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ALT SETI Live record button logo. Text: More Radio Bursts? with Lauren Sgro and Mawson Sammos, Thursday, 22 October 2026, 10:00 am PDT / 1:00 pm EDT. Background: A galaxy cluster in multi-wavelengths: X-rays in blue, visible light in green, and infrared light in red, with a sound wave graphic going from the center to the upper right corner. Inset: Photos of Lauren Sgro and Mawson Sammons.

ALT Top - Live colouration of adult paratypes of ๐๐๐๐๐๐๐ก๐๐๐ข๐ ๐๐ข๐๐๐๐ข๐๐ข๐ , from Guaporรฉ River, tributary of Madeira River basin, Rondรดnia, Brazil. Bottom - Portion of a larger lateritic block (approx. 45 kg, 1.5 m in length, 0.6 m in width) containing numerous interconnected tunnels, from which specimens of ๐๐๐๐๐๐๐ก๐๐๐ข๐ ๐๐ข๐๐๐๐ข๐๐ข๐ were collected. The block was taken from the riverbed of the โGuaporรฉ River (type locality),โ Rondรดnia, Brazil.

ALT On the left is a large image of a star cluster and nebula, which takes up two-thirds of the view. Wispy filaments of pink-purple fill the middle, curving left and right on either side of the center. The filaments on the right side form a dramatic loop that seems to extend toward the viewer. At lower left, additional filaments are yellowish. Two prominent, bright stars near the center show Webbโs eight-point diffraction spikes. Dozens of fainter stars are scattered across the image. In the bottom third, three small areas are circled and labeled 1, 2, and 3. On the right is a column of three smaller boxes labeled 1, 2, and 3, showing enlarged sections of the full image that align to the numbers in the larger image at left. A pair of faint stars are shown in box 1, while boxes 2 and 3 each highlight a single faint star. The background in the top two images looks light brown, while the background in the third is dark gray.

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ALT An edge-on spiral galaxy. Its rusty-brown dust lanes bisect the galaxy lengthwise. Bright-blue points dot the galaxy and seem to be more dense on its left side. A bright foreground star shines just to the left of the galaxy's center. The background is black and dotted with distant galaxies and a smattering of foreground stars, which are easily identified by their diffraction spikes.



























