New evidence challenges the idea that Earth and Mars formed the same way
Earth and Mars may have formed through surprisingly different mixtures of pebble accretion, planetesimal collisions and giant impacts, despite growing beside each other in the same young Solar System. Chemical modeling suggests at least 75% of Earth’s mass came from two protoplanets that grew mainly by capturing pebbles, while roughly 73% of Mars came from volatile-depleted planetesimals. The study uses the loss of moderately volatile elements as a record of planetary growth, providing a possible new way to reconstruct the formation and habitability of rocky worlds around other stars. Earth and Mars emerged from the same swirling disk of gas and dust, separated today by less than 80 million kilometers at their closest approach. Their common birthplace might suggest that the two rocky planets were assembled through broadly similar processes. Their chemistry tells a different story. A University of Copenhagen-led study finds that Earth appears to have been built primarily from large protoplanets that themselves grew by sweeping up millimeter- to centimeter-sized pebbles. Mars, by contrast, acquired most of its mass from collisions with much …









