Solar System Physics I Dr Martin Hendry 5 lectures, beginning Autumn 2007 Department of Physics and Astronomy Astronomy 1X Session 2007-08.
200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 200 300 400 500 100 Earth-Sun-Moon Seasons Solar System Stars Laws and.
More Light, History, Gravity, Distance, Relativity, and Space-time.
Std. IE 1k- Students will recognize the cumulative nature of scientific evidence Objective 1: Compare models of the solar systems Objective 2: Summarize.
Astronomy 100 Tuesday, Thursday 2:30 - 3:45 pm Tom Burbine [email protected].
Lesson 1-3 Classical Astronomy (500B.C. to 1400 A.D.)
1 Gravity and Motion II Heliocentric Astronomy. 2 Topics l Recap l Heliocentric Astronomy l Copernicus l Brahe l Kepler l Galileo l Newton l Summary.
History of Solar System Understanding How do we know the Earth goes around the Sun?
Kepler’s laws Kepler’s laws. Ancient Astronomy Ancient civilizations observed the skies Many built structures to mark astronomical events for religious.
The Scien”terrific”! Revolution 1543-1687 c. ~1300 oFr science; “knowledge (of something) acquired by study.” (L; scientia) c. ~1300 oFr science; “knowledge.
Planetary Motions and Lessons in Science. Can One Prove that the Earth is Round? Shadow of the Earth during a lunar eclipse Height of Polaris above the.
Ch 22 Astronomy. Ancient Greeks 22.1 Early Astronomy Astronomy is the science that studies the universe. It includes the observation and interpretation.