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Earth Science An overview of the Solar System
Geocentric Theory  ,[object Object],[object Object],[object Object]
 
Problems with Geocentric ,[object Object],[object Object],[object Object],[object Object]
Heliocentric Theory ,[object Object],[object Object],[object Object]
 
Galileo ,[object Object],[object Object]
Adding to Copernicus ,[object Object],[object Object],[object Object],[object Object]
Cont. ,[object Object]
Gravity The mechanisms of Newton's law of universal gravitation; a point mass  m 1 attracts another point mass  m 2 by a force  F 2 which is proportional to the product of the two masses and inversely proportional to the square of the distance ( r ) between them. Regardless of masses or distance, the magnitudes of | F 1| and | F 2| will always be equal.  G  is the gravitational constant.
General relativity ,[object Object],[object Object],[object Object]
[object Object],Newton Vs. Einstein ,[object Object]
The Sun ,[object Object],[object Object],[object Object]
Mercury ,[object Object],[object Object],[object Object]
Venus ,[object Object],[object Object]
Earth ,[object Object],[object Object],[object Object]
EARTH ,[object Object],[object Object],[object Object],[object Object],[object Object]
Moon
Mars ,[object Object],[object Object],[object Object]
Moons of Mars ,[object Object],[object Object]
Jupiter
Jupiter’s Red Spot ,[object Object],[object Object]
Moons of Jupiter ,[object Object],[object Object]
Io ,[object Object],[object Object]
Europa ,[object Object],[object Object],[object Object],[object Object]
Ganymede ,[object Object],[object Object]
Callisto ,[object Object],[object Object]
Saturn ,[object Object],[object Object]
Rings of Saturn ,[object Object],[object Object]
Uranus ,[object Object],[object Object],[object Object]
Neptune ,[object Object],[object Object],[object Object]
Pluto ,[object Object],[object Object]

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Solar System

  • 1. Earth Science An overview of the Solar System
  • 2.
  • 3.  
  • 4.
  • 5.
  • 6.  
  • 7.
  • 8.
  • 9.
  • 10. Gravity The mechanisms of Newton's law of universal gravitation; a point mass m 1 attracts another point mass m 2 by a force F 2 which is proportional to the product of the two masses and inversely proportional to the square of the distance ( r ) between them. Regardless of masses or distance, the magnitudes of | F 1| and | F 2| will always be equal. G is the gravitational constant.
  • 11.
  • 12.
  • 13.
  • 14.
  • 15.
  • 16.
  • 17.
  • 18. Moon
  • 19.
  • 20.
  • 22.
  • 23.
  • 24.
  • 25.
  • 26.
  • 27.
  • 28.
  • 29.
  • 30.
  • 31.
  • 32.