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25 ii 2011 25 ii 2011

25 ii 2011 - PowerPoint Presentation

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25 ii 2011 - PPT Presentation

NASM 1 Exploring the Crab Nebula with the Hubble Chandra and Fermi Space Telescopes Roger Blandford KIPAC Stanford Anasazi Indians 25 ii 2011 NASM 2 Charles Messier 25 ii 2011 NASM 3 ID: 216422

nasm 2011 synchrotron tev 2011 nasm tev synchrotron crab rays telescope nebula radiation gamma scattering compton radio neutron star

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Slide1

25 ii 2011

NASM

1

Exploring the Crab Nebula with theHubble, Chandra and FermiSpace Telescopes

Roger BlandfordKIPACStanfordSlide2

Anasazi Indians

25 ii 2011

NASM

2Slide3

Charles Messier

25 ii 2011

NASM

3Slide4

Sam Okoye

discovers compact radio source

25 ii 2011

NASM4Slide5

Franco Pacini

predictsCrab Nebula Powered by Neutron Star

25 ii 2011

NASM5Slide6

Jocelyn Bell Discovers Pulsars

25 ii 2011

NASM

6Slide7

John Bahcall (1934-2005)

25 ii 2011

NASM

Astrophysicist

Astronomical LeaderMentor to Young ScientistsChampion of Hubble Space Telescope7Slide8

Hubble Space Telescope

25 ii 2011

NASM

8Slide9

Chandra X-ray Telescope

25 ii 2011

NASM

9Slide10

25 ii 2011

NASM

10

High Energy Astronomy!

VERITAS/H.E.S.S.LIGOIce 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

RadioSlide11

25 ii 2011

NASM

11

Fermi(the scientist and the telescope)Slide12

The Pulsing

g

-ray Sky

Pulses at

1/10

th

true rate

25 ii 2011

12

NASMSlide13

25 ii 2011

NASM

H.E.S.S.

13Slide14

Supernova Explosion

25 ii 2011

NASM

14

Supernova 1987a in Magellanic CloudSlide15

Crab Nebula at Different Wavelengths

25 ii 2011

NASM

15Slide16

Optical and X-rays Combined

25 ii 2011

NASM

16Slide17

The Entire Spectrum

25 ii 2011

NASM

17Radio

Gamma RaysTeVSynchrotronRadiationComptonScatteringSlide18

Synchrotron Radiation

Maximum Synchrotron Photon Energy ~ 100

MeV

25 ii 2011

18NASM~0.01 Gauss10

keV

10

TeVSlide19

Compton Scattering

25 ii 2011

NASM

19

0.1 eV Infrared Photon

10 TeV Electron

5

TeV

Electron

5

TeV

Gamma-

rayPhotonSlide20

Neutron Star

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NASM

20Wilson

Mass: 1.5 sunsRadius: 10 km Density: million, billion x waterRotation Rate: 30 per secondMagnetic Field: 1 trillion Gauss Slide21

Crab Pulsar

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NASM

21Slide22

25 ii 2011

NASM

22

Faraday’s Disk

MagnetConducting DiskCrank

Voltage: 50

PetaVolts

Current: 300

TeraAmps

Power: 100,000 SunsSlide23

The

Restless Crab

Hester

25 ii 201123

NASMSlide24

Fermi

Flares

25 ii 2011

24NASMSlide25

Spectral

Changes

September Flare

4 day variation

SynchrotronRadiationCompton Scattering25 ii 2011

25

NASM

SynchrotronRadiationLimitSlide26

Where is the Flare?

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NASM

26

JetTorus

PulsarSlide27

Let’s Keep Exploring the Crab Nebula

25 ii 2011

NASM

27

Thank You