During the final evolutionary stages of massive stars, silicon burning produces a cascade of nuclear reactions that create elements up to iron.

In stars of more than eight solar masses that have exhausted their helium supply, carbon burning converts carbon into neon, sodium, magnesium, and other elements, driving the star toward later fusion stages.

In models of massive stars, oxygen burning is the nucleosynthesis phase that follows carbon burning, during which neon disintegrates and oxygen fuses to form silicon, phosphorus, sulfur, and other elements up to atomic number 40.

Hydrogen burning in stars under 1.2 solar masses primarily fuels the conversion of hydrogen into helium, deuterium, and traces of lithium, shaping their long-term structure and evolution.

In the cores of red giants, helium burning begins once temperatures exceed 10^8 K, converting helium into carbon and subsequently into oxygen, neon, and magnesium.

During the heated demonstration, several protesters were arrested for flag-burning outside the embassy.

The villagers adopted burn-clearing to prepare the soil before planting the next season's crops.

After the fall, he inspected the road burn on his knee and covered it with a sterile dressing.

After hours outside without gloves, he developed a severe frost burn on his fingertips.

At dusk, the old fishermen still burn the water to catch salmon, their torches throwing orange reflections across the river.