DO NOW QUESTION What life stage is our Sun currently in? What do you think will happen to our Sun as it gets older?

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Presentation transcript:

DO NOW QUESTION What life stage is our Sun currently in? What do you think will happen to our Sun as it gets older?

The Life Cycle of Stars

Stage 1: Formation  Enters first stage as a ball of gas and dust  Gravity pulls the gas and dust together into a sphere  As the sphere becomes denser, it gets hotter and the hydrogen changes into helium

Stage 2: Main Sequence  The longest stage  In the core of this type of star, hydrogen atoms fuse into helium atoms releasing a huge amount of energy

Nuclear Fusion  Occurs when hydrogen changes to helium  This process releases energy that fuels the star 2 hydrogen atoms combine 1 helium atoms is produced 1 hydrogen atom 1 hydrogen atom + energy is released

Stage 3: Red Giant  The star expands and cools once it uses all of its hydrogen  The center of the star shrinks  The star’s atmosphere then grows very large and cools  The star is reddish in color Red giants size comparison to our Sun. Note, red giants can vary in size.

Stage 4: White Dwarf  Final stage of a star’s life cycle  Has the same mass as the sun or smaller  A small hot star that is the leftover center of an older stare  There is no hydrogen left and can no longer generate energy by fusing hydrogen atoms into helium atoms About the same size as Earth

Supernova  At the end of its life, a massive star may explode in a large, bright flash called a supernova  A gigantic explosion in which a massive star collapses and throws its outer layers into space Chandra, Hubble, and Spitzer Space Telescope image of Crab Nebula supernova remnant

Neutron Star  Following a supernova, the center of the collapsed star contracts to form a neutron star  A star that has collapsed under gravity to the point at which all of the stars particles are neutrons

Pulsar  A spinning neutron star that sends out radiation across space  This radiation (radio waves) is detected on Earth by radio telescopes Vela pulsar, picture taken by Chandra X-Ray Observatory

Black Hole  An object that is so massive that light cannot escape  If the center of a collapsed star has a mass that is more than 3 times the mass of the sun, the star may contract further because of gravity  The force of the contractions crushes the dense center of the star and leaves a black hole