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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.
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Roger Blandford KIPAC Stanford Exploring the Crab Nebula with theHubble, Chandra and FermiSpace Telescopes NASM
Anasazi Indians NASM
Charles Messier NASM
Franco Pacini predictsCrab Nebula Powered by Neutron Star NASM
John Bahcall (1934-2005) Astrophysicist Astronomical Leader Mentor to Young Scientists Champion of Hubble Space Telescope NASM
VERITAS/H.E.S.S. High Energy Astronomy! eVkeVMeVGeVTeVPeVEeVZeV LIGO X Radio Gamma-Rays Cosmic Rays Ice Cube Electromagnetic waves comprise particles calledPhotons Cosmic rays comprise mainly Protons and Electrons NASM
The Pulsing g-ray Sky Pulses at 1/10th true rate NASM
H.E.S.S. NASM
Supernova Explosion Supernova 1987a in Magellanic Cloud NASM
The Entire Spectrum TeV Synchrotron Radiation Compton Scattering Gamma Rays Radio NASM
Synchrotron Radiation 10 TeV ~0.01 Gauss 10 keV Maximum Synchrotron Photon Energy ~ 100 MeV NASM
Compton Scattering 10 TeV Electron 0.1 eV Infrared Photon 5 TeV Electron 5 TeV Gamma-rayPhoton NASM
Neutron Star • Mass: 1.5 suns • Radius: 10 km • Density: million, billion x water • Rotation Rate: 30 per second • Magnetic Field: 1 trillion Gauss Wilson NASM
Crab Pulsar NASM
Faraday’s Disk Magnet Conducting Disk Crank Voltage: 50 PetaVolts Current: 300 TeraAmps Power: 100,000 Suns NASM
The Restless Crab Hester NASM
FermiFlares NASM
Spectral Changes September Flare 4 day variation Synchrotron Radiation Limit Compton Scattering Synchrotron Radiation NASM
Where is the Flare? Pulsar Torus Jet NASM
Let’s Keep Exploring the Crab Nebula Thank You NASM