Title Page Title Page Janet Moore NASA Educator Ambassador
Mar 26, 2015
Title PageTitle Page
Janet Moore
NASA Educator Ambassador
What is a Black Hole?What is a Black Hole?
Definition: a place where the escape velocity is faster than the speed of light.
Close-up Picture of a Black HoleClose-up Picture of a Black Hole
Escape VelocityEscape Velocity
Definition: the velocity at which something must travel
away from an object such that the gravity
of the object cannot stop it.
Escape Velocity (2)Escape Velocity (2)
Escape velocity depends on the
gravitygravityof the object
Escape Velocity (3)Escape Velocity (3)
Lowmass
Mediummass
Highmass
Very high mass
for a given radius
^
Escape Velocity (4)Escape Velocity (4)radius decreases increases
What is a Black Hole?What is a Black Hole?
It’s an object of high enough It’s an object of high enough mass mass
and small enough radius and small enough radius such that such that
the escape velocity is the escape velocity is faster than light.faster than light.
Nothing can escape.
Or, put another way …Or, put another way …
QuickTime™ and ampeg4 decompressor
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The First Way A Black The First Way A Black Hole Can Kill YouHole Can Kill You
1.2.3.4.5.6.7.
Falling in
Down the DrainDown the Drain
Forcing the IssueForcing the IssueThe force of gravity from an object depends on
1) the mass of the object2) your distance from it
Black holes are really massive, And you can get
really, really close
But this means….
Gm1m2
F=
r2
So if it’s really massive, or you’re really close, the force is high.
Forcing the Issue (2)Forcing the Issue (2)The force you feel CHANGES as you get closer.
Something closer to the black hole feels MORE force.
If you fall in feet first, you have a problem.
STRETTTTTCH!
There is a TideThere is a TideThe change in force is called a TIDE
Tides on surface of Earth (distance = 6400 km) : 1/1,000,000th of a g
DISTANCE FORCE (g)
6400 km 0.5
2000 18
1000 144
100 150,000
10150,000,000B
LA
CK
HO
LE
TID
ES
6400 km
Fup
Fdown
(for a 3 solar mass black hole)
The Second Way A The Second Way A Black Hole Can Kill YouBlack Hole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettification
Why the long face?Why the long face?
The Third Way A Black The Third Way A Black Hole Can Kill YouHole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornBe near one when it’s born
Cold War, Hot TopicCold War, Hot Topic
Vela Satellites flown to detect
nuclear explosions on Earthin 1960s and 1970s
by looking for gamma rays
Over their lifetime, they detected 73 events.
NOT ONE WAS OF THIS EARTH
Gamma Ray BurstsGamma Ray Bursts
GRBs happen every day, somewhere in the Universe
The Birth of a Black HoleThe Birth of a Black Hole
Hypernova!
Coalescing neutron stars
Birth PangsBirth PangsEnergy generated in a GRB = 1052 ergs
This is 10x the Sun’s total energy
over its entire lifetime.
Enough energy to vaporize the Earth
100 billion times over.
Pfffssssst!Pfffssssst!
NASA’s Swift ResponseNASA’s Swift Response
Swift detects
>100 GRBs per year
LaunchedNovember 20, 2004
The Fourth Way A Black The Fourth Way A Black Hole Can Hole Can KillKill You You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornBe near one when it dies
Pare ProductionPare ProductionParticles created here
Buh bye!Free at last!
Black hole
Hawking Radiation:2 particles created, one particle leaves
Net Effect: Black holes radiate
away energy
Size Does MatterSize Does Matter
Hawking radiation depends on size/mass of the black hole:smaller holes radiate faster!
In fact, radiation emitted goes as 1/mass3
Stellar black hole lives for 1067 years
A mini black hole (mass =1012 kg)
would be exploding now
Emits higher energy radiation faster as size shrinks.
KABOOM!
The Fifth Way A Black The Fifth Way A Black Hole Can Kill YouHole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornJust passing throughBe near one when it dies
notnot It’s a Wonderful Day in the It’s a Wonderful Day in the Neighborhood Neighborhood
What if . . .What if . . .
What would happenif the sun became ablack hole?
Solar System Black HoleSolar System Black Hole
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The Sixth Way A Black The Sixth Way A Black Hole Can Kill YouHole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornJust passing throughBe nearby when they merge
Be near one when it dies
When Galaxies CollideWhen Galaxies Collide
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Wave Bye ByeWave Bye Bye
Gravitational waves expand and contract space itself
The Long and the Short of ItThe Long and the Short of It
ESA’s Response: LISAESA’s Response: LISA
3 “Wagon wheels”That will detect
passing gravitational
waves
Target launch: 2014
The Seventh Way A The Seventh Way A Black Hole Can Kill YouBlack Hole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornJust passing throughBe nearby when they merge
Be near one when it dies
Fried by the light
Traveling CompanionTraveling CompanionHD 226868: just your typicalbloated supergiant star… but it has a secret
HD 226868 in X-rays(100,000x energy of Sun!)
Cygnus X-1
Hey, where is it?
The Hideous VortexThe Hideous Vortex
Disks and Fields and Jets, Oh MyDisks and Fields and Jets, Oh My
Not-so-compact DiskNot-so-compact Disk
Angry NeighborsAngry Neighbors
Cygnus A
M 87
(600 million light years)
(60 million light years)
Our GLAST (Fermi) ResortOur GLAST (Fermi) Resort
Gamma-RayLarge AreaSpace Telescope
Launched: June 2008
Fermi will see thousands
of active galaxies
The Seven Ways A Black The Seven Ways A Black Hole Can Kill YouHole Can Kill You
1.2.3.4.5.6.7.
Falling inSpaghettificationBe near one when it’s bornJust passing throughBe nearby when they merge
Fried by the light
Be near one when it dies
What’s on the other side…?What’s on the other side…?
Questions?Questions?
The Sky by EyeThe Sky by Eye
DIRBE’s Milky WayDIRBE’s Milky Way
EXTREME Close upEXTREME Close up
The Monster in the MiddleThe Monster in the Middle
Video DiskVideo Disk