Moon and Mars

If you look at an elevation map of Mars, one thing really stands out: The northern hemisphere is a lot lower than the southern hemisphere. And planetary scientists are still trying to figure out why.

On average, the northern third of Mars is a mile or two lower than the rest of the planet. And there’s evidence that water once pooled there, forming a giant ocean.

There are several possible explanations for the difference in the two hemispheres.

One is that another planet-sized body slammed into Mars when it was young. The other world could have hit the northern hemisphere, excavating the deeper northern plains. Or it could have hit near the south pole, melting the upper layers of rock in the southern hemisphere. As the magma cooled, it left the southern hemisphere with a thicker crust.

Another idea is that the northern hemisphere was pounded by several big impacts.

And yet another says the cause was home-grown. Early Mars might have had plate tectonics like those on Earth. Motions in the crust and mantle could have piled up rocks in the southern hemisphere, making the crust there about 15 miles thicker than in the north.

Each of these ideas has problems, though. So there’s no final explanation for the “deep” difference in the Martian hemispheres.

Look for Mars near the Moon tonight. It looks like a bright orange star. It’s above the Moon at nightfall, and to the right of the Moon as they set in the wee hours of Thanksgiving.

Script by Damond Benningfield