Friday, March 22, 2024

Declining fertility is a huge problem for Denmark



We know a lot about why Danes are having fewer children, but not nearly enough to do anything about it. Rune Lindahl-Jacobsen, Professor of Epidemiology and Biodemography, takes us through the factors at play. And offers his take on a path to the solution



UNIVERSITY OF SOUTHERN DENMARK FACULTY OF HEALTH SCIENCES





Fertility is now firmly on the public agenda after Mette Frederiksen’s New Year’s speech and current TV and article series.

In today’s Denmark, one in eight children are born through fertility treatment, and this is part of a major societal problem that we are only now beginning to realise.

But why are we having fewer and fewer children? The short answer from Rune Lindahl-Jacobsen, Professor of Epidemiology and Biodemography, is that we don’t know.

- We know several factors that are important, but we don’t know how much each factor matters.

But there’s also a longer, more nuanced answer.

- It is only now that we as a society are realising that low birth rates pose a significant societal problem. And the problem must be seen in connection with the fact that we are living longer and longer.

Fewer children and more elderly people

Globally, far fewer children are being born than just a few years ago. In 1970, the average woman had 5 children. Today, women have 2.3 children on average, and that number is dropping sharply.

In Denmark, the figure is as low as 1.5 children per woman. In countries such as Italy, only 1.2 children are now born per woman. The magic number is 2.1, which is the number of children that must be born per woman to maintain the population size.

- We need to replace our parents. That’s the two children. And then we calculate an extra 0.1 child because some children die before reaching adulthood, Rune Lindahl-Jacobsen explains.

At the same time, we’re living longer and longer. For every year we live, we gain an extra three months or six hours every 24 hours if the trend in life expectancy continues as it has for the last 150 years.

And even though we know that we get less sick at a given age, the number of sick people increases dramatically. This happens because the risk of getting sick increases with age.

This means that the number of elderly people will increase, which will ultimately represent an increased cost for the healthcare system and society as a whole.

- This is why we need hands to create value in society and why we need sustainable fertility.

Young people must support the elderly

After 2050, at current fertility rates, the labour force (15–69-year-olds) will start to decline. And that’s problematic.

For the individual, because he or she may not be able to have the children they want. For society, because there won’t be enough hands to keep society running and support the elderly, a demographic which is going to increase in the coming years.

- National fertility forecasts have been overly optimistic for many years, and significantly fewer children have been born than predicted. We are therefore in dialogue with the forecasters, and they have already lowered their expectations for future fertility rates. That’s pretty significant, he says.

The 7,000 too many children that have been predicted to be born since 2017, but never came, means fewer childcare places, fewer educators, fewer school teachers and fewer education places. And that also means there the labour force will decrease.

If the trend continues as predicted, a situation will arise where there will be too few people contributing income to society compared to those who are costing society money (see figure).

- Importing young people from other countries is of course a solution, but somehow it seems unethical to remove labour when you know that fertility is also declining in middle-income countries, such as China, where the birth rate is 1.28 children per woman, and India, where the birth rate is 2.0 children per woman, just like in low-income countries.

Explanations for declining birth rates

There are many socio-cultural factors that we know can influence our fertility. Education in particular is cited as a factor that has had an impact, as higher education levels of women in a country means lower fertility.

On an individual level, this isn’t necessarily the case. In today’s Denmark, highly educated women have the most children.

- Of course, there are also several other social, economic and cultural factors that influence and can affect women’s behaviour. For example, women can control their fertility using contraception and induced abortion.

According to Rune Lindhardt-Jacobsen, most sociologists and demographers believe that socio-cultural and economic factors explain the fertility rate decline and that the ability to have children (fertility) is constant.

But at the same time, we know that one in six couples globally struggle to have children, as documented in a 2023 WHO report

- We also know that trends in a number of biological markers of our ability to have children show that our reproduction has deteriorated. Our ability to have children, and therefore our reproductive health, has deteriorated over time.

This is exactly what Rune Lindhardt-Jacobsen and colleagues summarised in an article in Nature Reviews Endocrinology.

Decreasing sperm quality

Male sperm quality is decreasing, a trend observed for years in high-income countries. Men’s ability to father children has simply worsened.

A good indicator of this is a study based on semen samples that young men aged 18 were invited to provide when being selected for National Service.

- Here we see that sperm quality is dangerously low. And we’re talking about 18-year-olds who have the best sperm quality they will have in their lifetime.

When comparing sperm quality with historical data from Danish men examined at an infertility clinic in the 1940s, men examined in the 1940s had a sperm concentration of approximately 60 million per millilitre, whereas the young men examined in 2000 only had 45 million per millilitre.

- This is alarming, as 40–50% of young men had sperm concentrations below 40 million per millilitre and will have trouble fathering children.

What affects fertility?

The growing need and demand for fertility treatment speaks volumes about the desire to have children. It is a clear sign that not only social and cultural factors play a role; reproductive health also needs to be considered.

- It is essential to investigate how all the substances we are exposed to in our everyday lives affect fertility. And here, men are easier to examine as it is much more difficult to test women’s fertility, such as determining the quality of a woman’s eggs.

One thing that researchers around the world are focusing on to find the causes of fertility problems is testicular cancer. Testicular cancer is a kind of canary in the coal mine.

In the same way that a dead canary in a coal mine was a sign that there were dangerous substances in the air, the incidence of testicular cancer is a good measure of reproductive problems.

Things go wrong in the foetal stage

Precursors to testicular cancer can be traced all the way back to foetal life. Up until the 12th week of pregnancy, a key process takes place in which the so-called gonads are formed. In women, the gonads become ovaries; in boys, testicles. These are the genitals that produce eggs and sperm, respectively.

If this formation goes wrong due to environmental influences such as endocrine disruptors, it leads to lower sperm quality and precursors to testicular cancer, as well as genital malformations and reduced testosterone levels.

- This means we can trace low sperm quality and precursors to testicular cancer all the way back to the foetal stage. If a woman has been exposed to something environmental, such as endocrine disruptors, it damages the ability of the male foetus to reproduce.

- Therefore, when looking for the causes of low sperm quality, we also consider the incidence of testicular cancer – and on a global level, it’s rising sharply, just as we’re seeing a decline in men’s sperm quality.

A link to fossil fuels

Rune Lindahl-Jacobsen has looked at cases of testicular cancer in men conceived during World War II, and the number is relatively lower than in other periods. There is thus reason to believe that the environmental factors that were different during World War II have an impact on our fertility.

- We observe that fossil fuel use and testicular cancer go hand in hand. The more fuel used, the more cases of cancer.

Fossil fuels are not only used for heating, but also to produce petrochemicals, which is a huge economic market (DKK 4,266 billion annually). Petrochemicals are in everything we surround ourselves with: Clothing, packaging, electronics, cosmetics, furniture and more.

- An example of a little-known fact is that almost everything you buy at the chemist’s is 99% petrochemicals. And we find them in rivers and drinking water around the world.

Petrochemicals are not natural to our bodies and therefore have the potential to reduce our fertility.

- We know this is true for some substances, such as PFAS and phthalates, but there are a myriad of products made using petrochemicals and the ways in which they can affect us, so it’s almost impossible to get an overview of possible effects.

The population must be examined

- As a society, we act on the issue by offering treatment for infertility. It’s great for the individual to get extra help in the form of fertility treatment, now also with free help for a second child, but it doesn’t matter demographically, i.e. on a population level.

Rune Lindahl-Jacobsen believes that there is a need for a national study of Danish fertility so that we can learn more about where to focus our efforts.

- How do we best prevent? How do we get women to start having children earlier? How do we prevent women from being exposed to these environmental impacts that jeopardise the sperm quality of their male children? We need to find out if we want to do something about it.

- The fact is that we know a lot of individual socio-cultural and biological factors that have an impact on fertility, but we don’t know how big their effects are in relation to the others. Therefore, it is difficult to intervene and prevent so that fertility becomes sustainable based on current knowledge.

To find out, Rune Lindhardt-Jacobsen calls for a study to be made of both the socio-cultural (mainly behavioural factors) and the biological (mainly our ability to have children) factors.

- In 1990, the Danish Parliament set up a life expectancy committee, headed by then Minister of Health Ester Larsen, due to the stagnating life expectancy. Similarly, we currently need an interdisciplinary study of Danish fertility if we want to change the low fertility rate. Until that happens, we won’t know how to increase fertility, not only in Denmark but also in other countries.

More info

Rune Lindahl-Jacobsen and colleagues have proposed population studies, in part in a publication published in the European Endocrine Views  and by participating in an expert panel in the European Society of Human Reproduction and Embryology. A fact sheet will be published in March to advise the EU Commission.


Exploring China's water usage trends and sustainability



 NEWS RELEASE 
MAXIMUM ACADEMIC PRESS





Against the backdrop of growing global concern over water scarcity, China, has been grappling with the complexities of water dynamics and their impact on economic growth and environmental protection. A recent study published in the journal Advances in Water Science has shed light on the intricate interplay between China's water usage, demand, and the factors influencing it, which is crucial for understanding the future trajectory of the country's water resources.

Led by Academician of Chinese Academy of Engineering Zhang Jianyun, the research team delved into the concept of water peaking, which refers to the point where water consumption reaches a maximum and then stabilizes or declines. This phenomenon is vital for comprehending the future of China's water resources.

The researchers analyzed China's water usage patterns, identifying three distinct phases: a period of rapid growth, a stable growth phase, and a gradual decline since 2013. However, this decline is attributed to a combination of factors, including stringent water resource management policies, technological advancements in water efficiency, and adjustments in statistical reporting methods. The study emphasizes that China's current economic and social development indicators, such as GDP per capita, industrial structure, and urbanization levels, do not yet align with those of developed countries that have experienced water peaking. This suggests that China may not have reached its peak water demand, and future water demand remains uncertain.

The study also highlights the urgent issue of water scarcity in China, with significant challenges in agriculture, industry, domestic water use, and ecological conservation. Despite efforts to improve water efficiency and implement water-saving measures, researchers believe there is still considerable room for improvement in water resource management and conservation.

In light of these findings, researchers call for a comprehensive top-level design of China's national water grid, emphasizing the need to enhance the optimization of water resource allocation at various scales. They argue that this is essential for ensuring water security and supporting the country's high-quality development amidst increasing demands and environmental constraints.

As China continues to balance its economic growth with sustainable water resource management, the international community will closely monitor its strategies and their impact on global water resource management. The study serves as a reminder of the critical role water plays in the sustainable development of any country and the importance of proactive planning and management in addressing water-related challenges.

###

References

DOI

10.14042/j.cnki.32.1309.2024.01.001

Original Source URL

http://skxjz.nhri.cn/cn/article/doi/10.14042/j.cnki.32.1309.2024.01.001

Funding information

The study is financially supported by the National Key R&D Program of China (No. 2021YFC3200204) and the National Natural Science Foundation of China (No. 52121006).

Journal

Advances in Water Science

SPACE

Researchers identify two of the Milky Way's earliest building blocks



MAX PLANCK INSTITUTE FOR ASTRONOMY

A visualisation of the Milky Way galaxy, with the stars  belonging to Shiva and Shakti 

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A VISUALIZATION OF THE MILKY WAY GALAXY, WITH THE STARS THAT KHYATI MALHAN AND HANS-WALTER RIX IDENTIFIED IN THE GAIA DR3 DATA SET AS BELONGING TO SHIVA AND SHAKTI SHOWN AS COLORED DOTS. SHIVA STARS ARE SHOWN IN GREEN AND SHAKTI STARS IN PINK. THE COMPLETE ABSENCE OF GREEN AND PINK MARKERS IN SOME REGIONS DOES NOT MEAN THAT THERE ARE NO STARS FROM SHIVA OR SHAKTI THERE, AS THE DATA SET USED FOR THIS STUDY ONLY COVERS SPECIFIC REGIONS WITHIN OUR GALAXY.

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CREDIT: S. PAYNE-WARDENAAR / K. MALHAN / MPIA




The early history of our home galaxy, the Milky Way, is one of joining smaller galaxies, which makes for fairly large building blocks. Now, Khyati Malhan and Hans-Walter Rix of the Max Planck Institute for Astronomy have succeeded in identifying what could be two of the earliest building blocks that can still be recognized as such today: proto-galactic fragments that merged with an early version of our Milky Way between 12 and 13 billion years ago, at the very beginning of the era of galaxy formation in the Universe. The components, which the astronomers have named Shakti and Shiva, were identified by combining data from ESA’s astrometry satellite Gaia with data from the SDSS survey. For astronomers, the result is the equivalent of finding traces of an initial settlement that grew into a large present-day city.

Tracing the origins of stars that came from other galaxies

When galaxies collide and merge, several processes happen in parallel. Each galaxy carries along its own reservoir of hydrogen gas. Upon collision, those hydrogen gas clouds are destabilized, and numerous new stars are formed inside. Of course, the incoming galaxies also already have their own stars, and in a merger, stars from the galaxies will mingle. In the long run, such “accreted stars” will also account for some of the stellar population of the newly-formed combined galaxy. Once the merger is completed, it might seem hopeless to identify which stars came from which predecessor galaxy. But in fact, at least some ways of tracing back stellar ancestry exist.

Help comes from basic physics. When galaxies collide and their stellar populations mingle, most of the stars retain very basic properties, which are directly linked to the speed and direction of the galaxy in which they originated. Stars from the same pre-merger galaxy share similar values for both their energy and what physicists call angular momentum – the momentum associated with orbital motion or rotation. For stars moving in a galaxy’s gravitational field, both energy and angular momentum are conserved: they remain the same over time. Look for large groups of stars with similar, unusual values for energy and angular momentum – and chances are, you might find a merger remnant.

Additional pointers can assist identification. Stars that formed more recently contain more heavier elements, what astronomers call “metals”, than stars that formed a long time ago. The lower the metal content (“metallicity”), the earlier the star presumably formed. When trying to identify stars that already existed 13 billion years ago, one should look for stars with very low metal content (“metal-poor”).

Virtual excavations in a large data set

Identifying the stars that joined our Milky Way as parts of another galaxy has only become possible comparatively recently. It requires large, high-quality data sets, and the analysis involves sifting the data in clever ways so as to identify the searched-for class of objects. This kind of data set has only been available for a few years. The ESA astrometry satellite Gaia provides an ideal data set for this kind of big-data galactic archeology. Launched in 2013, it has produced an increasingly accurate data set over the past decade, which by now includes positions, changes in position and distances for almost 1.5 billion stars within our galaxy.

Gaia data revolutionized studies of the dynamics of stars in our home galaxy, and has already led to the discovery of previously unknown substructures. This includes the so-called Gaia Enceladus/Sausage stream, a remnant of the most recent larger merger our home galaxy has undergone, between 8 and 11 billion years ago. It also includes two structures identified in 2022: the Pontus stream identified by Malhan and colleagues and the “poor old heart” of the Milky Way identified by Rix and colleagues. The latter is a population of stars that newly formed during the initial mergers that created the proto-Milky Way, and continue to reside in our galaxy’s central region.

Traces of Shakti and Shiva

For their present search, Malhan and Rix used Gaia data combined with detailed stellar spectra from the Sloan Digital Sky Survey (DR17). The latter provide detailed information about the stars’ chemical composition. Malhan says: “We observed that, for a certain range of metal-poor stars, stars were crowded around two specific combinations of energy and angular momentum.”

In contrast with the “poor old heart”, which was also visible in those plots, the two groups of like-minded stars had comparatively large angular momentum, consistent with groups of stars that had been part of separate galaxies which had merged with the Milky Way. Malhan has named these two structures Shakti and Shiva, the latter one of the principal deities of Hinduism and the former a female cosmic force often portrayed as Shiva’s consort.

Their energy and angular momentum values, plus their overall low metallicity on par with that of the “poor old heart”, makes Shakti and Shiva good candidates for some of the earliest ancestors of our Milky Way. Rix says: “Shakti and Shiva might be the first two additions to the ‘poor old heart’ of our Milky Way, initiating its growth towards a large galaxy.”

Several surveys that are either already ongoing or bound to start over the next couple of years promise relevant additional data, both spectra (SDSS-V, 4MOST) and precise distances (LSST/Rubin Observatory), should enable astronomers to make a firm decision on whether or not Shakti and Shiva are indeed a glimpse of our home galaxy's earliest prehistory.

Heat to blame for space pebble demise


Pebbles are destroyed proportional to the peak temperature they reach along their orbit



SETI INSTITUTE

MeteorCluster-20221030-Norway1 

IMAGE: 

THIS METEOROID BROKE UP BY THERMAL STRESSES JUST BEFORE ENTERING EARTH'S ATMOSPHERE, CREATING A CLUSTER OF METEORS OVER NORWAY ON OCTOBER 30, 2022, RECORDED BY ALLSKY7 STATION AMS119 OPERATED BY GAUSTABANEN AND STEINAR MIDTSKOGEN OF THE NORWAY METEOR NETWORK. 

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CREDIT: MIKE HANKEY, AMERICAN METEOR SOCIETY




March 21, 2024, Mountain View, CA -- The dust of comets fills the space between the planets, collectively called the zodiacal cloud. Still, severe breakdown has reduced that dust in size so much that it now scatters sunlight efficiently, causing the faint glow in the night sky known as the "zodiacal light."

It was long thought that high-speed collisions pulverized the comet ejecta, but now a 45-member team of researchers reports, in a paper published online in the journal Icarus this week, that heat is to blame.

“Comets eject most debris as large sand-grain to pebble-sized particles, called meteoroids, that move in meteoroid streams and cause the visible meteors in our meteor showers,” says Dr. Peter Jenniskens, meteor astronomer at the SETI Institute. “In contrast, the zodiacal cloud is mostly composed of particles the size of tobacco smoke that even radars have difficulty detecting as meteors.”

Why do pebbles pulverize after they leave the comet?

“Meteor showers show us this loss of pebbles over time, because older showers tend to contain fewer bright meteors than young showers,” said Jenniskens. “We set out to investigate what is responsible.”

Jenniskens leads a NASA-sponsored global network called “CAMS” that monitors the night sky for meteors with low-light video security cameras. Most co-authors on the paper are the researchers and citizen scientists who built and operate the 15 CAMS camera networks in ten countries.

“We developed software that detects meteors in videos recorded from different locations and then triangulates their trajectory in the atmosphere,” said detection specialist Peter S. Gural. “Meteors arriving from the same direction each day belong to a meteor shower.”

Nightly maps showing from what direction those meteors arrive at Earth are at the website: https://meteorshowers.seti.org. After 13 years of observations, the combined maps were recently published as a book, “Atlas of Earth’s Meteor Showers”, an encyclopedia of information on each known meteor shower.

“As part of this work, we determined the age of meteor showers from how much they had dispersed,” says Stuart Pilorz of the SETI Institute, “and then examined how rapidly they were losing their large meteoroids compared to the smaller ones.”  

To investigate what is responsible, the team examined of how close those streams came to the Sun. If collisions were to blame, then the pebbles were expected to be destroyed faster directly proportionally to their proximity to the Sun.

“Because there is more comet dust closer to the Sun, we had expected collisions there would pulverize the pebbles that much faster,” says Jenniskens. “Instead, we found that the pebbles survived better than expected.” 

The research team concluded that, instead, the pebbles are destroyed proportional to the peak temperature they reach along their orbit.  Thermal stresses are likely to blame for breaking up the large meteoroids near Earth, and all the way to the orbit of Mercury, while deep inside the orbit of Mercury the particles are heated so much that they fall apart from losing material.

“Here at Earth, we sometimes see that process in action when in a short time of say 10 seconds we detect ten or twenty meteors in part of the sky, a meteor cluster, the result of a meteoroid having fallen apart by thermal stresses just before entering Earth’s atmosphere,” says Jenniskens.

Manuscript online at: https://authors.elsevier.com/sd/article/S0019-1035(24)00093-9

About the SETI Institute
Founded in 1984, the SETI Institute is a non-profit, multi-disciplinary research and education organization whose mission is to lead humanity’s quest to understand the origins and prevalence of life and intelligence in the Universe and to share that knowledge with the world. Our research encompasses the physical and biological sciences and leverages expertise in data analytics, machine learning and advanced signal detection technologies. The SETI Institute is a distinguished research partner for industry, academia and government agencies, including NASA and NSF.


Same meteor cluster from a different perspective.

CREDIT

Steinar Midtskogen and Mike Hankey


New geological study: Scandinavia was born in Greenland



The oldest Scandinavian bedrock was 'born' in Greenland according to a new geological study from the University of Copenhagen. The study helps us understand the origin of continents and why Earth is the only planet in our solar system with life.


 NEWS RELEASE 
UNIVERSITY OF COPENHAGEN - FACULTY OF SCIENCE

Finnish outcrop 

IMAGE: 

IN A FINNISH OUTCROP NESTLED BETWEEN SOME OF NORTHERN EUROPE'S OLDEST MOUNTAINS, RESEARCHERS HAVE FOUND TRACES OF A PREVIOUSLY HIDDEN PART OF EARTH'S CRUST THAT POINTS MORE THAN THREE BILLION YEARS BACK IN TIME AND NORTH TOWARDS GREENLAND.

THESE TRACES WERE FOUND IN THE MINERAL ZIRCON, WHICH AFTER CHEMICAL ANALYSES, INDICATED TO RESEARCHERS FROM THE DEPARTMENT OF GEOSCIENCES AND NATURAL RESOURCE MANAGEMENT THAT THE "FOUNDATION" UPON WHICH DENMARK AND SCANDINAVIA REST, WAS PROBABLY 'BORN' FROM GREENLAND APPROXIMATELY 3.75 BILLION YEARS AGO.

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CREDIT: ANDREAS PETERSSON




In a Finnish outcrop nestled between some of Northern Europe's oldest mountains, researchers have found traces of a previously hidden part of Earth's crust that points more than three billion years back in time and north towards Greenland.

These traces were found in the mineral zircon, which after chemical analyses, indicated to researchers from the Department of Geosciences and Natural Resource Management that the "foundation" upon which Denmark and Scandinavia rest, was probably 'born' from Greenland approximately 3.75 billion years ago.

"Our data suggest that the oldest part of Earth's crust beneath Scandinavia originates in Greenland and is about 250 million years older than we previously thought," says Professor Tod Waight, a geologist at the Department of Geosciences and Natural Resource Management.

The researchers’ study of the zircon showed that, in several ways, its chemical fingerprint matches those of some of the oldest rocks on the planet found in West Greenland’s North Atlantic Craton.

"The zircon crystals we found in river sand and rocks from Finland have signatures that point towards them being much older than anything ever found in Scandinavia, while matching the age of Greenlandic rock samples. At the same time, the results of three independent isotope analyses confirm that Scandinavia's bedrock was most likely linked to Greenland," says Department of Geosciences and Natural Resource Management researcher Andreas Petersson.

A water world without oxygen

Denmark, Sweden, Norway and Finland rest atop a part of Earth's crust known as the Fennoscandian Shield, or the Baltic Shield. The researchers believe that it broke away from Greenland as a "seed" and shifted for hundreds of millions of years until it "took root" where Finland is today.

Here, the plate grew as new geological material accumulated around it, until it became Scandinavia. At the time of the crust’s detachment from Greenland, the planet looked very different than today.

"Earth was probably a watery planet, like in the movie Waterworld, but without any oxygen in the atmosphere and without emergent crust. But, because that’s so far back in time, we can’t be really be sure about what it actually looked like," says Tod Waight. 

According to the researchers, the fact that Earth even has a continental crust composed of granite is quite special when they look out into space and compare it with other planets in our galactic neighborhood.

"This is unique in our solar system. And, evidence of liquid water and a granite crust are key factors when trying to identify habitable exoplanets and the possibility of life beyond Earth," explains Andreas Petersson.

Continents are the key to life

The new study adds pieces to a primordial continental puzzle that began long before life on Earth truly blossomed, but which has largely paved the way for both human and animal life.

"Understanding how continents formed helps us understand why ours is the only planet in the solar system with life on it. Because without fixed continents and water in between them, we wouldn't be here. Indeed, continents influence both ocean currents and climate, which are crucial for life on Earth," says Andreas Petersson.

Furthermore, the new study contributes to a growing number of studies which reject the means used thus far to calculate how continents have grown – especially during the first billion years of Earth's history.

"The most commonly used models assume that Earth’s continental crust began to form when the planet was formed, about 4.6 billion years ago. Instead, our and several other recent studies suggest that the chemical signatures showing growth of the continental crust can only be identified about a billion years later. This means that we may need to revise much of what we thought about how early continents evolved," says Professor Waight. 

At the same time, results of the study add to previous research that found similar "seeds" from ancient crusts in other parts of the world.

"Our study provides us with another important clue in the mystery of how continents formed and spread across Earth – especially in the case of the Fennoscandian Shield. But there is still plenty that we don't know. In Australia, South Africa and India, for example, similar seeds have been found, but we’re unsure of whether they all come from the same "birthplace", or whether they originated independently of one another in several places on Earth. This is something that we would like to investigate more using the method we used in this study," concludes Professor Waight.

 

About the study

  • The study demonstrates that the oldest part of Earth's crust beneath Scandinavia comes from Greenland and is about 250 million years older than once thought.
  • Therefore, Denmark and Scandinavia’s geologic foundation was most likely connected to Greenland approximately 3.75 billion years ago.
  • The researchers analysed zircons from modern river sand and rock samples from the remote Pudasjärvi and Suomujärvi regions of Finland, whose geological origins have been little studied.
  • The zircon crystals found in the Finnish river sand originally crystallized in granitic magmas deep within the crust. These granites were then lifted to the surface and eroded to eventually form sand.
  • The researchers used isotopic compositions of lead, hafnium and oxygen to trace the chemical fingerprint from the Fennoscandian Shield back to Greenland. 
  • The study has been published in the scientific journal Geology.

 

The zircon crystals we found in river sand and rocks from Finland have signatures that point towards them being much older than anything ever found in Scandinavia, while matching the age of Greenlandic rock samples. At the same time, the results of three independent isotope analyses confirm that Scandinavia's bedrock was most likely linked to Greenland

CREDIT

Andreas Petersson

  • The researchers analysed zircons from modern river sand and rock samples from the remote Pudasjärvi and Suomujärvi regions of Finland, whose geological origins have been little studied.
  • The zircon crystals found in the Finnish river sand originally crystallized in granitic magmas deep within the crust. These granites were then lifted to the surface and eroded to eventually form sand.

CREDIT

Tod Waight


 

Researchers take major step toward developing next-generation solar cells



UNIVERSITY OF COLORADO AT BOULDER




The solar energy world is ready for a revolution. Scientists are racing to develop a new type of solar cell using materials that can convert electricity more efficiently than today’s panels. 

In a new paper published February 26 in the journal Nature Energy, a University of Colorado Boulder researcher and his international collaborators unveiled an innovative method to manufacture the new solar cells, known as perovskite cells, an achievement critical for the commercialization of what many consider the next generation of solar technology.

Today, nearly all solar panels are made from silicon, which boast an efficiency of 22%. This means silicon panels can only convert about one-fifth of the sun’s energy into electricity, because the material absorbs only a limited proportion of sunlight’s wavelengths. Producing silicon is also expensive and energy intensive.

Enter perovskite. The synthetic semiconducting material has the potential to convert substantially more solar power than silicon at a lower production cost.

“Perovskites might be a game changer,” said Michael McGehee, a professor in the Department of Chemical and Biological Engineering and fellow with CU Boulder’s Renewable & Sustainable Energy Institute. 

Scientists have been testing perovskite solar cells by stacking them on top of traditional silicon cells to make tandem cells. Layering the two materials, each absorbing a different part of the sun’s spectrum, can potentially increase the panels’ efficiency by over 50%.

“We're still seeing rapid electrification, with more cars running off electricity. We’re hoping to retire more coal plants and eventually get rid of natural gas plants,” said McGehee.  “If you believe that we're going to have a fully renewable future, then you're planning for the wind and solar markets to expand by at least five to ten- fold from where it is today.” 

To get there, he said, the industry must improve the efficiency of solar cells.

But a major challenge in making them from perovskite at a commercial scale is the process of coating the semiconductor onto the glass plates which are the building blocks of panels. Currently, the coating process has to take place in a small box filled with non-reactive gas, such as nitrogen, to prevent the perovskites from reacting with oxygen, which decreases their performance.  

“This is fine at the research stage. But when you start coating large pieces of glass, it gets harder and harder to do this in a nitrogen filled box,” McGehee said. 

McGehee and his collaborators set off to find a way to prevent that damaging reaction with the air. They found that adding dimethylammonium formate, or DMAFo, to the perovskite solution before coating could prevent the materials from oxidizing. This discovery enables coating to take place outside the small box, in ambient air. Experiments showed that perovskite cells made with the DMAFo additive can achieve an efficiency of nearly 25% on their own, comparable to the current efficiency record for perovskite cells of 26%. 

The additive also improved the cells’ stability. 

Commercial silicon panels can typically maintain at least 80% of their performance after 25 years, losing about 1% of efficiency per year. Perovskite cells, however, are more reactive and degrade faster in the air. The new study showed that the perovskite cell made with DMAFo retained 90% of its efficiency after the researchers exposed them to LED light that mimicked sunlight for 700 hours. In contrast, cells made in the air without DMAFo degraded quickly after only 300 hours. 

While this is a very encouraging result, there are 8,000 hours in one year, he noted. So longer tests are needed to determine how these cells hold up overtime. 

“It’s too early to say that they are as stable as silicon panels, but we're on a good trajectory toward that,” McGehee said. 

The study brings perovskite solar cells one step closer to commercialization. At the same time, McGehee’s team is actively developing tandem cells with a real-world efficiency of over 30% that have the same operational lifetime as silicon panels. 

McGehee leads a U.S. academic–industry partnership called Tandems for Efficient and Advanced Modules using Ultrastable Perovskites (TEAMUP). Together with researchers from three other universities, two companies and a national laboratory, the consortium received $9 million funding from the U.S. Department of Energy last year to develop stable tandem perovskites that can feasibly be used in the real world and are commercially viable. The goal is to create tandem more efficient than conventional silicon panels and equally stable over a 25-year period. 

With higher efficiency and potentially lower price tags, these tandem cells could have broader applications than existing silicon panels, including potential installation on the roofs of electric vehicles. They could add 15 to 25 miles of range per day to a car left out in the sun, enough to cover many people’s daily commutes. Drones and sailboats could also be powered by such panels.  

After a decade of research in perovskites, engineers have built perovskite cells that are as efficient as silicon cells, which were invented 70 years ago, McGehee said. “We are taking perovskites to the finish line.  If tandems work out well, they certainly have the potential to dominate the market and become the next generation of solar cells,” he said.