The gravity of the Red Planet causes the asteroid's surface material to shift, exposing fresh material, which explains the colour variation previously observed.
Richard Binzel, a professor of planetary sciences at Massachusetts Institute of Technology (MIT) and colleague Francesca DeMeo calculated the orbits of 60 refreshed asteroids, and found that 10 per cent of these never cross Earth's orbit.
Instead, these asteroids only come close to Mars, suggesting that the Red Planet can refresh the surfaces of these asteroids.
The idea that Mars may shake up the surface of an asteroid is a surprising one: The planet is one-third the size of Earth, and one-tenth as massive - and therefore exerts a far weaker gravitational pull on surrounding objects.
But Mars' position in the solar system places the planet in close proximity with the asteroid belt, increasing the chance of close asteroid encounters.
"So that may be a balancing factor," said Binzel.
DeMeo, who suspected that Mars may have a hand in altering asteroid surfaces, looked through an asteroid database created by the International Astronomical Union's Minor Planet Center.
The researchers looked at 60 asteroids, mapping out the orbit of each and determining which orbits had intersected with those of Earth or Mars.
DeMeo then calculated the probability, over the last 500,000 years, that an asteroid and either planet would have intersected, creating a close encounter that could potentially generate asteroid quakes.
"If they just barely miss each other, that's close enough for Mars' gravity to tug on (the asteroid) and shake it up. It ends up being this random process as to how these things happen, and how often," said Binzel.
From their calculations, the researchers found that 10 per cent of their sample of asteroids only cross Mars' orbit, and not Earth's.
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