A long-lost moon could explain Mars' weird shape and extreme terrain

A long-lost moon could explain why Mars is so different from the other rocky planets in the solar system.

Today, Mars has two tiny moons. But early in its history, the Red Planet may have had a much larger moon, which might be responsible for Mars' weird shape and extreme terrain, Michael Efroimsky, an astronomer at the U.S. Naval Observatory in Washington, D.C., proposes in a paper that has been submitted to the Journal of Geophysical Research: Planets and is available as a preprint via arXiv.

Mars hosts some of the most extreme terrain in the solar system, including the largest canyon, the tallest mountain and the greatest highland region. This highland region, known as the Tharsis bulge or Tharsis rise, dominates Mars' western hemisphere near its equator. The Tharsis region is about 3,100 miles (5,000 kilometers) wide and rises up to 4.4 miles 7 (km) high, excluding its massive shield volcanoes, which rise even higher. Almost exactly on the opposite side of the planet from Tharsis sits Terra Sabaea and Syrtis Major, another highland region and massive shield volcano, respectively.

Either way, Nerio's significant mass altered the shape of Mars with its gravity, raising tides in the magma oceans the same way Earth's moon raises tides in our planet's oceans today. But because Mars is smaller than Earth, it cooled much more quickly and its tidal bulges became locked into the resulting form of the planet.

Somehow, Nerio got lost, Efroimsky wrote. It could have been obliterated by a collision, leaving behind Mars' current moons, Phobos and Deimos, he proposed, or it could have been scattered out of the solar system through a gravitational interaction with another body.

Such collisions and scatterings were common in the early solar system. Astronomers think Earth gained its moon through a collision with a Mars-size protoplanet and scatterings among the outer planets shifted their initial orbits, which were once much closer to the sun, into their present positions.

But as long as Nerio stayed around long enough to deform Mars as it cooled, it could have set the stage for that planet's dramatic landscape, Efroimsky said. Further geologic processes could have continued the work, uplifting the highlands and leading to Mars' odd shape.