Adult Friendships Can Triumph Over Childhood Trauma, Even in Baboons

Members of a baboon group in Amboseli, Kenya, relax and groom together, a baboon's way of social bonding.
Photo Credit: Susan C. Alberts, Duke University

Decades of research show that experiencing traumatic things as a child -- such as having an alcoholic parent or growing up in a tumultuous home -- puts you at risk for poorer health and survival later in life.

But mounting evidence suggests that forging strong social relationships can help mitigate these effects. And not just for people, but for our primate cousins, too.

Drawing on 36 years of data, a new study of nearly 200 baboons in southern Kenya finds that adversity early in life can take years off their lifespan, but strong social bonds with other baboons in adulthood can help get them back.

“It’s like the saying from the King James Apocrypha, ‘a faithful friend is the medicine of life,’” said senior author Susan Alberts, professor of biology and evolutionary anthropology at Duke University.

Baboons who had challenging childhoods were able to reclaim two years of life expectancy by forming strong friendships.

The findings were published May 17 in the journal Science Advances.

New study explains how a common virus can cause multiple sclerosis

Olivia Thomas and Mattias Bronge
Photo Credit: Erik Holmgren

Researchers at Karolinska Institutet have found further evidence for how the Epstein-Barr virus can trigger multiple sclerosis or drive disease progression. A study published in Science Advances shows that some individuals have antibodies against the virus that mistakenly attacks a protein in the brain and spinal cord.

The Epstein-Barr virus (EBV) infects most people early in life and then remains in the body, usually without causing symptoms. The link between EBV and the neurological disease multiple sclerosis (MS) was discovered many years ago and has puzzled researchers ever since. Increasing evidence, including two papers published in Science and Nature last year, suggests that EBV infection precedes MS and that antibodies against the virus may be involved. However, the molecular mechanisms seem to vary between patients and remain largely unknown.

“MS is an incredibly complex disease, but our study provides an important piece in the puzzle and could explain why some people develop the disease,” says Olivia Thomas, postdoctoral researcher at the Department of Clinical Neuroscience, Karolinska Institutet and shared first author of the paper. “We have discovered that certain antibodies against the Epstein-Barr virus, which would normally fight the infection, can mistakenly target the brain and spinal cord and cause damage.”

How Breast Cancer Arises

Breast cancer: polyploid giant cancer cell (PGCC)
Image Credit: National Cancer Institute

In what may turn out to be a long-missing piece in the puzzle of breast cancer, Harvard Medical School researchers have identified the molecular sparkplug that ignites cases of the disease currently unexplained by the classical model of breast-cancer development.

A report on the team’s work is published May 17 in Nature.

“We have identified what we believe is the original molecular trigger that initiates a cascade culminating in breast tumor development in a subset of breast cancers that are driven by estrogen,” said study senior investigator Peter Park, professor of Biomedical Informatics in the Blavatnik Institute at HMS.

The researchers said as many as one-third of breast cancer cases may arise through the newly identified mechanism.

The study also shows that the sex hormone estrogen is the culprit behind this molecular dysfunction because it directly alters a cell’s DNA.

Most, though not all, breast cancers are fueled by hormonal fluctuations. The prevailing view of estrogen’s role in breast cancer is that it acts as a catalyst for cancer growth because it stimulates the division and proliferation of breast tissue, a process that carries the risk for cancer-causing mutations. The new work, however, shows that estrogen causes mischief in a far more direct manner.

Genetic research offers new perspective on the early evolution of animals

Some representatives of comb jellies - (a) Beroe ovata, (b) Euplokamis sp., (c) Nepheloctena sp., (d) Bathocyroe fosteri, (e) Mnemiopsis leidyi, and (f) Ocyropsis sp.
Image Credits: a, b, e, f: Joseph F. Ryan; c: R. Griswold, National Oceanic and Atmospheric Administration; d: Marsh Youngbluth, National Oceanic and Atmospheric Administration.

Mapping gene linkages provides clear-cut evidence for comb jellies as sibling group to all other animals

A study published by University of Vienna and MBARI researchers and their collaborators today in Nature provides new insights into one of the earliest points in animal evolution that happened more than 700 million years ago.

For more than a century, scientists have been working to understand the pivotal moment when an ancient organism gave rise to the diverse array of animals in the world today. As technology and science have advanced, scientists have investigated two alternative hypotheses for which animals—sponges or comb jellies, also known as ctenophores—were most distantly related to all other animals. Identifying this outlier—known as the sibling group—has long eluded scientists.

In the new study, a team of researchers from MBARI, the University of Vienna, the University of California, Berkeley, and the University of California, Santa Cruz, mapped sets of genes that are always found together on a single chromosome, in everything from humans and hamsters to crabs and corals, to provide clear evidence that comb jellies are the sibling group to all other animals. Understanding the relationships among animals will help shape our thinking about how key features of animal anatomy, such as the nervous system or digestive tract, have evolved over time.

Radio signal reveals supernova origin

Artist impression of the double star system with a compact white dwarf star accreting matter from a helium-rich donor companion, surrounded by dense and dusty circumstellar material. It was the interaction of the exploded star and the material left over from this companion that gave rise to the strong radio signal, the conspicuous helium lines in the optical spectra and the infrared emission from SN 2020eyj.
Video Credit: Adam Makarenko/W. M. Keck Observatory

In the latest issue of the journal Nature, an international team including astronomers from University of Turku reveal the origin of a thermonuclear supernova explosion. Strong emission lines of helium and the first detection of such a supernova in radio waves show that the exploding white dwarf star had a helium-rich companion.

Thermonuclear (Type Ia) supernovae are important for astronomers since they are used to measure the expansion of the Universe. However, the origin of these explosions remains an open question. While it is established that the explosion is that of a compact white dwarf star somehow accreting too much matter from a companion star, the exact process and the nature of the progenitor is not known. The new discovery of supernova SN 2020eyj established that the companion star was a so-called helium star that had lost much of its material just prior to the explosion of the white dwarf.

“Once we saw the signatures of strong interaction with the material from the companion, we tried to detect it also in radio emission”, explains Erik Kool, post-doc at the Department of Astronomy at Stockholm University and lead author of the paper. “The detection in radio is actually the first one of a Type Ia supernova – something astronomers have tried to do for decades.”

Scales or feathers? It all comes down to a few genes

From left to right: Rory Cooper, a post-doctoral researcher in Michel Milinkovitch’s laboratory, and Michel Milinkovitch, professor in the Department of Genetics and Evolution at the Faculty of Science of the UNIGE. 
Photo Credit: UNIGE

Scales, spines, feathers and hair are examples of vertebrate skin appendages, which constitute a remarkably diverse group of micro-organs. Despite their natural multitude of forms, these appendages share early developmental processes at the embryonic stage. Two researchers from the University of Geneva (UNIGE) have discovered how to permanently transform the scales that normally cover the feet of chickens into feathers, by specifically modifying the expression of certain genes. These results, published in the journal Science Advances, open new perspectives for studying mechanisms that have enabled radical evolutionary transitions in form among species.

The skin of terrestrial vertebrates is adorned with diverse keratinized appendages, such as hair, feathers, and scales. Despite the diversity of forms within and among species, the embryonic development of skin appendages typically begins in a very similar way. Indeed, all of these structures develop from cells that produce a localized thickening on the skin surface and express particular genes. One of these genes, called Sonic hedgehog (Shh), controls a signaling pathway - a communication system that allows the transmission of messages within and between cells. Shh signaling is involved in the development of diverse structures, including the neural tube, limb buds and skin appendages.

New Model for Human Evolution Suggests Homo Sapiens Arose from Multiple Closely Related Populations

View of the village of Kuboes, on the border of South Africa and Namibia. DNA samples were collected from Nama individuals who have historically lived in the region.
Photo Credit: Brenna Henn/UC Davis

In testing the genetic material of current populations in Africa and comparing against existing fossil evidence of early Homo sapiens populations there, researchers have uncovered a new model of human evolution — overturning previous beliefs that a single African population gave rise to all humans. The new research was published today, May 17, in the journal Nature.

Although it is widely understood that Homo sapiens originated in Africa, uncertainty surrounds how branches of human evolution diverged and how people migrated across the continent, said Brenna Henn, professor of anthropology and the Genome Center at UC Davis, corresponding author of the research.

“This uncertainty is due to limited fossil and ancient genomic data, and to the fact that the fossil record does not always align with expectations from models built using modern DNA,” she said. “This new research changes the origin of species.”

Research co-led by Henn and Simon Gravel of McGill University tested a range of competing models of evolution and migration across Africa proposed in the paleoanthropological and genetics literature, incorporating population genome data from southern, eastern and western Africa.

Are Earth and Venus the only volcanic planets? Not anymore.

LP 791-18 d is an Earth-size world about 90 light-years away. The gravitational tug from a more massive planet in the system, shown as a blue disk in the background, may result in internal heating and volcanic eruptions – as much as Jupiter’s moon Io, the most geologically active body in the solar system.
Illustration Credit: NASA’s Goddard Space Flight Center/Chris Smith/KRBwyle

Scientific Frontline: "At a Glance" Summary

• Main Discovery: The identification of LP 791-18 d, an Earth-sized exoplanet orbiting a red dwarf star 90 light-years away, which is likely covered in active volcanoes due to intense gravitational heating.
• Methodology: Researchers utilized photometric data from NASA’s Transiting Exoplanet Survey Satellite (TESS) and the retired Spitzer Space Telescope to detect the planet and analyze its orbit, specifically measuring transit timing variations caused by the gravitational tug of a larger neighboring planet, LP 791-18 c.
• Key Data: LP 791-18 d has a radius and mass consistent with Earth (approximately 1.03 Earth radii and 0.9 Earth masses) and orbits its host star every 2.8 days; its massive neighbor passes as close as 1.5 million kilometers, generating sufficient tidal friction to fuel volcanic activity comparable to Jupiter’s moon Io.
• Significance: This finding provides a rare analog for studying the long-term evolution of terrestrial planets and how extensive volcanic outgassing can sustain an atmosphere on tidally locked worlds, potentially allowing water to condense on the planet's dark side.
• Future Application: The planet serves as a prime target for the James Webb Space Telescope (JWST) to conduct atmospheric spectroscopy, aiming to detect potential biosignatures or volcanic gases like sulfur dioxide.
• Branch of Science: Exoplanetary Astronomy, Planetary Science.
• Additional Detail: The planet is tidally locked, meaning one side faces the star permanently, but the suspected global volcanic activity could transport heat and maintain an atmosphere across the night side.

Researchers develop new method to synthesize cannabis plant compound

Photo Credit: Matthew Brodeur

A group of researchers at Leipzig University has developed a new method for synthesizing cis-tetrahydrocannabinol (THC) – a natural substance found in the cannabis plant that produces the characteristic psychoactive effect and has many potential applications, including in the pharmaceutical industry. “Our strategy makes it possible to produce cis-tetrahydrocannabinoids and test them for their biological activity,” explains researcher Caroline Dorsch, who, together with Professor Christoph Schneider from the Institute of Organic Chemistry, has published her findings in the journal Angewandte Chemie.

She points out that until now there has been no way of synthesizing this structural class in a consistent way. With their simple, inexpensive and nature-based synthesis, the Leipzig researchers have for the first time made the substance class of cis-tetrahydrocannabinoids accessible for a broad range of applications. The researcher notes that because previous methods required many steps and large amounts of chemicals and solvents, their approach is clearly superior. The substance can be synthesized with high overall yields and excellent optical purities using the new method.  

Study Finds Carrying Pollen Heats Up Bumble Bees, Raising New Climate Change Questions

Photo Credit: Malia Naumchik.

A new study from North Carolina State University finds carrying pollen is a workout that significantly increases the body temperature of bumble bees. This new understanding of active bumble bee body temperatures raises questions about how these species will be impacted by a warmer world due to climate change.

Spend a bit of time at a nearby flower patch and you will spot a fuzzy bumble bee with yellow bumps on her back legs. These yellow bumps are solid packets of pollen that have been carefully collected during the bees’ foraging trip for transport back to their nests. And while bees may seem to move from flower to flower with ease, these pollen packets can weigh up to a third of their body weight. This new study found that – after accounting for environmental temperature and body size – the body temperature of bumble bees carrying pollen was significantly hotter than the temperature of bees that were empty-legged.

Specifically, the researchers found that bee body temperatures rose 0.07°C for every milligram of pollen that they carried, with fully laden bees being 2°C warmer than unladen bees.