Once there was…
…a Sun that, even after the height of Solar Cycle 25, still had a talent for surprising us—and a James Webb Space Telescope (JWST) that kept spotting tiny, puzzling red dots in the early universe.
Every day,
Solar astronomers watched the Sun’s corona for openings in its magnetic “skin,” tracking coronal holes—regions where magnetic field lines open into space and let high-speed solar wind escape.
And every day, cosmologists sifted through JWST’s deep-field images, trying to understand what those compact, intensely red objects were—especially because they appeared when the universe was only about 700 million years old.
Until one day,
On January 16, 2026, the Laboratory of Solar Astronomy at the Institute of Space Research (IKI) of the Russian Academy of Sciences detected something rare: an unusually shaped coronal hole resembling a huge inverted number “1.”
It was enormous—about 1 million km tall—and its strange outline stood out against a backdrop of declining solar activity that began in early 2025, after the October–December 2024 solar peak.
At nearly the same time, another long-running mystery got a dramatic new answer: those JWST “mysterious red dots” weren’t what many had assumed.
Because of that,
The Sun’s inverted “1” wasn’t just a curiosity—it arrived during a phase when solar activity was trending downward, but the space-weather consequences were not necessarily calming down. In fact, the same reports noted that this shift has been accompanied by increased magnetic storms, and that more events like this may appear in 2026, potentially exceeding prior years’ magnetic storm counts.
Adding to that tension, on January 15, the Sun released a strong M-class solar flare. It didn’t meaningfully affect Earth—but it served as a reminder that even in a declining cycle, the Sun can still snap, and further events were anticipated within 1–2 days.
Because of that,
Far beyond our solar neighborhood, the JWST’s red dots finally started to make sense in a way that also sharpened the stakes of what we’re learning about the early cosmos.
According to University of Copenhagen researchers, published in Nature on January 14, 2026, these compact red objects are best explained as newborn black holes—not the giant, fully formed monsters some theories leaned toward, but much smaller young black holes rapidly growing. They are embedded in dense gas cocoons, and as the black holes feed, the surrounding gas heats up and glows red through the shroud, creating the distinct JWST signature.
The payoff is big: this explanation helps show how the universe could produce early supermassive black holes without invoking new exotic events—just fast growth under the right, heavily gas-rich conditions.
Ever since then,
The story of 2026 has started to feel like two versions of the same lesson.
On the Sun, a million-kilometer “inverted 1” coronal hole is a reminder that solar behavior doesn’t have to look “typical” to be impactful—especially in a year expected to bring more frequent magnetic storms even as overall activity declines.
And in the deep universe, those tiny red JWST dots are a reminder that the most important objects aren’t always the biggest—not at first. Sometimes they begin as small, heavily hidden engines, growing quickly inside thick cocoons until they become the giants that shape galaxies.
In other words: whether it’s space weather above Earth or black hole birth in the early cosmos, the universe is still writing its plot twists in plain sight—if we know how to read the light.
Leave a Reply