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Keplers Laws

Keplers Laws

Assessment

Presentation

•

Science

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9th - 12th Grade

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Easy

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NGSS
HS-ESS1-4, MS-ESS1-2, MS-ESS1-3

+2

Standards-aligned

Created by

Tim Gault

Used 16+ times

FREE Resource

17 Slides • 7 Questions

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Kepler's Laws
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Learning Objectives
  • Describe the roles of gravity and tangential velocity in maintaining a planetary orbit.

  • Explain Kepler's three laws of planetary motion.

  • Define key orbital terms including ellipse, perihelion, and aphelion.

  • Relate a planet's orbital speed and period to its distance from the Sun.

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Key Vocabulary

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Gravity

The force that pulls objects together and keeps planets in their orbits around the Sun.

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Ellipse

An oval shape with two focal points, representing the true path of a planet's orbit around the Sun.

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Perihelion

The point in a planet's orbit where it is closest to the Sun, moving at its fastest speed.

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Aphelion

The point in a planet's orbit where it is farthest from the Sun, moving at its slowest speed.

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Orbital Period

The time it takes for a planet to complete one full orbit around the Sun, also known as its year.

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What Keeps a Planet in Orbit?

  • Gravity acts as the centripetal force, pulling a planet toward the Sun.

  • The planet's tangential velocity keeps it moving forward along its orbital path.

  • Gravity's strength depends on objects' mass and the distance between them.

  • A gravity well illustrates how massive objects have stronger gravitational pulls.

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Planets orbit the sun in an elliptical path.

​First Law

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web page not embeddable

Kepler’s Laws of Orbital Motion | How Things Fly

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Multiple Choice

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What does Kepler's 1st Law state?

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all planets move in elliptical shaped orbits around the sun

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all ellipses have one foci

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the area that a planet revolves around the sun is equal

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the speed that a planet revolves around the sun changes

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Planets move faster when they are closer to the Sun and slower when they are farther away.

​Second Law

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web page not embeddable

Kepler’s Laws of Orbital Motion | How Things Fly

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Kepler's Second Law
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This law provides a relationship between the distance of a planet from the Sun and the time it takes to complete one orbit. Planets that are farther from the Sun have longer orbital periods.

​Third Law

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web page not embeddable

Kepler’s Laws of Orbital Motion | How Things Fly

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​Keplers Third Law

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On your own, answer the remaining 6 Questions.

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Multiple Choice

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When do gravitational forces exist between two objects?

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They only exist between microscopic objects.

2

They are always present between any two objects.

3

Gravitational forces only act on objects falling on Earth.

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They only exist for objects in space.

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Multiple Choice

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What effect does increasing the distance between the two objects do to the gravitational force?

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The distance between two objects has no effect on the gravitational force

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It increases

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It stays the same

4

It decreases

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Multiple Choice

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A planet moves __________ when it is farthest from the sun.
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faster
2
slower

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Multiple Choice

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Where is the planet moving faster?

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Position A to B
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Position B to C
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Position H to I
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Position I to J

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Multiple Choice

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Based on the table, which planet in our solar system will have the fastest orbital speed?

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Venus

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Earth

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Saturn

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Mercury

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Multiple Choice

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You discover a new planet in our solar system. You measure it's orbital period to be 246 years.


Where is this planet likely to be located based on this information?

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Closer to the Sun than Mercury.

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Located between Earth and Jupiter.

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Located between Uranus and Neptune.

4

Located beyond Neptune.

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Kepler's Laws
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