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When Earth was a very young planet, around 4.5 billion years ago, temperatures were extremely high due to intense volcanic activity, frequent asteroid impacts, and the decay of radioactive isotopes. Estimates suggest that surface temperatures may have reached around 1,000 degrees Celsius (1,832 degrees Fahrenheit) or more. This molten state gradually cooled, leading to the formation of a solid crust and eventually allowing for the accumulation of water and the development of a more stable climate.

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