Press Release
Parker Solar Probe Sheds New Light on the Sun
The Parker Solar Probe mission has returned unprecedented data from near the Sun, culminating in new discoveries published on Dec. 4, 2019, in the journal Nature. Among the findings are new understandings of how the Sun’s constant outflow of material, the solar wind, behaves. Seen near Earth — where it can interact with our planet’s natural magnetic field and cause space weather effects that interfere with technology — the solar wind appears to be a relatively uniform flow of plasma. But Parker Solar Probe’s observations reveal a complicated, active system not seen from Earth. Johns Hopkins APL designed, built and manages the mission for NASA.
Credit: NASA Goddard Space Flight Center
Wed, 12/04/2019 - 16:24
Sarah Frazier/NASA Goddard Space Flight Center
In August 2018, NASA’s Parker Solar Probe launched to space, soon becoming the closest-ever spacecraft to the Sun. With cutting-edge scientific instruments to measure the environment around the spacecraft, Parker Solar Probe — designed, built and managed for NASA by the Johns Hopkins Applied Physics Laboratory — has completed three of 24 planned passes through never-before-explored parts of the Sun’s atmosphere, the corona. On Dec. 4, 2019, four new papers in the journal Nature describe what scientists have learned from this unprecedented exploration of our star — and what they look forward to learning next.
These findings reveal new information about the behavior of the material and particles that speed away from the Sun, bringing scientists closer to answering fundamental questions about the physics of our star. In the quest to protect astronauts and technology in space, the information Parker has uncovered about how the Sun constantly ejects material and energy will help scientists rewrite the models we use to understand and predict the space weather around our planet and understand the process by which stars are created and evolve.
“This first data from Parker reveals our star, the Sun, in new and surprising ways,” said Thomas Zurbuchen, associate administrator for science at NASA Headquarters in Washington. “Observing the Sun from up close rather than from a much greater distance is giving us an unprecedented view into important solar phenomena and how they affect us on Earth, and gives us new insights relevant to the understanding of active stars across galaxies. It’s just the beginning of an incredibly exciting time for heliophysics with Parker in the vanguard of new discoveries.”
“Parker Solar Probe has performed exceptionally well over the past year, and we are thrilled the spacecraft has been able to carry these instruments into previously unexplored regions around the Sun to collect so much new insight into how our star works,” said Jason Kalirai, civil space mission area executive at Johns Hopkins APL.
Though it may seem placid to us here on Earth, the Sun is anything but quiet. Our star is magnetically active, unleashing powerful bursts of light, deluges of particles moving near the speed of light and billion-ton clouds of magnetized material. All of this activity affects our planet, injecting damaging particles into the space where our satellites and astronauts fly, disrupting communications and navigation signals, and even — when intense — triggering power outages. It’s been happening for the Sun’s entire 5-billion-year lifetime, and will continue to shape the destinies of Earth and the other planets in our solar system into the future.
“The Sun has fascinated humanity for our entire existence,” said Nour E. Raouafi, project scientist for Parker Solar Probe at APL. “We’ve learned a great deal about our star in the past several decades, but we needed a mission like Parker Solar Probe to go into the Sun’s atmosphere. It’s only there that we can really learn the details of these complex solar processes. And what we’ve learned in just these three solar orbits alone has changed a lot of what we know about the Sun.”
Making this mission possible are key technologies developed by APL. The revolutionary 4.5-inch-thick (11.43 cm) carbon-composite thermal protection system — or heat shield — keeps the spacecraft and most of its instruments at a comfortable 85 degrees Fahrenheit, even as the spacecraft plunges deeper into the Sun’s fiery corona. The solar-powered spacecraft houses active water-cooled solar arrays (a first in space) that retract and extend as Parker Solar Probe swings toward or away from the Sun, making sure the panels stay at appropriate temperatures while providing the necessary power to operate the spacecraft and instruments autonomously. At its closest passes the spacecraft must survive solar intensity of about 500 times what we experience here at Earth on the hottest day of the year.
What happens on the Sun is critical to understanding how it shapes the space around us. Most of the material that escapes the Sun is part of the solar wind, a continual outflow of solar material that bathes the entire solar system. This ionized gas, called plasma, carries with it the Sun’s magnetic field, stretching it out through the solar system in a giant bubble — the heliosphere — that spans more than 10 billion miles.
“The information that the Parker team has gathered during the first year of the mission is unprecedented,” said APL's Rob Decker, Parker Solar Probe deputy project scientist. “We are starting to get some of the missing pieces of the coronal puzzle, like glimpses of how the solar wind behaves, but there is still more to explore and observe in the next several years as Parker Solar Probe gets closer and closer to the Sun. Parker Solar Probe is opening our eyes to a new reality of the corona and solar wind.”
The Dynamic Solar Wind
Observed near Earth, the solar wind is a relatively uniform flow of plasma, with occasional turbulent tumbles. But by that point it’s traveled over ninety million miles — and the signatures of the Sun’s exact mechanisms for heating and accelerating the solar wind are wiped out. Closer to the solar wind’s source, Parker Solar Probe saw a much different picture: a complicated, active system.
Like the Sun itself, the solar wind is made up of plasma, where negatively charged electrons have separated from positively charged ions, creating a sea of free-floating particles with individual electric charge. These free-floating particles mean plasma carries electric and magnetic fields, and changes in the plasma often make marks on those fields. The FIELDS instruments surveyed the state of the solar wind by measuring and carefully analyzing how the electric and magnetic fields around the spacecraft changed over time, along with measuring waves in the nearby plasma.
These measurements showed quick reversals in the magnetic field and sudden, faster-moving jets of material — all characteristics that make the solar wind more turbulent. These details are key to understanding how the wind disperses energy as it flows away from the Sun and throughout the solar system.
One type of event in particular drew the eye of the science teams: flips in the direction of the magnetic field, which flows out from the Sun, embedded in the solar wind. These reversals — dubbed “switchbacks” — last anywhere from a few seconds to several minutes as they flow over Parker Solar Probe. During a switchback, the magnetic field whips back on itself until it is pointed almost directly back at the Sun. Together, FIELDS and SWEAP, the solar wind instrument suite led by the University of Michigan and managed by the Smithsonian Astrophysical Observatory, measured clusters of switchbacks throughout Parker Solar Probe’s first two flybys.
Parker Solar Probe observed switchbacks — traveling disturbances in the solar wind that caused the magnetic field to bend back on itself — an as-yet-unexplained phenomenon that might help scientists uncover more information about how the solar wind is accelerated from the Sun.
Credit: NASA Goddard Space Flight Center/Conceptual Image Lab/Adriana Manrique Gutierrez
“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 for SWEAP — short for Solar Wind Electrons Alphas and Protons — at the University of Michigan in Ann Arbor. “We are detecting remnants of structures from the Sun being hurled into space and violently changing the organization of the flows and magnetic field. This will dramatically change our theories for how the corona and solar wind are being heated.”
The exact source of the switchbacks isn’t yet understood, but Parker Solar Probe’s measurements have allowed scientists to narrow down the possibilities.
Among the many particles that perpetually stream from the Sun are a constant beam of fast-moving electrons, which ride along the Sun’s magnetic field lines out into the solar system. These electrons always flow strictly along the shape of the field lines moving out from the Sun, regardless of whether the north pole of the magnetic field in that particular region is pointing toward or away from the Sun. But Parker Solar Probe measured this flow of electrons going in the opposite direction, flipping back toward the Sun — showing that the magnetic field itself must be bending back toward the Sun, rather than Parker Solar Probe merely encountering a different magnetic field line from the Sun that points in the opposite direction. This suggests that the switchbacks are kinks in the magnetic field — localized disturbances traveling away from the Sun, rather than a change in the magnetic field as it emerges from the Sun.
Parker Solar Probe’s observations of the switchbacks suggest that these events will grow even more common as the spacecraft gets closer to the Sun. The mission’s next solar encounter on Jan. 29, 2020, will carry the spacecraft nearer to the Sun than ever before, and may shed new light on this process. Not only does such information help change our understanding of what causes the solar wind and space weather around us, it also helps us understand a fundamental process of how stars work and how they release energy into their environment.
The Rotating Solar Wind
Some of Parker Solar Probe’s measurements are bringing scientists closer to answers to decades-old questions. One such question is about how, exactly, the solar wind flows out from the Sun.
Near Earth, we see the solar wind flowing almost radially — meaning it’s streaming directly from the Sun, straight out in all directions. But the Sun rotates as it releases the solar wind; before it breaks free, the solar wind was spinning along with it. This is a bit like children riding on a playground park carousel — the atmosphere rotates with the Sun much like the outer part of the carousel rotates, but the farther you go from the center, the faster you are moving in space. A child on the edge might jump off and would, at that point, move in a straight line outward, rather than continue rotating. In a similar way, at some point between the Sun and Earth, the solar wind transitions from rotating along with the Sun to flowing directly outward, or radially, like we see from Earth.
Exactly where the solar wind transitions from a rotational flow to a perfectly radial flow has implications for how the Sun sheds energy. Finding that point may help us better understand the life cycle of other stars or the formation of protoplanetary disks, the dense disks of gas and dust around young stars that eventually coalesce into planets.
Now, for the first time — rather than just seeing that straight flow that we see near Earth — Parker Solar Probe was able to observe the solar wind while it was still rotating. It’s as if Parker Solar Probe got a view of the whirling carousel directly for the first time, not just the children jumping off it. Parker Solar Probe’s solar wind instrument detected rotation starting more than 20 million miles from the Sun, and as Parker approached its perihelion point, the speed of the rotation increased. The strength of the circulation was stronger than many scientists had predicted, but it also transitioned more quickly than predicted to an outward flow.
“The large rotational flow of the solar wind seen during the first encounters has been a real surprise,” said Kasper. “While we hoped to eventually see rotational motion closer to the Sun, the high speeds we are seeing in these first encounters is nearly ten times larger than predicted by the standard models.”
Dust Near the Sun
Another question approaching an answer is the elusive dust-free zone. Our solar system is awash in dust — the cosmic crumbs of collisions that formed planets, asteroids, comets and other celestial bodies billions of years ago. Scientists have long suspected that, close to the Sun, this dust would be heated to high temperatures by powerful sunlight, turning it into a gas and creating a dust-free region around the Sun. But no one had ever observed it.
For the first time, Parker Solar Probe’s imagers saw the cosmic dust begin to thin out. Because WISPR — Parker Solar Probe’s imaging instrument, led by the Naval Research Lab — looks out the side of the spacecraft, it can see wide swaths of the corona and solar wind, including regions closer to the Sun. These images show dust starting to thin a little over 7 million miles from the Sun, and this decrease in dust continues steadily to the current limits of WISPR’s measurements at a little over 4 million miles from the Sun.
Parker Solar Probe saw cosmic dust — scattered throughout our solar system — begin to thin out close to the Sun, supporting the idea of a long-theorized dust-free zone near the Sun.
Credit: NASA Goddard Space Flight Center/Scott Wiessinger
“This dust-free zone was predicted decades ago, but has never been seen before,” said Russ Howard, principal investigator for the WISPR suite — short for Wide-field Imager for Solar Probe — at the Naval Research Laboratory in Washington, D.C. “We are now seeing what’s happening to the dust near the Sun.”
At the rate of thinning, scientists expect to see a truly dust-free zone starting a little more than 2–3 million miles from the Sun — meaning Parker Solar Probe could observe the dust-free zone as early as 2020, when its sixth flyby of the Sun will carry it closer to our star than ever before.
Putting Space Weather Under a Microscope
Parker Solar Probe’s measurements have given us a new perspective on two types of space weather events: energetic particle storms and coronal mass ejections.
Charged particles — both electrons and ions — are accelerated by explosive solar activity, creating storms of energetic particles. Events on the Sun, like flares and coronal mass ejections, can send these particles rocketing out into the solar system at nearly the speed of light, meaning they reach Earth in under half an hour and can impact other worlds on similarly short time scales. These particles carry a lot of energy, so they can damage spacecraft electronics and even endanger astronauts, especially those in deep space, outside the protection of Earth’s magnetic field — and the short warning time for such particle storms makes them difficult to avoid.
Parker Solar Probe has made new observations of energetic particles — like those seen here impacting a detector on ESA and NASA’s Solar and Heliospheric Observatory — which will help scientists better understand how these events are accelerated.
Credit: ESA/NASA/SOHO
Understanding exactly how these particles are accelerated to such high speeds is crucial. But even though they zip to Earth in as little as a few minutes, that’s still enough time for the particles to lose the signatures of the processes that accelerated them in the first place. By whipping around the Sun at just a few million miles away, Parker Solar Probe can measure these particles just after they’ve left the Sun, shedding new light on how they are released.
Already, Parker Solar Probe’s ISʘIS instruments, led by Princeton University, have measured several never-before-seen energetic particle events — events so small that all trace of them is lost before they reach Earth or any of our near-Earth satellites. These two instruments (APL built one of them, called EPI-Lo) have also measured a rare type of particle burst with a particularly high number of heavier elements — suggesting that both types of events may be more common than scientists previously thought.
“It’s amazing — even at solar minimum conditions, the Sun produces many more tiny energetic particle events than we ever thought,” said David McComas, principal investigator for the Integrated Science Investigation of the Sun suite, or ISʘIS, at Princeton University in New Jersey. “These measurements will help us unravel the sources, acceleration and transport of solar energetic particles and ultimately better protect satellites and astronauts in the future.”
Data from the WISPR instruments also provided unprecedented detail on structures in the corona and solar wind — including coronal mass ejections, billion-ton clouds of solar material that the Sun sends hurtling out into the solar system. CMEs can trigger a range of effects on Earth and other worlds, from sparking auroras to inducing electric currents that can damage power grids and pipelines. WISPR’s unique perspective, looking alongside such events as they travel away from the Sun, has already shed new light on the range of events our star can unleash.