Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your...

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Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your clickers. There’s a link from webct.
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Transcript of Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your...

Page 1: Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your clickers. There’s a link from webct.

Agenda

Types of star deaths Relativity Black holes Evidence for both

Start registering your clickers. There’s a link from webct.

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He core contracting

H fusing

Exterior expanding

H runs out: star becomes a red giant

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Mass alone determines death

Small mass: White dwarf

Med. Mass: Neutron star or pulsar

Large mass: Black hole

Determined by S. Chandreskhar

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What type of death will our Sun die?

What will happen to us?

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Sun’s fateD

iam

ete

r (t

ime

s p

rese

nt v

alu

e)

1

100

10

Age (billions of years)

0 5 10 12.1 12.2 12.3 12.3650 12.3655

Contraction

FirstRed giant

peakNow

Leaves Mainsequence

White dwarf

Orbits of:MarsEarth

VenusMercury

Helium shell

flashes

Page 6: Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your clickers. There’s a link from webct.

Sun’s fateD

iam

ete

r (t

ime

s p

rese

nt v

alu

e)

1

100

10

Age (billions of years)

0 5 10 12.1 12.2 12.3 12.3650 12.3655

Contraction

FirstRed giant

peakNow

Leaves Mainsequence

White dwarf

Orbits of:MarsEarth

VenusMercury

Helium shell

flashes

Page 7: Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your clickers. There’s a link from webct.

Sun’s fateD

iam

ete

r (t

ime

s p

rese

nt v

alu

e)

1

100

10

Age (billions of years)

0 5 10 12.1 12.2 12.3 12.3650 12.3655

Contraction

FirstRed giant

peakNow

Leaves Mainsequence

White dwarf

Orbits of:MarsEarth

VenusMercury

Helium shell

flashes

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Death of a low mass star

Red giant shrinks, becomes very hot Expands to become a red giant again Outer layers ejected into space.

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Death of a low mass star

Planetary

nebulae

are formed Eventually

becomes a

white dwarf

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On the HR diagrams, white dwarf stars are

A. On the upper right

B. On the upper left

C. On the lower right

D. On the lower left

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The Hertzsprung-Russell (HR) Diagram

O B A F G K M

15

5

10

-10

0

-5

Spectral Class

Sun

Main Sequence Stars

White Dwarf Stars

Red Giant Stars

Hot, not too bright

Abs

olut

e m

agni

tude

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Higher mass stars

Fusion ofheavier elements

Contraction (increasing temperature)

Cycle continues until core is made of Fe (iron)

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Death of higher mass stars

Explodes in a type II supernova Then becomes

a neutron star or a black hole

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Supernova 1987A (Type II)

1994 2003

Gas from the explosion hitting cool ring of gas

NASA

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Neutron stars

Fe core collapses Electrons enter nuclei, neutrons and

neutrinos formed Carries energy outward, causing an

explosion

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Neutron star or black hole?

If very massive it becomes a black hole Otherwise it the remaining core is

called a neutron star If this spins, we call

it a pulsar

Jocelyn Bell Burnell discovered pulsars!

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What’s a theory?

Start with an hypothesis Must fit evidence Testable Falsifiable

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Einstein’s theory of Relativity

Fits evidence?

Testable?

Falsifiable?

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Matter tells space-time how to curve

Relativity in a nutshell

Space-time tells matter how to move

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Evidence – time dilation

Viking Lander sent a signal to EarthSpace was stretched, so time was too!

Earth

Viking Lander

Sun

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Evidence – GPS

Many of us own GPS receivers.

Uses time signals from satellites orbiting Earth.

Does not work unless corrected for relativity!

wikipedia; DoD

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Evidence: Wobble of Mercury

Cornell

Shown by Einstein

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Evidence: gravitational lensing

Demo: bending light

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Evidence: gravitational lensing

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Evidence: gravitational lensing

Demo: Lensing in water

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When a star stops fusing

If it has more than 25 X M sun

No outward force can resist gravity It will become a black hole Nothing on the surface can escape

(including light)

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What forces act between a black hole and a nearby object?

Gravity is the only force acting!!!! Depends on:

Mass of objects Distance between them

If the sun turned into a black hole, what would happen to the Earth?

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Can you get sucked into a black hole?

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Escape velocity

How fast does the shuttle have to go in order to leave Earth’s surface?

7 miles every second! (25,000 mph) The moon? 5320 mph The Sun? 1.38 million mph

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Escape velocity

Depends on the gravity between you and the object you want to escape!

For a black hole, the escape velocity (inside the event horizon) is greater than the speed of light!

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Do Black Holes Really Suck?

event horizon

Normal Weird

Singularity

The center of a black hole is a sphere (so is the event horizon)

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Field trip to a black hole!!

event horizon

Normal Weird

Singularity

Volunteers?

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At the event horizon

Time slows waaaaayyy down Someone jumping in would die a nasty

death Someone watching would see the

person freeze in time

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Finding black holes

How can we see something that emits no light? Look for binary systems Make sure candidate is not a neutron star!

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Finding black holes

Matter near the black hole is traveling close to the speed of light

When it rubs together, it gives off x rays we can see

NASA/CXC

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Summary

Relativity tells us space and time can be stretched

Escape velocity, event horizon Black holes can be found, but not

directly seen