the life & death of stars. nuclear fusion nebula supernova black hole

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The Life & Death of Stars

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Let’s review: What is a star? Giant ball of hot gases The huge objects in the universe Our Sun is an example of a star Made of mainly hydrogen and some helium

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Page 1: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

The Life & Death of Stars

Page 2: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Nuclear fusion

Nebula

Supernova

Black hole

Page 3: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Let’s review: What is a star?

• Giant ball of hot gases• The huge objects in

the universe• Our Sun is an example

of a star• Made of mainly

hydrogen and some helium

Page 4: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

How do stars generate energy?

• Stars burn by a process called nuclear fusion• This process combines two hydrogen atoms

into one helium atom, which then fuse to form elements with even more protons

• This process gives off a lot of heat & energy• Gives the illusion of “burning”

Page 5: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Types of stars• 3 main sizes of stars

• Small/medium (like our Sun)• Large (aka giant)• Very large (aka supergiant or hypergiant)

• Different colours of stars indicate they’re different temperatures• Blue is hottest• Yellow is average• Red is ‘coolest’

• Usually, the bigger the star, the cooler it is• Most big stars are called Red Giants because they’re relatively cool• Blue giants are very rare

• The hotter the star, the shorter its lifespan

Page 6: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Sizes of stars1) small / med – most common2) large – rare3) extremely large – very rare

• The Sun is a med (average) sized star

• Small stars are called dwarf stars

• Large stars are called Giants

• Extremely large stars are called Supergiants

Page 7: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

The Birth of a Star• All stars start out the same way, as

a nebula• A nebula is a giant cloud of gas

and dust• Stars are created in a nebula as the

gases contract due to the force of gravity, turning into a hot, dense clump

• As they become larger, they heat up until they reach a temperature of 10 000 000 C

• At this temperature, nuclear fusion begins

Page 8: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

A Star’s Life • For the major part of a star’s life, it

undergoes nuclear fusion• Lower-mass stars can undergo this

process for up to 100 BILLION years!

• Stars like the Sun can last for about 10 billion years

• Higher-mass stars produce energy for only a few million years

• Fast-burning, hot (blue) stars only last for a million years… yikes!

Page 9: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

A Star’s Death • A Star begins to “die” when the

hydrogen that fuels it runs out • H has fused into new substances (He)

• Outer layers swell• Once the core fuses into lead, fusion

stops and the star collapses inward, followed by an outward projection of particles

• Depending of the star’s size, its collapse is either in the form of a planetary nebula or a supernova

• After that, it then becomes one of the following:1) White dwarf (small/medium-sized stars)2) Neutron star (large stars)3) Black hole (extremely large stars)

Page 10: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Supernovas• In 1987, Canadian astronomer

Ian Shelton discovered one while working at an observatory in Chile

• His discovery was by accident!• He was looking at images of

stars when he noticed something unusual: one star looked MUCH brighter than the others

• Named it SN 1987A and it is 163 000 light years away• This means Shelton was looking at the

supernova the way it was 163 000 yrs ago!

• SN 1987A was the closest one to Earth since 1604

Page 11: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

White DwarfsLife After Death of Small & Medium

Stars• When the star’s core

becomes lead it can not undergo fusion any longer

• This white hot ball of lead is called a white dwarf

• It cools over a loooong time to form a black dwarf star

Page 12: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Neutron Stars Life after death of a large star

• Sometimes a star is so heavy & under so much pressure that it cannot support its weight (even if it’s fused into lead!)

• The atoms collapse even further creating a ball of neutrons

• This forms a rapidly spinning neutron star that is only a few kilometers in size

• We see neutron stars from the radiation that shoots out of either end

Page 13: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Black holesThe Life After Death of Huge Stars

• Sometimes a star is so heavy that not even the neutrons can stay apart

• The neutrons crash together, forming a black hole

• After that we are not sure as this creates a black hole

• A black hole is an object so dense that not even light can escape it

• We can find black holes by looking for objects in space that are orbiting seemingly empty space

• These are very, very rare

Page 14: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

How will our Sun die?

Page 15: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Death of a Biiiig Star

Page 16: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Life Sequence of StarsStar’s Size Phases of a star’s “life & death”

Small/Mediumnebula nuclear fusion red giant planetary nebula white dwarf black dwarf

Largenebula nuclear fusion red supergiant supernova neutron star

Extremely Largenebula nuclear fusion red supergiant supernova black hole

Page 17: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole

Life cycle of Stars… in pictures

Page 18: The Life & Death of Stars. Nuclear fusion Nebula Supernova Black hole