Death By Black Hole Rob Sparks Pinon Teacher’s Workshop Presentation stolen shamelessly from Phil Plait (the Bad Astronomer)

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Presentation transcript:

Death By Black Hole Rob Sparks Pinon Teacher’s Workshop Presentation stolen shamelessly from Phil Plait (the Bad Astronomer)

DISCLAIMER! What you are about to see is for entertainment purposes only. No one has EVER been killed by a black hole in the entire history of the human race and everything in this presentation is EXTREMELY unlikely to harm life on Earth. So relax and enjoy!

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 Hole

Escape 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 depends on thegravity of the object

Escape Velocity (3) Low mass Medium mass High mass Very high mass for a given radius ^

Escape Velocity (4) radius decreasesincreases

What is a Black Hole? It’s an object of high enough mass and small enough radius such that the escape velocity is faster than light. Nothing can escape.

Four Types of Black Holes Mini-Black Holes – kg Stellar Mass Black Holes – 3 – 100 times the mass of our Sun Mid-Size Black Holes – a few thousand to 100,000 times the mass of our Sun Massive and Supermassive black holes – Millions to billions of times the mass of our Sun

The First Way A Black Hole Can Kill You Falling in

Down the Drain

Forcing the Issue The force of gravity from an object depends on 1) the mass of the object 2) your distance from it Black holes are really massive, And you can get really, really close But this means…. Gm 1 m 2 F= r 2 So if it’s really massive, or you’re really close, the force is high.

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 Tide The change in force is called a TIDE Tides on surface of Earth (distance = 6400 km) : 1/1,000,000 th of a g DISTANCEFORCE (g) 6400 km , ,000,000 BLACK HOLE TIDES 6400 km F up F down (for a 3 solar mass black hole)

The Second Way A Black Hole Can Kill You Falling in Spaghettification

Spaghetti what?

Why the long face?

The Third Way A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born

Cold War, Hot Topic Vela Satellites flown to detect nuclear explosions on Earth in 1960s and 1970s by looking for gamma rays Over their lifetime, they detected 73 events. NOT ONE WAS OF THIS EARTH

Gamma Ray Bursts GRBs happen every day, somewhere in the Universe

The Birth of a Black Hole Hypernova! Coalescing neutron stars

Birth Pangs Energy generated in a GRB = ergs This is 10x the Sun’s total energy over its entire lifetime. Enough energy to vaporize the Earth 100 billion times over.

Pfffssssst!

NASA’s Swift Response Swift will detect >100 GRBs per year Launched November 20, 2004 Detected over 200 burst so far

The Fourth Way A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born Be near one when it dies

Pare Production Particles 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 Matter Hawking radiation depends on size/mass of the black hole: smaller holes radiate faster! In fact, radiation emitted goes as 1/mass 3 Stellar black hole lives for years A mini black hole (mass =10 12 kg) created in the Big bang would be exploding now Emits higher energy radiation faster as size shrinks. KABOOM!

The Fifth Way A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born Just passing through Be near one when it dies

not It’s a Wonderful Day in the Neighborhood

Orbit Simulation Go to orbit animation

The Sixth Way A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born Just passing through Be nearby when they merge Be near one when it dies

When Galaxies Collide

Wave Bye Bye Gravitational waves expand and contract space itself

The Long and the Short of It

LIGO : Hunting Gravity Waves Two observatories (Washington and Louisiana) L-Shaped tubes Attempt to measure changes in length as gravity waves pass Sensitive to m Sensitive to short wavelength gravity waves

ESA’s Response: LISA 3 “Wagon wheels” That will detect passing gravitational Waves Target launch: 2011

The Seventh Way A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born Just passing through Be nearby when they merge Be near one when it dies Fried by the light

Traveling Companion HD : just your typical bloated supergiant star… but it has a secret HD in X-rays (100,000x energy of Sun!) Cygnus X-1 Hey, where is it?

The Hideous Vortex

Disks and Fields and Jets, Oh My

EXTREME Close up

The Monster in the Middle

Our GLAST Resort Gamma-Ray Large Area Space Telescope Launch in 2007 GLAST will see thousands of active galaxies

The Eight Ways A Black Hole Can Kill You Falling in Spaghettification Be near one when it’s born Just passing through Be nearby when they merge Fried by the light Be near one when it dies Roasted!

Black holes can only eat so fast Matter piles up inside a black hole creating a hot plasma VERY HOT PLASMA! In large black holes, tidal forces are weak, so you would be fried before you were spaghettified!

What’s on the other side…?