Old belief that the earth is plane or discoidal in form
Flat Earth Model
According to Egyptians, Mesopotamians, and Homer
According to Israelites
Spherical Earth Model
Introduced by Pythagoras in the 6th century BC
Arguments for a spherical Earth
Earth was spherical since the moon and the sun were both spherical
The North Star is closer to the horizon for places nearer the equator
When the ship sailed, the hull disappeared first, which implied that the surface of the earth was curved
Modern Evidence Supporting Spherical Earth Model
Satellitephotos show the earth is spherical
Astronauts in satellites orbiting in low Earth orbit personally observed curvature of the planet
Lunar eclipse shows a darkcircle on the moon indicating a spherical earth
Timezones can only be explained if the world is round and continuously rotating on its axis
Airplanes can travel in a straight line without falling off any edges and circle the earth without stopping
Astronomical Observations before the Advent of Telescopes
Observations of the sun, moon, lunar eclipse, solar eclipse, daily and annual motion of the stars, constellations, and planets Mercury, Venus, Mars, Jupiter, and Saturn
Earliest Astronomical Observations
Nebra sky disk from Northern Europe dated 1600BC
Petroglyph showing the 1006AD supernova that resulted in the Crab Nebula
Babylonian records dated 1600 BC trying to record positions of planets and timeeclipse events
Evidence from Chinese, American, and European cultures like the Stonehenge
Hellenistic Observations
Thales used Babylonian data to predicteclipses
Eratosthenes introduced the spherical Earth model and calculated the circumference of the earth
Plato introduced the geocentric solar system model
Heraclides presented the first solar system model with the earth at the center
Aristarchus presented the heliocentric solar system model with the sun at the center
Renaissance and Astronomical Observations
Nicolaus Copernicus reintroduced the heliocentric theory
Tycho Brahe made accurate measurements of planetary and star positions
Johannes Kepler used Brahe's data to formulate the laws of planetary motion
Galileo Galilei pioneered astronomicalobservation and constructed the first small refracting telescope
Kepler's Laws of Planetary Motion
1. Law of Ellipses: Planets orbit the sun in elliptical paths with the sun at onefocus
2. Law of EqualAreas: The line from the sun to the planet sweepsoutequalareas in equal timeintervals
3. Law of Harmonies: The ratio of the squares of the orbital periods to the cubes of the average distances from the sun is the same for allplanets
Kepler'slaws explain the motion of planets around the sun
Kepler's laws corrected conflicts on epicycles in the heliocentrictheory by introducing ellipticorbits