Discover Early Paleocene Fish Fossils: Bridging the 10 Million-Year Gap Post-Dinosaur Extinction

Approximately 66 million years ago, the end-Cretaceous extinction event drastically altered Earth’s biodiversity. However, the implications for marine fish remain a topic of debate due to gaps in the fossil record. A recent study conducted by paleontologists reveals a collection of marine fish fossils from the 62.2 million-year-old Quraya 3 site in Egypt’s eastern desert, shedding light on this transition. These discoveries include the earliest known fossil skeletons of horse mackerel, moonfish, and pipefish, which are relatives of seahorses.



Marine fish fossils from the early Paleocene site of Quraya 3 in Egypt’s Eastern Desert. Image credit: Ian Beilatry.

“The fossil record is limited, and there exists a substantial 10 million-year gap,” stated study lead author Sanaa El-Sayed, a doctoral candidate at the University of Michigan.

“While we know asteroids impacted marine environments, it remains unclear how these events shaped the ocean’s inhabitants, particularly modern fish species.”

“This site is remarkable in addressing when, where, and which species existed in modern oceans just a few million years post-dinosaurs.”

At the Quraya 3 site, El-Sayed and her colleagues identified fossils from 21 distinct fish species spanning nine orders.

“Most of these fish are percomorphs, a dominant group in today’s oceans, yet relatively rare during the dinosaur era,” noted co-author Professor Matt Friedman, director and curator of the University of Michigan Museum of Paleontology.

“This discovery reinforces the theory that a biological crisis tied to the end-Cretaceous mass extinction led to the loss of certain fish types, allowing modern-looking fish groups to flourish soon after.”

The “Patterson Gap,” named after the paleontologist who studied it, identifies the fossil-poor section of the record before and following the mass extinction at the end of the Cretaceous.

This gap obscures our understanding of how fish species were affected by extinction events.

“This early Cenozoic gap raises two critical questions,” added Professor Friedman.

“First, did the fish we traditionally associate with extinction at the end of the Cretaceous truly not continue into the Paleogene period? Or were they simply overlooked due to poor records?”

“Second, when did recognizable modern groups actually emerge?”

“This gap represents an extensive timeframe in which the details remain unclear, frustratingly coinciding with one of Earth’s most intriguing historical periods.”

“Our remarkable findings provide insights into this critical epoch.”

“We found numerous preserved skeletons; however, the species long believed extinct were absent.”

“Our research indicates that their absence likely reflects genuine extinction occurring around the end-Cretaceous event, rather than simply a record deficiency.”

“Moreover, this site offers concrete evidence that many modern fish groups were established quite early in the evolutionary timeline.”

The research team also contemplated the broader implications of their findings in the context of the fossil record following the end-Cretaceous mass extinction.

Upon comparing their findings with data from additional fossil deposits, they noted that most percomorphs discovered shortly after extinction events predominantly thrived in tropical regions.

Conversely, fewer percomorphs appeared at high latitudes, becoming more common only significantly later.

“An intriguing geographic pattern emerges regarding how contemporary fauna evolved,” Friedman said.

“It appears they predominantly developed in tropical regions, later dispersing to higher latitudes as climatic conditions changed.”

“As we enhance our fossil record, these conclusions will be put to further rigorous testing.”

These significant findings are published in this week’s edition of Scientific Progress.

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Sanaa El-Sayed et al. 2026. The Rise of Modern Marine Fishes Caught in Lagerstätte during the Early Paleocene. Scientific Progress 12(23); doi: 10.1126/sciadv.aec8978

Source: www.sci.news

Ancient Moon Metstone, 23.5 Billion Years Old, Bridges 100 Million-Year Gap in Lunar History

The examination of North West Africa (NWA) 16286 reveals a lunar metstone with a distinctive chemical profile, offering new perspectives on the evolution of the moon’s interior and emphasizing the enduring nature of its volcanic activity.



Backscattered electron images of NWA 16286 samples. Image credit: Joshu Asu Nape/University of Manchester.

Discovered in Africa in 2023, NWA 16286 is one of only 31 moon basalts officially identified on Earth.

The distinct composition of the 311-gram metstone, featuring melted glassy pockets and veins, indicates it was likely impacted by an asteroid or metstone on the lunar surface before being ejected and eventually landing on Earth.

A recent study by researchers at the University of Manchester supports the theory that the moon has maintained internal heat production processes responsible for lunar volcanic activity across various stages.

Lead isotopic analyses suggest that these rock formations are the youngest basalt lunar metstones identified on Earth, dating back approximately 2.35 billion years, a time when lunar samples are scarce.

The sample’s unique geochemical profile distinguishes it from those brought back by previous lunar missions, indicating that its chemical characteristics likely result from lava flows that solidified after ascending from the moon’s depths.

“While the moon rocks returned from sample return missions provide valuable insights, they are limited to the immediate areas around those landing sites,” stated Dr. Joshua Snape from the University of Manchester.

“In contrast, this sample could originate from impact craters located anywhere on the moon’s surface.”

“Thus, there is a unique coincidence with this sample. It fortuitously landed on Earth, unveiling secrets about lunar geology without the need for an extensive space mission.”

The sample contains notably large crystals of olivine and is classified as olivine basalt, characterized by medium titanium levels and high potassium content.

Alongside the atypical age of the samples, researchers found that the lead isotopic composition of the rocks—geochemical signatures preserved when the rocks formed—originates from internal lunar sources with unusually high ratios of uranium and lead.

These chemical markers can assist in identifying the mechanisms behind the moon’s prolonged internal heat production.

“The sample’s age is particularly intriguing as it fills a billion-year gap in the history of lunar volcanism,” Dr. Snape noted.

“It is younger than the basalts collected during the Apollo, Luna, and Chang-E 6 missions, yet significantly older than the more recent rocks retrieved by the Chang-E 5 missions in China.”

“Its age and composition indicate that volcanic activity persisted throughout this entire timeframe, and our analysis suggests a potentially continuous process of heat generation from radioactive elements that generates heat over extended periods.

“Moon rocks are a rarity, making it always exciting to acquire samples that stand out from the norm.”

“This specific rock presents new constraints on the timing and nature of volcanic activity on the moon.”

“We still have much to learn about the lunar geological history. Further analyses to trace surface origins will inform where future sample return missions might be directed.”

The researchers presented their results today at the Goldschmidt Conference 2025 in Prague, Czech Republic.

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Joshua F. Snape et al. Northwest Africa 16286: An investigation into the age and origin of new moon basalts. Goldschmidt Conference 2025

Source: www.sci.news