Simulation by SPH of the collapse and fragmentation of a molecular cloud presented in "The Formation of Stars and Brown Dwarfs and the Truncation of Protoplanetary Discs in a Star Cluster" by Matth...
Simulation by SPH of the collapse and fragmentation of a molecular cloud presented in "The Formation of Stars and Brown Dwarfs and the Truncation of Protoplanetary Discs in a Star Cluster" by Matthew R. Bate, Ian A. Bonnell, and Volker Bromm (http://www.ukaff.ac.uk/starcluster/).
The calculation models the collapse and fragmentation of a molecular cloud with a mass 50 times that of our Sun. The cloud is initially 1.2 light-years (9.5 million million kilometres) in diameter, with a temperature of 10 Kelvin (-263 degrees Celsius).
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To play an *.flv? Yeah, you don't need a super computer, but to compile asimulation which is depicted in the flv you'd need something better, since to make a single frame you'd need to recalculate the position of each individual particle based on the positions of other particles. Having said that, my above calculations are wrong since I misunderstood the term "CPU hours", the whole calculation didn't take 100.000hrs it took 64 times less and the power of each core was 64 times bigger.
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It's a lot, maybe in 20 years we'll be able to do this on our laptops.