The study of the universe as a whole
Galaxies in the infancy of the Universe are the building blocks of more modern galaxies. They began as small "shreds" of material that coalesced over time to form larger ones. That's why astronomers use observatories such as the James Webb Space Telescope (JWST) to study the young Universe. The light from those early objects appears in the infrared part of the spectrum, which JWST is tuned to see.
Little Red Dots are among the most intriguing discoveries made to date by the infrared-sensitive James Webb Space Telescope (JWST). They are distant, small objects that appear red in the JWST observations and they've only been known since 2024. More than 300 of them have been found as part of JWST's infrared surveys of the early Universe.
Astronomers aren't certain where Fast Radio Bursts come from. But they still have utility. They can use them to find the Universe's "missing matter."
It’s hard hunting down the oldest stars in the universe. These behemoths, known as Population (or Pop) III stars, are a missing link in cosmology between the primordial soup that was the early universe and the complex, “metal”-rich cosmos we’re familiar with today. But we’re slowly getting a better idea of where to look for them, and a new paper available in pre-print on arXiv from Alessandra Venditti of the University of Texas at Austin and her co-authors, highlights some of the recent advances and potential new surveying techniques that could eventually help us definitively find these massive, bright, early sparks in the universe.
There are parts of the universe that are extremely hard to see, even for our most advanced telescopes. Gas and dust don’t emit any light, and are only visible by the light that they happen to block from stars and galaxies. Magnetic fields are even harder since regular light typically passes right through them. However, according to a new paper available in pre-print on arXiv, by Manisha Caleb of the University of Sydney and their co-authors, we’re currently commissioning a potentially game-changing new tool that could use a particularly violent astronomical phenomenon to provide new insight into these hard to see places.
Swinburne University of Technology and CSIRO have combined telescope and gravitational wave data in an attempt to unlock the true value of the Universe's expansion. Existing measurements of the Hubble Constant have split cosmologists for more than a decade.
A study led by the University of Bonn presents new data that calls the existence of Dark Matter - a fundamental pillar of the current cosmological model - into question.
Astronomers using W. M. Keck Observatory on Maunakea, Hawaiʻi Island, have discovered the third known galaxy apparently lacking dark matter, part of a strange linear structure that may have formed during a violent collision between galaxies.
Astronomers have discovered a huge reservoir of cold molecular gas, the direct fuel for star formation, in REBELS-25, a massive, star-forming galaxy.The team, led from ​​Leiden University, focused on REBELS-25, seen when the universe was only about 700 million years old, around 5% of its current age. Astronomers use “redshift” to describe this distance, which measures how much the universe’s expansion has stretched a galaxy’s light to redder wavelengths.
Astronomers have detected a flickering quasar called J0439+1634 as it appeared only 850 million years after the Big Bang. That discovery raises fresh questions about black hole formation and activity in the early Universe. The flickering light of this distant cosmic lighthouse showed that black hole at the heart of the quasr has a flat, pancake-shaped accretion disk. That shape is more familiar in modern-day quasars, which leads astronomers to wonder how these objects formed so quickly in the infant cosmos?
We have spent centuries being knocked off our pedestal. Earth isn't the centre of the Solar System, the Sun isn't the centre of the Galaxy, and we are not the point around which everything else turns. Now two philosophers want to take the demotion one step further and apply it to the thing we hold most precious of all, our own conscious minds. If they're right, awareness may be far more widespread, and far stranger, than we ever dared imagine.
Last year, a study sent a quiet tremor through the field of cosmology. A team of researchers claimed that the universe's expansion might be slowing down, not speeding up, suggesting that dark energy, the mysterious force thought to be driving the cosmos apart, could be weakening. If true, it would have shaken the foundations of our understanding of the universe. Now, a new study including two Nobel laureates has looked carefully at the evidence and reached a clear verdict - crisis averted.
After decades of searches, cosmologists are within reach of finding cosmic dawn. A longtime observational cosmologist explains.
Using data from NASA’s James Webb Space Telescope, astronomers led by researchers at the University of California, Riverside have produced the most detailed map of the cosmic web ever made, tracing the network of galaxies all the way back to when the universe was one billion years old.
For nearly thirty years, dark energy has been cosmology's great get out of jail free card, the invisible, mysterious force we invented to explain why the universe is expanding faster than it should be. Now a team of mathematicians says we may never have needed it at all. And the implications are stranger than you might think.
An early galaxy cluster named after an Indian lake is teaching astronomers about influences on galaxy evolution in the infant Universe. Astronomer Ronaldo Laishram of the National Astronomical Observatory of Japan (NAOJ) used the Subaru Telescope’s wide-field camera, Hyper Suprime-Cam (HSC), to conduct a large sky survey to look for early galaxies with active star formation. The result was the discovery of a massive protocluster of galaxies that existed some 12.6 billion years ago, very early in cosmic time. Detailed study of this region could give new insight into how galaxies and their clusters form and evolve.
Researchers at the University of Alabama in Huntsville have found a new way to measure the mass of neighbouring galaxies using pulsars. Using the universe's most precise natural clocks it’s possible to detect tiny gravitational disturbances rippling through the Milky Way. By analysing 54 millisecond pulsars, the team directly measured the gravitational pull of both the Large Magellanic Cloud and the Sagittarius Dwarf Galaxy, including their dark matter. The same technique could eventually map dark matter across the entire Galaxy bringing us closer to understanding what it actually is.
How can astronomers observe ancient galaxies when they're so challenging to resolve? By looking at a whole bunch of them at once in a single spectral line and seeing how it changes over time. That's what a new instrument called the Tomographic Ionized-carbon Mapping Experiment (TIME) does.
The cosmological constant has been a problem in physics since Einstein, but new research may show why it takes the value that it does despite quantum fluctuations that should make its value practically infinite.
An international team of astrophysicists has just released one of the largest cosmological datasets ever assembled. A mouthwatering 2.5 petabytes of simulated universe, freely available to researchers anywhere in the world. Built using a supercomputer and a suite of simulations called FLAMINGO, the data models how matter has evolved since the Big Bang, tracing everything from individual galaxies to the vast cosmic web that stretches across billions of light years.
Universe Today