Gravitational Forces and Constants

Gravitational Forces and Constants

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video tutorial explains how to calculate the net gravitational force acting on the moon due to the Earth and the Sun. It begins by introducing the problem and making assumptions about the masses and distances of the celestial bodies involved. A diagram is used to represent the forces as vectors at a 90-degree angle. The tutorial then demonstrates how to calculate the individual forces using the gravitational constant and the Pythagorean theorem. Finally, the net force is calculated, and the direction of the moon's movement is discussed.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the mass of the Earth used in the problem?

5.98 x 10^24 kg

3.84 x 10^8 kg

7.35 x 10^22 kg

1.99 x 10^30 kg

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How are the Earth, Moon, and Sun positioned relative to each other in the problem?

At a 45-degree angle

In a triangular formation

At a 90-degree angle

In a straight line

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the distance between the Moon and the Earth used in the calculations?

7.35 x 10^22 meters

3.84 x 10^8 meters

1.50 x 10^11 meters

5.98 x 10^24 meters

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the approximate gravitational force on the Moon due to the Earth?

3.0 x 10^20 N

1.5 x 10^20 N

2.0 x 10^20 N

4.3 x 10^20 N

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the mass of the Sun used in the problem?

3.84 x 10^8 kg

7.35 x 10^22 kg

1.99 x 10^30 kg

5.98 x 10^24 kg

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the approximate gravitational force on the Moon due to the Sun?

3.0 x 10^20 N

2.0 x 10^20 N

4.3 x 10^20 N

1.5 x 10^20 N

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Which theorem is used to calculate the net force on the Moon?

Law of Universal Gravitation

Kepler's Third Law

Pythagorean Theorem

Newton's First Law

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