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PhET Activity for MS-ESS1-3: Gravity & Orbits

PhET Activity for MS-ESS1-3: Gravity & Orbits

Assessment

Passage

•

Science

•

6th Grade

•

Medium

Created by

Wayground Simulations

Used 4+ times

FREE Resource

15 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

3 mins • Ungraded

Media Image

DIRECTIONS:
1. Click on the 'Model' button on the initial screen.
2. Press the large blue play button at the bottom of the screen to start the simulation.
3. Observe the planet orbiting the sun.
4. Use the play/pause button to start and stop the motion.
5. On the right panel, check and uncheck the boxes for 'Velocity', 'Path', and 'Grid' to see what they do.
Spend 2-3 minutes exploring the simulation. Try the playback controls and the checkboxes on the right. Do not change any mass sliders or move the objects yet.

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

Yes

No

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

DIRECTIONS:
1. Click the circular arrow 'Reset' button in the top right panel.
2. Press the play button to start the orbit.
3. After the planet has moved for a few seconds, click the 'off' option on the 'Gravity' switch in the right panel.

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

It stops moving immediately.
It flies off in a straight line.
It crashes into the sun.
It continues to orbit the sun normally.

Answer explanation

The planet flies off 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 (gravity).

3.

FILL IN THE BLANKS QUESTION

1 min • 1 pt

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DIRECTIONS:
1. Click the big orange 'Reset' button in the bottom right corner. This will also turn gravity back on.
2. Check the box for 'Gravity Force' in the right panel.
3. Press the play button.

QUESTION: The blue gravity force arrows always point from the center of the planet towards the center of the ___ and from the center of the sun towards the center of the ___.

(a)  

Answer explanation

sun, planet

4.

DROPDOWN QUESTION

1 min • 1 pt

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DIRECTIONS:
1. Ensure the 'Gravity Force' box is still checked from the previous slide.
2. Now, check the box for 'Velocity' in the right panel.

QUESTION: The planet's velocity vector is always (a)   to the curved orbital path.

perpendicular
tangent
parallel
opposite

Answer explanation

The correct answer is 'tangent'. The velocity of an object in circular or elliptical motion is always tangent to its path at any given point.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Media Image

DIRECTIONS:
1. Click the small 'Reset' button in the top right corner.
2. In the right panel, move the 'Star Mass' slider all the way to the right, setting it to 2.0.
3. Check the boxes for 'Path' and 'Gravity Force'.
4. Press the play button.

QUESTION: When the star's mass is doubled, what happens to the gravitational force and the planet's orbit?

The force decreases, and the planet drifts away.
The force is unchanged, and the orbit is the same.
The force increases, and the planet is pulled into a tighter, faster orbit.
The force increases, but the planet's orbit does not change.

Answer explanation

The force increases, and the planet is pulled into a tighter, faster orbit. According to Newton's Law of Universal Gravitation, the force is directly proportional to the mass of the objects.

6.

OPEN ENDED QUESTION

3 mins • 1 pt

Media Image

DIRECTIONS:
1. Click the small 'Reset' button in the top right corner. This will reset the star's mass to its default value (Our Sun).
2. Move the 'Planet Mass' slider all the way to the right, setting it to 2.0.
3. Check the 'Path' box.
4. Press play and observe the orbit.

QUESTION: Describe what you observed when you doubled the planet's mass. Did it significantly change the planet's orbital path around the sun? Why do you think this is?

Evaluate responses using AI:

OFF

Answer explanation

A good answer should note that doubling the planet's mass has little to no visible effect on its orbital path. While it does technically increase the gravitational force, the planet's increased inertia cancels out the effect of the increased force, resulting in the same orbital path. The sun's mass is so dominant that the planet's mass change is negligible for the orbit's shape.

7.

MATCH QUESTION

1 min • 1 pt

DIRECTIONS:
1. Click the small 'Reset' button in the top right corner.
2. Check the 'Velocity' and 'Path' boxes if not already done.
3. With the simulation paused, click and drag the tip of the green velocity arrow to make it about half its original length without changing its direction.
4. Press play and observe the path.
5. Reset the simulation again. This time, drag the velocity arrow to make it about 50% longer again without changing its direction.
6. Press play and observe the path.

QUESTION: Match the initial velocity setting with the most likely outcome for the planet's orbit.

Stable, near-circular orbit
Significantly shorter velocity vector
Wider, elliptical orbit or escapes gravity
Significantly longer velocity vector
Planet falls into the star
Default velocity vector

Answer explanation

A shorter velocity means the planet isn't moving fast enough to counteract gravity, so it falls inward. The default velocity is balanced for a stable orbit. A much longer velocity means the planet has too much energy to be held in a tight orbit, so it moves into a wider orbit or escapes entirely.

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