1.
How did Copernicus, Tycho, and Kepler challenge the Earth centered model? •
proposed Sun-centered model (published 1543) used model to determine layout of
solar system (planetary distances in AU).
2.
What are Kepler's three laws of planetary motion?
a. The orbit of each planet around the Sun is an
ellipse with the Sun at one focus.
b. As a planet moves around its orbit, it sweeps out
equal areas in equal times.
c. More distant planets orbit the Sun at slower
average speeds, obeying the relationship
3.
How did Galileo solidify the Copernican revolution? Earth could not be moving
because objects in air would be left behind. Non-circular orbits are not
“perfect” as heavens should be. If Earth were really orbiting Sun, we’d detect
stellar parallax.
4.
How can we distinguish science from nonscience? Science: seeks explanations
that rely solely on natural causes; progresses through the creation and testing
of models of nature; models must make testable predictions.
5.
What is a scientific theory? A model that explains a wide variety of
observations in terms of a few general principles and that has survived
repeated and varied testing.
6.
In what sense is the moon imperfect? The moon is not a perfect circle shape. It
has deformities such as craters.
7.
Why did Kepler use ellipses instead of circles? The orbit of a planet around
the Sun is an ellipse having the center of mass of the planet-Sun system at one
focus.
8.
When was Tycho Brahe born? December 14, 1546
9.
When was Johannes Kepler born? December 27, 1571
10.
When was Galileo Galilei born? February 15, 1564
1 comment:
Good work.
Post a Comment