New commissioned piece for @proximareport!
Following the name, this is theorized exoplanet Proxima c, orbiting Proxima Centauri of the Alpha Centauri star system.
Always a pleasure working with these guys, so be sure to check out their work and give them a follow! 🌌 #b3d
The University of Arizona has been named the top public school in the nation for space science by U.S. News and World Report. kvoa.com/news/good-news/univ…
For a limited time, save 67% for your first 3 months of SuperGrok. One subscription for smarter research, image generation, and Grok's most advanced AI models.
Webb has delivered the strongest evidence yet that its discovery of mysterious Little Red Dots (LRD) are “black hole stars.” They appear starting ~600 million years after the big bang, and scientists are still working out exactly what they are. science.nasa.gov/missions/we…
ALT A field of galaxies against the black background of space. In the center is a bright-white elliptical galaxy that is the core of the Abell S1063 galaxy cluster. Around the core are short, curved red lines, which are distant background galaxies magnified and warped by gravitational lensing. A couple of foreground stars appear large and bright with Webb’s signature eight-point diffraction spike pattern. Toward the very bottom, slightly off center toward the right, is a small red dot that is highlighted by an orange square outline. A larger orange square in the top right corner shows the object in more detail. The object, labeled “GLIMPSE-17775” looks like a fuzzy red dot with a yellow core.
Astronomers have found that the supermassive black hole at the center of the Milky Way, known as Sagittarius A* (Sgr A*), is blowing a hot cosmic wind — something scientists have been hunting for over 50 years.
READ MORE >> chandra.harvard.edu/photo/20…
ALT This image centers on a bright, pinpoint white glow marking Sagittarius A* (Sgr A*), the supermassive black hole at the heart of the Milky Way, surrounded by a turbulent, cloud-like environment. Radiating outward from the center is a luminous swirl of blue X-ray emission from NASA's Chandra X-ray Observatory, forming a soft, irregular halo that is brightest near the core and fades into darker shades toward the edges. Interwoven with this blue glow are thick, patchy structures in orange, tracing colder gas mapped by radio observations from ALMA. These orange regions form a partial ring and clumpy arcs around the center, but notably break open to reveal a wide, cone-shaped cavity where little to no orange emission appears. This hollowed-out region is instead filled with the blue X-ray glow, emphasizing the contrast between hot and cold material. The scene feels dynamic and layered, with the interplay of blue and orange just a few light-years from the galaxy’s core.