How Terraforming Mars Will Work

We have been going to space for decades now, but until the year 2000, those stays in orbit were always temporary. However, when three astronauts moved into the International Space Station (ISS) for a four-month stay, it marked the beginning of a decade an­d a half of a permanent human presence in space. The arrival of these three astronauts at the ISS on Nov. 2, 2000, sparked one NASA official to remark, “We’re going into space forever with people first circling this globe, and then we’re going to Mars….”

Why would we ever want to go to Mars? As pictures beamed back from planetary probes and rovers since 1964 have shown, Mars is a desolate, lifeless planet with seemingly little to offer humans. It has a very thin atmosphere and no signs of existing life — but Mars does hold some promise for the continuation of the human race. There are more than six billion people on Earth, and that number continues to grow unabated. This overcrowding, or the possibility of planetary disaster, will force us to eventually consider new homes in our solar system, and Mars may have more to offer us than the photos of its barren landscape now show.
Mars has all of the elements needed to support life.
Mars has all of the elements needed to support life.
PHOTO COURTESY NASA
Mars has long held a special fascination in the human imagination, as is witnessed by the scores of books and movies that have been produced about the planet in the last century alone. Each story creates its own unique image of what might exists on the red planet. What is it about Mars that makes it the subject of so many tales? While Venus is often referred to as Earth’s sister planet, the conditions that exist on that fiery planet are far too uninhabitable. On the other hand, Mars is the next closest planet to us. And although it is a cold, dry planet today, it holds all of the elements that are needed for life to exist, including:

Water, which may be frozen at the polar ice caps
Carbon and oxygen in the form of carbon dioxide (CO2)
Nitrogen
There are amazing similarities between the Martian atmosphere that exists today and the atmosphere that existed on Earth billions of years ago. When the Earth was first formed, no oxygen existed on our planet and it, too, looked like a desolate, unlivable planet. The atmosphere was made entirely of carbon dioxide and nitrogen. It wasn’t until photosynthetic bacteria developed on Earth that enough oxygen was produced to allow for the development of animals. Similarly, the thin Mars atmosphere today is almost totally composed of carbon dioxide. Here is the composition of Mars’ atmosphere:

95.3 percent carbon dioxide
2.7 percent nitrogen
1.6 percent argon
0.2 percent oxygen
In contrast, Earth’s atmosphere consists of 78.1 percent nitrogen, 20.9 percent oxygen, 0.9 percent argon and 0.1 percent carbon dioxide and other gases. As you can see by this breakdown, any humans visiting Mars today would have to carry with them huge amounts of oxygen and nitrogen in order to survive. However, the similarity to the early Earth and modern Mars atmospheres has led some scientists to speculate the same process that turned the Earth’s atmosphere from mostly carbon dioxide into breathable air could be repeated on Mars. To do so would thicken the atmosphere and create a greenhouse effect that would heat the planet and provide a suitable living environment for plants and animals.

The average surface temperature on Mars is a frigid minus 81 degrees Fahrenheit (-62.77 degrees Celsius) with extremes that range from 75 degrees Fahrenheit (23.88 Celsius) to less than minus 100 degrees Fahrenheit (-73.33 Celsius). In comparison, Earth’s average surface temperature is about 58 degrees Fahrenheit (14.4 degrees Celsius). However, there are a few Martian features that are close enough to Earth’s to consider it for habitation, including:

A rotation rate of 24 hours 37 min (Earth: 23 hours 56 min.).
An axial tilt of 24 degrees (Earth 23.5 degrees).
A gravitational pull one-third of Earth’s
It is close enough to the sun to experience seasons. Mars is about 50 percent farther from the sun than Earth.
Other worlds have been considered as possible candidates for terraforming, including Venus, Europa (a Jupiter moon), and Titan (a Saturn moon). However, Europa and Titan are too far from the sun, and Venus is too close (the average temperature on Venus is about 900 degrees Fahrenheit (482.22 Celsius)). Mars stands alone as the one planet in our solar system, not including Earth, that might be able to support life. In the next section, learn how scientists plan to transform the dry, cold landscape of Mars into warm, livable habitat.

You may also like...