Milkyway@home/en

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Milkyway@Home uses the BOINC platform to harness volunteered computing resources, creating a highly accurate three dimensional model of the Milky Way galaxy using data gathered by the Sloan Digital Sky Survey. This project enables research in both astroinformatics and computer science.

In computer science, the project is investigating different optimization methods which are resilient to the fault-prone, heterogeneous and asynchronous nature of Internet computing; such as evolutionary and genetic algorithms, as well as asynchronous newton methods. While in astroinformatics, Milkyway@Home is generating highly accurate three dimensional models of the Sagittarius stream, which provides knowledge about how the Milky Way galaxy was formed and how tidal tails are created when galaxies merge.

Milkyway@Home is a joint effort between Rensselaer Polytechnic Institute's departments of Computer Science and Physics, Applied Physics and Astronomy.

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Milkyway@home
Start 2007
End
Status
Admin Jeffery M. Thompson
Institution Rensselaer Polytechnic Institute - AstroInformatics Group
Country USA
Area Astronomy
Apps
Win
Linux
Mac
64bit MilkyWay@Home N-Body Simulation 1.82 (mt) [win/linux]
PS3
ATI
CUDA
Intel
Android
RPi
NCI
System-Specs
VRAM SP DP
RAM
Runtime
HDD
Traffic dl/ul kb / kb
Deadline
Checkpoints