New Clues on How Jupiter and Saturn Formed
Astrophysicists and planetary geologists have long known that planets form around stars when dust particles accrete (gradually accumulate) to form pebbles which will coalesce into larger bodies, eventually becoming rocky planets or rocky cores of gaseous planets.
Figure 1. Illustration of planetary formation around a new-born star. Credit: Gemini Observatory/AURA Artwork by Lynette Cook
The problem, as with most astronomical phenomena, is the huge timescales in which things happen. We therefore rely on supercomputers to feed them data and get simulations which show us what happens in thousands, hundreds of thousands, millions, or billions of years.
Researchers at the Southwest Research Institute (Colorado, USA) and Queen’s University (Ontario, Canada) have fed these supercomputers gravitational effects, pebble generation and growth ratios, dust evolution, amounts of gas, velocity, collisional fragmentation and aerodynamic drag to simulate the formation of particles into full-sized planets, particularly in the case of the Solar System.
Their initial simulated results were standard for these studies, creating hundreds of Earth-sized objects in thousands of years, which we know is not consistent with our Solar System where only four rocky planets (Mercury, Venus, Earth and Mars) and five dwarf rocky planets (Ceres, Pluto, Haumea, Makemake and Eris) exist. So they came up with a novel idea: allowing the simulation to take longer to form the pebbles.
“It really is a paradigm shift for how planets form,” said lead author Harold Levison from the Southwest Research Institute to the journal Nature, where the work was recently published.
As we know little of the intricate details of the processes of planetary formation in nature, increasing the time scale in which these —> Read More