exploring the crab nebula with the hubble, chandra and fermi space telescopes

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25 ii 2011 NASM 1 Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes Roger Blandford KIPAC Stanford

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Roger Blandford KIPAC Stanford. Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes. Anasazi Indians. Charles Messier. Sam Okoye discovers compact radio source. Franco Pacini predicts Crab Nebula Powered by Neutron Star . Jocelyn Bell Discovers Pulsars. - PowerPoint PPT Presentation

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Page 1: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 125 ii 2011

Exploring the Crab Nebula with the

Hubble, Chandra and FermiSpace Telescopes

Roger BlandfordKIPAC

Stanford

Page 2: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 2

Anasazi Indians

25 ii 2011

Page 3: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 3

Charles Messier

25 ii 2011

Page 4: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 4

Sam Okoye discovers compact radio source

25 ii 2011

Page 5: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 5

Franco Pacini predictsCrab Nebula Powered

by Neutron Star

25 ii 2011

Page 6: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 6

Jocelyn Bell Discovers Pulsars

25 ii 2011

Page 7: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

7

John Bahcall (1934-2005)

25 ii 2011 NASM

AstrophysicistAstronomical LeaderMentor to Young ScientistsChampion of Hubble Space Telescope

Page 8: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 8

Hubble Space Telescope

25 ii 2011

Page 9: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 9

Chandra X-ray Telescope

25 ii 2011

Page 10: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 1025 ii 2011

High Energy Astronomy! VERITAS/H.E.S.S.

LIGO

Ice Cube

eV keV MeV GeV TeV PeV EeV ZeV

Cosmic Rays

Gamma-Rays

X

Electromagnetic waves comprise particles called Photons

Cosmic rays comprise mainly Protons and Electrons

Radio

Page 11: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 1125 ii 2011

Fermi(the scientist

and the telescope)

Page 12: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 12

The Pulsing g-ray Sky

Pulses at1/10th true rate

25 ii 2011

Page 13: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 1325 ii 2011

H.E.S.S.

Page 14: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 14

Supernova Explosion

25 ii 2011

Supernova 1987a in Magellanic Cloud

Page 15: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 15

Crab Nebula at Different Wavelengths

25 ii 2011

Page 16: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 16

Optical and X-rays Combined

25 ii 2011

Page 17: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 17

The Entire Spectrum

25 ii 2011 Radio Gamma Rays

TeV

SynchrotronRadiation

ComptonScattering

Page 18: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 18

Synchrotron Radiation

Maximum Synchrotron Photon Energy ~ 100 MeV

25 ii 2011

~0.01 Gauss 10 keV

10 TeV

Page 19: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 19

Compton Scattering

25 ii 2011

0.1 eV Infrared Photon

10 TeV Electron

5 TeV Electron

5 TeV Gamma-rayPhoton

Page 20: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 20

Neutron Star

25 ii 2011

Wilson

• Mass: 1.5 suns• Radius: 10 km • Density: million, billion x

water• Rotation Rate: 30 per

second• Magnetic Field: 1 trillion

Gauss

Page 21: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 21

Crab Pulsar

25 ii 2011

Page 22: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 2225 ii 2011

Faraday’s Disk

Magnet

Conducting DiskCrank

Voltage: 50 PetaVoltsCurrent: 300 TeraAmpsPower: 100,000 Suns

Page 23: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 23

The Restless Crab

Hester25 ii 2011

Page 24: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 24

Fermi Flares

25 ii 2011

Page 25: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 25

Spectral Changes

September Flare4 day variation

SynchrotronRadiation

Compton Scattering

25 ii 2011

SynchrotronRadiation

Limit

Page 26: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 26

Where is the Flare?

25 ii 2011 Jet Torus

Pulsar

Page 27: Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes

NASM 27

Let’s Keep Exploring the Crab Nebula

25 ii 2011

Thank You