Whitedwarf10 619x558

Life Cycle of a Star

  • 100,000 BCE

    Stellar Nebula

    Stellar Nebula
    Stellar Nebula 8 billion years ago, gravity began to pull together lots of gas and dust in space. This began the formation of our solar system, specifically our sun.
  • 60,000 BCE

    Protostar

    Protostar
    6 billion years ago, gravity began to pull at the enter of our solar system. This pulled all the gas and dust from the stellar nebula together. This began to create a disk shape forming billions of stars and planets.
  • 4600 BCE

    Our Sun was Born

    Our Sun was Born
    Our Sun formed 4.6 billion years ago. It began fusing Hydrogen to Helium. It was formed as a G2 main sequence star. It will stay this way for another 5 billion years.
  • Red Giant

    Red Giant
    Once all the Hydrogen runs out in the sun, gravity will lose grip and our sun will expand to a red giant.
  • Planetary Nebua

    Planetary Nebua
    11 billion years after the sun formed, all of the Hydrogen, Helium, Carbon, and Oxygen will run out.This means there's no more fuel left for the sun. All of the outer gases once held in by gravity will be released, leaving behind the core of the sun. This will occur in another 6.5 billion years.
  • White Dwarf

    White Dwarf
    White Dwarf Once all of the gas and dust have escaped from the core of the sun, all that will be left is a white dwarf. This is the last stage for our sun, meaning our star has died. The last bit that it burns are heavy metals like silver and iron. This will occur in 13 billion years.