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As the star

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The star’s main goal in life is to achieve stability, In a stable star, the gas pressure pushing out from the center is equal with the gravity pulling atoms inward to the center

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Main sequence stars have achieved nuclear fusion and are becoming hotter and brighter. The star slowly contracts over billions of years to compensate for the heat and light energy lost.

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Once Proto-stars reach a 10,000 degree temperature they begin nuclear fusion. They are very unstable and cannot be classified as real stars just yet.

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collections of gas and materials n space

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The Different masses  and particles are grouping together and coming and clustering together.  They explode and burst back out the center of This is called a proto-star. the newly formed star forces out any gas trying to crush it. The core starts to heat up to about 10,000 degrees kelvin.