Now, a new set of theoretical models from Carnegie's Alan Boss shows how an outburst event in the Sun's formative years could explain some of this disparate evidence.
His work could have implications for the hunt for habitable planets outside of our solar system.
One way to study the solar system's formative period is to look for samples of small crystalline particles that were formed at high temperatures but now exist in icy comets.
Another is to analyze the traces of isotopes-versions of elements with the same number of protons, but a different number of neutrons-found in primitive meteorites.
These isotopes decay and turn into different, so-called daughter, elements.
The initial abundances of these isotopes tell researchers where the isotopes may have come from, and can give clues as to how they traveled around the early solar system.
Stars are surrounded by disks of rotating gas during the early stages of their lives.
Observations of young stars that still have these gas disks demonstrate that sun-like stars undergo periodic bursts, lasting about 100 years each, during which mass is transferred from the disk to the young star.
But analysis of particles and isotopes from comets and meteorites present a mixed picture of solar system formation, more complicated than just a one-way movement of matter from the disk to the star.
The heat-formed crystalline grains found in icy comets imply significant mixing and outward movement of matter from close to the star to the outer edges of the solar system. Some isotopes, such as aluminum, support this view.
However, isotopes of the element oxygen seem to paint a different picture.
Boss' new model demonstrates how a phase of marginal gravitational instability in the gas disk surrounding a proto-sun, leading to an outburst phase, can explain all of these findings.
The results are applicable to stars with a variety of masses and disk sizes.
The study is published by The Astrophysical Journal.
--ANI (Posted on 25-07-2013)