The Sun is a source of life and energy for our planet, but it has a wild side too. It sends out harmful UV rays and can unleash powerful bursts of solar plasma. NASA is on a mission to learn more about this fiery star with the Parker Solar Probe, launched in 2018. This spacecraft is designed to get as close to the Sun as possible, nicknamed the mission to “touch the Sun.”
Each time it approaches, it sets a new record. Most recently, on December 24, 2024, it came within just 6.1 million kilometers (about 3.8 million miles) of the Sun’s surface. That’s incredibly close! Fortunately, the Parker Solar Probe is built with several protective layers, and it’s the fastest spacecraft ever, zooming at 692,000 km/h (430,000 mph) during its flyby.
One of the key instruments on the probe is WISPR, or the Wide-field Imager for Solar Probe. WISPR uses two robust cameras to capture stunning images of the solar corona and solar wind, allowing us to see these phenomena like never before. Nicky Fox, from NASA, said, “We are witnessing where space weather threats to Earth begin.” This data is crucial for predicting space weather, which can impact astronauts in space and technology back on Earth.
The solar wind is a constant stream of charged particles from the Sun. It’s beautiful, creating stunning auroras, but it can also disrupt power grids and satellites. Understanding this flow is essential as we increase satellite activity in space. Coronal mass ejections (CMEs) are more dangerous; they are bursts of plasma that can cause geomagnetic storms if they hit Earth. While earthbound satellites can be affected only by a few CMEs, they can do significant damage when they do.
The Parker Solar Probe is named after Eugene Parker, an American scientist who first described the solar wind in 1958. His groundbreaking ideas faced skepticism but changed our understanding of the Sun. Previous missions have explored the Sun, but none have come so close or used such advanced technology. The probe has revealed the mystery of “switchbacks,” magnetic field patterns that zigzag near the Sun and cause chaotic solar wind behavior.
When studying the solar wind from Earth, it appears steady. But closer to the Sun, things get wild. The Parker Solar Probe’s findings show that these switchbacks are more common than scientists initially thought and seem to cluster together. This research is crucial for uncovering how the solar wind escapes the Sun’s gravity, which has puzzled scientists for years.
Recent studies indicate that slow solar wind and switchbacks might have more complex relationships than we believed. As Adam Szabo, a scientist from NASA’s Goddard Space Flight Center, notes, “We have a whole lot of new intriguing data,” indicating that the understanding of solar phenomena is deeper than ever.
In just a few years, we’ve gained significant insights into the Sun’s behavior, and the Parker Solar Probe is set to continue this journey. Its next close approach will occur in September 2025, promising even more fascinating data and breathtaking images. Each mission is a step closer to answering our biggest questions about the Sun.
This exploration has implications not just for science but for our daily lives. As we depend on technology influenced by solar activity, understanding the Sun’s nuances becomes more critical with each passing day.
This article was originally published by Universe Today. Read the original article.