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proposed the first heliocentric model, suggested the stars were really far away, ideas were not widely accepted and were largely overshadowed by the geocentric model
wrote the "Almagest" which summarized ancient Greek astronomy, introduced the concept of epicycles, defined the concept of deferents and eccentrics
proposed the heliocentric model in his work "De revolutionibus orbium coelestium.", asserted that the sun was at the center of the universe, explained retrograde motion as Eartth moving relative to other planets
developed the tychonic system, discovered the supernova of 1572, built the Uraniborg observatory, introduced the concept of stellar parallax
formulated the three laws of planetary motion, planets move in elliptical orbits, published "Astronomia nova", played a crucial role in confirming the heliocentric model
made the first known telescopic observations of the heavens, discovered 4 moons of Jupiter, observed the phases of venus, studied sunspots, his work on inertia and falling objects laid the groundwork for Newton, faced the inquisition
formulated the law of universal gravitation, developed three laws of motion (inertia, F=ma, action-reaction), his work completed the scientific revolution
Large circular orbit followed by the center of the small epicycle in which a planet was thought to move
the apparent shift in the position of a nearby star (relative to distant objects) that occurs as we view the star from different positions in Earth's orbit of the Sun each year
point in a planet's orbit that is farthest from the sun
The place in the Earth's orbit where Earth is closest to the sun.
half of the major axis of an ellipse
A elongated circle, or oval shape, the shape of the planets orbit.
the extent to which Mars' orbit differs from a perfect circle
the smaller circles that the planets move in proposed by Ptolemy
the center of the epicycles moved in larger circles known as this
a framework of ideas and assumptions that represents our best possible explanation for something