Comet tails blowing in the solar wind

Comet C/2006 P1 -- also known as Comet McNaught, named for astronomer Robert McNaught, who discovered it in August 2006 -- was one of the brightest comets visible from Earth in the past 50 years. Throughout January 2007, the comet fanned across the Southern Hemisphere's sky, so bright it was visible to the naked eye even during the day. McNaught belongs to a rarefied group of comets, dubbed the Great Comets and known for their exceptional brightness. Setting McNaught apart further still from its peers, however, was its highly structured tail, composed of many distinct dust bands called striae, or striations, that stretched more than 100 million miles behind the comet, longer than the distance between Earth and the Sun. One month later, in February 2007, an ESA (European Space Agency) and NASA spacecraft called Ulysses would encounter the comet's long tail.

"McNaught was a huge deal when it came because it was so ridiculously bright and beautiful in the sky," Battams said. "It had these striae -- dusty fingers that extended across a huge expanse of the sky. Structurally, it's one of the most beautiful comets we've seen for decades."

How exactly the tail broke up in this manner, scientists didn't know. It called to mind reports of another storied comet from long ago: the Great Comet of 1744, which was said to have dramatically fanned out in six tails over the horizon, a phenomenon astronomers then couldn't explain. By untangling the mystery of McNaught's tail, scientists hoped to learn something new about the nature of comets -- and solve two cosmic mysteries in one.

A key difference between studying comets in 1744 and 2007 is, of course, our ability to do so from space. In addition to STEREO's serendipitous sighting, another mission, ESA/NASA's SOHO -- the Solar and Heliospheric Observatory -- made regular observations as McNaught flew by the Sun. Researchers hoped these images might contain their answers.

Now, years later, Oliver Price, a planetary science Ph.D. student at University College London's Mullard Space Science Laboratory in the United Kingdom, has developed a new image-processing technique to mine through the wealth of data. Price's findings -- summarized in a recently published Icarus paper -- offer the first observations of striations forming, and an unexpected revelation about the Sun's effect on comet dust.

Comets are cosmic crumbs of frozen gas, rock and dust left over from the formation of our solar system 4.6 billion years ago -- and so they may contain important clues about our solar system's early history. Those clues are unlocked, as if from a time capsule, every time a comet's elliptical orbit brings it close to the Sun. Intense heat vaporizes the frozen gases and releases the dust within, which streams behind the comet, forming two distinct tails: an ion tail carried by the solar wind -- the constant flow of charged particles from the Sun -- and a dust tail.

Understanding how dust behaves in the tail -- how it fragments and clumps together -- can teach scientists a great deal about similar processes that formed dust into asteroids, moons and even planets all those billions of years ago. Appearing as one of the biggest and most structurally complex comets in recent history, McNaught was a particularly good subject for this type of study. Its brightness and high dust production made it much easier to resolve the evolution of fine structures in its dust tail.

Price began his study focusing on something the scientists couldn't explain. "My supervisor and I noticed weird goings-on in the images of these striations, a disruption in the otherwise clean lines," he said. "I set out to investigate what might have happened to create this weird effect."

The rift seemed to be located at the heliospheric current sheet, a boundary where the magnetic orientation, or polarity, of the electrified solar wind changes directions. This puzzled scientists because while they have long known a comet's ion tail is affected by the solar wind, they had never seen the solar wind impact dust tails before.

Dust in McNaught's tail -- roughly the size of cigarette smoke -- is too heavy, the scientists thought, for the solar wind to push around. On the other hand, an ion tail's miniscule, electrically charged ions and electrons easily sail along the solar wind. But it was difficult to tell exactly what was going on with McNaught's dust, and where, because at roughly 60 miles per second, the comet was rapidly traveling in and out of STEREO and SOHO's view.

"We got really good data sets with this comet, but they were from different cameras on different spacecraft, which are all in different places," Price said. "I was looking for a way to bring it all together to get a complete picture of what's happening in the tail."

His solution was a novel image-processing technique that compiles all the data from different spacecraft using a simulation of the tail, where the location of each tiny speck of dust is mapped by solar conditions and physical characteristics like its size and age, or how long it'd been since it'd flown off the head, or coma, of the comet. The end result is what Price dubbed a temporal map, which layers information from all the images taken at any given moment, allowing him to follow the dust's movements.

The temporal maps meant Price could watch the striations form over time. His videos, which cover the span of two weeks, are the first to track the formation and evolution of these structures, showing how dust fragments topple off the comet head and collapse into long striations.

But the researchers were most excited to find that Price's maps made it easier to explain the strange effect that drew their attention to the data in the first place. Indeed, the current sheet was the culprit behind the disruptions in the dust tail, breaking up each striation's smooth, distinct lines. For the two days it took the full length of the comet to traverse the current sheet, whenever dust encountered the changing magnetic conditions there, it was jolted out of position, as if crossing some cosmic speed bump.

"It's like the striation's feathers are ruffled when it crosses the current sheet," University College London planetary scientist Geraint Jones said. "If you picture a wing with lots of feathers, as the wing crosses the sheet, lighter ends of the feathers get bent out of shape. For us, this is strong evidence that the dust is electrically charged, and that the solar wind is affecting the motion of that dust."

Scientists have long known the solar wind affects charged dust; missions like Galileo Cassini, and Ulysses watched it move electrically charged dust through the space near Jupiter and Saturn. But it was a surprise for them to see the solar wind affect larger dust grains like those in McNaught's tail -- about 100 times bigger than the dust seen ejected from around Jupiter and Saturn -- because they're that much heavier for the solar wind to push around.

With this study, scientists gain new insights into long-held mysteries. The work sheds light on the nature of striated comet tails from the past and provides a crucial lens for studying other comets in the future. But it also opens a new line of questioning: What role did the Sun have in our solar system's formation and early history?

"Now that we see the solar wind changed the position of dust grains in McNaught's tail, we can ask: Could it have been the case that early on in the solar system's history, the solar wind played a role in organizing ancient dust as well?" Jones said.