
u/The_Rise_Daily

The Squid Galaxy - A Beacon of Light in Swirls of Dust
Webb & Hubble find massive star clusters emerge faster
esa.intMost galaxies JWST finds this far back are blazing blue, young, hot, and dust-free. That's what the models predicted.
However, EGS-z11-R0 breaks that framework completely.
Here's the TLDR:
- Dust and carbon do not appear overnight. They require multiple generations of stars to live, explode, and seed the surrounding medium with heavy elements. This galaxy already had both just 400 million years after the Big Bang, making it an "anomaly among anomalies" at one of the earliest points in cosmic history.
- Red monsters shouldn't be confused with JWST's "little red dots." The closer comparison is the "blue monster" galaxies JWST has also found, which share the extreme mass but lack the dust buildup. Lead author Giulia Rodighiero (University of Padua in Italy) believes red and blue monsters may be ancestors and descendants in the same evolutionary story.
- "It's astonishing to think about how short these timescales are," says Yale astrophysicist Pieter van Dokkum, who was not involved in the study. "Sharks and turtles have been around for about that long." Given how long stars take to produce dust and carbon, EGS-z11-R0 suggests we could spot galaxies as early as 200 million years after the Big Bang.
Note: preprint study, not yet peer-reviewed.
Full paper: https://arxiv.org/abs/2603.15841
P.S. if you liked this, you'll love RISE!
Hey fellow space nerds, I've been enchanted by the "Little Red Dot" mystery for a while now and to me this new NASA/Chandra result is a big deal!
And because this sub has been tracking this topic for a while now, I went through the new NASA/Chandra release and traced it back through some recent research.
So here's where we stand:
- Using the first datasets released by JWST in 2022, an international team of scientists began spotting mysterious tiny red objects in the early universe, informally dubbed "universe breakers." They initially appeared to be impossibly mature galaxies, far older than models predicted for that era.
- By September 2025, a published a paper in Astronomy and Astrophysics by Penn State University proposed that these dots may not be galaxies at all, but an entirely new class of object called a "black hole star," giant spheres of hot gas so dense they look like the atmospheres of typical stars, but powered by a supermassive black hole at their center rapidly pulling in matter and converting it to light.
- That left one big open question that if LRDs are supermassive black holes embedded in gas, they should produce X-rays like other known accreting black holes. However, none had ever been detected doing so.
- This week that changed! Chandra detected object 3DHST-AEGIS-12014, located about 11.8 billion light-years away, with all the hallmarks of an LRD but uniquely glowing in X-ray light. Researchers propose it represents a transition phase that as the black hole consumes its surrounding gas, patchy holes open in the cloud and X-rays finally escape. How cool!
Lead author Raphael Hviding of the Max Planck Institute for Astronomy said: "Astronomers have been trying to figure out what little red dots are for several years. This single X-ray object may be -- to use a phrase -- what lets us connect all of the dots."
Future observations are planned to confirm their true nature. As co-author Andy Goulding of Princeton put it: "The X-ray dot had been sitting in our Chandra survey data for over ten years, but we had no idea how remarkable it was before Webb came along to observe the field."
JWST remains to me the coolest piece of space tech to date. Hope you enjoyed!
Article Source | NASA Press Release
Previous Research | Penn State Press Release
More from me :) | RISE
A study published today in the Astrophysical Journal may change how we think about stellar collapse.
3D simulations from Kyoto University show that a star's final spin before death isn't determined by its mass or age, but by the geometry of its internal magnetic field. That geometry can even spin the core up instead of down which was a finding that surprised the team. "We were surprised to discover that some configurations of the magnetic fields actually spin the core up," says co-author Lucy McNeill, "suggesting that the final spin rate will be unique to the star's properties." Slow rotation might even be forbidden in some classes of massive stars."
This isn't the first time magnetism has rewritten the rulebook recently. In March, Nagoya University used Japan's Fugaku supercomputer to overturn a 45-year-old theory about stellar rotation, one that turned out to be incomplete because older simulations weren't powerful enough to model magnetic fields accurately.
The pattern is slowly becoming hard to ignore. Could final spin determine what a collapsing star becomes? If that outcome is unique to each star's magnetic geometry, we may have been misreading the graveyard of stars for decades.
Article source: Kyoto University | Paper: The Astrophysical Journal, Shimada et al. (2026)
Press Release: Kyoto University
Source reporting: RISE | Space News
5 months from now, NASA's Roman telescope begins hunting for exoplanets. A study released today suggests it may find far more than anyone expected.
New simulations from the University of Lancashire show that once the protoplanetary disc extends beyond the "forbidden" inner zone of a binary system, it fragments more efficiently than around single stars. As lead supervisor Dr. Stamatellos puts it: "Once you get past the danger zone, planets can form quickly and in large numbers."
The Roman Space Telescope was built to survey over 100,000 exoplanets. Per a 2025 ESO review, at least half of all solar-like stars have a stellar companion. This research suggests Roman's final count could be far higher than anyone projected.
If binary stars are nurseries rather than graveyards, the universe is far more crowded than we imagined.