Mon 20 Sep 2010
I came across a post in the Through the Kaleidoscope blog that got me thinking. “Crowd science – where masses of people participate in data collection for science projects – is growing … Astronomy is the area in which crowd science has been most frequently used, which makes sense given the field’s massive scale and large datasets. One example is the ten-year old SETI@home project …” I must admit here that I’ve been participating in the latter project since May 1999—which puts me in the 89th percentile of all 1.1 million SETI enthusiasts :-) I run the project using UC Berkeley’s BOINC, a commonly-used, multiplatform open-source program for volunteer computing and grid computing. BOINC facilitates running several projects at the same time according to selected settings. For instance, I’m also active in other projects: Einstein@home, MilkyWay@home (astronomy), Climateprediction.net (climatology), Rosetta@home, Malariacontrol.net (medical research), SZTAKI Desktop Grid (math), Quake Catcher Network (seismology). At one time, I also participated in non-BOINC projects but that was too cumbersome. The BOINC projects have attracted a lot of creative programmers so that there are for example at least seven websites where you can easily access your statistics both by project as well as combined. Each project awards credits for work done, allowing cross-project comparison and combination of your “scores.” It all serves to involve the participants, make them feel invested. There is even a way to have important milestones in you efforts posted on your FaceBook account, e.g., on September 3, I passed the 6,000 credit milestone for Climateprediction.net.
So what could we do with this crowd-sourced/distributed-computing approach in archaeology? After all, just like astronomy and medical research, we too have a lot of goodwill from the general public directed at us. There has to be a way to channel some of this. Surely, we can find some huge data sets that need processing and whose results can be appealing to a general audience? In the above blog post, another angle is also discussed, e.g., Galaxy Zoo, a project in which people help classify galaxies from Hubble Telescope images, a task that is hard to computerize. Some museums are letting the public tag artifacts online, a way to enhance the often-brief information available in the database (see the Steve Project). This is still primarily for art though, not archaeological artifacts. We all know that our budgets won’t increase in the near future, on the contrary. Let’s get creative!