ch. 29 sec. 1 overview of solar system. early ideas humans have watched the sky for thousands of...
TRANSCRIPT
Ch. 29 Sec. 1Ch. 29 Sec. 1
Overview of Solar SystemOverview of Solar System
Early IdeasEarly Ideas Humans have watched the sky for thousands of Humans have watched the sky for thousands of
yearsyears Planets change position relative to the starsPlanets change position relative to the stars
• Easy to recognize the differenceEasy to recognize the difference Believed to be Believed to be Geocentric: Geocentric: earth centeredearth centered Copernicus in 1543 noticed a difference in Copernicus in 1543 noticed a difference in
movement of planetsmovement of planets• HeliocentricHeliocentric: Sun centered: Sun centered
Planet MotionPlanet Motion
Normal direction of planets is to the eastNormal direction of planets is to the east Occasionally a planet will move in opposite Occasionally a planet will move in opposite
directiondirection• Retrograde MotionRetrograde Motion
Kepler’s 1Kepler’s 1stst Law Law Kepler used his mentors data on planetary Kepler used his mentors data on planetary
motionmotion• Demonstrated that planets move in an ellipseDemonstrated that planets move in an ellipse• Kepler’s 1Kepler’s 1stst Law Law
Kepler’s 1Kepler’s 1stst Law Law EccentricityEccentricity
• A planets distance isn’t always the same from sunA planets distance isn’t always the same from sun• PerihelionPerihelion: Closest to sun: Closest to sun• AphelionAphelion: Furthest from sun: Furthest from sun• Measured from 0 – 1: 0 – circle / 1 - parabolaMeasured from 0 – 1: 0 – circle / 1 - parabola
Kepler’s 2Kepler’s 2ndnd Law Law
An imaginary line sweeps out from sun to An imaginary line sweeps out from sun to planet of equal area in equal amounts of planet of equal area in equal amounts of timetime• 2nd Law
Other DiscoveriesOther Discoveries
GalelioGalelio• Use 1Use 1stst telescopes telescopes• Discovered 4 moons around JupiterDiscovered 4 moons around Jupiter
NewtonNewton• Gravity: observed the orbits of planets and moonGravity: observed the orbits of planets and moon• Force is directly proportional to massForce is directly proportional to mass
GravityGravity Force of gravity grows stronger with an increase Force of gravity grows stronger with an increase
in massin mass Force of gravity grows smaller with increasing Force of gravity grows smaller with increasing
distancedistance Center of mass will be closer to the heavier objectCenter of mass will be closer to the heavier object