Sun yields its secrets to Parker Solar Probe
Scientists are 'blown away' by unprecedented data from the Sun-kissing mission, culminating in new discoveriesEuropost
NASA's Parker Solar Probe made the closest ever flyby of the Sun in August 2018, collecting massive amounts of data using cutting-edge scientific instruments from a distance of 15 million miles - a mission that also, incidentally, set the record for the fastest-ever human-made object of all time.
Now, scientists are starting to release what they learned from the data it collected. Four new papers published in the journal Nature on Wednesday reveal new findings that could rewrite the way we understand the way stars are born, evolve, and die. They could also help us find new ways to protect astronauts from harsh space weather during long distance trips through the Solar System.
"The complexity was mind-blowing when we first started looking at the data," said Stuart Bale, lead researcher for the probe's onboard instrument suite at the University of California, Berkeley. "Now, I've gotten used to it. But when I show colleagues for the first time, they're just blown away."
The most startling discovery the teams made was that magnetic fields emanating from our star seemed to unexpectedly flip back and forth, causing local disturbances - what scientists dubbed "switchbacks" - which can even cause them to point back at the Sun at times. The cause of these switchbacks is still a mystery to scientists, but they could eventually allow us to understand how energy flows away from the Sun and throughout the Solar System.
"Waves have been seen in the solar wind from the start of the space age, and we assumed that closer to the Sun the waves would get stronger, but we were not expecting to see them organize into these coherent structured velocity spikes," said Justin Kasper, principal investigator at the University of Michigan said in a statement..
Scientists were also surprised by what they found about the acceleration of the solar wind, the outward stream of protons, electrons and other particles emanating from the Sun. It was known that closer in, the Sun's magnetic field pulls this wind in the same direction as its rotation, so the team expected this effect would weaken further out.
"To our great surprise, as we neared the Sun, we've already detected large rotational flows - 10 to 20 times greater than what standard models of the Sun predict," Kasper said.
"So we are missing something fundamental about the Sun and how the solar wind escapes.This has huge implications. Space weather forecasting will need to account for these flows if we are going to be able to predict whether a coronal mass ejection will strike Earth, or astronauts heading to the Moon or Mars," he added.
The scientists also found that the Sun's radiation vaporizes cosmic dust particles around itself, leaving a 5.6 million km dust-free zone.
The mission also marks the first time that solar wind flows were observed still rotating around the Sun, rather than shooting off at a perpendicular velocity from the star - the kind of straight trajectories we observe from Earth.
"The Sun is the only star we can examine this closely," Nicola Fox, director of the Heliophysics Division at NASA Headquarters, said in the statement.
"Getting data at the source is already revolutionising our understanding of our own star and stars across the universe. Our little spacecraft is soldiering through brutal conditions to send home startling and exciting revelations."
The probe will be attempting to get even closer to the Sun during an encounter on 29 January, 2020.