About How our solar system was formed
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.
Four and a half billion years ago, our sun wasn't quite the shining star that it is today. It was.
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 planet.
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 Systemis thesystem of theand the objects thatit.Itwhen a dense region of acollapsed, forming the Sun and a . The Sun is a typical star that maintains aby theof hydrogen into helium at its , releasing this energy from its outer . Astronomers
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