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Pythagoras
First to propose a spherical Earth, using observations like North and South constellations and lunar eclipses.
Plato's Concept of Earth
Described Earth as a globe, equidistant from its center, and having perfect, eternal contributions.
Aristotle's Geocentric Universe
Proposed a geocentric model with a fixed spherical Earth at its center in "On the Heavens".
Eratosthenes
Accurately calculated the circumference of the Earth through non-scientific methods.
Geocentric Theorists
Scholars like Plato, Aristotle, Ptolemy, and Tycho Brahe who believed Earth was at the center of the universe.
Heliocentric Theorists
Proponents like Aristarchus, Copernicus, Galileo, and Kepler who placed the Sun at the center of the universe.
Eudoxus of Cnidus
Proposed 27 interconnected geocentric spheres.
Claudius Ptolemy's Model
Described Earth as spherical with fixed stars and independent moving planets.
Aristarchus of Samos
Estimated sizes and distances of the Sun and Moon compared to Earth.
Modern Astronomy Characteristics
Differentiated by quantitative observations and logical mathematical theories.
Copernicus' Heliocentric Theory
Proposed Earth is one of many planets, rotating and revolving around the Sun.
Tycho Brahe
Modified the geocentric model and made precise measurements of planets.
Galileo Galilei's Discoveries
Discovered sunspots, the rough surface of the Moon, and the four Galilean moons of Jupiter.
Kepler's First Law
States that the orbits of planets are ellipses with the Sun at one focus.
Kepler's Second Law
An imaginary line from the Sun to a planet sweeps equal areas in equal intervals.
Kepler's Third Law
The cube of the orbital radius of a planet is proportional to the square of its period of revolution.