A dense cloud of interstellar matter becomes unstable and collapses, resulting in a new star. Or so we are told. Perhaps there is a better explanation.
The great ball of hydrogen and helium, after a few billion years, is finally mature and ready to breed. It sends out electromagnetic energy, signaling a message about its willingness to propagate. With enthusiastic response, the trajectories of countless meteors are destined to arrive from the depths of interstellar space, aiming to collide with the massive star. Inevitably, millions of these willing fiery seedlings burn and disintegrate within the corona, unable to complete their journeys.
However, there is one proud meteor that purposefully makes it through the protective corona and successfully collides with the patiently waiting sun. The impact event introduces new elements, effectively resulting in stellar fertilization. In turn, the evolving embryonic Starseed grows for a period of a thousand years. Finally, with the assistance of a sudden increase of the radiative flux emitted from within the corona, the Starseed is released out into the surrounding blackness of interstellar space. A star is born.

