1. Kepler’s Laws and Universal Gravitation

2. Kepler’s Laws of Planetary Motion

3. Kepler’s 1st Law Planetary Motion
The path of the planets around the sun are ellipses with the sun at one of the focus points
Consequence: The planets traveling in their orbits are sometimes closer to the sun and other times further away
Note: The orbits are only slightly elliptical. They are close to circular.

4. Kepler’s 2nd Law of Planetary Motion
The planets sweep out equal areas in equal time intervals no matter how close or far away a planet is from the sun
Consequence: Planets speed up as they move closer to the sun and slow down as they move further away

5. Kepler’s 3rd Law Planetary Motion
3. The ratio of the squares of the Periods of any two planets going around the sun is equal to the ratio of the cubes of their Average Distances away from the sun.
Consequence: Planets that are farther away from the sun have a longer Period of Revolution

6. Equation for Kepler’s 3rd Law
Kepler’s 3rd Law can be written in an equation form.
(Ta)2 = (Ra)3
(Tb) (Rb)3
Kepler’s 3rd law applies to any two objects going around a third central object!
(2 planets around the sun or 2 moons around a planet)

7. Astronomical Units (A.U.)
Measurement of distance between two different planets
Ex) average distance between the Earth and the Sun is dE-S = 1.5 x m
1 A.U. = 1.5 x 1011 m
dE-S = 1A.U.

8. Universal Gravitation
aka. Gravity
A force of attraction between any two masses and that each mass pulls on the other with an equal and opposite force

9. Universal Gravitation
The Force of Gravity is directly proportional to the mass of each object
F a m
The Force of Gravity is inversely proportional to the square of the distance between the center of the masses
F a 1/d2 (Inverse Square Law)

10. Universal Gravitation Equation
Newton used his Law of Gravity (Universal Gravitation) to make the following equation:
Fg = G m1 m2 d2
Where “G” is the Universal Gravitational Constant! G = 6.67 x Nm2/kg2

11. Universal Gravitation Equation
Note: In using the Universal Gravitation Equation,
One mass(m1) doubles - Fg is doubled
Both masses(m1, m2) double– Fg is quadrupled (multiplied by 4)
Distance(d) doubles – Fg is divided by (22 = 4)
Note: d has to be measured from center to center! (Not center to SURFACE!)

12. Universal Gravitation and Acceleration Due to Gravity
The acceleration due to gravity (g) changes if you go to another planet or moon or as you move away from the surface of Earth
g = 9.8 m/s2 at the surface of the Earth
g will be greater on a larger planet (Jupiter gJ = 25 m/s2)
g will be smaller on a smaller planet (Mercury gM = 3.78 m/s2)

13. Satellites The Moon is a satellite of the Earth!
The Earth is a satellite of the Sun!
Jupiter’s Moons are satellites of Jupiter!
We put up man-made satellites around the Earth and other planets!
Most of the man-made satellites going around the Earth are Geosynchronous (have a period, T = 24 hours)

14. Gravitational Field
Gravity is not a contact force. Therefore, masses produce a Gravitational Field!
g measures the gravitational field strength acting on an object
g = Fg/m