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This view shows the scene in the region of the earth less than
a million years after the sun formed. Small grains of dust are aggregating
into "planetesimals". The planets grew by collisional aggregation of
these planetesimals. Scientists at PSI have developed the most advanced
and detailed theoretical computer
models to represent the processes
by which dust and asteroid-like particles aggregated to form the planets
of our solar system, and perhaps those of other solar systems as well.
Painting © William K. Hartmann
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