Lecture

Galileo's Defense

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In course

HUM-318: Sciences, raison et foi

Cet enseignement a pour but de revenir sur les conflits entre sciences et religions. Des conflits inévitables quand la science décida d'aborder des thèmes qui recouvrent ceux discutés dans les textes sacrés, en particulier la question de l'origine du monde ...

Description

This lecture explores Galileo's defense of the heliocentric theory against the geocentric model, his struggles with the Catholic Church, and the impact of his work on the relationship between science and religion. It delves into his discoveries, the controversy surrounding his publications, and the lasting consequences of his trial, shedding light on the evolution of scientific methodology and the autonomy of scientific inquiry.

Instructor

Jean-François Bert

Teaching & PhD Past EPFL PhD Students as codirector Alina Volynskaya Courses Anthropology of belief HUM-382 This course is an introduction to the question of conspiracy theories especially in the field of science Darwin, religion and science HUM-365 This course takes the long history of opponents of Darwin and Darwinism (creationists, neo-creationists, supporters of intelligent design) to try to understand their strategies and arguments. Sciences and religions I HU

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Related concepts (32)

Scientific community

The scientific community is a diverse network of interacting scientists. It includes many "sub-communities" working on particular scientific fields, and within particular institutions; interdisciplinary and cross-institutional activities are also significant. Objectivity is expected to be achieved by the scientific method. Peer review, through discussion and debate within journals and conferences, assists in this objectivity by maintaining the quality of research methodology and interpretation of results.

Copernican Revolution

The Copernican Revolution was the paradigm shift from the Ptolemaic model of the heavens, which described the cosmos as having Earth stationary at the center of the universe, to the heliocentric model with the Sun at the center of the Solar System. This revolution consisted of two phases; the first being extremely mathematical in nature and the second phase starting in 1610 with the publication of a pamphlet by Galileo.

Aristarchus of Samos

Aristarchus of Samos (ˌærəˈstɑrkəs; Ἀρίσταρχος ὁ Σάμιος, Aristarkhos ho Samios; 310-230 BCE) was an ancient Greek astronomer and mathematician who presented the first known heliocentric model that placed the Sun at the center of the known universe, with the Earth revolving around the Sun once a year and rotating about its axis once a day. He was a student of Strato of Lampsacus, who was the third head of the Peripatetic School in Greece. According to Ptolemy, during Aristarchus' time there, he observed the summer solstice of 280 BCE.

Conflict thesis

The conflict thesis is a historiographical approach in the history of science that originated in the 19th century with John William Draper and Andrew Dickson White. It maintains that there is an intrinsic intellectual conflict between religion and science, and that it inevitably leads to hostility. The consensus among historians of science is that the thesis has long been discredited, which explains the rejection of the thesis by contemporary scholars. Into the 21st century, historians of science widely accept a complexity thesis.

Relationship between religion and science

The relationship between religion and science involves discussions that interconnect the study of the natural world, history, philosophy, and theology. Even though the ancient and medieval worlds did not have conceptions resembling the modern understandings of "science" or of "religion", certain elements of modern ideas on the subject recur throughout history. The pair-structured phrases "religion and science" and "science and religion" first emerged in the literature during the 19th century.

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