Description
The origin of the solar system is a fascinating topic in astronomy and cosmology. While there are still uncertainties and ongoing research in this field, scientists have developed several theories to explain how our solar system formed roughly 4.6 billion years ago. One of the most widely accepted theories is the nebular hypothesis, which suggests that the solar system formed from the gravitational collapse of a giant molecular cloud composed mostly of hydrogen and helium, along with trace amounts of other elements
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