Mars Geological and Atmospheric Features

Mars Geological and Atmospheric Features

Assessment

Interactive Video

Science, Geography, History

9th - 12th Grade

Hard

Created by

Patricia Brown

FREE Resource

The video explores various intriguing anomalies on Mars, from the famous 'Face on Mars' to the mysterious reoccurring slope lineae, dust devils, and hemispherical dichotomy. It delves into Mars' magnetic anomalies, the discovery of hematite 'blueberries', and the unique aania form terrain. The video also discusses Mars quakes, methane spikes, and the vast Valis Marineris canyon, highlighting their significance in understanding Mars' geological history and potential for life.

Read more

10 questions

Show all answers

1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What was the 'face on Mars' in the Sidonia region later identified as?

A volcanic formation

A human-made structure

An alien artifact

A natural mesa

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are the recurring slope lineae (RSL) on Mars now thought to be caused by?

Liquid water

Ice melting

Dry granular flows

Lava flows

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What role do Martian dust devils play in the maintenance of rovers?

They protect from radiation

They recharge batteries

They clean solar panels

They provide energy

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What is the hemispherical dichotomy on Mars?

A variation in temperature

A difference in magnetic fields

A difference in atmospheric pressure

A contrast in terrain between hemispheres

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What do the magnetic anomalies on Mars suggest about its past?

Mars was once a gas giant

Mars had a thicker atmosphere

Mars had a global magnetic field

Mars was closer to the Sun

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What are the 'blueberries' discovered by the Opportunity Rover composed of?

Silicon dioxide

Iron oxide

Magnesium sulfate

Hematite

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

What causes the 'spider' formations near the Martian South Pole?

Wind patterns

Sublimation of carbon dioxide ice

Water erosion

Volcanic activity

Create a free account and access millions of resources

Create resources
Host any resource
Get auto-graded reports
or continue with
Microsoft
Apple
Others
By signing up, you agree to our Terms of Service & Privacy Policy
Already have an account?