Hydrogen and helium formed shortly after the Big Bang but did not ignite due to the lack of oxygen and the conditions of the early universe. Although hydrogen is flammable, burning requires oxygen, which was not present in significant amounts. The universe was too hot for electrons to orbit atomic nuclei until about 300,000 years post-Big Bang, preventing any chemical reactions. Instead, hydrogen fuses in stars like the Sun at a slow rate, allowing the universe to cool before significant quantities were converted. Helium, being a noble gas, does not readily combine with other elements, further explaining its stability in the early universe.