The differences between dusty Mars and lush, vibrant Earth are more than just skin deep. The two planets are different down to their very core.
Earth contains a heavy version of silicon that is absent from Mars.
The finding, detailed in today's issue of the journal Nature, suggests Earth’s core formed under very different conditions from those on Mars. It also supports the idea that the moon formed from material torn from early Earth by a collision with a planet-sized rock.
Rock samples from Mars and the giant asteroid Vesta show they contain a lighter form, or “isotope,” of silicate that is identical to those found in a primitive class of meteorites called chondrites. Scientists think chondrites are shed remnants of the original building blocks of planets that have fallen to Earth. Silicates are compounds made of silicon and oxygen mixed with other elements.
“The most likely explanation is that, unlike Mars or Vesta, the Earth’s silicon has been divided into two sorts—a portion that became a light element in the Earth’s core dissolved in metal and the greater proportion which formed the silicon-oxygen bonded silicate of the Earth’s mantle and crust,” said study team member Alex Halliday of Oxford University in the United Kingdom.
Earth is eight times more massive than Mars, and this could partly explain the differences in the planets’ core compositions, the scientists say. It might be that silicates in our planet’s core transformed into denser forms under the greater pressure conditions on Earth.
The finding is, however, consistent with the theory that our Moon was born when a Mars-sized planet, usually called “Theia,” collided with early Earth. The impact carved out a large molten chunk from Earth which eventually coalesced into the Moon.
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