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Unformatted text preview: form of neutrinos. The gas has almost zero opacity with the neutrinos so they pass right on through the star's gas in just a few seconds. The equation of state, hydrostatic equilibrium and the other physical principles are put together for each layer in a star. The equations are solved for each layer starting from the layer there is direct information of, the surface. That result gives the conditions for the next layer's equations. Solving the layer's equations gives the conditions for the layer below it and this process continues on down toward the center layer by layer. In order to get sufficient detail for accurate results, the star's interior is divided into hundreds of layers. To save on time, the equations are solved using a computer....
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This note was uploaded on 12/15/2011 for the course AST AST1002 taught by Professor Emilyhoward during the Fall '10 term at Broward College.
- Fall '10