Answer:
Flattens out into the ecliptic plane and spins faster due to conservation of angular momentum.
Explanation:
A star is formed in a molecular cloud of gas and dust, mainly composed of hydrogen and helium. The Nebular Theory establishes, for the formation of the solar system, that the cloud starts to collapse under its own gravity when it receives a shock wave from a near event, for example, a supernova explosion. That results in the cloud breaking in small pieces, and those pieces constitute a possible future star.
Then it begins to accrete and rotate as a consequence of the angular momentum.
[tex]L = mrv\sin \theta[/tex] (1)
Where m is the mass, r is the radius and v is the velocity and [tex]\theta[/tex] is the angle between the velocity and r.
