your place in the cosmos - mit

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Andrew Friedman & Ryan Andrew Friedman & Ryan Hickox Hickox Harvard Harvard - - Smithsonian Center For Astrophysics Smithsonian Center For Astrophysics Dudley House Crosstalk: Thursday, December 8th 2005 Dudley House Crosstalk: Thursday, December 8th 2005 Your place in the cosmos Your place in the cosmos From Planets to Stars to Galaxies and Beyond From Planets to Stars to Galaxies and Beyond

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Page 1: Your place in the cosmos - MIT

Andrew Friedman & Ryan Andrew Friedman & Ryan HickoxHickoxHarvardHarvard--Smithsonian Center For AstrophysicsSmithsonian Center For Astrophysics

Dudley House Crosstalk: Thursday, December 8th 2005Dudley House Crosstalk: Thursday, December 8th 2005

Your place in the cosmosYour place in the cosmosFrom Planets to Stars to Galaxies and BeyondFrom Planets to Stars to Galaxies and Beyond

Page 2: Your place in the cosmos - MIT

AstrologyAstrology

“Yeah, m-maybe... by leaving her predictions vague and generalized, there's less of a chance of someone findin' out she's a phoney.”

-Bobby Boucher, The Waterboy

Page 3: Your place in the cosmos - MIT

The Copernican PrincipleThe Copernican Principle

Sun & Solar SystemSun & Solar System Spiral GalaxySpiral Galaxy

Galaxy Clusters Galaxy Clusters & & SuperclustersSuperclusters

Other Other Universes?...Universes?...

A Small Piece of A Small Piece of Our Observable Our Observable

UniverseUniverse

EarthEarthPeoplePeople

Page 4: Your place in the cosmos - MIT

Nuclear fusion in starsNuclear fusion in stars

Our StarOur StarThe SunThe Sun

Where do heavy elements come from?Where do heavy elements come from?

The Periodic TableThe Periodic Table

Page 5: Your place in the cosmos - MIT

SupernovaESupernovaE

SN 1994dSN 1994dHubble Space TelescopeHubble Space Telescope

SN 1999bh SN 1999bh –– KatzmannKatzmannAutomated Imaging Automated Imaging Telescope & AndyTelescope & Andy

Page 6: Your place in the cosmos - MIT

GammaGamma--ray bursts (ray bursts (GRBsGRBs))The Brightest Explosions in the Universe!

Long Duration GRBsOccur along with

supernovae of some massive stars

Short Duration GRBsProbably merging

neutron stars

Page 7: Your place in the cosmos - MIT

Supernova REMNANTSSupernova REMNANTS

•What’s left over after the explosion?

Page 8: Your place in the cosmos - MIT

We are all made of starsWe are all made of stars

Page 9: Your place in the cosmos - MIT

Cosmic RaysCosmic Rays

DNA MoleculeDNA Molecule

SNeSNe & & GRBsGRBsBursts Produce Bursts Produce HighHigh--Energy Energy Cosmic RaysCosmic Rays

Cosmic Ray Cosmic Ray Air ShowerAir Shower

Cosmic Rays Cosmic Rays From Space Set From Space Set the Background the Background Rate of Genetic Rate of Genetic

Mutation on Mutation on Earth!Earth!

Page 10: Your place in the cosmos - MIT

Astrophysical disastersAstrophysical disasters

Asteroid ImpactsAsteroid Impacts

Supernovae in our own Supernovae in our own Galaxy or GammaGalaxy or Gamma--Ray Ray Bursts even in distant Bursts even in distant

galaxies!galaxies!

Page 11: Your place in the cosmos - MIT

conclusionsconclusions

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HISTORICAL SUPERNOVAEHISTORICAL SUPERNOVAE

Year Report Supernove Remnant 1006 China, Japan, Korea, Arab lands, Europe Identified with radio SNR

1054 China, Japan Crab Nebula

1181 China, Japan Possible identification with radio SNR 3C58

1572 Europe (Tycho Brahe), China, Japan Tycho's remnant

1604 Europe (Kepler), China, Japan, Korea Kepler's remnant

1987 SN 1987A – Large Magellanic Cloud Remnant still observable

Supernovae in our galaxy (or a nearby galaxy)Supernovae in our galaxy (or a nearby galaxy)

Page 29: Your place in the cosmos - MIT

Neutron starsNeutron stars

Page 30: Your place in the cosmos - MIT

PULsarsPULsars

•Pulsars are rapidly rotating neutron stars with radio or X-ray beams like lighthouses•Pulsars rotate with precise regularity that beats our best atomic clocks.

Crab NebulaCrab NebulaPulsar MoviePulsar Movie

Page 31: Your place in the cosmos - MIT

Quark starsQuark stars

Page 32: Your place in the cosmos - MIT

Star warsStar wars

Astrophysical ObjectAstrophysical Object Force Fighting GravityForce Fighting Gravity

PeoplePeople ElectromagnetismElectromagnetism

PlanetsPlanets ElectromagnetismElectromagnetism

ProtostarsProtostars Thermal Pressure Thermal Pressure (gravitational contraction)(gravitational contraction)

Main Sequence StarsMain Sequence Stars Thermal Pressure Thermal Pressure (nuclear fusion)(nuclear fusion)

White DwarfsWhite Dwarfs electron degeneracy pressureelectron degeneracy pressure

Neutron StarsNeutron Stars neutron degeneracy pressureneutron degeneracy pressure

Quark StarsQuark Stars quark pressure?quark pressure?

Black HolesBlack Holes NOTHING!NOTHING!

Page 33: Your place in the cosmos - MIT

Type Type IaIa SupernovaESupernovaEThermonuclear Bombs in Space!Explosions of White Dwarfs in Binary Systems

WD Accretion From Main Sequence Companion

Merger of 2 White Dwarfs

Page 34: Your place in the cosmos - MIT

Type I i SupernovaeType I i SupernovaeGravity Bombs!Gravitational Core Collapse of Massive Stars

Star with M > 8 Star with M > 8 MMsunsun

The SunThe Sun

Page 35: Your place in the cosmos - MIT

Stellar Explosion Stellar Explosion MOVIEsMOVIEs

Core Collapse Supernova Movie

Page 36: Your place in the cosmos - MIT

GammaGamma--ray bursts (ray bursts (GRBsGRBs))The Brightest Explosions in the Universe!

Long Duration GRBsOccur along with core collapse supernovae of

some massive stars

Short Duration GRBsProbably merging

neutron stars

Page 37: Your place in the cosmos - MIT

Stellar Explosion Stellar Explosion MOVIEsMOVIEs

Gamma Ray Burst Movie

Page 38: Your place in the cosmos - MIT

Leftover Leftover COMpactCOMpact objectsobjects

Type of Stellar Explosion

Compact Remnant

Type Ia NOTHING!

Failed Type Ia NEUTRON STAR?

NEUTRON STARType II

BLACK HOLE

Gamma-Ray Burst BLACK HOLE

Page 39: Your place in the cosmos - MIT

Black holesBlack holes

The SchwarzchildRadius

Page 40: Your place in the cosmos - MIT

Evidence for Black holesEvidence for Black holes

SupermassiveBlack Holes

M ~ 106 – 109 Msun

Stellar MassBlack Holes

M ~ 3 – 20 Msun