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In triggered star formation, one of several events might occur to compress a molecular cloud and initiate its gravitational collapse. Molecular clouds may collide with each other, or a nearby supernova explosion can be a trigger, sending shocked matter into the cloud at very high speeds.
These knots contain sufficient mass that the gas and dust can begin to collapse from gravitational attraction. As it collapses, pressure from gravity causes the material at the center to heat up, creating a protostar. One day, this core becomes hot enough to ignite fusion and a star is born.
Stars form in large clouds of gas and dust called molecular clouds. Molecular clouds range from 1,000 to 10 million times the mass of the Sun and can span as much as hundreds of light-years. Molecular clouds are cold which causes gas to clump, creating high-density pockets.
Star formation happens in interstellar molecular clouds: opaque clumps of very cold gas and dust. The process starts when some of those clumps docHub a critical mass, allowing them to collapse under their own gravity.
Star formation can be triggered by compression from wind or supernova-driven shock waves that sweep over molecular clouds.
Structuring your STAR interview responses Situation: Briefly set the scene with relevant context (1-2 sentences). Task: Describe your responsibility or the goal you needed to achieve (1-2 sentences). Action: Explain the specific steps you took to address the situation, focusing on your contributions (3-4 sentences).
All stars form in nebulae, which are huge clouds of gas and dust. Though they shine for many thousands, and even millions of years, stars do not last forever.
The formation of the star process will take around a million years from the time when the initial gas cloud starts to collapse till the star is formed and shines like a sun.