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New images from the now-decommissioned Atacama Cosmology Telescope (ACT) provide the most precise glimpse yet of the universe just 380,000 years after the Big Bang. These images of the cosmic microwave background (CMB), captured before ACT ceased operations in 2022, reveal how the first structures that would later form stars and galaxies began taking shape.

Breakthrough in Understanding Early Cosmic Structures

According to reports, the images depict the intensity and polarisation of the earliest light with unprecedented clarity, validating the standard model of cosmology. Researchers found that these findings align with previous observations, reinforcing current theories on the universe’s evolution. The data also reveal the movement of ancient gases under gravitational influence, tracing the formation of primordial hydrogen and helium clouds that later collapsed to birth the first stars.

ACT director and Princeton University researcher Suzanne Staggs said in a statement that they are seeing the first steps towards making the earliest stars and galaxies. They are seeing the polarisation of light in high resolution. It is a determining factor distinguishing ACT from Planck and other earlier telescopes, she added.

Imaging the Universe’s First Light

As per reports, before 380,000 years post-Big Bang, the universe was opaque due to a hot plasma of unbound electrons scattering photons. Once the universe cooled to approximately 3,000 Kelvin, electrons bound with protons to form neutral atoms, allowing light to travel freely. This event, known as the ‘last scattering,’ made the universe transparent, leaving behind the CMB—a fossil record of the first light.

ACT, positioned in the Chilean Andes, captured this ancient light, which has been traveling for over 13 billion years. Previous studies from the Planck space telescope provided a detailed image of the CMB, but ACT’s data offers five times the resolution and improved sensitivity.

Insights into Cosmic Evolution and Expansion

The high-resolution images also track how primordial hydrogen and helium gases moved in the universe’s infancy. According to reports, variations in the density and velocity of these gases indicate the presence of regions that eventually formed galaxies. These fluctuations, frozen in the CMB, serve as markers of the universe’s expansion history.

Using ACT data, researchers also estimated the universe’s total mass, which is equivalent to around 2 trillion trillion suns. Sources report that approximately 100 zetta-suns of this mass consist of ordinary matter, while 500 zetta-suns correspond to dark matter, and 1,300 zetta-suns are attributed to dark energy.

Addressing the Hubble Tension

One of the biggest challenges in cosmology is the discrepancy in measuring the universe’s expansion rate, known as the Hubble tension. Measurements from nearby galaxies suggest a Hubble constant of around 73-74 km/s/Mpc, while CMB observations, including those from ACT, yield a lower value of 67-68 km/s/Mpc.

Columbia University researcher Colin Hill, who studied the ACT data, told that they wanted to see if they could find a cosmological model that matched the data and also predicted a faster expansion rate. He further added that they have used the CMB as a detector for new particles or fields in the early universe, exploring previously uncharted terrain.
However, reports confirm that ACT findings align with prior CMB-based measurements, offering no evidence for alternative cosmic models that could explain the discrepancy.

Looking Ahead

ACT concluded its observations in 2022, and astronomers have now shifted focus to the Simons Observatory in Chile, which promises even more advanced studies of the universe’s early light. The new ACT data has been made publicly available through NASA’s LAMBDA archive, with related research published on Princeton’s Atacama Cosmology Telescope website.

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

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NASA’s Hubble and Webb Discover Bursting Star Formation in Small Magellanic Cloud

Scientists from NASA observed the bursting expansion of gas, stars, and dust from the glittering territory of the dual star clusters using Hubble and Webb space telescopes. NGC 460 and NGC 456 stay in the Small Magellanic Cloud, which are open clusters, with dwarf galaxies and orbit the Milky Way. These clusters are part of the extensive star complex clusters and nebulae that are most likely to be linked to each other. Stars are born upon the collapse of clouds.

Hubble and Webb Reveal Explosive Star Births in Small Magellanic Cloud

As per a report from NASA, the open clusters are from anywhere from a few dozen to many young stars, which are loosely bound by gravity. The images captured by Hubble capture the glowing and ionised gas, which comes from stellar radiation and blows bubbles in the form of gas and dust, which is blue in colour. The infrared of Webb shows the clumps and delicate filament-like structures and dust, which is red in colour.

NGC 460 and NGC 456: A Window into Early Universe Star Formation

Hubble shows the images of dust in the form of a silhouette against the blocking light; however, in the images of Webb, the dust is warmed by starlight and glows with infrared waves. The blend of gas and dust between the stars of the universe is called the interstellar medium. The region holding these clusters is known as the N83-84-85 complex and is home to multiple, rare O-type stars. These are hot and extremely massive stars that burn hydrogen like the Sun.

Such a state mimics the condition in the early universe; therefore, the Small Magellanic Cloud gives a nearby lab to find out the theories regarding star formation and the interstellar medium of the cosmos’s early stage.

With these observations, the researchers tend to study the gas flow from convergence to divergence, which helps in refining the difference between the Small Magellanic Cloud and its dwarf galaxy, and the Large Magellanic Cloud. Further, it helps in knowing the interstellar medium and gravitational interactions between the galaxies.

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

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New Interstellar Object 3I/ATLAS Could Reveal Secrets of Distant Worlds

The entry of a third known object into our solar system has been confirmed on July 1, 2025 by the astronomers. This object is named 3I/ATLAS, where 3I stands for “Third Interstellar”, having a highly hyperbolic (eccentricity ≈ 6.2) orbit, confirming it is not bound to the Sun but is a true interstellar visitor. Only two such visitors, 1I/ʻOumuamua (2017) and 2I/Borisov (2019), had been seen before. Notably, 3I/ATLAS appears to be the largest and brightest interstellar wanderer yet discovered.

Comparison with previous interstellars

According to NASA, astronomers from the ATLAS survey first spotted the object on July 1, 2025, using a telescope in Chile. It immediately drew attention for its unusual motion. Shortly after discovery, observers saw a faint coma and tail, leading to its classification as comet C/2025 N1 (ATLAS).

This comet-like appearance is shared with 2I/Borisov, the second interstellar visitor. Global observatories now track 3I/ATLAS. It poses no threat but offers a rare opportunity to study alien material. Since 1I/ʻOumuamua was observed only as it was leaving the solar system, it was difficult for astronomers to get enough data on it to confirm its exact nature — hence the crazy theories about it being an alien spaceship — though it’s almost certainly an asteroid or a comet.

Size and Significance

3I/ATLAS is much larger and brighter than earlier interstellar visitors. It is about 15 kilometers (km) [9 miles] in diameter, with huge uncertainty, compared to 100m for 1I/’Oumuamua and less than 1km for 2I/Borisov. This brightness and size makes it a a better target for study. Astronomers are planning to analyze its light for chemical signatures from its home system to get clues about the formation of distant planetary systems.

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Scientists Recreate Cosmic Ray Physics Using Cold Atom in New Laboratory Study

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Scientists Recreate Cosmic Ray Physics Using Cold Atom in New Laboratory Study

For the first time, researchers have managed to simulate a fundamental process of cosmic particle acceleration in a laboratory: the first series of discoveries that will transform our understanding of cosmic rays. Now, scientists from the Universities of Birmingham and Chicago have created a tiny, 100-micrometre Fermi accelerator, in which mobile optical potential barriers collide with trapped atoms, in a partial replica of how cosmic particles pick up energy in space. The technique not only replicates cosmic ray behaviour but also sets a new benchmark in quantum acceleration technology.

Lab-Built Fermi Accelerator Using Cold Atoms Validates Cosmic Ray Theory and Advances Quantum Tech

As per findings published in Physical Review Letters, this fully controllable setup demonstrated particle acceleration through the Fermi mechanism first proposed by physicist Enrico Fermi in 1949. Long theorised to underlie cosmic ray generation, the process had never been reliably replicated in a lab. By combining energy gains with particle losses, researchers created energy spectra similar to those observed in space, offering the first direct validation of Bell’s result, a cornerstone of cosmic ray physics.

In Fermi acceleration, ultracold atoms are accelerated to more than 0.5 metres per second using laser-controlled barriers. Dr Amita Deb, a coauthor and researcher at the University of Birmingham, mentioned, ‘Our chimney is more powerful than conventional quantum nano-measurements, which are the best acceleration tools in the world so far, and while its simplicity and small size can be compelling, its lack of a theoretical speed limit is the most attractive feature.’ The ultracold atomic jets could be readily controlled with high precision in the subsequent experiments.

This progress means that, for the first time, complicated astrophysical events like shocks and turbulence can be studied in a laboratory, lead author Dr Vera Guarrera stated. This opens new avenues for high-energy astrophysics and also for applications in quantum wavepacket control and quantum chemistry.

Researchers plan to find out how different behaviour affects energy cutoffs and acceleration rates. A compact Fermi accelerator of this type could be a cornerstone for studies of fundamental physics and also connect to emerging technologies such as atomtronics.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


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