Ay [T6.5] - Kepler's Laws Flashcards
Both Kepler's Laws of Planetary Motion, and Newton's Universal Law of Gravitation
Name law 1 of the 3 laws of planetary motion
The orbit of all the planets is an ellipse with the sun at one foci.
Name law 2 of the 3 laws of planetary motion
An imaginary line connecting the planet to the sun “sweeps out” equal areas in equal times
Name law 3 of the 3 laws of planetary motion
The square of the orbital period is proportional to the cube of it’s mean distance from the sun
T²∝R³
Define aphelion
The furthest point from the sun on an orbit
Define perihelion
The closest point to the sun on an orbit
Define eccentricity
A measure of how stretched an elliptical orbit is
When is the aphelion for Earth’s orbit?
In the summer
When is the perihelion for Earth’s orbit?
In the winter
In the 2nd law of the 3 laws of planetary motion, where is a celestial body in it’s orbit moving the slowest and where is it moving the fastest?
Closer to the object that it’s orbiting, the celestial body moves quicker. (It’ll have the most kinetic energy here.)
Further away from the object that it’s orbiting, the celestial body moves slower. (It’ll have the least kinetic energy here.)
What is the equation related to Kepler’s 3rd law for anything that orbits the sun?
T(y)² / R(AU)³ = 1
T measured in years (y)
R measured in AU
If T² / R³ = k, and you’re using the data of 2 objects that orbit the same object, what can you do?
If constant doesn’t change, you can remove it.
(T1²) / (R1³) = (T2²) / (R2³)
The k in Kepler’s 3rd law depends on what?
The mass of the central object - the bigger the mass, the smaller k is
What is the ratio of masses equations for Kepler’s 3rd law?
k1 / k2 = m2 / m1
1 = the sun
2 = the new star
In Newton’s Universal Law of Gravitation, the size of the force acting between bodies depends on what things?
The mass of each body in the situation
The distance between the two bodies
In Newton’s Law of Universal Gravitation, what is force proportional to (both words and equations)?
Force is directly proportional to both masses of both objects, and force is inversely proportional to distance squared
F ∝ (m1 × m2) / r²