Lifeboat Foundation

“This makes agri-PV systems increasingly attractive for agriculture, because it provides a way to keep domestic agriculture competitive with the international market and to enable farmers to earn additional income,” explains Max Trommsdorff, project manager at Fraunhofer ISE. “At the same time, we can drive the expansion of renewable energies, reduce pressure on scarce land and increase resilience to weather extremes and climate change in different farming systems.”

Nevertheless, only a few projects have been realised so far. Those involved in the project see one of the crucial hurdles in the existing legal framework. These include inadequate incentive systems and comparatively complex approval processes. In addition, there are growing concerns about the acceptance of the local population and the attractiveness of the landscape.

Such economic, legal and social hurdles are to be compiled within the framework of the project. Subsequently, the participants want to work out proposals for solutions on how to reduce and overcome these hurdles. The focus should be on the optimal use of the potentials and the avoidance of wrong decisions in the application of agriphotovoltaics.

Unnecessary Playing with nature.

The stem-cell-derived embryos could shed new light on the earliest stages of human pregnancy.

The most massive star known by astronomers is truly of gargantuan proportions. Dubbed R136a1, this is the most massive and luminous star ever discovered in the cosmos. Additionally, it belongs to the Large Magellanic Cloud and is one of the hottest stars out there, and it is very, very different than our Sun.

Astronomers have obtained the sharpest image ever of star R136a1, the most massive known star in the Universe, with the 8.1-meter Gemini South telescope in Chile, part of the International Gemini Observatory operated by NSF’s NOIRLab. Researchers at NOIRLab, led by Venu Kalari, challenge our understanding of the most massive stars and suggest their mass may be lower than previously believed.

The formation of the biggest stars – those with 100 times the mass of the Sun – is still a mystery to astronomers. Observing these giants, which normally reside within dust-shrouded star clusters, is challenging. A giant star’s fuel reserves are depleted in less than a million years. Compared with our Sun, which has a lifespan of about 10 billion years, ours is less than halfway through. Individual massive stars in clusters are difficult to distinguish due to their densely packed nature, short lifetimes, and vast astronomical distances.

A new technique makes it possible to capture videos of single atoms “swimming” at the interface between a solid and a liquid for the first time. The approach uses stacks of two-dimensional materials to trap the liquid, making it compatible with characterization techniques that usually require vacuum conditions. It could enable researchers to better understand how atoms behave at these interfaces, which play a crucial role in devices such as batteries, catalytic systems and separation membranes.

Several techniques exist to image single atoms, including scanning tunnelling microscopy (STM) and transmission electron microscopy (TEM). However, they involve exposing atoms on the surface of the sample to a high-vacuum environment, which can change the material’s structure. Techniques that do not require a vacuum, meanwhile, are either lower-resolution or only work for short time periods, meaning that the atoms’ motion cannot be captured on video.

Researchers led by materials scientists Sarah Haigh of the University of Manchester’s National Graphene Institute (NGI) have now developed a new approach that enables them to track the motion of single atoms on a surface when that surface is surrounded by liquid. They showed that the atoms behave very differently under these circumstances than they do in vacuum. “This is crucial,” explains Haigh, “since we want to understand atomic behaviour for realistic reaction/environmental conditions that the material will experience in use – for example, in a battery, supercapacitor and membrane reaction vessels.”

Researchers have developed a new type of high-efficiency photodetector inspired by the photosynthetic complexes plants use to turn sunlight into energy. Photodetectors are used in cameras, optical communication systems and many other applications to turn photons into electrical signals.

Researchers developed a new type of high-efficiency photodetector that is similar to the photosynthetic complexes plants use to turn sunlight into energy. The new design integrates a simple organic detector into the propagation region to produce efficient polariton-to-charge conversion over distances of up to 100 microns. (Image: Bin Liu, University of Michigan)

“Our devices combine long-range transport of optical energy with long-range conversion to electrical current,” said research team leader Stephen Forrest from the University of Michigan. “This arrangement, analogous to what is seen in plants, has the potential to greatly enhance the power generation efficiency of solar cells, which use devices similar to photodetectors to convert sunlight into energy.”

Demonstration of concept I first developed for The Millennial Project at the turn of the century. Even had the same name.

https://tmp2.fandom.com/wiki/Inchworms.

Continue reading “The GITAI IN1, an inchworm-type robotic arm” »

Scientists had previously theorised that extremely high pressure and temperatures turn hydrogen and carbon into solid diamonds thousands of kilometres below the surface of the ice giants.

Now new research, published in Science Advances, inserted oxygen into the mix, finding that “diamond rain” could be more common than thought.

Ice giants like Neptune and Uranus are thought to be the most common form of planet outside our Solar System, which means diamond rain could be occurring across the universe.

It is long-established that innervation-dependent production of neurotrophic factors is required for blastema formation and epimorphic regeneration of appendages in fish and amphibians. The regenerating mouse digit tip and the human fingertip are mammalian models for epimorphic regeneration, and limb denervation in mice inhibits this response. A complicating issue of limb denervation studies in terrestrial vertebrates is that the experimental models also cause severe paralysis therefore impairing appendage use and diminishing mechanical loading of the denervated tissues. Thus, it is unclear whether the limb denervation impairs regeneration via loss of neurotrophic signaling or loss of mechanical load, or both. Herein, we developed a novel surgical procedure in which individual digits were specifically denervated without impairing ambulation and mechanical loading. We demonstrate that digit specific denervation does not inhibit but attenuates digit tip regeneration, in part due to a delay in wound healing. However, treating denervated digits with a wound dressing that enhances closure results in a partial rescue of the regeneration response. Contrary to the current understanding of mammalian epimorphic regeneration, these studies demonstrate that mouse digit tip regeneration is not peripheral nerve dependent, an observation that should inform continued mammalian regenerative medicine approaches.

Ken Muneoka has a history of shaking up the field of regeneration; for instance, in a 2019 groundbreaking article published in Nature, the Texas A&M University College of Veterinary Medicine & Biomedical Sciences (CVMBS) professor proved the possibility of joint regeneration in mammals for the first time.

His team is already questioning further long-held notions about the underlying science of the subject, this time in relation to how mammals might regenerate damaged parts of the body.

Only some organs, like the liver, and certain tissues, like the epidermis, the top layer of skin, can naturally regenerate in humans.