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The latest phase of the AMoRE (Advanced Mo-based Rare Process Experiment) project has yielded significant findings in the search for neutrinoless double beta decay, a process that could redefine understanding of fundamental particle physics. Conducted at the Yangyang Underground Laboratory in Korea, the study involved the use of molybdate scintillating crystals at extremely low temperatures to detect this elusive nuclear event. While no clear evidence was observed, the research has set a new upper limit on the decay halflife of molybdenum-100, refining the parameters for future experiments in the field.

New Constraints Established

According to the study published in Physical Review Letters, the AMoRE collaboration utilised multiple kilograms of molybdenum-100, a radioactive isotope, in the form of scintillating crystals. The experiment aimed to detect whether two neutrons in a nucleus could decay into two protons without emitting neutrinos, a phenomenon that would confirm the neutrino and antineutrino as identical particles. Detection of this process is considered crucial for exploring matter-antimatter asymmetry in the universe.

In an interview with Phys.org, Yoomin Oh, corresponding author of the study, explained that the neutrino is one of the elementary particles in the Standard Model. It was ‘invented’ by Wolfgang Pauli about a hundred years ago and discovered a couple of decades later than that. He added that while neutrinos are among the most abundant particles, their properties, including mass, remain largely unknown.

Next Phase: AMoRE-II at Yemilab

AMoRE-I achieved the highest sensitivity ever recorded for detecting neutrinoless double beta decay in molybdenum-100, but no definitive signal was found. This outcome has refined the experimental approach, with the next phase, AMoRE-II, currently being developed at Yemilab, a newly constructed underground research facility in Korea.

The upcoming phase will involve a significantly larger quantity of molybdenum-based crystal detectors and an upgraded low-temperature detection system. The AMoRE collaboration aims to achieve an even lower background environment, enhancing the sensitivity of the experiment. Data collection for AMoRE-II is expected to begin within the next year, with researchers hoping to uncover new insights into the nature of neutrinos.

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Water on Ancient Mars? New Study Challenges the Cold Planet Theory

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Water on Ancient Mars? New Study Challenges the Cold Planet Theory

Despite being a vast and inhospitable planet today, scientists believe Mars, the Red Planet, used to look much like Earth, the Blue Planet. Over the last four years, NASA’s Perseverance rover has wandered across an area of Mars where researchers believe a powerful river once poured into a crater, forming a sizable delta. According to computer models, ancient Mars most likely had frequent snowfall and rain, which shaped the enormous networks of lakes and river basins. In the Journal of Geophysical Research: Planets, a recent study found that the distribution of these land characteristics is more consistent with precipitation models than with only the consequences of melting ice caps.

Investigating Early Martian Climate Through Modeling

The researchers published their findings April 21 in the Journal of Geophysical Research: Planets. According to the research by geologists at the University of Colorado in Boulder, our planetary neighbour, on average 140 million miles away in space, was warm and wet billions of years ago. This challenges a long-held belief that early Mars was mostly cold and icy. However, there’s a vital mystery buried in the story: It’s unclear where Mars’ water could have come from, and most climate models predict the world exhibits surface temperatures that are far too cold to sustain liquid water, raising questions about how those visible geological features could have formed.

“It’s very hard to make any kind of conclusive statement,” Amanda Steckel, a postdoctoral researcher at the California Institute of Technology’s Division of Geological and Planetary Sciences, said in a statement. “But we see these valleys beginning at a large range of elevations. It’s hard to explain that with just ice,” she further added in the official blog posted by University of Colorado. 

Through computer simulations, Steckel and her team explored what Mars might have looked like during the Noachian epoch, when water may have drastically shaped the planet’s surface, some 4 billion years ago. Initially created for Earth, their model was modified to simulate how Mars’ landscape changed near the equator, where expansive channel networks extend from the highlands and drain into ancient lakes, possibly even an ocean. NASA’s Perseverance rover is currently exploring one of these sites, Jezero Crater, where a once-powerful river poured into the basin.

Comparing Climate Models and Implications for Planetary History

The group explored two major simulation models, the ice-melt model and the wet and warm model for how precipitation might have created the valleys on Mars: one in which the planet was warm and humid, and another in which ice briefly melted at the edge of a huge ice cap, signifying a cold, arid climate. With valley roots showing up in radically diverse places, each scenario produced a very different Mars.

Their goal was to determine whether ancient Mars may have had a more Earth-like climate, at least for a while. While more evidence is needed and answers to questions, such as how the planet stayed warm enough for rain or snow, are part of an ongoing investigation. Still, Hynek said the study offers valuable clues, not just about Mars, but about the early history of Earth as well.

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SpaceX launches 28 Starlink satellites, nails booster landing

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SpaceX launches 28 Starlink satellites, nails booster landing

SpaceX added to its growing Starlink mega-constellation with a launch to orbit and booster recovery. A Falcon 9 rocket launched from Cape Canaveral Space Force Station’s Launch Complex-40 at 9:52 p.m. EDT (0152 GMT on April 25), carrying 28 new satellites into low Earth orbit. The spacecraft were stacked vertically inside the rocket’s nose cone, where they sat on the Falcon 9’s nine first-stage Merlin engine stack that blasted them into the sky over Florida’s Space Coast.

According to a SpaceX mission update, the Falcon 9’s first stage, booster B1069, separated from the upper stage about 2.5 minutes after launch. Roughly six minutes later, it executed a precise landing on the autonomous droneship A Shortfall of Gravitas, stationed in the Atlantic Ocean. This marked the 23rd successful flight for B1069 and the 19th time it supported a Starlink mission. The rocket’s second stage continued on its course, deploying the 28 satellites into low Earth orbit one hour into the mission.

These satellites come as new additions to the mission (Starlink 6-74), which is now amplifying an extensive network of no less than 7000+ operational units established in orbit. Starlink’s gates are inching open, as each new flight strengthens global service, and the company aims to beam high-speed internet to nearly every location on Earth, except the polar region. In the days to come, the new arrivals will gradually drift into their assigned orbital slots.

SpaceX is still maintaining a breakneck launch tempo for 2025, with Thursday’s flight being the 47th Falcon 9 mission of the year and the 30th carrying Starlink satellites only. The timeline reflects the firm’s determination to broaden satellite broadband deployment, particularly to rural and poorly served parts of the world. Each new batch enhances service reliability and builds resilience into the constellation’s structure.

The Starlink program continues to reshape global internet accessibility, backed by the Falcon 9’s proven reusability and precision recovery. As they tick off their successful booster landing and payload deployment, SpaceX continues to redefine both space travel logistics and satellite-powered access on Earth.

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Scientists Reportedly Found a Potential Sign of Life on a Distant Planet: What You Need to Know

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Scientists Reportedly Found a Potential Sign of Life on a Distant Planet: What You Need to Know

A team of astronomers have reportedly discovered biological activity outside the solar system. The scientists have revealed that the distant planet, named K2-18 b, comprises more than one molecule in its atmosphere that potentially has been generated by living things. However, this revelation has made a sensation among astronomers across the world, more specifically for those who study biosignatures in exoplanet atmospheres.

 

According to report by Nature.com, K2-18 b is a planet that is smaller than Neptune. It lies at a distance of 38 parsecs above the Earth.

About the Discovery

Dimethyl sulphide (DMS) has been discovered by scientists from the University of Cambridge, UK, in the atmosphere of K2-18b. The DMS molecule is generated by living organisms, which has raised speculations about the potential for life on this distant planet. The scientists used the James Webb Space Telescope (JWST) to implement research. Also, the discovery happened when a molecule was detected in the starlight filtering through the planet’s atmosphere. These chemicals have raised curiosity amongst astronomers as they are generated by living organisms on the planet Earth.

This discovery first came into the light in the year 2023. However, the new revelations have been made as a result of the follow-up on similar findings. This time, the scientists used different wavelengths and a research strategy to support their discovery of molecules on the distant planet. .

Significance of this Discovery

For decades, scientists have been engrossed in studying life beyond Earth. Now that the pieces of evidence are hinting towards the potential existence of DMS or DMDS on K2-18 b. If proven, this will be a historic win for the scientists. Furthermore, this discovery is a step towards understanding planets from a broader perspective. Overall, more than 5,800 planets have been detected throughout the Universe.

Reason Behind Uncertainty by Other Researchers

The scientists are sceptical about this discovery as they doubt whether DMS or DMDS are really present or is K2-18 b is barren. While some of the researchers are not confident about the discovery, the expert team of scientists from the University of Cambridge, UK, is working extensively to provide a proven base to support their findings.

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