Was there ever a fifth rocky, terrestrial planet in our Solar System? If so, it was located beyond the orbit of Mars in what is now the asteroid belt. John Chambers (Carnegie Institute of Washington) likes to call the hypothetical world ‘Artemis,’ and at the 2006 Astrobiology Science Conference in Washington DC this March, he described how the planet might have formed.

The trick, of course, is to account for the orbits of the giant planets, which some believe underwent a shift from almost circular to more highly eccentric (elliptical) orbits. If you set up a simulation with Jupiter in a circular orbit, terrestrial worlds form out to about 2.2 AU. From an abstract of Chambers’ presentation:

Artemis could have formed in a region that was stable before the giant planets’ shift, but unstable thereafter, probably between 1.8-2.2 AU. We simulate the giant planets’ orbital shift to explore Artemis’ demise, varying Artemis’ mass and starting location. In each simulation, the giant planets’ eccentricity jump causes a increase in the terrestrial planets’ eccentricities, sometimes causing their orbits to cross and collisions to occur.

What Chambers finds is that in most scenarios involving collisions or ejection of a planet from the Solar System, the remaining terrestrial worlds are pushed into orbits that are more elliptical than we observe today. If Artemis ever existed, it must have been destroyed quickly to make today’s orbits possible. An abstract of Chambers’ paper “Planet Artemis: the case for the formation and delayed destruction of a fifth Solar System terrestrial planet” can be found here.