Universe Today

Astronomers find a nearly metal-free star in our own back yard, which tells us a few interesting things about early star formation.

Duplicating expensive resources is expensive and wasteful, and most people would agree it's unnecessary. However, the planned increase in major satellite constellations is currently causing a massive duplication of resources as individual companies and even countries try to set up their own infrastructure in space. What’s more, there is a relatively limited amount of space in Low Earth Orbit (LEO), where many of these satellites are supposed to go - any more than that and a single collision could cause Kessler Syndrome, where many of the ones already in orbit would be destroyed and we wouldn’t be able to launch any more for a long time. A new paper from researchers at the National University of Defense Technology in China suggests an alternative to these multiple megaconstellations - a single, modular system similar to how cloud computing works on the current internet.

The China National Space Administration on Wednesday released a breathtaking image captured by the Tianwen-2 probe, showing the spacecraft and Earth framed together in a "celestial selfie."

Dark matter, as its name suggests, is really dark, so dark in fact that it doesn’t interact in any way with light or any other part of the electromagnetic spectrum. Even thought it makes up about 80 percent of all matter in the universe and plays a vital role in galaxy formation we still don’t really know what it is. Of all the methods and techniques used to try and unravel this mystery, never would I think I would be writing about the Moon and how it could help us. However, a new piece of research suggests that future missions to the far side of the Moon could help us determine the mass of individual dark matter particles.

Gamma ray bursts are among the most luminous explosions in the universe, briefly outshining entire galaxies in a violent flash of energy. For decades, scientists have debated what powers these incredibly powerful detonations and, to date, the leading candidates have been black holes or highly magnetised neutron stars called magnetars. Distinguishing between the two has proven frustratingly difficult though but a new study has just provided the clearest evidence yet that magnetars can indeed power some of these extreme events, and they did it by detecting something unexpected, the "heartbeat" of a newborn star.

arXiv:2508.00249v1 Announce Type: new Abstract: Any population of artificial radio broadcasts in a galaxy contributes to its integrated radio luminosity. If this radio emission is bright enough, inhabited galaxies themselves form a cosmic population of artificial radio galaxies. We can detect these broadcasts individually or set constraints from their collective emission. Using the formalism in Paper I and II, I set bounds on the artificial radio galaxy population using both of these methodol...

October 2025 may provide a memorable sky scene, as Comet C/2025 A6 Lemmon puts on an encore appearance at dusk. The comet joins Comet R2 SWAN, which slides 0.26 Astronomical Units (AU) past Earth on October 20th. Both are currently fine objects for binoculars or a small telescope, vying for top spot at magnitude +6.

Peering back into the early years of the universe requires scientists to make a lot of assumptions. But sometimes, we get better instruments that then allow them to either confirm or replace those assumptions. That happened recently when it came to our study of J0529, a supermassive black hole that is currently the brightest known quasar in the universe. A new paper from a massive team of researchers used the GRAVITY+ instrument on the European Southern Observatory’s (ESO’s) Very Large Telescope (VLT) Interferometer to map this unique object’s Broad Line Region (BLR), and thereby calculated a new, updated mass that is 10 times smaller than previous estimates.

I remember the first time I pointed my 25cm telescope at the Ring Nebula in Lyra. Even through modest amateur optics, that surreal view of the ring hanging in space was breathtaking, the glowing embers of a dying star. Planetary nebulae like the Ring have long been favourites among amateur astronomers, not just for their visual beauty but because they represent the end of a star's life. However, new research is revealing equally fascinating structures at the opposite end of stellar evolution, the discs where planets are born, and they're not quite what we expected.

This ESA/Webb Picture of the Month shows eight stunning examples of gravitational lensing. Gravitational lensing, which was first predicted by Einstein, occurs because massive objects like galaxies and clusters of galaxies dramatically warp the fabric of spacetime. When a massive foreground object lines up just so with a background galaxy, the light from the background galaxy bends as it navigates the warped spacetime on its way to our telescopes.

Black have no hair, but the material surrounding them does, and the two can interact in unusual ways. As observations from the Event Horizon Telescope show, the magnetic fields surrounding a black hole can change extremely fast.

Interstellar visitor 3I/ATLAS has been constantly changing as it makes its way through our solar system. That’s to be expected, as, for the first time in potentially billions of years, it's getting close to the energy put out by a star. Scientists have been keeping a close watch on those changes, both to ensure there’s nothing unexplainable by our current understanding, but also to compare 3I/ATLAS to both previous interstellar visitors as well as comets in our own solar system. A recent paper from European researchers describes how the changes in a particular material ratio in 3I/ATLAS’ coma fit with our current understanding of cometary geology.

When astronomers pointed their telescopes at a distant galaxy called HerS-3, they discovered something really quite remarkable. The galaxy, located 11.6 billion light years away, appeared not once but five times in their observations, arranged in a nearly perfect cross pattern. This rare phenomenon, known as an Einstein Cross, has revealed exciting evidence for a massive halo of dark matter lurking in the space between us and that distant galaxy.

How will NASA’s upcoming Habitable Worlds Observatory (HWO) mission differentiate Earth-sized exoplanets from other exoplanets, specifically Earth-sized exoplanets within the habitable zone, also called exoEarths? This is what a recent study accepted for publication in The Astronomical Journal hopes to address as an international team of researchers investigated the potential future capabilities of HWO and what shortcomings need to be addressed for it to conduct groundbreaking science, specifically with discovering exoEarths.

What type of lander could touch down on Jupiter’s volcanic moon, Io? This is what a recent paper presented at the AIAA 2025 Regional Student Conference hopes to address as a team of student engineers from Spartan Space Systems at San Jose State University investigated a novel concept for landing a spacecraft in Io, which is the most volcanically active planetary body in the solar system. This study has the potential to help scientists and engineers develop new mission concepts from all levels of academia and industry.

While no evidence of life beyond Earth has been found (yet), it is assumed that life and habitable planets are the norm (per the Copernican Principle). Meanwhile, exoplanet studies have revealed several rocky planets orbiting within the habitable zones of nearby dwarf suns. But as Columbia University Professor David Kipping argues in a recent paper, there is evidence that Earth could be an outlier, while rocky planets orbiting red dwarfs may not be capable of supporting advanced life.

If a new proposal by MIT physicists bears out, the recent detection of a record-setting neutrino could be the first evidence of elusive Hawking radiation.

New observations made with the European Southern Observatory’s Very Large Telescope (ESO’s VLT) identified an enormous a rogue planet with the strongest growth rate ever recorded. These observations reveal that this free-floating planet is eating up gas and dust from its surroundings at a rate of six billion tonnes a second.

By modeling the limb darkening of a star, astronomers can get a better measure of the transit depth of an exoplanet. This will allow us to get better measurements of the size of exoplanets.

The JWST observed the moon-forming disk around a Jupiter-mass planet about 625 light years away. The telescope gave astronomers a detailed view of the circumplanetary disk and found that it's rich in carbon. Its researchers first opportunity to characterize these disks in detail.