Venus: Geological and Atmospheric Features

Venus: Geological and Atmospheric Features

Assessment

Interactive Video

Science

9th - 10th Grade

Hard

Created by

Patricia Brown

FREE Resource

Venus, our closest planetary neighbor, is a world of extremes with a dense, toxic atmosphere and a surface temperature reaching 900°F. Despite its harsh conditions, Venus holds clues to planetary evolution and climate change. Its unique retrograde rotation and long day-night cycle contribute to its mystique. Historical and geological studies suggest Venus may have once harbored oceans. Future missions aim to uncover more secrets, offering insights into planetary climates and the delicate balance needed for life.

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10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What makes Venus similar to Earth?

Its magnetic field

Its surface temperature

Its size and mass

Its atmosphere

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the primary cause of Venus's high surface temperatures?

Lack of water

Greenhouse effect

Volcanic activity

Proximity to the Sun

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is a unique feature of Venus's atmosphere?

It has a strong magnetic field

It is thin and clear

It is composed of nitrogen

It contains sulfuric acid clouds

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What geological feature covers over 80% of Venus's surface?

Ice caps

Oceans

Deserts

Volcanic plains

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why is Venus's surface pressure so high?

Because of its distance from the Sun

Because of its thick atmosphere

Due to its fast rotation

Due to its magnetic field

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

How does Venus's rotation differ from Earth's?

It has a retrograde rotation

It has a 24-hour day

It rotates faster

It rotates in the same direction

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is believed to be the composition of Venus's core?

Iron and nickel

Silicon and oxygen

Carbon and hydrogen

Magnesium and aluminum

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