The First Results Are in From NASA’s Closest Flyby of the Sun

NASA's Parker Solar Probe Sheds New Light on the Sun

The Parker Solar Probe team is kind of blowing everyone away with some unprecedented findings of the behavior of our sun, solar wind and the star’s peculiar magnetic field. Since its launch in 2018, the Parker Solar Probe has been busy collecting data to help answer some of the biggest unsolved mysteries about the star at the center of our solar system. As a refresher, Parker is a highly specialized craft that is capable of getting us closer than ever to its surface.

This new batch of record-breaking data was collected by the probe between late 2018 and April 2019 after completing just two of its 24 planned flybys, where it managed to get just 38 million km away from the star. So far, the Parker team has been focused on measuring the behavior of the solar wind, the Sun’s constant outflow of charged particles. While these solar particles do eventually reach our humble blue planet, they really can’t tell us much about the solar wind and the complex systems on the surface of the Sun.





New Discoveries from NASA's Parker Solar Probe

So what exactly has Parker found that’s got everyone so excited? Well, from its close vantage point to the Sun, the new data collected has presented the possible source for “slow” solar wind, a phenomenon that has been a long-standing mystery within the scientific community. Not to be confused with the fast solar wind, which scientists know a lot more about. These winds travel between 500 and 1,000 kilometers per second and they come from large coronal holes at the sun's north and south poles. ‘Slow’ solar wind, on the other hand, moves at speeds less than 500 km per second, and its source has remained unknown until now.

After spending roughly a week observing the coronal holes—areas of colder, darker low-density plasma—Parker was able to strongly correlate coronal holes located near the Sun's equator, to the origin of the slow solar wind. But that wasn’t the most surprising part! Parker also revealed a previously unknown feature of the solar wind.

found rapid reversals in the direction of the magnetic field

The probe’s measurements found rapid reversals in the direction of the magnetic field, which moves outward from the sun embedded in the solar wind. Known as switchbacks, these phenomena bend back on themselves in moments that can last anywhere from several seconds to several minutes.

Parker observed that these switchbacks occurred quite frequently, causing the slow winds to accelerate to form long tubes of a fast wind containing plasma with around twice the energy of the background solar wind. Researchers are speculating that these energetic bursts could help explain why the Sun’s atmosphere is so much hotter than its surface. But more research is needed before we're able to know for sure. All of this is to say that this brand new information is making us completely rethink the physics of the Sun.

Scientists hope that Parker's subsequent flybys and further data analysis will help them build models to understand and predict space weather in order to better protect astronauts and avoid disruption in our satellites and electrical grid systems. So what we learned from Solar Probe will definitely play very seriously into our understanding of space weather, of the dynamics of the Earth's magnetic field, the communication networks, the power grid on Earth is an extraordinary, complex electromagnetic system. And so having big disturbances from the Sun that can generate large currents in our power grid, in our communications grid, is potentially a very serious thing.

Another thing that surprised scientists

Now Parker's data on the solar wind and weird magnetic field wasn't the only thing that took scientists by surprise. It has long been suspected that the area around the Sun is completely void of cosmic dust. That's the stuff left over by celestial collisions from the formation of our galaxy. The long-held theory suggested that as dust approaches the star, it’s heated to high temperatures and turned into a gas, resulting in a dust-free zone at roughly three to 4.8 million km away from the Sun. And the Parker probe just found the very first evidence of this cosmic phenomenon.

Its imaging instrument WISPR looked out onto large sections of the corona and solar wind, observing dust that started to thin out at roughly 11 million km and this decrease continued until WISPR hit its limit of what it could measure, at around six million km from the Sun. Scientists expect to explore this preliminary finding in more detail as early as 2020. As Parker continues on its fourth flyby of the Sun, what’s really amazing is that all this data came from the spacecraft’s first two flybys, so who knows what they’ll find next.





Barker will continue his journey