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What is Seti@Home?

Most of the SETI programs in existence today, including those at UC Berkeley build large computers that analyze that data from the telescope in real time. None of these computers look very deeply at the data for weak signals nor do they look for a large class of signal types (which we'll discuss further on...) The reason for this is because they are limited by the amount of computer power available for data analysis. To tease out the weakest signals, a great amount of computer power is necessary. It would take a monstrous supercomputer to get the job done. SETI programs could never afford to build or buy that computing power. There is a trade-off that they can make. Rather than a huge computer to do the job, they could use a smaller computer but just take longer to do it. But then there would be lots of data piling up. What if they used LOTS of small computers, all working simultaneously on different parts of the analysis? Where can the SETI team possibly find thousands of computers they'd need to analyze the data continuously streaming from Arecibo? 
The UC Berkeley SETI team has discovered that there are already thousands of computers that might be available for use. Most of these computers sit around most of the time with toasters flying across their screens accomplishing absolutely nothing and wasting electricity to boot. This is where SETI@home (and you!) come into the picture. The SETI@home project hopes to convince you to allow us to borrow your computer when you aren't using it and to help us "�search out new life and new civilizations." We'll do this with a screen saver that can go get a chunk of data from us over the internet, analyze that data, and then report the results back to us. When you need your computer back, our screen saver instantly gets out of the way and only continues it's analysis when you are finished with your work.

It's an interesting and difficult task. There's so much data to analyze that it seems impossible! Fortunately, the data analysis task can be easily broken up into little pieces that can all be worked on separately and in parallel. None of the pieces depends on the other pieces. Also, there is only a finite amount of sky that can be seen from Arecibo. In the next two years the entire sky as seen from the telescope will be scanned three times. We feel that this will be enough for this project. By the time we've looked at the sky three times, there will be new telescopes, new experiments, and new approaches to SETI. We hope that you will be able to participate in them too!

Project Plan

Project Plan

A history and future schedule of SETI@home:

1996: David Gedye, along with Craig Kasnoff, conceived the idea for SETI@home and formed the initial project team. A scientific plan was developed that received widespread academic support at the 5th International Conference in Bioastronomy in July 1996.

1997: The signal analysis code and prototypes of the client and server software were developed.

1998: Most of this year has been devoted to fundraising. In 9/98 we began working on the data recording system and on the final version of the client software. In 11/98 we plan to begin recording data and to begin testing the client software.

1999: From 1/99 through 3/99 we will test and debug the client software, develop the final version of the server software, and prepare the web site for launch. The launch is scheduled for 4/99.

2000-2001: To survey as much of the sky as possible, the experiment will run for two years. The web site will be updated regularly with progress reports, and explanations of the results found so far.

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