Mission to Mars: Learning Resource

Introduction to Mars

Mars, often called the "Red Planet," is the fourth planet from the Sun in our solar system. It's named after the Roman god of war because of its reddish appearance, which is due to iron oxide, commonly known as rust, on its surface.

Mars has a thin atmosphere composed mainly of carbon dioxide, with traces of nitrogen and argon. The surface of Mars is rocky, with features such as volcanoes, valleys, deserts, and polar ice caps. It's a cold desert world, with temperatures often dropping to -80 degrees Fahrenheit (-60 degrees Celsius).

Key Topics: Mars' Environment

Atmosphere

Mars has a very thin atmosphere, about 100 times thinner than Earth's. It's mostly made up of carbon dioxide (95%), with small amounts of nitrogen (2.7%) and argon (1.6%). There is very little oxygen and water vapor. Because of this thin atmosphere, Mars cannot retain heat, leading to extreme temperature fluctuations.

Surface Conditions

The surface of Mars is a cold, barren desert. It's covered with dust and rocks, and experiences massive dust storms that can last for weeks. Mars has the largest volcano in the solar system, Olympus Mons, and a canyon system, Valles Marineris, that is 4,000 kilometers long and up to 7 kilometers deep.

Potential for Human Life

The potential for human life on Mars is a topic of great interest. The planet's extreme conditions, lack of liquid water, and harmful radiation make it a challenging environment for humans. However, scientists are exploring ways to create sustainable habitats, grow food, and generate water and oxygen from the Martian environment.

Quiz: Journey to Mars

Oxygen
Carbon Dioxide
Nitrogen
Lack of liquid water
Too much vegetation
High oxygen levels

Matching Activity: Mars Environment

Atmosphere
Surface Conditions
Potential for Human Life
Thin layer, mostly carbon dioxide
Rocky terrain with dust storms
Lack of water, extreme temperatures