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Gravity and Orbits PhET Simulation

Rated 4.64 out of 5, based on 22 reviews
4.6 (22 ratings)
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Sarah's STEM stuff
3k Followers
Grade Levels
6th - 8th
Resource Type
Standards
Formats Included
  • PDF
  • Google Apps™
Pages
5 pages
$2.75
$2.75
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Sarah's STEM stuff
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Includes Google Apps™
The Teacher-Author indicated this resource includes assets from Google Workspace (e.g. docs, slides, etc.).

What educators are saying

Grab-and-go. Easy to use. Kept my students focused on how mass and distance affect gravitation force -- key points in our study of gravity. I broke this up into 2 days for our homeschool, to allow time for independent exploration with the simulator and discussion.
The content quality was exceptional, and the creativity of the materials kept my students enthusiastic and eager to participate. As an educator, I greatly appreciated the resource's versatility and the ease of implementation in my classroom.
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Description

Students use a PhET computer simulation of the Earth and Sun orbit to see how different variables affect the orbit and the force of gravity between the two objects.
In this computer model, students change variables (mass and distance) of the Earth and Sun to see how they affect the force of gravity and the orbit of the Earth. In the first part of the activity, students observe the Earth’s orbit around the sun under ”normal” conditions. In part 2, students look at the relationship between mass and the force of gravity and how that affects the Earth’s orbit around the sun. In part 3, the students investigate the relationship between distance from the sun and the force of gravity and how that affects Earth’s orbit.


NGSS Alignment:
MS-ESS1-2. Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.
MS-PS2-4. Construct and present arguments using evidence to support the claim that gravitational interactions are attractive and depend on the masses of interacting objects.

This activity can be printed and used in class or use a link to make a copy of a digital google doc to complete it electronically.

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Total Pages
5 pages
Answer Key
Included
Teaching Duration
45 minutes
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Standards

to see state-specific standards (only available in the US).
NGSSMS-PS2-4
Construct and present arguments using evidence to support the claim that gravitational interactions are attractive and depend on the masses of interacting objects. Examples of evidence for arguments could include data generated from simulations or digital tools; and charts displaying mass, strength of interaction, distance from the Sun, and orbital periods of objects within the solar system. Assessment does not include Newton’s Law of Gravitation or Kepler’s Laws.
NGSSMS-ESS1-2
Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system. Emphasis for the model is on gravity as the force that holds together the solar system and Milky Way galaxy and controls orbital motions within them. Examples of models can be physical (such as the analogy of distance along a football field or computer visualizations of elliptical orbits) or conceptual (such as mathematical proportions relative to the size of familiar objects such as students’ school or state). Assessment does not include Kepler’s Laws of orbital motion or the apparent retrograde motion of the planets as viewed from Earth.

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