K
kk434
Guest
A quick description how astronomers calculate the D.M. halo:
Firsth you create a computer model that simulates the orbital speed of the stars. You place all the visible mass and run the model, it shows that the outermost stars have a lower than observed speed. Then you place invisible mass at specific places in the galaxy and run the model again, if you placed the mass at the right places it maches the observed rorational curve.
Does anyone know what set of equations are used? How complicated the simplest model is ?
Firsth you create a computer model that simulates the orbital speed of the stars. You place all the visible mass and run the model, it shows that the outermost stars have a lower than observed speed. Then you place invisible mass at specific places in the galaxy and run the model again, if you placed the mass at the right places it maches the observed rorational curve.
Does anyone know what set of equations are used? How complicated the simplest model is ?