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For the first time in human history, a spacecraft has entered the Sun’s outer atmosphere. The Parker Solar Probe crossed the Alfvén critical surface and began directly sampling the solar corona, a region where temperatures reach millions of degrees and magnetic forces dominate the motion of plasma. What it found is reshaping our understanding of how the solar wind forms, why the corona is so much hotter than the Sun’s surface, and how solar storms are born. In this long-form deep dive, we explore how the probe survived temperatures near 2,500 degrees Fahrenheit, how it became the fastest human-made object ever built, and what its instruments discovered inside the Sun’s magnetic environment. From switchbacks in the solar wind to turbulence that may explain coronal heating, this mission is changing solar physics in real time. The Parker Solar Probe is still active today, still looping around the Sun, and still sending back data from deeper inside the corona than any spacecraft before it. This is the story of how we touched the Sun, and what we are learning from within.