Wanna Do Some Science?

I’ve been running Seti@Home on my computer for a few years now and have managed to crank out a few thousand work units for the cause. Its seems like an easy-enough contribution to science: donate unused computer cycles to some giant distributed-computing project. I like the screensaver—it’s spiffy-looking and gives me some idea of the progress my machine is making as it crunches data from stellar signals.

So, why not try it? If you’re interested, you can sign up and get started over at
Seti@Home.

If searching for signals from ET isn’t your cup of tea, maybe you’d like to help out with some astrophysical researchers trying to detect gravitational waves. These are ripples in the fabric of space and time, emanating from such violent events in the cosmos as black hole collisions and supernovae, the action around rapidly rotating compact stars, and between active members of binary systems. These ripples travel through space, carrying information both about their source and about the nature of gravity itself. And there are two groups of astrophysicists trying to detect them: the LIGO and the GEO-600 collaboration. Their measurements are producing data that needs crunching, and why not use the world’s desktops as a powerful tool, just as the Seti@Home folks do with their distributed computing? If you’re interested in that project, you can visit the Einstein@Home project.

These are two of many other distributing computer projects that make solid contributions to science every day. I think it’s pretty cool that people and their home computers can be a part of Big Science!

Saturn’s Aurorae on the Move


Still from aurora movie
Still from aurora movie

Ever since the Pioneer and Voyager missions to the outer planets in the late 70s and early 80s, planetary scientists have known about Saturn’s aurorae. Hubble Space Telescope scientists have tracked the eerie glows over the past decade and a half using ultraviolet filters and instruments to study the characteristics of these emissions-related events. Recent studies using the Hubble Space Telescope and Cassini spacecraft show that the dancing light of the auroras on Saturn behaves in ways different from how scientists have thought possible for the last 25 years.

To get the image above, astronomers combined HST and Cassini ultraviolet images of Saturn’s southern polar region with visible-light images of the planet and its rings to make this picture. The auroral display appears blue because of the glow of ultraviolet light. In reality, the aurora would appear red to an observer at Saturn because of the presence of glowing hydrogen in the atmosphere. On Earth, charged particles from the Sun collide with nitrogen and oxygen in the upper atmosphere, creating auroral displays colored mostly green and blue.

If you click on the link above, you’ll see a “movie” of the Saturnian aurorae,dancing around the auroral “oval” at one of the planets’ poles. For more pictures and videos, visit the European Space Agency’s Hubble releases page.