pulsar stage and neutron star
TRANSCRIPT
Neutron Star
and
Pulsar Stage
Mattia Sibilia VDa.s. 2013/14
Introduction
Star
White Dwarf
Black Dwarf
Red Supergiant
Planetary Nebula
SNR (SuperNovae Remnant)
Neutron Star / Pulsar
Black Hole
Supernova
The Birth
Red Supergiant
Supernova explosion
Outward (external strata)
Inward ( central core )
Compression in a sphere ( 10 miles )
Neutron Star
The structure
Compression
Change of structure
electrons and protons
neutrons
Central core
Dense, super-hot mass
The properties - Density
Neutron Star
dense object
No empty space in his structure
Teaspoon of neutron star's matter
100 million tons
On Earth it would disappear instantly
The properties - Surface
Enormous Gravity force
No hills or bumps
Perfect glass ball
Attraction of debris
Pressed on surface
Part of solid crust
The properties - spin
During supernova explosion
Mass spin very fast
Principle of Conservation of Angular Momentum
Normally 30 times/sec
The fastest one 600 times/sec
The properties - Temperature
Temperature
500 million degrees
X-rays
White
The Magnetic Fields
Supernova explosion
Magnetic forces
debris around the star
Impact the surface of neutron star (due to the gravity force)
jets
Pulsar
Matter impacted
turn back away from star
Into two narrow beams of matter
jets
Point at Earth
Pulsing Neutron Star or Pulsar
The Death
Slowly the rest of supernova gases (fuel of neutron star)
Will run out:
No Jets
colour: from white to red
The spin decelerate
Black frigid sphere with a powerful gravity
Black Dwarf
bibliography
Celestia's educational activity nr. 6 (Star)
Geografia Generale (Crippa-Fiorani)
http://en.wikipedia.org/wiki/Neutron_star
http://www.nasa.gov/ ( for images )