Tuesday, November 19, 2024

Hundreds of 19th-century skulls collected in the name of medical science tell a story

The Conversation
November 18, 2024

Human Skull (AFP)

When I started my research on the Samuel George Morton Cranial Collection, a librarian leaned over my laptop one day to share some lore. “Legend has it,” she said, “John James Audubon really collected the skulls Morton claimed as his own.” Her voice was lowered so as not to disturb the other scholars in the hushed archive.

As my work progressed, I uncovered no evidence to substantiate her whispered claim. Audubon had collected human skulls, several of which he then passed on to Morton. But birds and ornithology remained Audubon’s passion.

Nevertheless, the librarian’s offhanded comment has proven useful – a touchstone of sorts that continues to remind me of the controversy and confusion long surrounding the Morton Collection.

Morton was a physician and naturalist who lived in Philadelphia from 1799 until the end of his life in 1851. A lecture he delivered to aspiring doctors at the Philadelphia Association for Medical Instruction outlined the reasons for his cranial compulsion:
“I commenced the study of Ethnology in 1830; in which year, having occasion to deliver an introductory lecture on Anatomy, it occurred to me to illustrate the difference in the form of the skull as seen in the five great races of men … When I sought the materials for my proposed lecture, I found to my surprise that they could be neither bought nor borrowed.”

He would go on to acquire almost 1,000 human skulls.

Morton used these skulls to advance an understanding of racial differences as natural, easily categorizable and able to be ranked. Big-brained “Caucasians,” he argued in the 1839 publication “Crania Americana,” were far superior to small-skulled American Indians and even smaller-skulled Black Africans. Many subsequent scholars have since thoroughly debunked his ideas.

Certainly, condemnation of Morton as a scientific racist is warranted. But I find this take represents the man as a caricature, his conclusions as foregone. It provides little insight into his life and the complicated, interesting times in which he lived, as I detail in my book “Becoming Object: The Sociopolitics of the Samuel George Morton Cranial Collection.”

My research demonstrates that studies of skulls and diseases undertaken by Morton and his medical and scientific colleagues contributed to an understanding of U.S. citizenship that valued whiteness, Christianity and heroic masculinity defined by violence. It is an exclusionary idea of what it means to be American that persists today.

Yet, at the same time, the collection is an unintended testament to the diversity of the U.S. population during a tumultuous moment in the nation’s history.


Samuel Morton wasn’t a lone voice on the fringe of medicine. 'Memoir of the life and scientific labors of Samuel George Morton' by Henry S. Patterson, CC BY


Men of science and medicine

As a bioarchaeologist who has studied the Morton Collection for many years, I have sought to better understand the social, political and ideological circumstances that led to its creation. From my work – analyzing archival sources including letters, laws, maps and medical treatises, as well as the skulls themselves – I’ve learned that, over a lifetime, Morton fostered a professional network that had far-reaching tentacles.

He had plenty of help amassing the collection of skulls that bears his name.

The physician connected with medical colleagues – many of whom, like him, received degrees from the University of Pennsylvania – gentleman planters, enslavers, naturalists, amateur paleontologists, foreign diplomats and military officers. Occupational differences aside, they were mostly white, Christian men of some financial means.

Their interactions took place during a pivotal moment in American history, the interlude between the nation’s revolutionary consolidation and its violent civil unraveling.

Throughout this stretch of time, Morton and his colleagues catalyzed biomedical interventions and scientific standards to more effectively treat patients. They set in motion public health initiatives during epidemics. They established hospitals and medical schools. And they did so in the service of the nation.

Not all lives were seen as worthy of these men’s care, however. Men of science and medicine may have fostered life for many, but they also let others die. In “Becoming Object,” I track how they represented certain populations as biologically inferior; diseases were tied to nonwhite people, female anatomy was pathologized, and poverty was presumed inherited.

From person to specimen

Such representations made it easier for Morton and his colleagues to regulate these groups’ bodies, rationalize their deaths and collect their skulls with casual cruelty from almshouse dissecting tables, looted cemeteries and body-strewn battlefields. That is, a sizable portion of the skulls in Morton’s collections were not culled from ancient graves but belonged to those of the recently alive.

It is no coincidence that Morton began his scientific research in earnest the same year Andrew Jackson signed the Indian Removal Act of 1830. Men of science and medicine benefited from the expansionist policies, violent martial conflicts and Native displacement that underpinned Manifest Destiny.


A drawing from Morton’s book of the skull of a Seminole man killed by American troops. A bullet hole is visible on the left side of the man’s head. 'Crania Americana' by Samuel George Morton, CC BY


The collection reveals these acts of nation-building as necropolitical strategies – techniques used by sovereign powers to destroy or erase certain, often already vulnerable, populations from the national consciousness. These skulls attest to precarious existences, untimely deaths and trauma experienced from cradle to beyond the grave.

In the specific case of Native Americans, skeletal analysis testifies to the violent effects of U.S. military campaigns and forced removal. Native skulls that Morton labeled “warriors” have evidence of unhealed fractures and gunshot wounds. Children’s skulls bear the marks of compromised health; such pathology and their young ages at death are evidence of long-standing malnutrition, poverty and deprivation or stress.


To effectively transform subjects into objects – human beings into specimens – collected crania were ensconced in the institutional spaces of medical school lecture halls and museum storage cabinets.

There, Morton first numbered them sequentially. These numbers along with information about race, sex, age, “idiocy” or “criminality,” cranial capacity and provenance were inked on skulls and written in catalogs. Very rarely was the person’s name recorded. If used as teaching tools, Morton drilled holes to hang the skulls for display and notated them with the names of skeletal elements and features.

As dehumanizing as this process was, the Morton Collection does contain evidence of resilience and heterogeneous lives. There are traces of people with mixed-race backgrounds such as Black Indians. Several people may have also bent gender to navigate dire conditions or in keeping with social norms, such as native Beloved Women, who were active in warfare and political life.



In contrast to those whose skulls ended up in his collection, Samuel Morton’s own grave was memorialized with a monument. Pamela L. Geller


What these bones mean today


As anthropologists now recognize, it is through the repatriation of the remains of the people in the Morton Collection to their descendants, among other types of reparations, that current practitioners may begin to atone for the sins of intellectual forebears. Indeed, all institutions housing legacy collections must contend with this issue.

There are other, valuable lessons – about diversity and suffering – that the Morton Collection has to impart in today’s interesting times.

The collection demonstrates that the American body politic has always been a diverse one, despite efforts of erasure by men like Morton and his colleagues. Piecing together the stories of past, disenfranchised lives – and acknowledging the silences that have made it difficult to flesh them out – counters past white nationalism and xenophobia and their current resurgence.

The collection, I believe, also urges the repudiation of violence, casual cruelty and opportunism as admirable attributes of masculinity. Valorizing men who embody these qualities has never served America well. Particularly in the mid-1800s, when Morton amassed skulls, it led to a nation divided and hardened to suffering, an unfathomable death count and the increasing fragility of democracy.

Pamela L. Geller, Associate Professor of Anthropology, University of Miami

This article is republished from The Conversation under a Creative Commons license. Read the original article.
SPACE / COSMOS

Egg-shaped galaxies may be aligned to the black holes at their hearts, astronomers find


The Conversation
November 18, 2024

The active galaxy Centaurus A, with jets emanating from the central black hole. ESO/WFI (Optical); MPIfR/ESO/APEX/A.Weiss et al. (Submillimetre); NASA/CXC/CfA/R.Kraft et al. (X-ray), CC BY

Black holes don’t have many identifying features. They come in one color (black) and one shape (spherical).

The main difference between black holes is mass: some weigh about as much as a star like our Sun, while others weigh around a million times more. Stellar-mass black holes can be found anywhere in a galaxy, but the really big ones (known as supermassive black holes) are found in the cores of galaxies.

These supermassive behemoths are still quite tiny when seen in cosmic perspective, typically containing only around 1% of their host galaxy’s mass and extending only to a millionth of its width

However, as we have just discovered, there is a surprising link between what goes on near the black hole and the shape of the entire galaxy that surrounds it. Our results are published in Nature Astronomy.

When black holes light up

Supermassive black holes are fairly rare. Our Milky Way galaxy has one at its centre (named Sagittarius A*), and many other galaxies also seem to host a single supermassive black hole at their core.


Under the right circumstances, dust and gas falling into these galactic cores can form a disk of hot material around the black hole. This “accretion disk” in turn generates a super-heated jet of charged particles that are ejected from the black hole at mind-boggling velocities, close to the speed of light.

When a supermassive black hole lights up like this, we call it a quasar.

How to watch a quasar

To get a good look at quasar jets, astronomers often use radio telescopes. In fact, we sometimes combine observations from multiple radio telescopes located in different parts of the world.

Using a technique called very long baseline interferometry, we can in effect make a single telescope the size of the entire Earth. This massive eye is much better at resolving fine detail than any individual telescope.

As a result, we can not only see objects and structures much smaller than we can with the naked eye, we can do better than the James Webb Space Telescope.



Black holes are millions of times smaller than galaxies, yet make jets that are pointed in the same direction as the entire galaxy. Optical image: NASA, ESA, R.M. Crockett (University of Oxford, U.K.), S. Kaviraj (Imperial College London and University of Oxford, U.K.), J. Silk (University of Oxford), M. Mutchler (Space Telescope Science Institute, Baltimore, USA), R. O'Connell (University of Virginia, Charlottesville, USA), and the WFC3 Scientific Oversight Committee. Top right: MOJAVE Collaboration, NRAO/NSF. Bottom right: Event Horizon Telescope / ESO (same as before) CC BY-SA

This is the technique that was used to make the first “black hole image” in 2019, showing the halo of light generated around the supermassive black hole hosted by the galaxy M87.


Quasar jets that can be detected using very long baseline interferometry can be millions of light years long and are almost always found in elliptical galaxies. Using very long baseline interferometry, we can observe them all the way down to a few light years or so from their black hole of origin.

The direction of the jet near its source tells us about the orientation of the accretion disk, and so potentially the properties of the black hole itself.


Connection to the host galaxy


What about the host galaxies? A galaxy is a three-dimensional object, formed of hundreds of billions of stars.

But it appears to us (observed in optical or infrared) in projection, either as an ellipse or a spiral. We can measure the shape of these galaxies, tracing the profile of starlight, and measure the long axis and short axis of the two-dimensional shape.

In our paper, we compared the direction of quasar jets with the direction of this shorter axis of the galaxy ellipse, and found that they tend to be pointing in the same direction. This alignment is more statistically significant than you would expect if they were both randomly oriented.

This is surprising, as the black hole is so small (the jets we measure are only a few light years in length) compared to the host galaxy (which can be hundreds of thousands or even millions of light years across).

It is surprising that such a relatively small object can affect, or be affected by, the environment on such large scales. We might expect to see a correlation between the jet and the local environment, but not with the whole galaxy.
How galaxies form

Does this have something to say about the way galaxies form?


Spiral galaxies are perhaps the most famous kind of galaxy, but sometimes they collide with other spirals and form elliptical galaxies. We see these three-dimensional egg-shaped blobs as two-dimensional ellipses on the sky.

The merger process triggers quasar activity in ways we don’t fully understand. As a result, almost all quasar jets that can be detected using very long baseline interferometry are hosted in elliptical galaxies.

The exact interpretation of our results remains mysterious, but is important in the context of the recent James Webb Space Telescope discovery of highly massive quasars (with massive black holes), which have formed much earlier in the universe than expected. Clearly, our understanding of how galaxies form and how black holes influence that needs to be updated.


David Parkinson, Research Scientist in Astrophysics, The University of Queensland and Jeffrey Hodgson, Assistant Professor in Astrophysics, Sejong University

This article is republished from The Conversation under a Creative Commons license. Read the original article.


AnalySwift receives NASA STTR contract to transform spacecraft infrastructure for secondary uses during long-duration missions



Company and Purdue will develop composite heater layer and better engineering tools for composites



Purdue University

Kawai Kwok, Purdue University and AnalySwift, NASA STTR contract, reassembly 

image: 

Kawai Kwok, an associate professor in Purdue University’s School of Aeronautics and Astronautics, will be the primary investigator on a project with commercial software provider AnalySwift LLC. NASA has awarded AnalySwift a $156,424 Phase I Small Business Technology Transfer contract for the research.

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Credit: (Purdue University photo/Alan Cesar)




WEST LAFAYETTE, Ind. — AnalySwift LLC, a Purdue University-affiliated company, has received a Phase I STTR (Small Business Technology Transfer) contract from NASA worth $156,424.

Allan Wood, AnalySwift president and CEO, said the contract will fund two advancements: processes and hardware to disassemble spacecraft components and reassemble them for a secondary use, and software for multiphysics simulation and analysis of the involved thermoplastics.

Kawai Kwok, associate professor in Purdue’s School of Aeronautics and Astronautics, is the principal investigator.

Wood said long-duration crewed missions to the moon, Mars and beyond require infrastructure, such as trusses, to be constructed sustainably on these surfaces. But there are immense logistical challenges in transporting heavy and large payloads to space.

“The AnalySwift project proposes a novel method of disassembling and reassembling thermoplastic composite joints in space,” he said. “Our proposed method enables reconfiguration of truss structures in space, transitioning away from the current one-time use model to a scalable and sustainable approach.”

Kwok said spacecraft components could be quickly and easily repurposed into vastly different geometries.

“For example, a lunar lander support truss could become a vertical solar array support truss,” he said. “There are other applications, depending on mission needs using the same set of structural elements and innovative multiphysics modeling.”

Contract deliverables

Kwok said AnalySwift will develop a composite heater layer for the trusses and other infrastructure; it will be embedded with nanostructured carbon fillers. The layer will be made from the same thermoplastic matrix as the adhered composite parts. The layer will bring the matrix to the processing temperature for interface debonding by mechanical forces.

“Lightweight conductive nanocarbon thin films will be encapsulated inside semicrystalline thermoplastics such as PEEK (polyether ether ketone),” he said. “The disassembled struts and joints will be reassembled to the repurposed configuration via resistance welding using the same or additional heaters. The proposed in situ heating and reassembly method enables spacecraft components to be reutilized, which greatly reduces the logistical footprint to deliver technologies to space.”

Liang Zhang, senior research scientist at AnalySwift, said the company also will develop better engineering tools for composites, enabling reliable multiphysics simulation of their technique to repurpose lightweight structures made from thermoplastics.

“Theoretical and computational developments will include a new software tool or module, Thermoplastic Composites Multiphysics,” he said. “This multiphysics modeling framework will simulate the debonding and bonding processes of thermoplastic composite joint-strut interfaces using embedded carbon nanoheaters.”

Kwok said the framework has broader applications for thermoplastics.

“Advancements include developing multiphysics models and data for electrical heating and welding, including establishing relations between bonding strength and the process conditions of temperature, pressure and time,” he said. “More specifically, the disassembly and assembly processes of a nanocomposite is simulated using a third-party commercial finite element code with user subroutines defining the governing behavior of the material system.”

Zhang said AnalySwift’s multiphysics simulation tool will determine force, pressure and temperature histories during assembly and disassembly processes.

“More specifically, it will incrementally solve the constitutive relations as an initial value problem, extract temperature distributions at specific time points, and calculate the time and power required for completion,” he said.

Non-space applications

Wood said the processes and hardware advancements for disassembly and reassembly are more applicable to space applications, but the software has other potential uses.

“It can be particularly useful where simulation tools can improve utilization possibilities for high-performance thermoplastics,” he said. “Additional applications can be likely for aerospace, defense, automotive, marine, energy, electronics, sporting goods and medical devices. Applications also extend beyond simulation and into repair for thermoplastics.”

About AnalySwift

AnalySwift LLC is a provider of composite simulation software, which enables an unprecedented combination of efficiency and accuracy, including multiphysics structural and micromechanics modeling. Drawing on cutting-edge university technology, AnalySwift’s powerful solutions save orders of magnitude in computing time without a loss of accuracy so users can consider more design options and arrive at the best solution more quickly. The technologies deliver the accuracy of detailed 3D finite element analysis at the efficiency of simple engineering models. SwiftComp was developed at Purdue University and licensed from the Purdue Research Foundation. Contact AnalySwift at info@analyswift.com.

About Purdue Innovates Office of Technology Commercialization

The Purdue Innovates Office of Technology Commercialization operates one of the most comprehensive technology transfer programs among leading research universities in the U.S. Services provided by this office support the economic development initiatives of Purdue University and benefit the university’s academic activities through commercializing, licensing and protecting Purdue intellectual property. In fiscal year 2024, the office reported 145 deals finalized with 224 technologies signed, 466 invention disclosures received, and 290 U.S. and international patents received. The office is managed by the Purdue Research Foundation, a private, nonprofit foundation created to advance the mission of Purdue University. Contact otcip@prf.org for more information.

About Purdue University

Purdue University is a public research institution demonstrating excellence at scale. Ranked among top 10 public universities and with two colleges in the top four in the United States, Purdue discovers and disseminates knowledge with a quality and at a scale second to none. More than 105,000 students study at Purdue across modalities and locations, including nearly 50,000 in person on the West Lafayette campus. Committed to affordability and accessibility, Purdue’s main campus has frozen tuition 13 years in a row. See how Purdue never stops in the persistent pursuit of the next giant leap — including its first comprehensive urban campus in Indianapolis, the Mitch Daniels School of Business, Purdue Computes and the One Health initiative — at https://www.purdue.edu/president/strategic-initiatives.

Media contact: Steve Martin, sgmartin@prf.org


New idea may crack enigma of the Crab Nebula’s ‘zebra’ pattern



University of Kansas
Zebra-pattern pulsar 

image: 

Medvedev modeled wave diffraction off a circular reflecting region with radially varying index of refraction outside of it to better understand the Crab Nebula’s zebra pattern.

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Credit: Mikhail Medvedev




LAWRENCE — A theoretical astrophysicist from the University of Kansas may have solved a nearly two-decade-old mystery over the origins of an unusual "zebra" pattern seen in high-frequency radio pulses from the Crab Nebula.

His findings have just been published in Physical Review Letters (PRL), among the most prestigious physics journals.

The Crab Nebula features a neutron star at its center that has formed into a 12-mile-wide pulsar pinwheeling electromagnetic radiation across the cosmos.

“The emission, which resembles a lighthouse beam, repeatedly sweeps past Earth as the star rotates,” said lead author Mikhail Medvedev, professor of physics & astronomy at KU. “We observe this as a pulsed emission, usually with one or two pulses per rotation. The specific pulsar I’m discussing is known as the Crab Pulsar, located in the center of the Crab Nebula 6,000 light years away from us.”

The Crab Nebula is the remnant of a supernova that appeared in 1054.

“Historical records, including Chinese accounts, describe an unusually bright star appearing in the sky,” said the KU researcher.

But unlike any other known pulsar, Medvedev said the Crab Pulsar features a zebra pattern — unusual band spacing in the electromagnetic spectrum proportional to band frequencies, and other weird features like high polarization and stability.

“It’s very bright, across practically all wave bands,” he said. “This is the only object we know of that produces the zebra pattern, and it only appears in a single emission component from the Crab Pulsar. The main pulse is a broadband pulse, typical of most pulsars, with other broadband components common to neutron stars. However, the high-frequency interpulse is unique, ranging between 5 and 30 gigahertz — frequencies similar to those in a microwave oven.”

Since this pattern was discovered in a 2007 paper, the KU researcher said the pattern had proved “baffling” for investigators.

“Researchers proposed various emission mechanisms, but none have convincingly explained the observed patterns,” he said.

Using data from the Crab Pulsar, Medvedev established a method using wave optics to gauge the density of the pulsar’s plasma – the “gas” of charged particles (electrons and positrons) — using a fringe pattern found in the electromagnetic pulses.

“If you have a screen and an electromagnetic wave passes by, the wave doesn’t propagate straight through,” Medvedev said. “In geometrical optics, shadows cast by obstacles would extend indefinitely — if you’re in the shadow, there’s no light; outside of it, you see light. But wave optics introduces a different behavior — waves bend around obstacles and interfere with each other, creating a sequence of bright and dim fringes due to constructive and destructive interference.”

This well-known fringe pattern phenomenon is caused by consistent constructive interference but has different characteristics when radio waves propagate around a neutron star.

“A typical diffraction pattern would produce evenly spaced fringes if we just had a neutron star as a shield,” the KU researcher said. “But here, the neutron star’s magnetic field generates charged particles constituting a dense plasma, which varies with distance from the star. As a radio wave propagates through the plasma, it passes through dilute areas but is reflected by dense plasma. This reflection varies by frequency: Low frequencies reflect at large radii, casting a bigger shadow, while high frequencies create smaller shadows, resulting in different fringe spacing.”

In this way, Medvedev determined the Crab Pulsar’s plasma matter causes diffraction in the electromagnetic pulses responsible for the neutron star’s singular zebra pattern.

“This model is the first one capable of measuring those parameters,” Medvedev said. “By analyzing the fringes, we can deduce the density and distribution of plasma in the magnetosphere. It's incredible because these observations allow us to convert fringe measurements into a density distribution of the plasma, essentially creating an image or performing tomography of the neutron star's magnetosphere.”

Next, Medvedev said his theory can be tested with collection of more data from the Crab Pulsar and fine-tuned by factoring in its powerful and strange gravitational and polarization effects. The new understanding of how a plasma matter alters a pulsar’s signal will change how astrophysicists understand other pulsars.

“The Crab Pulsar is somewhat unique — it’s relatively young by astronomical standards, only about a thousand years old, and highly energetic,” he said. “But it’s not alone; we know of hundreds of pulsars, with over a dozen that are also young. Known binary pulsars, which were used to test Einstein’s general relativity theory, can also be explored with the proposed method. This research can indeed broaden our understanding and observation techniques for pulsars, particularly young, energetic ones.”

Pope Francis urges genocide probe of Israel's war on Gaza

Brett Wilkins, 
Common Dreams
November 18, 2024 

Pope Francis (Tiziana FABI)

In a new book set to be released this week, Pope Francis I endorsed a genocide investigation into Israel's war on Gaza—which has killed or maimed more than 150,000 Palestinians and forcibly displaced, starved, or sickened millions more over the past 13 months.


"In the Middle East, where the open doors of nations like Jordan or Lebanon continue to be a salvation for millions of people fleeing conflicts in the region: I am thinking above all of those who leave Gaza in the midst of the famine that has struck their Palestinian brothers and sisters given the difficulty of getting food and aid into their territory," the pontiff wrote in his latest book, which goes on sale in some countries on November 19.

"According to some experts, what is happening in Gaza has the characteristics of a genocide," the Pope added. "It should be carefully investigated to determine whether it fits into the technical definition formulated by jurists and international bodies.


The Pope's words echo last week's finding by a United Nations expert panel that Israel's annihilation of Gaza is "consistent with the characteristics of genocide."

The International Court of Justice—a U.N. organ—is currently weighing a South Africa-led genocide case against Israel backed by more than 30 nations and regional blocs as well as hundreds of groups and experts around the world.

Meanwhile, the prosecutor of the International Criminal Court is seeking arrest warrants for Israeli Prime Minister Benjamin Netanyahu and former Israel Defense Minister Yoav Gallant, as well as three former Hamas leaders assassinated by Israel, for alleged war crimes and crimes against humanity, including extermination.

Many jurists, scholars, and other expertsincluding some of Israel's leading Holocaust historians—have called Israel's policies and actions in Gaza genocide. Early in the war, Raz Segal—an Israeli historian and professor of Holocaust and genocide studies at Stockton University in New Jersey—called Israel's Gaza onslaught "a textbook case of genocide."

Numerous world leaders and other international officials, artists, entertainers, and others—including half of Democratic voters in the United States surveyed in May—also agree that Israel is committing genocide in Gaza.

Many Palestinian Christians have been killed, injured, or otherwise harmed by Israeli forces during the bombardment, invasion, and siege of Gaza. With just 800 to 1,000 people believed remaining in Gaza, members of the world's oldest Christian community warned early in the war that they were "under threat of extinction."

In their most infamous attack on Gaza Christians, Israeli forces bombed the 12th century Saint Porphyrius Greek Orthodox Church, Gaza's oldest, in October 2023, killing 18 Palestinians including numerous children. Among the victims were two women and an infant related to former Republican U.S. Congressman Justin Amash of Michigan.

After an Israeli sniper fatally shot an elderly woman and her daughter on the grounds of a Catholic church in Gaza City last December, Pope Francis condemned what he called an act of "terrorism."


Amid the death and destruction wrought by Israel's assault on Gaza, last December's Christmas celebrations were canceled in Bethlehem, the purported birthplace of Jesus Christ.

"How can we celebrate when we feel this war—this genocide—that is taking place could resume at any moment?" asked Palestinian Lutheran pastor Munther Isaac at the time.