Article ID: CBB573664538

How to Make the Earth Orbit the Sun in 1614 (2019)

unapi

In 1614 the Jesuit astronomer Christoph Scheiner and his student, Johann Georg Locher, proposed a physical mechanism to explain how the Earth could orbit the sun. An orbit, they said, is a perpetual fall. They proposed this despite the fact that they rejected the Copernican system, citing problems with falling bodies and the sizes of stars under that system. In 1651 and again in 1680, Jesuit writers Giovanni Battista Riccioli and Athanasius Kircher, respectively, considered and rejected outright this idea of an orbit as a perpetual fall. Thus this important concept of an orbit was proposed, considered, and rejected well before Isaac Newton would use an entirely different physics to make the idea that an orbit is a perpetual fall the common way of envisioning and explaining orbits.

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Authors & Contributors
Marcacci, Flavia
Graney, Christopher M.
Gambaro, Ivana L.
Maciel Pinheiro
Ghalandari, Hanif
Tirapicos, Luís
Journals
Annals of Science: The History of Science and Technology
Tarikh-e Elm (The Iranian Journal for the History of Science)
Physis: Rivista Internazionale di Storia della Scienza
Physics in Perspective
Nuncius: Annali di Storia della Scienza
Galilæana: Journal of Galilean Studies
Publishers
University of Notre Dame Press
Pavia University Press
Verlag Harri Deutsch
Olschki
Meiner
Concepts
Cosmology
Astronomy
Physics
Science and religion
Orbits; planets
Geocentrism
People
Riccioli, Giovanni Battista
Galilei, Galileo
Brahe, Tycho
Scheiner, Christoph
Copernicus, Nicolaus
Ptolemy
Time Periods
17th century
16th century
Early modern
Renaissance
Medieval
Ancient
Places
Italy
Europe
Bologna (Italy)
Spain
Portugal
Germany
Institutions
Jesuits (Society of Jesus)
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