the Boston Area Colloquium of Ancient Philosophy 25 (1):69-108.
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  • A natureza matemática: da alma da Terra como potência geometrizante no opúsculo Da neve hexagonal de Johannes Kepler.Anastasia Guidi Itokazu - 2008 - Trans/Form/Ação 31 (1):73-86.
    Na física celeste apresentada em sua Astronomia nova, Kepler explica os movimentos planetários através da ação de uma certa força ou potência motriz solar. Em vista da aproximação feita no livro entre física celeste e explicações baseadas em “causas corpóreas”, chamam a atenção as numerosas passagens onde Kepler refere-se às noções de alma e mente planetária. No presente artigo discutimos esses trechos pouco comentados da Astronomia nova. Com o objetivo de iluminar a discussão, abordamos na segunda seção a definição de (...)
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  • Kepler's Optical Part of Astronomy (1604): Introducing the Ecliptic Instrument.Giora Hon & Yaakov Zik - 2009 - Perspectives on Science 17 (3):307-345.
    The year 2009 marks the 400th anniversary of the publication of one of the most revolutionary scientific texts ever written. In this book, appropriately entitled, Astronomia nova, Johannes Kepler developed an astronomical theory which departs fundamentally from the systems of Ptolemy and Copernicus. One of the great innovations of this theory is its dependence on the science of optics. The declared goal of Kepler in his earlier publication, Paralipomena to Witelo whereby The Optical Part of Astronomy is Treated , was (...)
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  • Kepler's move from.Bernard R. Goldstein & Giora Hon - 2005 - Perspectives on Science 13 (1):74-111.
    : This study of the concept of orbit is intended to throw light on the nature of revolutionary concepts in science. We observe that Kepler transformed theoretical astronomy that was understood in terms of orbs [Latin: orbes] (spherical shells to which the planets were attached) and models (called hypotheses at the time), by introducing a single term, orbit [Latin: orbita], that is, the path of a planet in space resulting from the action of physical causes expressed in laws of nature. (...)
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  • Kepler Then and Now.Owen Gingerich - 2002 - Perspectives on Science 10 (2):228-240.
  • Kepler’s optics without hypotheses.Sven Dupré - 2012 - Synthese 185 (3):501-525.
    This paper argues that Kepler considered his work in optics as part of natural philosophy and that, consequently, he aimed at change within natural philosophy. Back-to-back with John Schuster’s claim that Descartes’ optics should be considered as a natural philosophical appropriation of innovative results in the tradition of practical and mixed mathematics the central claim of my paper is that Kepler’s theory of optical imagery, developed in his Paralipomena ad Vitellionem (1604), was the result of a move similar to Descartes’ (...)
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  • Constructing copernicus.Peter Barker - 2002 - Perspectives on Science 10 (2):208-227.
    : This paper offers my current view of a joint research project, with Bernard R. Goldstein, that examines Kepler's unification of physics and astronomy. As an organizing theme, I describe the extent to which the work of Kepler led to the appearance of the form of Copernicanism that we accept today. In the half century before Kepler's career began, the understanding of Copernicus and his work was significantly different from the modern one. In successive sections I consider the modern conception (...)
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  • The method of astronomy following Kepler.Claudemir Roque Tossato & Pablo Rubén Mariconda - 2010 - Scientiae Studia 8 (3):339-366.
    This article deals with the methodological procedures employed by Johannes Kepler, particularly those used in the process of elaboration of the two first laws of planetary movements. Its aim is to show that the astronomical practice of Kepler is linked with the proposal of (physical and mathematical) hypothesis and with valuing precision in observational data, with the goal of obtaining, by means of rigorous procedures, the (mathematically expressed) regularities of planetary motions. It was only afterwards that Kepler looked for an (...)
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