lives of stars section 3

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Lives of Stars Section 3

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Lives of Stars Section 3. Nebula. Large cloud of gas and dust spread out in an immense volume All stars are born in a nebula , large cloud of gas and dust. Protostar. Gas and dust begin to collect due to gravity . Once enough material has formed together, a protostar is created. - PowerPoint PPT Presentation

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Page 1: Lives of Stars Section 3

Lives of StarsSection 3

Page 3: Lives of Stars Section 3

Protostar

• Gas and dust begin to collect due to gravity.

• Once enough material has formed together, a protostar is created.

• This is the beginnings of what will become a star. A star is born when nuclear fusion begins.

Page 4: Lives of Stars Section 3

Lifetimes of Stars

• Like automobiles burning through their gas, the length a star lives depends on its mass.

• Larger, more massive stars live shorter while less massive stars live longer.

Page 5: Lives of Stars Section 3

Deaths of Stars

• As the star runs out of fuel, its core shrinks and gets hotter.

• As it does so, it heats the gases surrounding it which causes the outer layers to expand.

• The star will then become a black dwarf or black hole dependent upon its starting mass.

Page 6: Lives of Stars Section 3

Less Massive Stars

Nebula Protostar

Low-mass or medium-mass star

Red Giant Planetary Nebula

White Dwarf Black Dwarf

Page 7: Lives of Stars Section 3
Page 8: Lives of Stars Section 3

Medium Sized Stars

• Medium sized stars are the most common in the universe. An example is our sun. Medium size stars are 10 times more massive than a red dwarf

Page 9: Lives of Stars Section 3

Red Giant

• 10-100 times the size of our sun. It shines red and it is about 3000oC.

Page 10: Lives of Stars Section 3

Planetary Nebula

• After the red giant, the star will create a planetary nebula, which is the glowing gas of the outer layers as they expand away from the core.

Page 11: Lives of Stars Section 3

White Dwarf

• The only thing that remains after is the core of the star, a very hot dense, white dwarf. After billions of years this will eventually cool to become a black dwarf.

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Page 13: Lives of Stars Section 3

Greater Mass Stars

• Nebula Protostar

High-mass star Supergiant

Supernova Neutron Star

Black Hole

Page 14: Lives of Stars Section 3
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Supernova Images

Page 19: Lives of Stars Section 3

Neutron Stars

• The lower mass high mass stars will instead become neutron stars.

• Neutron stars spin rapidly and emit radio waves.

Page 20: Lives of Stars Section 3

Black Holes

• However, only the most massive will become black holes.

• Remains of a supernova which contains enough gravity that light cannot escape

• After a very massive star dies in a supernova explosion, more than 5 times the mass of the sun may be left

• The gravity of this mass is so strong that the gas is pulled inward, packing the gas into smaller and smaller space.

Page 21: Lives of Stars Section 3

Black Holes

• Not able to detect a black hole directly because no light, no radio waves, or any other form of radiation can ever get out of a black hole

• Detect black hole indirectly• Gas near a black hole is pulled so strongly that it

revolves faster and faster around the black hole• Friction heats the gas up• Astronomers can detect X-rays coming from the

hot gas and infer that a black hole is present

Page 22: Lives of Stars Section 3

                                                                                    

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Reminders

• Only stars with more than 40 times the mass of the sun form black holes when they die

• Other high mass stars become neutron stars when they die

• When a star begins to run out of hydrogen, it can become a red giant or supergiant

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