Connect with us

Published

on

Scientists say that dinosaurs weren’t doomed when an asteroid hit Earth. Fossil unearthings before the asteroid collision, at the end of the Cretaceous epoch, show that dinosaurs were losing variety and numbers. At first, some scientists thought this alteration showed dinosaurs were headed toward extinction even before the fatal asteroid incident. Nevertheless, this concept has long been argumentative, with other researchers insisting that dinosaur diversity was doing just fine at the time of their loss of life.

Challenging the Long-Held Narrative

According to a report by Live Science, the visible rarity of dinosaurs before their extinction may merely be due to a low fossil record. Emphasizsng four families—that is, the Ankylosauridae, Ceratopsidae, Hadrosauridae, and Tyrannosauridae—the studies of the scientists reveal records of approximately 8,000 fossils from North America dating to the Campanian age (83.6 million to 72.1 million years ago) and Maastrichtian age (72.1 million to 66 million years ago).

Th range of dinosaurs peaked 76 million years ago and started to shrink after the asteroid collision wiped off the nonavian dinosaurs. This drift was more pronounced than in the 6 million years before the mass annihilation, with the number of fossils from all four families reducing in the geological record.

Fossil Records and Statistical Models Paint a New Picture

Vegetation either covered or obscured geological outcrops from the Maastrichtian period in North America. Specifically, rock from this time that might contain dinosaur fossils was not easily accessible to the researchers who were searching for them. The study’s encapsulation might also have worldwide branching due to North America being home to half of the familiar fossils from this age.

A Catastrophic Exception, Not a Gradual End

There is no evidence of environmental conditions or other aspects that would specifically elaborate the reason of this decline, the researchers landed. All of the dinosaur broods were far-flung, as per models come into being developed by the researchers — and consequently at low risk for extinction, barring a catastrophic event such as the asteroid effect.

In the group of 8,000 fossil records evaluated, the team found that ceratopsians—a group that includes horned dinosaurs like Triceratops and its relatives — were the most common; most likely, they inhabited plain regions that were most conducive to preservation during the Maastrichtian era.

Continue Reading

Science

New Dwarf Planet Discovery Challenges Planet Nine Hypothesis

Published

on

By

New Dwarf Planet Discovery Challenges Planet Nine Hypothesis

Discovery of a new potential dwarf planet in the outer reaches of the solar system has posed the greatest challenge yet to the hypothesis that a ninth planet lurks far from the sun. This newly found trans-Neptunian object (TNO) named 2017 OF201 has incredibly elongated orbit (1,600 times that of the Earth’s orbit) that takes it more than 157 billion miles (244 billion kilometers) from the sun. According to researchers it is very rare to discover an object both large (estimated diameter of 435 miles) and with an exotic orbit.

The New Dwarf Planet

According to the pre-print of a paper describing the discovery, with an estimated diameter of 435 miles, 2017 OF201 is large enough to be considered a dwarf planet. It was detected with the help of the data from both DECaLS and the Canada–France–Hawaii Telescope. The closest point of its orbit to the sun (perihelion) is 44.5 astronomical units (AU)—comparable to Pluto—while its farthest point (aphelion) stretches over 1,600 AU. 2017 OF201 is too far away to be seen with current telescopes; it could only be discovered because its last perihelion came in 1930, and that it’s still relatively close.

Scattered Disk, a realm with icy bodies on highly elongated and inclined orbits is situated beyond the Kuiper belt of outer solar system. This discovery hints that many similar objects could exist in the Scattered Disk and beyond. It makes discovery of a trans-Neptunian object (TNO) on a greatly elongated orbit is vital for piecing together the mystery of the outer solar system.

Discarding Planet Nine

The discovery challenges the Planet Nine hypothesis, which suggests a massive, unseen planet is influencing the orbits of distant TNOs. While most extreme TNOs show a clustered pattern that supports this idea, 2017 OF201 does not—its orbit is unusually unclustered.

Although Planet Nine could allow for such deviations, its gravitational pull would render those orbits unstable over millions of years. This mismatch between theory and observation puts Planet Nine’s existence under scrutiny.

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.


Gajaana Now Streaming on JioHotstar: What You Need to Know About A Mythical Tale of Yali, Forests, and Fate

Related Stories

Continue Reading

Science

Venus May Be Geologically Active: New Study Reveals Tectonic Processes Shaping Its Surface

Published

on

By

Venus May Be Geologically Active: New Study Reveals Tectonic Processes Shaping Its Surface

A recent study, published in the Journal Science Advances on May 14, 2025, suggests that Venus, previously considered inactive, may be geologically active. This may be the result of tectonic plate activity. Further research shows that the mysterious circular landforms on Venus. These are called coronae and get their shape due to the rising plumes of hot rocks under the surface. This activity, similar to Earth’s tectonic plates, changes Venus’ behaviour as a dead planet. Further, it triggers the questions about its dynamic past and habitability in future.

Unravelling the Mystery of Coronae

The research published in the Journal Science Advances was led by Geal Cascioli, an assistant research scientist at the University of Maryland and NASA’s Goddard Space Flight Center. The research team analysed NASA’s Magellan mission Data after it orbited Venus in the 1990s to know the coronae, which are circular and vast in geological structure.

In 1983, when Venus coronae was discovered, it puzzled the scientists because of its unique and circular shape. The recent research shows that the structures are formed by the hot material plumes originating from the mantle of Venus. Such plumes despised the crust, making circular ridges and valleys on its surface.

Gravity Data Unlocks Hidden Activity

With NASA’s Magellan data, researchers found plumes under 52 coronae. The observations, like a change in the gravity because of the underground difference in the density, confirm the predictions made by the simulations and give strong evidence that Venus is not inactive geologically.
Subduction Without Plates

Venus has no tectonic plates like Earth; however, the new findings indicate the possibility of subduction at the edges of coronae. Plumes from beneath push outward, causing the surrounding crust to bend and dive under the coronae. These zones could be at the place where Venus experiences strong seismic activity.

Looking Toward Future Missions

The research indicates that Venus is tectonically active at present. This signals that if Venus is active geologically now, it might have a habitable milieu, signalling the new possibilities in terms of future habitat potential and planetary evolution.

Continue Reading

Science

Genetic Study Reveals Maya Civilization’s Collapse Was a Reorganization

Published

on

By

Genetic Study Reveals Maya Civilization’s Collapse Was a Reorganization

A new study reshapes our perspective on the decline of of classic Maya civilization. Though archaeological records long suggested a dramatic population fall around 1,200 years ago, new genetic evidence confirms that the Maya people never truly disappeared. The study, published in Current Biology, analysed genomes from seven ancient individuals from the ancient city of Copán, a major center of the classic Maya world, which lies beneath western Honduras. The results highlight a strong thread of genetic continuity from the Late Archaic period to modern Maya populations, offering new insight into migration, elite integration, and the enduring legacy of the Maya civilization.

Copan’s Cultural Fusion

According to the study, Copán was first settled during the Early Preclassic period (before ~1000 BCE) by small farming communities. Monumental architecture and sophisticated inscriptions indicates that the city had become a major maya center by the early Classic period (300–400 CE). A royal dynasty began in 426/427 CE when K’inich Yax K’uk’ Mo’, an outsider, assumed power—an event supported by both epigraphic and genomic evidence. Genetic data reveal that he, and others in the elite class, likely came from highland Mexican populations, such as those near Chichén Itzá.

Archaeological and historical records long suggested that elite Maya migrants intermarried with local non-Maya populations to establish the kingdom. The new genetic study supports this theory. Researchers found strong genetic continuity from the late archaic era to modern Maya groups, along with about 6% gene flow from highland Mexican populations, indicating regional integration and elite movement.

Collapse and Continuity

The DNA analysis of the study reveals that despite the big decline in the population of Copan around the beginning of 750 CE, the genetic continuity persisted. It indicates that local populations remained even as elite structures crumbled.

Traditional narratives described the Maya collapse as a mysterious vanishing. But this study indicates that Maya people did not vanish suddenly but they reorganised by adapting, migrating, and redefining their identities.

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.


Realme Narzo 80 Lite 5G May Launch in India Soon; RAM, Storage, and Colour Options Tipped

Continue Reading

Trending