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