3. T-Tauri Phase
A T-Tauri star begins when materials stop falling into the Protostar and release tremendous amounts of energy. The mean temperature of the Tauri star isn’t enough to support nuclear fusion at its core.
The T-Tauri star lasts for about 100 million years, following which it enters the most extended phase of development – the Main sequence phase.
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This Idea helps to know how a star evolves and through what process it goes to become a star like "The sun" and ultimately end up to star remnants.
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