New Study Uncovers How the Pelvis Evolved and Helped Our Ancestors Stand Upright

The pelvis is often described as the keystone for upright locomotion. Over millions of years, it has undergone significant transformations, enabling us to walk on two legs more effectively than any other part of our lower body. However, the specifics of this remarkable adaptation have been largely unknown. Recent research has uncovered two crucial genetic changes that reshaped the pelvis, permitting it to evolve into the upright structure that our ancestors utilized while traversing the Earth.

Ardipithecus ramidus Humanity resided in Africa over 4 million years ago. Illustrations by Arturo Asensio, via Quo.es

Anatomists have long recognized that the human pelvis is distinct among primates.

In our closest relatives, African apes (chimpanzees, bonobos, and gorillas) possess hipbones that are tall, narrow, and flat from front to back. When viewed from the side, they resemble thin blades.

The pelvic structure of an ape supports large muscles essential for climbing.

In contrast, human hip bones rotate sideways, forming a bowl shape. This flaring of the hip bones allows for muscle attachment critical for maintaining balance while shifting weight from one foot to the other during upright locomotion.

Nonetheless, the mechanisms behind this transformation have been elusive until now.

In a recent study, Professor Terrence Capelini from Harvard University and his team pinpointed vital genetic and developmental shifts that facilitated the evolution from the pelvis of tetraleaf monkeys to bipedalism.

“Our findings illustrate a complete mechanistic shift in human evolution,” stated Professor Capelini.

“There is no parallel to this among other primates.”

The researchers analyzed 128 samples of embryonic tissue from humans housed in museums in the US and Europe, along with nearly 20 other primate species.

These collections included specimens over 100 years old, preserved on glass slides or in bottles.

Using CT scans and histological analysis, they investigated pelvic anatomy during the early stages of development.

Their research revealed that the evolution of the human pelvis unfolded in two major phases.

Initially, the growth plate shifted 90 degrees, widening the human ilium instead of extending its height.

Following this adjustment, the timeline for embryonic bone formation was altered.

Typically, bones in the lower body develop when chondrocytes align along the long axis of the growing bone.

This cartilage becomes rigid through a process known as ossification.

At the early stages of development, similar to other primates, human growth plates formed from the head and continued to develop.

However, by day 53, the growth plate had notably shifted vertically from its initial orientation, resulting in a shorter and broader hip joint.

“When I examined my pelvis, it wasn’t initially on my radar,” Professor Capelini remarked.

“I anticipated a gradual modification to shorten and widen it, but histology indicated a complete 90-degree reversal.”

Group of Australopithecus afarensis. Image credit: Matheus Vieira.

A further significant alteration was the timeline of bone formation.

In most cases, bones develop along the primary ossification center located in the center of the bone shaft.

However, in humans, the ilium diverges from this norm, with ossification beginning at the posterior region in the sacrum and expanding radially.

This mineralization remains restricted to the peripheral layer, while internal ossification is postponed by 16 weeks, allowing bones to grow and maintain their shape during their geometric transitions.

To uncover the molecular mechanisms driving these changes, the team employed techniques like single-cell multiomics and spatial transcriptomics.

The researchers identified over 300 active genes, including three with notable roles: Sox9 and PTH1R (which control growth plate shifts) and runx2 (which governs ossification changes).

The significance of these genes is underscored by diseases arising from their dysfunction.

For example, mutations in Sox9 can lead to Campomelic dysplasia, a disorder characterized by an abnormally narrow hip joint lacking lateral flaring. Similarly, mutations in PTH1R result in narrow hip joints and various skeletal disorders.

The scientists propose that these adaptations began with the reorientation of the growth plate around the time our ancestors separated from African apes, estimated to have occurred between 5 and 8 million years ago.

They believe the pelvis has served as a focal point for evolutionary transformations over millions of years.

As brain size increased, the pelvis encountered selective pressures known as the obstetric dilemma—the trade-off between a narrow pelvis for efficient movement and a broader one for accommodating the birth of larger babies.

Researchers suspect that the delay in ossification likely occurred within the last two million years.

The oldest pelvic fossil, dated at 4.4 million years, belongs to Ardipithecus from Ethiopia—a species exhibiting a blend of upright walking and tree-climbing features, with pelvic characteristics akin to those of humans.

The renowned 3.2 million-year-old skeleton of Lucy (Australopithecus afarensis) showcases further adaptations for bipedalism, including the distinctively flaring hip blades.

“From that point onwards, all hominin fossils displayed pelvises that diverged significantly from those of earlier primates,” stated Professor Capelini.

“The implications of brain size and its subsequent changes should not be interpreted through growth models applicable to chimpanzees and unassociated primates.”

“Models should focus on the developments between humans and their own lineage.”

“Post-fetal growth occurred against the backdrop of novel methods for constructing the pelvis.”

This study is set to be published in the journal Nature.

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G. Senevilas et al. The evolution of hominin bipedal walking in two steps. Nature Published online on August 27th, 2025. doi:10.1038/s41586-025-09399-9

Source: www.sci.news

New Study Suggests Photons from Dwarf Galaxies Helped Reionize the Early Universe

Reionization of the universe happened about 500 million to 900 million years after the Big Bang. This represents the transformation of neutral hydrogen into an ionized gas and marks the end of the “Dark Ages” in the history of the universe. Currently, astronomers using the NASA/ESA/CSA James Webb Space Telescope have obtained spectra of eight ultrafaint dwarf galaxies that existed less than a billion years after the Big Bang. Their observations could help settle long-standing scientific debates about the driving force of reionization and could also be essential to understanding the formation of the first galaxies.

Astronomers estimate that 50,000 near-infrared sources are represented in the Webb image of galaxy cluster Abel 2744. Image credits: NASA / ESA / CSA / I. Labbe, Swinburne Institute of Technology / R. Bezanson, University of Pittsburgh / A. Pagan, STScI.

There is still much we don’t understand about the period in the early history of the universe known as the Era of Reionization.

It was a time of darkness, without stars or galaxies, and filled with a thick fog of hydrogen gas, until the first stars ionized the surrounding gas and light began to pass through.

Astronomers have spent decades trying to identify sources that emit radiation powerful enough to gradually remove this hydrogen fog that blanketed the early universe.

“Our discovery reveals the important role played by ultrafaint galaxies in the evolution of the early universe,” said astronomer Dr. Irina Chemelinska from the Paris Institute of Astrophysics.

“They produce ionizing photons that convert neutral hydrogen into ionized plasma during the reionization of the universe.”

“This highlights the importance of understanding low-mass galaxies in shaping the history of the universe.”

“These cosmic power plants collectively emit more than enough energy to accomplish their work,” said Dr. Hakim Atek, also of the Paris Institute of Astrophysics.

“Despite their small size, these low-mass galaxies produce large amounts of energetic radiation, and their abundance during this period is so great that their collective impact alters the state of the entire universe can do.”

In the study, astronomers captured and analyzed the spectra of eight very faint galaxies magnified by the lensing star cluster Abel 2744.

They found that these galaxies emit large amounts of ultraviolet light, at levels four times higher than previously thought.

This means that most of the photons that reionized the Universe likely came from these dwarf galaxies.

“With the web, we have stepped into uncharted territory,” said Dr. Themiya Nanayakkara, an astronomer at Swinburne University of Technology.

“Our study reveals more provocative questions that must be answered in efforts to chart the evolutionary history of our beginnings.”

of result It was published in the magazine Nature.

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H. Atek other. 2024. Most of the photons that reionized the universe came from dwarf galaxies. Nature 626, 975-978; doi: 10.1038/s41586-024-07043-6

Source: www.sci.news