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ALT Close-up, frame-filling view of the oval-shaped, spiral galaxy, NGC 2566, captured by the NASA/ESA/CSA James Webb Space Telescope. This galaxy is located in the constellation Puppis. Its core is a compact, pale spot that glows brightly, filling the disc with bluish light. Faint strands of pale reddish dust swirl out from the core to the far sides of the disc. They each join up with an arm of thick, cloudy, red dust with brighter orange patches that follows the edge of the disc around to the opposite end and a little off the galaxy.

ALT A screenshot of the Galaxy Zoo website, where users classify galaxies based on their appearance. The image displays a distant galaxy with a bright central area and a spiral arm. On the right, users are prompted to determine if the galaxy is smooth and rounded or if it has features like a disk. Image credit: Galaxy Zoo, Zooniverse, and the Cosmic Evolution Early Release Science Survey. Inset galaxy: NASA/STScI/CEERS/TACC/S. Finkelstein/M. Bagley/Z. Levay/A. Pagan.

ALT A bright ball at the center of the image represents a white dwarf star that glows in pale yellow. Surrounding the star is a disk of material. The disk starts a little distance away from the star and is tilted down to the right. The disk glows in orange closest to the star and fades to grays out to its edges. In the lower left is a blotchy cloud of white gas and dust with a trail leading to the edge of the material disk. The image is watermarked “Artist’s concept” and “Credit: NASA’s Goddard Space Flight Center/Scott Wiessinger.”

ALT Earth, seen from the International Space Station, at night and covered with the wispy, bright green swirls of the aurora borealis. Beneath the aurora borealis are bright yellow dots of light from cities. The Space Station’s solar arrays are in shadow and cut through the center of the image. Credit: NASA/Josh Cassada

ALT Hot stars burn brightly in this ultraviolet image of the Andromeda galaxy from NASA's Galaxy Evolution Explorer. Blue-white bands making up the galaxy's striking rings are neighborhoods that harbor hot, young, massive stars. Dark blue-gray lanes of cooler dust show up starkly against these bright rings, tracing regions where stars currently form in dense cloudy cocoons. Eventually, these dusty lanes will blow away when the forming stars ignite nuclear fusion in their core. Meanwhile, the central orange-white ball reveals a congregation of cooler, old stars that formed long ago. This image is watermarked “Credit: NASA/JPL-Caltech”



















