The Galaxy Rotation with Dark Mater model shows that the actual rotation of spiral galaxies cannot be accounted for by visible matter alone. Newtonian dynamics allows us to compute the amount of additional matter, that we call "dark", needed to compute correctly the observed galaxy rotation curve. Here we use a simple model to simulate the galaxy rotation curve and the distribution of visible matter (namely, stars) within the galaxy. It is possible to vary the parameters of the dark matter distribution in order to improve the interpretation of the rotation of the galaxy.
The Galaxy Rotation with Dark Mater model was created using the Easy Java Simulations (EJS) modeling tool. It is distributed as a ready-to-run (compiled) Java archive. Double click the ejs_astro_GalaxyRotation.jar file to run the program if Java is installed.
Please note that this resource requires
at least version 1.5 of
Galaxy Rotation with Dark Matter Source Code
The source code zip archive contains an EJS-XML representation of the Galaxy Rotation with Dark Matte Model. Unzip this archive in your EJS workspace to compile and run this model using EJS. download 137kb .zip
Last Modified: June 6, 2014
Pisani, A. (2011). Galaxy Rotation with Dark Matter Model (Version 1.0) [Computer software]. Retrieved December 5, 2016, from http://www.compadre.org/Repository/document/ServeFile.cfm?ID=11512&DocID=2444
%0 Computer Program %A Pisani, Armando %D October 14, 2011 %T Galaxy Rotation with Dark Matter Model %7 1.0 %8 October 14, 2011 %U http://www.compadre.org/Repository/document/ServeFile.cfm?ID=11512&DocID=2444
Disclaimer: ComPADRE offers citation styles as a guide only. We cannot offer interpretations about citations as this is an automated procedure. Please refer to the style manuals in the Citation Source Information area for clarifications.