Pulsars, Neutron Stars and Black Holes Model of a Neutron Star.

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Presentation transcript:

Pulsars, Neutron Stars and Black Holes Model of a Neutron Star

The Crab Nebula and the pulsar

Lighthouse Model Pulsar = Rotating Neutron Star Crab nebula in X-rays

Observational Evidence – X-ray Binaries

Black Holes -- depends on mass of collapsed core

A Little Bit of Relativity Special Relativity --- basic concepts Your physical reality is independent of how fast you are moving. The speed of light is a constant independent of your velocity The equivalence of matter and energy ( E= mc 2 ) Consequences --- length contraction time dilation mass increases (faster than light space ships?)

General Relativity -- with gravitation and acceleration How space (its shape) and time change in the presence of mass The shape of space is distorted – space curvature -- and time slows down Curvature or warping of space due to gravity

The 3 famous astronomical tests of general relativity the curvature of space time alters the path and wavelength of light. 1.Deflection of light by Sun -- eclipses 2. the advancement of the perihelion of Mercury 3. Gravitational redshift measured in spectra of stars

A GRAVITATIONAL SINGULARITY -- A.K.A. “BLACK HOLE”

Schwarzschild radius or event horizon R s = 3 M BH /M sun

Observational Evidence – affect on the environment

Journey into a Black Hole -- what do you and the intrepid astronaut observe, experience?

On the fringes --- white holes and wormholes, interstellar travel and you