4.57 billion years ago the Sun and the planets coalesced from a vast
nebular cloud of gas and dust. About
a million years later the Sun began shining when it accrued enough mass to ignite its
hydrogen fusion furnace. The ensuing solar wind purged the infant solar
system of much of its nebular origins, while leaving dust
and debris, including asteroids and planetoids, in the plane of the ecliptic
to be swept up by the
forming planets.
This rendering suggests how the newly formed
Earth and sun may have appeared shortly after the Sun's heat and solar
wind cleared the inner solar system of cooler gases. The entire Earth is molten due to
radioactive heating and frequent, heat-generating collisions with the
remaining debris.
Far above and below the Earth's orbit thousands of icy comets swarm around the Sun like bees around a hive. Some
of these comets will eventually collide with the Earth and other planets,
delivering water and other rare materials to these fledgling worlds.