H
harmonicaman
Guest
<p>(OK, Bonzelite, I'll expand on my thoughts - but it's mere speculation and begs supporting evidence...)<br /><br />I think the ignition of a star and the ensuing Solar Wind are important developments in a new Solar System's creation. I would propose that this event causes fundamental changes to the orbital mechanics of the accretion disc and the newly forming planets. <br /><br />This change in the status quo of the accretion disc likely contributes to the creation of spherical Kuiper Belt and Oort Cloud like debris fields and may be a common factor in Solar System formation.<br /><br />The Solar Wind's pressure, using our Sun as an example, is normally about 2-3 nanopascals (much less than a baby's breath); but can exceed 10 nanopascals during a CME (Coronal Mass Ejection). This pressure primarily effects the tiniest left over accretion disc debris (gas and dust) and the atmospheres of the inner (now rocky) planets1. <br /><br />Since this debris is mostly located in the plane of the accretion disc, as the Sun pushes it away, it would likely be perturbed (or captured) by other planets which also happen to lie in this orbital plane. <br /><br />This likely planetary perturbation would cause the debris to find new orbits which may occur outside the plane of the accretion disc. The debris finally settles in a new orbit where the pressure of the Solar Wind is balanced by the attraction of the systems gravity.<br /><br />This debris then collects with other expelled material and outer accretion disc particles to form the objects we see in the Kuiper Belt and Oort Cloud.<br /><br />The total amount material in the Kuiper Belt and Oort Cloud is thought to be greater than the Earth's mass but less than Jupiter's (from one web source).<br /><br />I believe we can account for the creation of spherical debris fields around Solar Systems if we carefully examine the effects of the Solar Wind on accretion discs during Solar System formation. <br /><br />1. The</p>