As Comet Schwassmann-Wachmann 3 continues what may be its final trip around the Sun(breaking up along the way), astronomers are turning everything they have toward it. While it isn’t as bright to the naked eye as Hyakutake or Hale-Bopp were a few years back, S-W3 is turning out to be dazzler in other wavelengths, most notably x-rays. In fact, it’s the brightest x-ray comet ever. The folks using the Chandra Observatory, the XMM-Newton satellite, and the Suzaku satellite (all three in orbit around Earth) are all getting ready to study the x-rays streaming off the comet.

The image above is what the comet looks like in x-ray wavelengths. It was taken using the NASA Swift satellite, which studied the comet recently. The data showed that the comet is about 20 times brighter in x-ray wavelengths of light.

How can a comet produce x-rays? It seems somewhat counterintuitive that such a cold, icy object would glow in wavelengths more commonly associated with hot, active events and objects. Astronomers are still characterizing the interactions that occur that cause cometary x-rays, but the basic story is this: as the comet plows through the solar wind, something called “charge exchange” occurs. Okay, that sounds appropriately mysterious, but what does it mean?

The solar wind is a stream of particles (electrons and protons). The comet is a lump of ices and dust. As it moves through the solar wind, those particles and gases fly away from the comet, particularly as the ices are warmed by the Sun. Those cometary bits are usually particles of molecules of water, methane, and carbon dioxide. When they the high-speed, high-energy particles from the solar wind encounter these lower-energy particles from the comet, electrons get “stolen” from the cometary chemical particles. In the process, a tiny bit of charge is exchanged and the result is a spark of energy, which results in an x-ray. So, it’s a collisional process that depends on an interaction between the comet and the solar wind. It’s not just from something the comet itself is generating.

Now, if you know enough about the x-ray energies that are given off in these collisions, you can make some deductions about the content of the solar wind and the makeup of the gases and materials being emitted by the comet. And this is one of the results of studying x-rays (and other high-energy emisssions) from such events as comets plowing through the solar wind.