
© NASA / JPL-Caltech / T. Pyle (SSC)Artist rendering of an early solar system.
The solar system's current planetary orbits seem stable, but that's only because the planets have settled into them
over billions of years. The early solar system was a much different place than that seen today, and for almost 20 years, scientists thought they had a good handle on how it got that way. But more recently, data had started pointing to some flaws in that understanding - especially about how the giant planets in the outer solar system got where they are today. Now an international team of astrophysicists thinks they have a better understanding of that process, and they believe it could help solve a long-standing argument about the early solar system.
Currently, the best model scientists have for the formation of the solar system is known as the Nice model, after the town in France, where it was first developed in 2005. As part of this model, the gas giants that currently reside in the outer fringes of this solar system originally orbited what became the sun much more closely with more circular orbits.
However, something caused instability in the system that kicked those planets out into the much more unevenly spaced and oblong orbits we see them in today.What exactly caused that anomaly has thus far been a mystery. However, a team comprised of researchers from Michigan State University, Zhejiang University, and the University of Bordeaux think they have an answer. It's as simple as dust in the (solar) wind.
Comment: See also: Did Earth 'Steal' Martian Water?