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Lecture

Origins of Earth: Religious & Scientific Perspectives

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 delves into the historical evolution of Earth's origin theories, from religious narratives to scientific inquiries. It explores the transition from mythological interpretations to rational scientific approaches, highlighting key figures like Thales and Copernicus. The presentation covers the clash between religious beliefs and emerging scientific discoveries, focusing on Copernicus' heliocentric model and the subsequent controversies it sparked. It also discusses the contributions of Thomas Digges and Giordano Bruno in expanding the understanding of the universe. The lecture concludes with the persecution faced by Bruno for advocating an infinite universe, challenging traditional theological views.

Instructor

Jean-François Bert

Official source

Ontological neighbourhood

Astronomy

Astrophysics: Physical cosmology

Related concepts (32)

Objections to evolution

Objections to evolution have been raised since evolutionary ideas came to prominence in the 19th century. When Charles Darwin published his 1859 book On the Origin of Species, his theory of evolution (the idea that species arose through descent with modification from a single common ancestor in a process driven by natural selection) initially met opposition from scientists with different theories, but eventually came to receive overwhelming acceptance in the scientific community.

Geocentric model

In astronomy, the geocentric model (also known as geocentrism, often exemplified specifically by the Ptolemaic system) is a superseded description of the Universe with Earth at the center. Under most geocentric models, the Sun, Moon, stars, and planets all orbit Earth. The geocentric model was the predominant description of the cosmos in many European ancient civilizations, such as those of Aristotle in Classical Greece and Ptolemy in Roman Egypt.

Copernican heliocentrism

Copernican heliocentrism is the astronomical model developed by Nicolaus Copernicus and published in 1543. This model positioned the Sun at the center of the Universe, motionless, with Earth and the other planets orbiting around it in circular paths, modified by epicycles, and at uniform speeds. The Copernican model displaced the geocentric model of Ptolemy that had prevailed for centuries, which had placed Earth at the center of the Universe.

Shape of the universe

The shape of the universe, in physical cosmology, is the local and global geometry of the universe. The local features of the geometry of the universe are primarily described by its curvature, whereas the topology of the universe describes general global properties of its shape as a continuous object. The spatial curvature is described by general relativity, which describes how spacetime is curved due to the effect of gravity.

Cosmology

Cosmology () is a branch of physics and metaphysics dealing with the nature of the universe. The term cosmology was first used in English in 1656 in Thomas Blount's Glossographia, and in 1731 taken up in Latin by German philosopher Christian Wolff, in Cosmologia Generalis. Religious or mythological cosmology is a body of beliefs based on mythological, religious, and esoteric literature and traditions of creation myths and eschatology. In the science of astronomy, cosmology is concerned with the study of the chronology of the universe.

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