Chapter 3 Flashcards
(8 cards)
1
Q
Kepler
A
- inherited Brahe’s data
- focused on fitting Mars into the data
- started over and observed that ellipses fit the data of the planets
2
Q
ellipse
A
- a circle with an eccentricity <0
- major and minor axis
3
Q
Kepler’s Laws of Planetary Motion
A
1st: The path of the planets about the sun is elliptical in shape, with the center of the sun being located at one focus
2nd: An imaginary line drawn from the center of the sun to the center of the planet will sweep out equal areas in equal intervals of time.
3rd: Distance planets have slower orbital periods
4
Q
Galileo
A
-birth of modern science
5
Q
Aristotelian Objections
A
- Earth can not be moving because the objects in the air would be left behind
- no circular orbits are not as perfect as the heavens should be
6
Q
Galileo’s answers Aristotelian Objections
A
- an object in motion will stay in motion unless acted on by an external force
- Tycho showed heavens are changing and thus not perfect
- used a telescope to detect stellar parallax
7
Q
Elements of modern science
A
- all theories must be falsifiable
- must rely solely on natural causes
- the simplest model is usually true (Occam’s razor)
- theories must match reality
8
Q
Asreology
A
- search for influences of the stars, planets
- supernatural explanations of natural events
- predictions fail to pass rigorous tests