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PhET Activity for MS-ESS1-1: Gravity & Orbits

PhET Activity for MS-ESS1-1: Gravity & Orbits

Assessment

Passage

•

Science

•

6th Grade

•

Hard

Created by

Wayground Simulations

FREE Resource

17 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

3 mins • Ungraded

Media Image

DIRECTIONS:
1. You should be on the initial screen with two options: 'Model' and 'To Scale'. Click on the 'Model' image on the left side of the screen.
2. You are now in the 'Model' tab with the 'Sun and Planet' preset. Observe the central star and the orbiting planet.
3. In the control panel on the right, check the boxes for 'Velocity', 'Gravity Force', 'Path', and 'Grid'.
4. At the bottom of the screen, locate the Play/Pause button and the simulation speed controls.
5. Press the play button to start the simulation and observe the planet's motion.
Spend 2-3 minutes exploring the simulation. Press play and pause. Use the speed controls to see the simulation run faster or slower. Click the reset button (circular arrow in the top-right panel) to see how it works. Do not change the mass sliders yet.

QUESTION: Are you acquainted with the tools in this simulation?

Yes

No

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

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DIRECTIONS:
1. Ensure you are in the 'Model' tab with the 'Sun and Planet' preset.
2. Click the reset button (circular arrow in the top-right panel).
3. Make sure the 'Gravity Force' checkbox on the right panel is checked. You should see blue arrows on the star and planet.
4. Press the play button and observe the direction of the blue force arrows as the planet orbits.

QUESTION: What do the blue arrows represent, and what is their effect on the planet?

They represent the planet's speed, which pushes it away from the star.
They represent the gravitational force, which pulls the planet toward the star and keeps it in orbit.
They represent a magnetic force, which has no effect on the orbit.
They represent the star's energy, which is transferred to the planet.

Answer explanation

The blue arrows show the gravitational force. This force acts as a centripetal force, constantly pulling the planet towards the star, which prevents it from moving in a straight line and instead keeps it in a curved orbital path.

3.

FILL IN THE BLANKS QUESTION

1 min • 1 pt

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DIRECTIONS:
1. Start in the 'Model' tab with the 'Sun and Planet' preset. Click the reset button (circular arrow in the top-right panel).

2. Ensure the 'Gravity Force' and 'Path' checkboxes are selected.
3. Press play and let the planet complete one orbit to see the default path.
4. While the simulation is running, use the 'Star Mass' slider in the bottom-right panel to increase the mass to its maximum value (2.0).
5. Observe the change in the size of the force arrows and the planet's new path.

QUESTION: When the star's mass is increased, the gravitational force ___ and the planet is pulled into a ___ orbit.

(a)  

Answer explanation

increases, smaller

4.

DROPDOWN QUESTION

1 min • 1 pt

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DIRECTIONS:
1. Click the reset button (circular arrow in the top-right panel).
2. Press play and observe the default orbit.
3. While the simulation is running, use the 'Planet Mass' slider to change its mass from 'Earth' to maximum (2.0).
4. Carefully observe the planet's orbital path.

QUESTION: Changing the planet's mass has a (a)   effect on its orbital path.

very large
negligible
reversing

Answer explanation

The correct answer is 'negligible'. While the planet's mass does affect the gravitational force, the star's mass is so dominant in this model that changing the planet's mass doesn't noticeably alter its orbit. Both objects actually orbit a common center of mass, but it's very close to the center of the massive star.

5.

OPEN ENDED QUESTION

3 mins • 1 pt

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DIRECTIONS:
1. Click the reset button (circular arrow in the top-right panel).
2. Set the 'Star Mass' slider to its minimum value (0.5).
3. Set the 'Planet Mass' slider to its maximum value (2.0).
4. Make sure 'Path' is checked. Press play.
5. Observe the motion of the star.

QUESTION: Describe what you observe about the star's motion when its mass is low and the planet's mass is high. Why do you think this happens?

Evaluate responses using AI:

OFF

Answer explanation

A good answer should state that the star is observed to wobble or move in a small circle. This happens because the planet's gravity is also pulling on the star, just as the star's gravity pulls on the planet. Both objects are orbiting a common center of mass, which is now noticeably outside the center of the star.

6.

MATCH QUESTION

1 min • 1 pt

DIRECTIONS:
1. Click the reset button (circular arrow in the top-right panel).
2. Make sure the simulation is paused. The green velocity vector should be visible on the planet.
3. Experiment by clicking and dragging the head of the green velocity vector to make it shorter or longer before pressing play.
4. Reset the simulation after each trial to test a new velocity.

QUESTION: Match the change in initial velocity to the resulting orbital outcome.

Causes the planet to crash into the star
Significantly increasing the initial speed

Creates a larger, elliptical (oval) obit

Significantly decreasing the initial speed
Causes the planet to escape the star's gravity
Slightly increasing the initial speed

Answer explanation

Slightly increasing speed leads to an elliptical orbit. Decreasing speed too much means the planet can't maintain its distance and falls into the star. Increasing speed too much allows the planet to achieve escape velocity and leave the system.

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

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DIRECTIONS:
1. Click the reset button (circular arrow in the top-right panel).
2. Press play and let the planet travel for a few seconds.
3. While the planet is moving, turn gravity off using the 'Gravity' toggle switch in the right-hand panel.

QUESTION: What happens to the planet's motion when gravity is turned off?

It stops moving immediately.
It continues in a straight line tangent to its previous orbit.
It flies directly away from the star.
It continues to orbit but in a much larger circle.

Answer explanation

The planet continues in a straight line. This demonstrates Newton's First Law of Motion (inertia): an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force. The straight line is tangent to the point in the orbit where gravity was turned off.

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