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Johnlukes Astronomy Haiku Deck

Published on Nov 20, 2015

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PRESENTATION OUTLINE

ASTRONOMISTS

ARISTOTLE

  • A greek philosopher
  • His model placed the moon,sun, planets,and stars on a series of circles that surround the earth.
  • He thought that if Earth went around the sun, then the relative position of stars would change as earth moves.
  • He lived from 384-322 BCE

ARISTARCHUS

  • A greek astronomer and mathmetician
  • His model that he created was not widely known and liked.
  • He attempted to measure the relative distance from the moon and the sun.
  • His ratio of distance was to small but was important in the use of observation and gemoetry to solve a scientific problem.
  • Lived from 310-230 BCE

PTOLEMY

  • An astronomef, geographer, and mathematician.
  • His book, that was named "Almagest" is one of the few books we have from this early in time.
  • The book was on the observation of planets going back as much as 800 years ago.
  • His theory was that planets moved on larger circles. " wheels on wheels"
  • Lived from 100-170 BCE

COPERNICUS

  • He thought that Ptolemy's theory was to complicated.
  • He used "wheels on wheels" system, he thought that they should travel in perfect circles.
  • He also thought that earth circled the sun.
  • 1473-1543

KEPLER

  • He realized that requiring planetary motion to be exactly circular did not fit.
  • He took another path and found that ellipses fit best.
  • Lives from 1571-1630

GALILEO

  • Scientific method
  • He helped improve the telescope.
  • Observed the moons Io, Europa, Callisto, and orbiting jupiter.
  • Lived from 1564-1642

KEPLERS 1ST LAW

  • He carefully plotted the orbit of mars, and it showed a deformed circle.
  • After 8 years, he realized that this was an ellipse.
  • Kepler placed the sun at one of the foci of the ellipse.

KEPLERS 2ND LAW

  • Using the shape of an ellipse, he looked deeper in to the data.
  • He found that when planets get closer to the sun, they get faster.

KEPLERS 3RD LAW

  • He calculated the orbital period and the distance from the sun for the planets using tycho's data.
  • He discovered that the square of the orbital period was proportional to the cube of the planets distance from the sun.