Kepler, Galileo & Newton: Foundations of Astronomy

Kepler's Laws of Planetary Motion and Early Pioneers in Astronomy

Administrative Updates

  • Test grades have been posted and are available for review.

  • If lab notes for Tuesday's session were not submitted, please send them to avoid a zero grade. (Notes are currently marked as zero until submitted).

  • An unanimous vote decided against changing lab partners.

  • M&M's were forgotten but are now packaged in small bags where lab packets are stored (on a bench in Bracey, near the back door, in a box for our class). Students are encouraged to retrieve them promptly as M&M's have a tendency to disappear quickly once word spreads. These will be used in a future lab session, not today or next Tuesday.

Kepler's Laws of Planetary Motion

  • Historical Context

    • Johannes Kepler used Tycho Brahe's data (obtained after Brahe's death, possibly illicitly) to deduce the laws of planetary motion.

    • He spent four years on these calculations; a task that would take mere moments with modern computers and calculators.

  • Validity and Significance

    • Kepler's laws, discovered in the 1600s, are still fundamental and valid today, used even for launching spacecraft.

    • This stands in stark contrast to most 16th-century knowledge (e.g., medicine, which might involve leeches).

Kepler's First Law: The Law of Ellipses
  • Statement: Planets orbit the Sun in ellipses with the Sun at one focus.

  • Correction of Ancient Bias

    • Earlier beliefs (a bias that the universe must be perfect) held that orbits were perfect circles, considering the circle the only