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Gravitational Forces

Gravitational Forces

Assessment

Presentation

Science

8th Grade

Hard

Created by

Joseph Anderson

FREE Resource

9 Slides • 5 Questions

1

Gravity Part 2

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2

Effects of Mass & Distance on Gravitational Force

  • The more massive an object, the greater it's gravitational pull

  • The closer the distance between objects, the greater the gravitational pull

  • The gravitational pull between the Sun and each planet or between Earth and it's moon causes distinct motions between and among the objects

3

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4

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5

Multiple Select

If the mass of an object increases, what happens to the gravitational pull?

1

Increases

2

Decreases

6

Multiple Select

The closer that two objects come together, what happens to the gravitational pull?

1

Decreases

2

Increases

7

Effects of Gravity on Planetary Orbits

  • The Sun's gravitational attraction along with a planet's inertia (continued forward motion), keeps the planets moving in an elliptical orbit (slightly oval) & determines how fast they move.

8

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9

Effects of Gravity on Planetary Orbits

  • Planets nearer to the Sun move/orbit faster due to the higher gravitational pull from the Sun.

  • Planets farther from the Sun move/orbit slower due to the gravitational pull becoming less the farther from the Sun a planet is located.

10

Mercury, Venus, Earth, Mars

4 planets closest to the Sun that orbit faster because of higher gravitational pull between them and the Sun

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11

Jupiter, Saturn, Uranus, Neptune

Even though these 4 planets are more massive, the large distance that they are from the Sun reduces the gravitational pull the Sun has on them.

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12

Multiple Choice

Inertia is:

1

Forward motion

2

Reverse motion

3

Sideways motion

13

Multiple Choice

Planets closer to the sun have:

1

More gravitational pull with the Sun

2

Less gravitation pull with the sun

14

Multiple Choice

What keeps planets in elliptical orbits?

1

Gravitational attraction

2

Inertia

3

Both gravitational attraction & inertia

4

Neither one

Gravity Part 2

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