WebSilicon burning begins when gravitational contraction raises the star's core temperature to 2.7–3.5 billion kelvin ( GK ). The exact temperature depends on mass. When a star has completed the silicon-burning phase, no further fusion is possible. The star catastrophically collapses and may explode in what is known as a Type II supernova . WebApr 11, 2024 · How long the fire could burn is still unknown. "The fire chief tells me the fire is somewhat contained on three sides," Snow said at around 6:30 p.m. Tuesday, adding that fire departments from ...
Richmond industrial fire: School canceled after
WebAnswer 3: Very large stars explode when they run out of fuel. Stars burn hydrogen (H) in their core throughout their lifetime. We call it "burning", but what is really happening is that H atoms are crashing together to form helium (He) atoms. H and He are what make up stars. WebGravity wins, everything is over. Eventually the cycle of star birth and death will come to an … inc 表示
Types Stars – NASA Universe Exploration
WebApr 11, 2024 · How long the fire could burn is still unknown. "The fire chief tells me the fire … WebMar 22, 2024 · Here’s how NASA explains it: “Massive stars burn huge amounts of nuclear fuel at their cores, or centers. This produces tons of energy, so the center gets very hot. Heat generates pressure, and the pressure created by a star’s nuclear burning also keeps that star from collapsing. A star is in balance between two opposite forces. WebJun 3, 2024 · When stars like our Sun die, they leave a stellar remnant behind known as a white dwarf: a core of dense atoms typically comprised of carbon and oxygen atoms. Many stars are like our Sun, but... include page number in word