Ancient Demosponges: The First Animals on Earth, According to Research

Researchers from MIT and other institutions have discovered chemical fossils possibly left by ancient sponges on rocks dating back over 541 million years. These fossils consist of a distinctive type of sterlan, a stable variant of sterols found within the cell membranes of complex organisms. The team linked these sterlans to a category of sea sponges known as demosponges.



It highlights the picture representation of the ancient Stellan timeline, highlighting important compounds and their possible biological sources. Image credit: Shawar et al. , doi: 10.1073/pnas.2503009122.

“While I cannot precisely describe what these creatures looked like, I can assert they inhabited the ocean, had soft bodies, and likely lacked a silica skeleton,” stated MIT professor Roger Sammons.

In 2009, the researcher discovered the first chemical fossil believed to have originated from ancient sponges.

The team examined rock samples from outcrops in Oman and found an abundant sterlan they deduced to be a remnant of 30 carbon (C30) sterols—a rare steroid form attributed to ancient sea sponges.

Stellan was identified in very old rocks formed during the Ediacaran era (635-541 million years ago).

This era preceded the Cambrian period, which was marked by a sudden global explosion of complex, multicellular life forms.

The findings imply that ancient sponges may have existed far earlier than most multicellular organisms, potentially being one of the first animals on Earth.

Nevertheless, following the publication of these findings, alternative hypotheses emerged regarding the origin of C30 sterlan, suggesting that these chemicals could arise from other biological sources or non-organic geological processes.

The current study bolsters the initial hypothesis that ancient sponges produced this chemical record, as the researchers found new chemical fossils within the same promelat rock that were almost certainly biogenic.

Similar to previous studies, they searched for chemical fossils in rocks dating back to the Ediacaran period.

Samples were collected from drill cores and outcrops in Oman, West India, and Siberia, with analyses focused on the signatures of geologically stable sterols present in all eukaryotes (including plants, animals, and organisms with nuclear membranes).

“Without sterols or comparable membrane lipids, you cannot be classified as a eukaryote,” Professor Sammons remarked.

The chemical fossil identified in 2009 was 30-carbon sterols.

Additionally, the team deduced that these compounds could be synthesized due to distinct enzymes encoded by genes prevalent in demosponges.

“Finding sterols with 30 carbons is quite rare,” noted Dr. Lubna Shawar, a researcher at Caltech.

In this study, scientists concentrated on the chemistry of these compounds, observing that genes from the same sponge can produce even scarcer sterols with 31 carbon atoms (C31).

Upon analyzing rock samples of C31 sterlan, they discovered it was rich in the aforementioned C30 sterlan.

“These unique sterlans have been present all along,” Dr. Shawar remarked.

“We had to inquire the right questions to uncover them and truly comprehend what they signify and their origin.”

The researchers additionally procured samples of modern demosponges to examine for C31 sterols.

They determined that it is indeed a biological precursor of C31 sterlan found in rocks, observed in several species of contemporary demosponges.

Going further, they chemically synthesized eight different C31 sterols as reference materials to verify chemical structures.

The molecules were subjected to conditions simulating how sterols transform during deposition, burial, and pressurization over millions of years.

They found that two sterol-only products closely matched the structure of C31 sterols located in ancient rock samples.

The evidence from both substances strongly indicates that these compounds were created by living organisms rather than random non-biological processes.

Moreover, these organisms are likely ancestors of demosponges and still possess the capability to produce this set of compounds.

“It’s a blend of what’s present in the rock, what’s within the sponge, and what’s demonstrated in the lab,” explained Professor Sammons.

“Three supportive and concordant pieces of evidence strongly suggest these sponges are among Earth’s earliest animals.”

“This study illustrates how to authenticate biomarkers and confirm that the signals arise from life forms rather than contamination or abiogenic chemistry,” Dr. Shawar stated.

New Results were published this week in Proceedings of the National Academy of Sciences.

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Lubuna Shawar et al. 2025. Chemical characterization of C31 sterols from the sponge and Neoproterozoic fossil star counterpart. PNAS 22 (41): E2503009122; doi: 10.1073/pnas.2503009122

Source: www.sci.news

Astronomers Say: Infant Space Is Warm, Not Cold, Before It Begins to Illuminate

Astronomers utilizing CSIRO’s Murchison Wide Field Array (MWA) telescope are on the quest to uncover the elusive period of reionization. This early stage in the universe’s history has been theorized but remains undetected by radio telescopes. This period marks the end of the universe’s dark ages, occurring approximately a billion years post-Big Bang, during which intergalactic gases transform from opaque to transparent, enabling light from the first stars and galaxies to permeate the cosmos.

A glimpse of the sky observed in radio waves by the Murchison Wide Field Array. Image credit: Nunhokee et al. / ICRAR / Curtin University.

“Our research was conducted in two phases,” stated Dr. Riddhima Nunhokey, an astronomer at Curtin University Node of the International Center for Radio Astronomical Research for All Sky Astrophysics (ICRAR).

“In the initial phase, we discovered the first signs of heating in the intergalactic gas—the intergalactic medium—around 800 million years after the Big Bang.”

“To examine this primordial phase of the universe, we must isolate faint signals from this epoch while eliminating all other sources of cosmic radio emissions.”

“These sources include emissions from nearby celestial bodies, interference from Earth’s atmosphere, and even noise generated by the telescope itself.”

“Only after meticulously subtracting these ‘foreground signals’ can we discern the signals from the era of reionization.”

“From this study, we have developed methods to manage foreground contamination and remove unwanted signals, thus enhancing our understanding of telescopes and improving the clarity of detected signals.”

“We are also able to integrate nearly a decade’s worth of MWA data, allowing us to make observations over a longer timeframe than before.”

“This is another reason we are closer than ever to detecting the signals.”

The team asserts that the enhanced quality and quantity of this new dataset made this discovery feasible.

The cold universe is producing signals that resemble these new data.

This absence of signals indicates that reionization must have commenced from a “cold start,” implying that the universe was “preheated” prior to the reionization phase.

“As the universe expands, intergalactic gases cool down, and thus we expect them to become extremely cold,” explained Professor Cathryn Trott, an astronomer at ICRAR’s Curtin University Node, associated with Astro 3D and the Curtin Institute of Radio Astronomy.

“Our measurements suggest that there is a certain level of heating present. While it may not be substantial, it does indicate that extremely cold reionization is unlikely, and that’s quite intriguing.”

“This study implies that this heating is probably influenced by energy from early black holes and primordial X-ray sources resulting from stellar remnants spread across the universe.”

The findings are presented in two papers in the Astrophysical Journal.

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CD Nunhokee et al. 2025. The 21 cm power spectrum limit of z = 6.5–7.0 based on Murchison wide field array observations. APJ 989, 57; doi:10.3847/1538-4357/adda45

Cathryn M. Trott et al. 2025. Utilizing Gaussian information to enhance the limit of the 21 cm signal at z = 6.5–7.0 using Murchison wide field array data. APJ 991, 211; doi: 10.3847/1538-4357/adff80

Source: www.sci.news

IVF Enhances Reef Recovery by Promoting Reproduction

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Source: www.nbcnews.com

Discovering Why the Belly Button Turns Into an “Innie”

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Why do most people have the “Innie” belly button?

Tatiana Gorbunova / Alamy

The belly button, often overlooked, is both well-researched and under-researched. A recent study may have uncovered the reason most individuals have “innie” belly buttons, potentially linked to a previously unknown structure that pulls the belly button inward.

Researchers made this discovery while investigating optimal techniques for abdominal and hernia repair surgery.

The team’s goal was to minimize occurrences of what is known as an “uncised hernia of the umbilical,” a condition where muscle weakness from prior surgeries allows abdominal tissue to push outward, causing bulging around the belly button.

Satori Muro from the Japanese Institute of Science mentions that this issue often arises, despite the fact that the anatomical details of the umbilical area have not been extensively reported. The researchers conducted a meticulous microscopic analysis of the ventral buttons from five donated human bodies and subsequently created a 3D model of the structure.

The belly button is essentially the remnant of the fetal umbilical cord, which connects to the placenta until birth. Approximately 90% of people show a concave depression where the umbilical scar has healed. However, Muro’s team identified a “fibrous tunnel-like structure” just beneath the skin of the umbilical tissue, seamlessly extending into the deeper layers of tissue. This underlying tissue, known as the abdominal fascia, plays a critical role in stabilizing the abdomen and securing the organs.

This structure is composed of densely packed collagen fibers oriented circumferentially, resembling the umbilical cord. “This sheath seems to anchor the inward curl of the belly button to the deep fascia in multiple directions,” Muro explains, helping to maintain the unique inward shape of the belly button.

However, the team was unable to include individuals with “outie” belly buttons in their study, indicating that further research is necessary to explore the variations in umbilical cord structures among individuals.

“Differences in umbilical cord development or strength may contribute to whether someone’s belly button protrudes outward,” Muro adds.

Kat Sanders from the University of Sydney emphasizes that belly buttons are indeed vital anatomical features, but more extensive research is needed, as five subjects cannot provide a comprehensive understanding for all variations of belly buttons.

“This study reveals aspects of anatomy that are infrequently examined. Given that this area is frequently accessed during laparoscopic procedures, there’s substantial surgical interest,” Sanders states.

Michelle Moscova from the University of New South Wales believes this research will enhance understanding of the structural integrity of the abdomen.

“Umbilical hernias are a common complication after abdominal surgery, where contents such as intestines protrude through a weaker area in the abdomen, leading to inflating around the belly button,” Moscova notes.

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Source: www.newscientist.com