5.8 Ancient Astronomers Timetoast Timeline

  • 240 BCE

    240 BCE ; Eratoshenes

    In 240 B.C, Eratosthenes Measures the Earth. By around 500 B.C., most ancient Greeks believed that Earth was round, not flat. But they had no idea how big the planet is until about 240 B.C., when Eratosthenes devised a clever method of estimating its circumference.
  • 126 BCE

    126 ; Ptolemy

    Ptolemy was an astronomer and mathematician. He believed that the Earth was the center of the Universe. The word for earth in Greek is geo, so we call this idea a "geocentric" theory.t gives in detail the mathematical theory of the motions of the Sun, Moon, and planets. Ptolemy made his most original contribution by presenting details for the motions of each of the planets. His theories were not superseded until a century after Copernicus presented his heliocentric theory in 1543.
  • 1514

    1514 ; Nicholas Copernicus

    Copernicus developed his own celestial model of a heliocentric planetary system. Around 1514, he shared his findings in the Commentariolus. His second book on the topic, De revolutionibus orbium coelestium, was banned by the Roman Catholic Church decades after his May 24, 1543 death in Frombork.
  • Feb 13, 1578

    1578 ; Tycho Brache

    Danish astronomer whose work in developing astronomical instruments and in measuring and fixing the positions of stars paved the way for future discoveries. Tycho Brahe was a Danish nobleman and astronomer, and he was one of the individuals whose work helped overturn that belief in favor of a heliocentric model of the universe, with the sun at the center.
  • 1604 - 1611 Johannes Kepler

    German astronomer who discovered three major laws of planetary motion, conventionally designated as follows: the planets move in elliptical orbits with the Sun at one focus; the time necessary to traverse any arc of a planetary orbit is proportional to the area of the sector between the central body and that arc (the “area law”); and there is an exact relationship between the squares of the planets’ periodic times and the cubes of the radii of their orbits (the “harmonic law”).
  • 1687 ; Sir Isaac Newton

    Newton developed the three laws of motion which form the basic principles of modern physics. His discovery of calculus led the way to more powerful methods of solving mathematical problems.
  • 1921 ; Albert Einstein

    As a physicist, Einstein had many discoveries, but he is perhaps best known for his theory of relativity and the equation E=MC2, which foreshadowed the development of atomic power and the atomic bomb. Einstein developed a theory of Brownian motion in terms of fluctuations in the number of molecular collisions with an object, providing further evidence that matter was composed of atoms.