About How was the solar system formed
Learn how a supernova, a nebula, and planetesimals shaped the planets and their orbits in this article by astrophysicist Paul Sutter. Discover the evidence, the theories, and the challenges of solar system formation.
I can't help but start with: In the beginning, there was nothing. But it wasn't quite nothing. All stars form from the collapse of nebulae, which are loose clouds of gas and dust, and our sun — and solar system — are no different. Astronomers call it the "pre-solar nebula".
Once the planets matured, however, all was not calm in the solar system. The inner rocky worlds had stabilized, and the sun had ignited nuclear fusion. But the outer giant planets were surrounded by swarms of hangers-on — the leftover bits of debris from the.
Four and a half billion years ago, our sun wasn't quite The Shining star that it is today. It was compact and very, very hot, but it hadn't reached.
The nebular hypothesis says that the Solar System formed from theof a fragment of a giant ,most likely at the edge of a .The cloud was about 20(65 light years) across,while the fragments were roughly 1 parsec (three and a quarter ) across.The further collapse of the fragments led to the formation of dense cor. The Solar System formed approximately 4.6 billion years ago from a dense region of a molecular cloud that collapsed, giving rise to the Sun and a protoplanetary disc123. Astronomers believe this collapse was triggered by a nearby exploding star, possibly a supernova2. The solar system consists of the Sun and the objects that orbit it1.
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