Question Description
Everything should be under this but if anything else is needed, let me know:
The fusion of deuterium and tritium isotopes fuels the Sun. This reaction also explains the existence of helium in the Sun and other stars. But what about the other elements? How did heavier elements, like oxygen, nitrogen, and sulfur, first form? Are they still forming today? If so, where and how? To investigate these questions, you will journey into a star and carry out the two-part exploration outlined below. Click each tab to review the assignment.
Part 1: The Elements: Forged in Stars
Visit The Elements:
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