Title: The Solar Nebula on Fire: A Solution to the Carbon Deficit in the Inner Solar System Authors: Jeong-Eun Lee, Edwin A. Bergin, Hideko Nomura
Despite a surface dominated by carbon-based life, the bulk composition of the Earth is dramatically carbon poor when compared to the material available at formation. Bulk carbon deficiency extends into the asteroid belt representing a fossil record of the conditions under which planets are born. The initial steps of planet formation involve the growth of primitive sub-micron silicate and carbon grains in the Solar Nebula. We present a solution wherein primordial carbon grains are preferentially destroyed by oxygen atoms ignited by heating due to stellar accretion at radii < 5 AU. This solution can account for the bulk carbon deficiency in the Earth and meteorites, the compositional gradient within the asteroid belt, and for growing evidence for similar carbon deficiency in rocks surrounding other stars.
Carbon deficit on Earth tied to fire in Solar System
Though our planet supports carbon-based life, it has a mysterious carbon deficit, but the element is thousands of times more abundant in comets in the outer solar system than on the earth, even the sun is rich in carbon. The conventional explanation for the deficit is that in the inner region of the dust disc where earth formed, temperatures soared above 1800 Kelvin, enough for carbon to boil away. But observations of developing solar systems suggested that at earth's distance from the sun, the temperature would be too cool to vaporise carbon dust. Now a team of astronomers from Sejong University in Seoul and the University of Michigan in Ann Arbor said fire sweeping through the inner solar system had "scorched away much of the carbon from earth and the other inner planets".