life cycle of stars. what is a star? a ball of gas that makes light. a luminous celestial body, made...

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Life Cycle of Stars

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Life Cycle of Stars

Life Cycle of Stars

What is a star?

•A ball of gas that makes light.•A luminous celestial body, made up of plasma, forming a sphere.•The Sun is one of billions of stars in the Milky Way galaxy.

L I F E O F A S T A R

Star Birth

Star Birth

Star Cluster N81

DUST and GAS

•Come closer together due to gravity.

•Mostly Hydrogen and Helium.

Dust and Gas

PROTOSTAR

•Gas condenses due to gravity.

•Planets may form.

•Temperature increases.

Star Birth

Dust and Gas

GravityProtostar

Star Birth

Dust and Gas

Gravity

At a distance of 7000 light years this nebula contains the largest protostar yet to be discovered. This protostar is 300 times the size of our own solar system. A protostar is a gas cloud that "shrinks" its way to becoming a star.

Protostar

FUSION

•Hydrogen molecules smash together to form Helium and energy.

•Star begins to shine.

•Bigger the star the faster it “burns”.

Star Birth

FUSION

•Hydrogen molecules smash together to form Helium and energy.

•Star begins to shine.

•Bigger the star the faster it “burns”.

Star Birth

Dust and Gas

GravityProtostar

Fusion

MAIN SEQUENCE STAR•Type of Main Sequence star depends on initial mass. •Bigger = Higher Temperature = Change in color.

Dust and Gas

GravityProtostar

Fusion Main

Sequence

Star

Star Birth

Red Dwarfs

Sun Class

Blue Giants MAIN SEQUENCE STAR•Type of Main Sequence star depends on initial mass. •Bigger = Higher Temperature = Change in color.

Star Birth

Dust and Gas

GravityProtostar

Fusion Main

Sequence

Star

Birth Main Sequence Star Death

Blue GiantsSun Class

Red Dwarfs

L I F E O F A S T A R

Star Birth

Small Star Death

Small Star Death

Small

MSS

SMALL MAIN SEQUENCE STAR•Star uses all of its Hydrogen. It runs out of fuel. •Star cools and expands.

Fuel u

sed u

p

Small Star Death

RED GIANT

•Hydrogen is used up.

•Star expands and cools.

•Really big.

Small

MSSFue

l use

d up

Red Giant

Small Star Death

PLANETARY NEBULA

•Core condenses due to gravity.

•Outer gasses expand outward.

Small

MSSFue

l use

d up

Red GiantCor

e

Collap

se

Small Star Death

PLANETARY NEBULA

•Core condenses due to gravity.

•Outer gasses expand outward.

Small

MSSFue

l use

d up

Red GiantCor

e

Collap

se

Planeta

ry

nebu

la

Spirograph Nebula

Small Star Death

Eight Burst Nebula

Small Star DeathLittle Ghost Nebula

Small Star DeathHelix Nebula

A mere seven hundred light years from Earth, in the constellation Aquarius, a sun-like star is dying. Its last few thousand years have produced the Helix Nebula (NGC 7293), a well studied and nearby example of a Planetary Nebula, typical of this final phase of stellar evolution. Nearly 11 hours of exposure time have gone into creating this remarkably deep view of the nebula. It shows details of the Helix's brighter inner region, about 3 light-years across, but also follows fainter outer halo features that give the nebula a span of well over six light-years. The white dot at the Helix's center is this Planetary Nebula's hot, central star.

Small Star Death

WHITE DWARF

•Outer nebula expands away.

•Small dense core remains.

•Size of the Earth, but the mass of the Sun.

•Will eventually burn out and become a Black Dwarf.

Small

MSSFue

l use

d up

Red GiantCor

e

Collap

se

Planeta

ry

nebu

la White

Dwarf

L I F E O F A S T A R

Star Birth

Small Star Death

Large Star Death

Large

MSS

To be large a star must be 4-5 times more massive than out Sun. A good example is Rigel in the Orion constellation. It is as bright as 70,000 Suns.

Large Star Death

Large

MSS

Large Star Death

Large

MSS

To be large a star must be 7 times more massive than out Sun. A good example is Rigel in the Orion constellation.

Rigel

Large Star Death

SUPER GIANT

•Hydrogen is used up.

•Star expands and cools.

•Really big.

Large

MSSFue

l use

d up

Superg

iant

Supernova RemnantSUPERNOVA

•Explosion of outer gasses.

•Very quick.

•Collapse of core.

Large

MSSFue

l use

d up

Superg

iant

Blow up

Supern

ova

Large Star Death

Crab NebulaSUPERNOVA

•Explosion of outer gasses.

•Very quick.

•Collapse of core.

Large

MSSFue

l use

d up

Superg

iant

Blow up

Supern

ova

Large Star Death

Star Collapse

STAR COLLAPSE

•Outward force of fusion is gone.

•Gravity dominates.

Supern

ova Neu

tron

Star

Large Star Death

A neutron star is about 12 miles in diameter and has the mass of about 1.4 times that of our Sun. This means that a neutron star is so dense that on Earth, one teaspoonful would weigh a billion tons! Because of its small size and high density, a neutron star possesses a surface gravitational field about 200,000,000,000 times that of Earth.

Pulsating Neutron Star = Pulsar

NEUTRON STAR

•Collapse of core.

•Very dense.

Supern

ova Neu

tron

Star

Large Star Death

BLACK HOLE

•Complete collapse of the core.

•Infinitely small. Infinitely dense.

Center of Milky Way

Supern

ova Neu

tron

Star

Black

Hole

Large Star Death

Supern

ova Neu

tron

Star

Black

Hole

Large Star Death

L I F E O F A S T A R

The sun is a mass of incandescent gasA gigantic nuclear furnaceWhere hydrogen is built into heliumAt a temperature of millions of degrees

Yo ho, it's hot, the sun is notA place where we could liveBut here on Earth there'd be no lifeWithout the light it gives

We need its lightWe need its heatWe need its energyWithout the sun, without a doubtThere'd be no you and me

The sun is a mass of incandescent gasA gigantic nuclear furnaceWhere hydrogen is built into heliumAt a temperature of millions of degrees

The sun is hot

It is so hot that everything on it is a gas: iron, copper, aluminum, and many others.

The sun is large

If the sun were hollow, a million Earths could fit inside. And yet, the sun is only a middle-sized star.

The sun is far away

About 93 million miles away, and that's why it looks so small.

And even when it's out of sightThe sun shines night and day

The sun gives heatThe sun gives lightThe sunlight that we seeThe sunlight comes from our own sun'sAtomic energy

Scientists have found that the sun is a huge atom-smashing machine. The heat and light of the sun come from the nuclear reactions of hydrogen, carbon, nitrogen, and helium.

The sun is a mass of incandescent gasA gigantic nuclear furnaceWhere hydrogen is built into heliumAt a temperature of millions of degrees

Life Cycle of Stars