About Mars


As the fourth planet from the Sun, Mars is our terrestrial neighbor. Though this cold and dusty world has many differences compared to Earth, it also has many similarities. It has seasons, dry river beds, polar ice caps and volcanoes. The length of a day on Mars is only 40 minutes longer than on Earth, and though It is half the size of our home world, it has roughly the same land area because there is no liquid water on the surface. The Red Planet, as it is sometimes called, is one of the most explored bodies in our solar system. Multiple space agencies have undertaken missions to Mars using landers, rovers, orbiters and a wide variety of instruments. The international effort to understand this fascinating world continues to grow, as we prepare to send the first human crews. With mounting evidence that it once had a wet, warm climate, Mars is suspected to have hosted life in the past.


The Red Planet took form roughly 4.5 billion years ago through a process known as accretion. Particles of gas and dust orbiting our sun were slowly pulled together by the force of gravity to form the single mass we now call Mars. It is classified as a terrestrial planet as a result of the fact that it is made primarily of rock and metal, with a core of iron, nickel and sulfur. The mantle and crust covering this core are composed of rock, iron, magnesium, aluminum, calcium and potassium. 


The surface of Mars is rugged, having been shaped over billions of years through a combination of asteroid impacts, wind, volcanoes and chemical reactions. The reddish hue that gives the Red Planet its nickname comes from the rusting (oxidization) of iron, which is distributed in Martian rocks, regolith and dust. This ancient, battered landscape features some of our solar system’s most striking geological features. The volcano Olympus Mons towers at 13.6 miles in height, more than two and a half times taller than Mount Everest, and is so wide that from the perspective of an astronaut at the summit, it would appear to stretch to the horizon. The Martian canyon of Valles Marineris is so large (2,500 miles long, 4 miles deep) that some mountain ranges on Earth could be hidden inside it. 


The atmosphere on Mars is made mostly of carbon dioxide, nitrogen and argon gas. It is very thin, at roughly 1% the density of our atmosphere on Earth, because it has been blowing away in solar winds for millennia due to the lack of a planetary magnetic field. The thinness of the Martian atmosphere provides little protection against radiation or asteroid impact on the surface, but it offers a significant reservoir of valuable gas for the production of oxygen and fuel. The temperature on Mars varies between 70 and negative 225 degrees Fahrenheit, though this variability is much less in specific regions such as the equator. The winds on Mars can blow up to 60 miles per hour, however, since the atmosphere is so sparse, this would only feel like a light breeze here on Earth. 

This artist’s impression shows how Mars may have looked about four billion years ago. The young planet Mars would have had enough water to cover its entire surface in a liquid layer about 140 metres deep, but it is more likely that the liquid would have pooled to form an ocean occupying almost half of Mars’s northern hemisphere, and in some regions reaching depths greater than 1.6 kilometres.

Water On Mars

Mars has enormous volumes of water trapped in the form of ice. It is estimated that the entire surface would be covered in a layer of water 35 meters deep, if that ice were melted. It is also suspected that additional water exists below the surface in the form of a highly saline (salty) brine, and that perhaps a large quantity is trapped in minerals within the planet’s crust. It is thought that this water was once in liquid form on the Martian surface. This theory is supported by substantial evidence, including the apparent presence of dried river beds. This vast amount of water may have harbored life in the past (and perhaps still today), and will be a valuable resource for human explorers on the Red Planet.

Life on Mars

The only place we have ever discovered life is here on Earth, for now. All living things on our home world require a source of energy (or food) and liquid water. Mars once had a warm and wet climate, and still has many essential nutrients for life such as potassium, magnesium and nitrogen. Not only is it possible that Mars once hosted life, but there is also a chance that organisms still exists beneath the surface. We continue to search for signs of Martian life, most recently with the NASA Perseverance rover. Discovering proof of past or present organic activity on Mars would have significant implications for the prevalence of life in our galaxy.

Future Mars colonists may have children who have never known the earthly blue skies of their parents origin but instead call Mars home.

Mars Settlement

To be written

Mars Geology

To be written