Solar System

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Solar System
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  • FUSION
  • Our story starts about 4.6 billion years ago, with a wispy cloud of stellar dust.This cloud was part of a bigger cloud called a nebula.At some point, the cloud collapsed—possibly because the shockwave of a nearby exploding star caused it to compress.
  • When it collapsed, it fell in on itself, creating a disk of material surrounding it. Finally the pressure caused by the material was so great that hydrogen atoms began to fuse into helium, releasing a tremendous amount of energy. Our Sun was born!
  • Even though the Sun gobbled up more than 99% of all the stuff in this disk, there was still some material leftover.Bits of this material clumped together because of gravity. Big objects collided with bigger objects, forming still bigger objects. Finally some of these objects became big enough to be spheres—these spheres became planets and dwarf planets
  • And like that, the solar system aswe know it today was formed.Gas and icy stuff collected furtheraway, creating the gas and ice giants.Rocky planets, like Earth, formednear the Sun, because icy and gaseous material couldn’t survive close to allthat heat.Andlike that, the solar system as we know it today was formed
  • Way off in the outer reaches of thesolar system are comets. These icy bits haven’t changed much at all since thesolar systems formation.Asteroids in the asteroid belt arethe bits and pieces of the early solar system that could never quite form aplanet.There are still leftover remains ofthe early days though.
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