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Kepler's Laws and Planetary Motion

Kepler's Laws and Planetary Motion

Assessment

Interactive Video

Physics, Science, Mathematics

9th - 10th Grade

Practice Problem

Hard

Created by

Patricia Brown

FREE Resource

The video tutorial covers Kepler's Second Law of Planetary Motion, explaining that a line between a planet and the sun sweeps out equal areas in equal time periods. This implies that a planet's speed increases as it approaches the sun and decreases as it moves away. The tutorial also discusses the concept of angular momentum, which remains constant in an elliptical orbit, and hints at a future lesson on deriving Kepler's Second Law. The video concludes with a discussion on the accuracy of the animation used to illustrate these concepts.

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8 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What does Kepler's Second Law of Planetary Motion state?

The distance between a planet and the sun remains constant.

An imaginary line between the sun and a planet sweeps out equal areas in equal time periods.

The speed of a planet is constant throughout its orbit.

Planets move in circular orbits around the sun.

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

According to Kepler's Second Law, what happens to the speed of a planet as it approaches the sun?

The speed becomes zero.

The speed remains constant.

The speed decreases.

The speed increases.

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the sun referred to as in the solar system?

The Satellite or Orbiting Body

The Secondary or Outer Body

The Minor or Distant Body

The Primary or Central Body

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the acceleration of a satellite in orbit behave?

It varies and is not constant.

It is uniformly accelerated.

It is constant.

It decreases uniformly.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is necessary to derive Kepler's Second Law?

The constant mass of the satellite.

The constant speed of the satellite.

The constant angular momentum of the satellite.

The constant distance from the sun.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why might the animation not perfectly represent Kepler's Second Law?

The areas are not exactly equal.

The orbits are shown as perfectly circular.

The planets are shown as stationary.

The sun is depicted as smaller than the planets.

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why was the eccentricity of the ellipse exaggerated in the animation?

To demonstrate the sun's movement.

To show the planets' actual orbits.

To make the animation more clear.

To make the animation more entertaining.

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