Understanding Planet Formation and the Kuiper Belt

Understanding Planet Formation and the Kuiper Belt

Assessment

Interactive Video

Physics

9th - 10th Grade

Hard

Created by

Nancy Jackson

FREE Resource

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the primary mission of NASA's New Horizons spacecraft in 2019?

To capture images of MU69 in the Kuiper Belt

To land on the moon

To explore the surface of Mars

To study the atmosphere of Jupiter

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How did MU69 form according to the video?

By the fusion of multiple small asteroids

Through volcanic activity on a larger planet

Through the gentle coalescence of two orbiting bodies

By a high-speed collision of two planetesimals

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the core accretion model?

A process for creating artificial satellites

A theory explaining the formation of stars

A method for measuring the age of the solar system

A model describing how planets form from dust, pebbles, and planetesimals

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why are planets in the outer solar system generally larger than those closer to the sun?

They are closer to the gravitational pull of the sun

They are made of denser materials

They formed earlier than inner planets

They have more solid material to form from beyond the frost line

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the frost line in the context of the solar system?

The boundary where the sun's heat is strongest

The point where water freezes and becomes solid ice

The region where planets stop forming

The area where comets originate

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does the presence of water ice beyond the frost line affect planet formation?

It doubles the amount of solid planet-forming material

It makes the planetesimals less sticky

It decreases the amount of solid material available

It prevents the formation of gas giants

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a key challenge in applying the core accretion model to Jupiter's formation?

The timing to build a core is too long compared to the sun's heat increase

The model predicts too rapid a formation

The model suggests Jupiter should be smaller

The model does not account for Jupiter's moons

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