One of the pleasures of being an historian of science - turned - futurist is that my past and present lives often meet in unexpected ways. This recently happened with the announcement of the eSTAR project, an effort that uses grid computing and intelligent agents to identify and track unexpected astronomical events. As a news release explained,
"Intelligent Agent" computer programs are roaming the Internet and watching the skies. It may sound like science fiction, but these programs, using Grid computing technology, will help astronomers detect some of the most dramatic events in the universe, such as massive supernova explosions....
Dr. Alasdair Allan, on the eSTAR team at the University of Exeter, said "The universe currently does things faster than we can respond to them. To study the most rapid and violent events in the universe, we need to be able to follow them quickly."
As well as supernova explosions, many other astronomical events happen suddenly and unpredictably. These include the detection of near-Earth asteroids as they move across the sky, rapid changes in the swirling gases being swallowed by black holes, and the subtle changes in the brightness of stars which may indicate planets in orbit around them.
The Intelligent Agent programs communicate with telescopes and each other using technology designed for the Grid - the "next generation Internet". They make observations with the telescopes, which they can analyse and immediately follow up with further observations, without the need for human intervention.
Prof. Tim Naylor, who led the eSTAR team and is also at the University of Exeter, said "We're creating a network of telescopes which can respond automatically to objects of great astronomical importance."
eSTAR currently is only running on one telescope, the
United Kingdom Infrared Telescope, located on Mauna Kea in Hawaii, but the hope is to be able to connect a number of telescopes to eSTAR in the next few years. They're even
considering "a Java based interface which could run on the user's mobile phone" that would "provide up to the minute information for an astronomer who is out of the office, but still wants to monitor their observations."
This is only the latest chapter in astronomy's long history of dealing with information overload. The Babylonians, who performed what are probably the first systematic, quantitative observations of celestial events, generated thousands of tablets of data; ever since, astronomers have often had too much information at their disposal.
One strategy has been to pursue what we would describe as collaborative, open-source work. In the nineteenth century, the discipline's agenda was crowded with international projects to create star catalogs, standards for photometric and spectroscopic research, and to attack important problems.
Likewise, astronomy has long been a distributed science-- that is, the data-collection and analysis have taken place in a variety of places. Astronomers would farm out photographs or spectrographs to former students for analysis. Young scientists at schools that didn't have research facilities got access to data and the chance to remain scientifically productive, while observatories got to ease some of their backlogs of data. Astronomers weren't the only ones who did this. For example, T. H. Morgan's laboratory, which was renowned for its research on the genetics of Drosophila melanogaster (fruit flies), was the center of a large network that shared strains of flies and experimental data with high-school teachers and professors at small colleges. (There's a brilliant book on this network called Lords of the Fly: Drosophila Genetics and the Experimental Life, written by Robert Kohler.) Arguably, though, the portability of astronomical data-- tables of star positions, photographs, and spectrographs-- made it easier for them to distribute their research.
A third strategy was to create what essentially little factories for analyzing data. The growth in the nineteenth century of factory-like systems for analyzing masses of data. The Greenwich Observatory under George Airy was famous for the methodical, disciplined way it handled its celestial mechanics data; likewise the Harvard College Observatory under Edward Pickering built a staff (nicknamed "Pickering's harem" because it consisted entirely of women) to analyze its spectroscopic data. (It was in places like this that the term "computers" came to be used-- but not for machines, for people.)
So the digitization of astronomical research in the twentieth century-- the replacement of photographic plates with CCDs and digital cameras, the replacement of atlases and tables with computer files, and the emergence of radio astronomy-- didn't so much upset the discipline, as made it possible for them to adapt or update traditional ways of working. Astronomers had been sharing data and organizing long-distance collaborations for a long time; the Internet made it easier to do that work. Automated systems for detecting anomalies or taking measurements had also been around for decades, and computers allowed astronomers to increase the volume of data they could analyze this way. In a curious way, computers and networks appealed to both the open source and factory traditions in astronomy. (In a sense, observatories were merely exchanging one kind of "computer" for another, though of course the reality was quite a bit more complex.)
There are two new things here, though.
First is the emphasis on pace. Older distributed, collaborative systems in astronomical research were mainly designed to deal with backlogs of data, while eSTAR's purpose is to respond to quickly-moving events. There is a tradition within astronomy of collective action around unique events like solar eclipses or Transits of Venus, but even those are often known in advance. The aim here, as Allen put it, is to observe the "most rapid and violent events in the universe"-- and the unexpected.
Second, eSTAR invests a degree of intelligence and decision-making power in the network itself. As Allen told the BBC,
"What is so important here is that we have developed an intelligent observing system.... It thinks and reacts for itself, deciding whether something it has discovered is interesting enough to need more observations. If more observations are needed, it just goes ahead and gets them."
One final, broader observation. eSTAR is a great example of how a technological system can be innovative not because it contains a large amount of completely new technology, but because it combines existing technologies in new ways. eSTAR's tremendous potential depends on the fact that it creatively recombines a heterogeneous assortment of existing technologies. It uses existing telescopes, computer networks, even cell phones; the agents and telescopes communicate using RTML (remote Telescope Markup Language, an XML dialect). It treats the Internet and global telescope networks as a gigantic commons, the kind that Lawrence Lessig discusses in The Future of Ideas; and it won't work without a system that recognizes how deeply innovative technologies and services are indebted to their predecessors.
Grid Computing for Astronomers [Roland Piquepaille's Technology Trends]
Grid technology helps astronomers keep pace with the Universe [EurekAlert]
Smart software watches the skies [BBC]
Robert Kohler, Lords of the Fly: Drosophila Genetics and the Experimental Life (University of Chicago Press, 1994) [Amazon link]
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