Planetesimals begin to form within the swirling
disk.
Small planetesimals collide with larger ones, and
the planets begin to grow.
The excess dust and gas is gradually removed
from the solar nebula, which leaves planets
around the sun and thus created a new solar
system.
As the solar nebula rotates, it flattens and
becomes warmer near its center.
The young solar nebula begins to collapse
because of gravity.
As planetesimals grow, their gravitational pull
increase. The largest planetesimals begin to
collect more of the gas and dust of the nebula.
Planetesimals begin to form within the swirling
disk.
Small planetesimals collide with larger ones, and
the planets begin to grow.
The excess dust and gas is gradually removed
from the solar nebula, which leaves planets
around the sun and thus created a new solar
system.
As the solar nebula rotates, it flattens and
becomes warmer near its center.
The young solar nebula begins to collapse
because of gravity.
As planetesimals grow, their gravitational pull
increase. The largest planetesimals begin to
collect more of the gas and dust of the nebula.
Planetesimals begin to form within the swirling
disk.
Small planetesimals collide with larger ones, and
the planets begin to grow.
The excess dust and gas is gradually removed
from the solar nebula, which leaves planets
around the sun and thus created a new solar
system.
As the solar nebula rotates, it flattens and
becomes warmer near its center.
The young solar nebula begins to collapse
because of gravity.
As planetesimals grow, their gravitational pull
increase. The largest planetesimals begin to
collect more of the gas and dust of the nebula.