In the inky blackness of interstellar space, a cloud of gas and dust sits motionless. It has remained that way for billions of years, occasionally jostled by the weak gravitational ripples of events in its galactic neighbourhood. More time passes and nothing much continues to occur. But eventually a much larger ripple passes through the cloud – a shock wave caused by a distant supernova, perhaps, or a collision with another gas cloud. This disturbance pushes the material together, and it begins to contract under its own gravity.
The dust in the cloud, which mostly comprises hydrogen and helium atoms, begins to clump together, orbiting around itself. It pulls in more and more material from the cloud, otherwise known as a nebula. As these clumps grow larger, the pressure of…
