JWST has given astronomers a much sharper look at Tc 1, a planetary nebula more than 10,000 light-years away in the constellation Ara, already famous because it was the first place where “buckyballs” were confirmed in space. These molecules, also called buckminsterfullerene or C60, are made of 60 carbon atoms arranged in a hollow, soccer-ball-like structure. They were first synthesized in the laboratory in 1985, but their presence in space was not confirmed until 2010, with NASA’s Spitzer Space Telescope. Now, using JWST’s Mid-Infrared Instrument, the Western University team has obtained a far more detailed view of the nebula. The new image combines nine infrared filters, from 5.6 to 25.5 microns, revealing structures that were previously invisible: shells of gas, fine filaments, rays, wisps of cooler material, and a curious curved feature near the center that resembles an upside-down question mark. The colors in the image are not what the human eye would see directly, but a way of translating infrared information into visible form: bluer tones trace hotter gas at shorter mid-infrared wavelengths, while redder tones trace cooler material at longer wavelengths. The most scientifically important part is not only the image itself, but the spectroscopy behind it. JWST’s MIRI can record the chemical fingerprint of the gas and dust across the nebula, allowing researchers to connect the shape of Tc 1 with its temperature, density, chemistry and motion. This is especially useful because planetary nebulae are not just beautiful remnants; they are laboratories for studying how dying Sun-like stars return processed material to space. In Tc 1, the central star has exhausted its nuclear fuel, expelled its outer layers, and left behind a hot core that illuminates the surrounding gas with ultraviolet radiation. One of the first results from the new data is that the buckyballs are not spread randomly through the nebula. Their emission appears concentrated in a thin spherical shell around the central star. In other words, microscopic hollow carbon spheres are distributed in a large hollow-sphere-like structure around the dying star. That geometry is striking, but its origin is still not fully understood. The researchers are now trying to determine why the molecules are located there, why they shine so brightly in Tc 1, and whether they formed through processes similar to those used to make them on Earth or through a different astrophysical pathway. The discovery matters because fullerenes are part of carbon chemistry in space. They may help explain unidentified infrared signals, trace how organic molecules survive or transform in harsh environments, and improve our understanding of how complex carbon-bearing material is produced and redistributed by evolved stars. The new JWST observations are therefore not just a spectacular image of a nebula, but a detailed physical and chemical map of one of the clearest known cosmic environments where these unusual molecules exist. Multiple scientific papers based on the dataset are still in preparation, so this image is likely only the first step in a broader study of how buckyballs form and behave in space. 👉 share.google/Puto8psnk402IUm…