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Newly born stars, often referred to as protostars, form from the gravitational collapse of gas and dust in molecular clouds. As the material gathers, it heats up, eventually igniting nuclear fusion at the core, which marks the transition to a main-sequence star. This process can take millions of years and is often accompanied by the formation of protoplanetary disks, where planets can also develop. Newly born stars are typically obscured by the surrounding dust and gas, making them difficult to observe directly in visible light.

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3w ago

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