Ay [T6.5] - Kepler's Laws Flashcards

Both Kepler's Laws of Planetary Motion, and Newton's Universal Law of Gravitation

1
Q

Name law 1 of the 3 laws of planetary motion

A

The orbit of all the planets is an ellipse with the sun at one foci.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Name law 2 of the 3 laws of planetary motion

A

An imaginary line connecting the planet to the sun “sweeps out” equal areas in equal times

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Name law 3 of the 3 laws of planetary motion

A

The square of the orbital period is proportional to the cube of it’s mean distance from the sun

T²∝R³

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Define aphelion

A

The furthest point from the sun on an orbit

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Define perihelion

A

The closest point to the sun on an orbit

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Define eccentricity

A

A measure of how stretched an elliptical orbit is

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

When is the aphelion for Earth’s orbit?

A

In the summer

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

When is the perihelion for Earth’s orbit?

A

In the winter

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

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?

A

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.)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

What is the equation related to Kepler’s 3rd law for anything that orbits the sun?

A

T(y)² / R(AU)³ = 1

T measured in years (y)
R measured in AU

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

If T² / R³ = k, and you’re using the data of 2 objects that orbit the same object, what can you do?

A

If constant doesn’t change, you can remove it.

(T1²) / (R1³) = (T2²) / (R2³)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

The k in Kepler’s 3rd law depends on what?

A

The mass of the central object - the bigger the mass, the smaller k is

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

What is the ratio of masses equations for Kepler’s 3rd law?

A

k1 / k2 = m2 / m1

1 = the sun
2 = the new star

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

In Newton’s Universal Law of Gravitation, the size of the force acting between bodies depends on what things?

A

The mass of each body in the situation

The distance between the two bodies

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

In Newton’s Law of Universal Gravitation, what is force proportional to (both words and equations)?

A

Force is directly proportional to both masses of both objects, and force is inversely proportional to distance squared

F ∝ (m1 × m2) / r²

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

In Newton’s Law of Universal Gravitation, what happens if you double one of the masses of one of the objects?

A

The magnitude of the forces on each object doubles

17
Q

In Newton’s Law of Universal Gravitation, what happens if you double both masses of both objects at the same time?

A

The magnitude of the forces on each object quadruples

18
Q

In Newton’s Law of Universal Gravitation, what happens if you half the distance between the objects?

A

The magnitude of the forces on each object quadruples

19
Q

In Newton’s Law of Universal Gravitation, what happens if you double the distance between the objects?

A

The magnitude of the forces on each object is divided by 4

20
Q

In Newton’s Law of Universal Gravitation, what happens if you triple the distance between the objects?

A

The magnitude of the forces on each object is divided by 9