The planet Mars shares numerous characteristics with our own. Both planets have roughly the same amount of land surface area, sustained polar caps, and both have a similar tilt in their rotational axes, affording each of them strong seasonal variability. Additionally, both planets present strong evidence of having undergone climate change in the past.

At the same time, our two planets are really quite different, and in a number of important ways. For instance, atmospheric pressure on Mars is only a fraction of what it is here on Earth – averaging 7.5 millibars on Mars to just over 1000 here on Earth. The average surface temperature is also lower on Mars, ranking in at a frigid -63 °C compared to Earth’s balmy 14 °C. And while the length of a Martian day is roughly the same as it is here on Earth (24 hours 37 minutes), the length of a Martian year is significantly longer (687 days).

But one big difference is that the gravity on Mars’ surface is much lower than it is here on Earth – 62% lower to be precise. At just 0.38 of the Earth standard, a person who weighs 100 kg on Earth would weigh only 38 kg on Mars.

This difference in surface gravity is due to a number of factors – mass, density, and radius being the foremost. Even though Mars has almost the same land surface area as Earth, it has only half the diameter and less density than Earth – possessing roughly 15% of Earth’s volume and 11% of its mass.

Scientists have calculated Mars’ gravity based on Newton’s theory of gravity, which states that the gravitational force exerted by an object is proportional to its mass. When applied to a spherical body like a planet with a given mass (in this case, Mars), the surface gravity will be approximately inversely proportional to the square of its radius. When applied to a spherical body with a given average density, it will be approximately proportional to its radius.

These proportionalities can be expressed by the formula *g* = *m*/*r*^{2}, where *g* is the surface gravity of Mars (expressed as a multiple of the Earth’s*,* which is 9.8 m/s²), *m* is its mass – expressed as a multiple of the Earth’s mass (5.976·10^{24} kg) – and *r* its radius, expressed as a multiple of the Earth’s (mean) radius (6,371 km).

For instance, Mars has a mass of 6.4185·10^{23} kg, which is 0.107 Earth masses. It also has a mean radius of 3,390 km, which works out to 0.532 Earth radii. The surface gravity of Mars can therefore be expressed mathematically as: 0.107/0.532², from which we get the value of 0.38. Based on the Earth’s own surface gravity, this works out to an acceleration of 3.724 meters per second².

Understanding Mars’ gravity and its affect on terrestrial beings is an important first step if we want to send astronauts, explorers, and even settlers there someday. Basically, the effects of long-term exposure to gravity that is just over one-third the Earth normal will be a key aspect of any plans for upcoming manned missions or colonization efforts.

For example, crowd-sourced projects like Mars One make allowances for the likelihood of muscle deterioration and osteoporosis for their participants. Citing a recent study of International Space Station (ISS) astronauts, they acknowledge that mission durations ranging from 4-6 months show a maximum loss of 30% muscle performance and maximum loss of 15% muscle mass.

Their proposed mission not only calls for many months in space to get to Mars, but for those volunteering to spend the rest of their lives living on the Martian surface. However, they also claim that they intend to lower these numbers and that their astronauts will be “well prepared with a scientifically valid countermeasures program that will keep them healthy, not only for the mission to Mars, but also as they become adjusted to life under gravity on the Mars surface.” What these measures are remains to be seen.

Learning more about Martian gravity and how terrestrial organisms fare under it could be a boon for space exploration and missions to other planets as well. And as more information is produced by the many robotic lander and orbiter missions on Mars, as well as planned manned missions, we can expect to get a clearer picture of what Martian gravity is like up close. As we get closer to NASA’s proposed manned mission to Mars, which is currently scheduled to take place in 2030, we can expect more research efforts to be attempted.

Here’s an article on Universe Today about how the reduced Martian gravity will be tested on mice in space. And another about how the lower gravity on Mars helps it make huge sand dunes.

Information on the Mars Gravity Biosatellite. And the kids might like this; a project they can build to demonstrate Mars gravity.

Finally, if you’d like to learn more about Mars in general, we have done several podcast episodes about the Red Planet at Astronomy Cast. Episode 52: Mars, and Episode 91: The Search for Water on Mars.

Sources:

http://solarsystem.nasa.gov/planets/profile.cfm?Object=Mars&Display=Facts

http://web.mit.edu/newsoffice/2004/mars-biosatellite.html

Mars One and how the mission will affect astronauts

{ 6 comments… add one }

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Sooo.. If we were to find a suitable lava tube on Mars and pressurize it, man COULD fly under his own power? Strap on a set of wings, and go for it!

Additionally, with only 3/8 gravity, how far could you leap or long jump? How fast could you run? Martian Olympic Games anyone? ON Mt. Olympus?

Long jump . . . probably about 40 feet for someone in good shape. Given that, I’d expect you could probably run about 40 mph. Only problem is, no atmosphere, so you’d be tied to a spacesuit, adding to your weight. Given some really huge lava tubes though, it could be riot.

You could not run faster on Mars because your feet would have less contact with the ground so you have less strides but your strides would be longer on Mars than they are running here on Earth, But you could throw a javelin for example much further on Mars than on Earth…Sounds like fun

Why are there comments from 2008 here?

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