Equation for Kepler’s Third Law
p^2 = a^3
p = planet’s orbital period in years
a = semi-major acid in AU
Newton’s Universal Law of Gravity
F = GMm/r^2
F = force of gravity
G = “big G”
M = bigger mass
m = smaller mass
r = radius; distance between centers of big and small masses
Newton’s Version of Kepler’s Third Law
M * P^2 = 4pi^2 / G * a^3
What does AU stand for?
Astronomical Unit - Distance from the Sun to the Earth
Value for Speed of Light
3.00 * 10^8 m/s
Brightness of Stars (to Determine Distance to Stars)
B = L / 4piD^2
Brightness = Luminosity/(Distance)^2
Stefan-Boltzmann Law
L = 4piR^2óT^4