Little Fe Configuration and GalaxSee Detection Code for Simulation the Planets with Pixels and Color Skin

Abstract

In this project we implemented a step by step procedure, of how to configure the portable cluster LittleFe, how to install the UNIX-LINUX operating system to the LittleFe (Server) and modifications to the GalaxSee Code. Also we will see a brief description of what is a LittleFe cluster and the associated hardware. The linux diestro used in this project is very powerful to complete tasks like this one. Galaxies are collections of billions of stars; our home galaxy, the Milky Way, is a typical example. New generations of stars are born out of gas that condenses within regions called giant molecular clouds, and the stars sometimes form into star clusters. When a star reaches the end of its evolution, it may return much of its gas back to the interstellar medium, which will be the source for a new generation of stars. Galaxies can be thought of as systems that turn gas into stars and back again. This is the reason why this project is so important to understand even more knowledge about galaxies. Key Terms -BCCD, CMOS, CUDA, MPI