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More than 130 scientists, lawyers, entrepreneurs, and government officials from five continents gathered at Harvard this week for an “exploratory” meeting to discuss the topic of creating genomes from scratch — including, but not limited to, those of humans, said George Church, Harvard geneticist and co-organizer of the meeting. The meeting was closed to the press, which drew the ire of prominent academics.
Synthesizing genomes involves building them from the ground up — chemically combining molecules to create DNA. Similar work by Craig Venter in 2010 created what was hailed as the first synthetic cell, a bacterium with a comparatively small genome.
In recent months, Church has been vocal in saying that the much-hyped genome-editing technology called CRISPR, which is only a few years old and which he helped develop, would soon be obsolete. Instead of changing existing genomes through CRISPR, Church has said, scientists could build exactly the genomes they want from scratch, by stringing together off-the-shelf DNA letters.
The topic is a heavy one, touching on fundamental philosophical questions of meaning and being. If we can build a synthetic genome — and eventually, a creature — from the ground up, then what does it mean to be human?
“This idea is an enormous step for the human species, and it shouldn’t be discussed only behind closed doors,” said Laurie Zoloth, a professor of religious studies, bioethics, and medical humanities at Northwestern University.
In response, she co-authored an article with Drew Endy, a bioengineering professor at Stanford University, calling for broader conversations around the research.
Church said that the meeting was originally going to be “an open meeting with lots of journalists engaged.” It was supposed to be accompanied by a peer-reviewed article on the topic. But, he said, the journal (which Church declined to identify) wanted the paper to include more information about the ethical, social, and legal components of synthesizing genomes — things that were discussed at the meeting.
Physicists at the Swiss Nanoscience Institute and the University of Basel have succeeded in measuring the very weak van der Waals forces between individual atoms for the first time. To do this, they fixed individual noble gas atoms within a molecular network and determined the interactions with a single xenon atom that they had positioned at the tip of an atomic force microscope. As expected, the forces varied according to the distance between the two atoms; but, in some cases, the forces were several times larger than theoretically calculated. These findings are reported by the international team of researchers in Nature Communications.
Van der Waals forces act between non-polar atoms and molecules. Although they are very weak in comparison to chemical bonds, they are hugely significant in nature. They play an important role in all processes relating to cohesion, adhesion, friction or condensation and are, for example, essential for a gecko's climbing skills.
Van der Waals interactions arise due to a temporary redistribution of electrons in the atoms and molecules. This results in the occasional formation of dipoles, which in turn induce a redistribution of electrons in closely neighboring molecules. Due to the formation of dipoles, the two molecules experience a mutual attraction, which is referred to as a van der Waals interaction. This only exists temporarily but is repeatedly re-formed. The individual forces are the weakest binding forces that exist in nature, but they add up to reach magnitudes that we can perceive very clearly on the macroscopic scale - as in the example of the gecko.
To measure the van der Waals forces, scientists in Basel used a low-temperature atomic force microscope with a single xenon atom on the tip. They then fixed the individual argon, krypton and xenon atoms in a molecular network. This network, which is self-organizing under certain experimental conditions, contains so-called nano-beakers of copper atoms in which the noble gas atoms are held in place like a bird egg. Only with this experimental set-up is it possible to measure the tiny forces between microscope tip and noble gas atom, as a pure metal surface would allow the noble gas atoms to slide around.
The researchers compared the measured forces with calculated values and displayed them graphically. As expected from the theoretical calculations, the measured forces fell dramatically as the distance between the atoms increased. While there was good agreement between measured and calculated curve shapes for all of the noble gases analyzed, the absolute measured forces were larger than had been expected from calculations according to the standard model. Above all for xenon, the measured forces were larger than the calculated values by a factor of up to two.
Via Mariaschnee, CineversityTV
Whether you have a huge honker, a puny proboscis, or a snubbed schnoz, the shape of your nose is in your genes. Now, researchers have sniffed out five of those stretches of DNA that control nose and chin shape. The team sequenced the genomes of more than 6000 men and women in Central and South America and used photographs of the participants to categorize 14 of their facial features—from cheekbone protrusion to lip shape. Then, the scientists analyzed whether any of the features were associated with certain genes. GLI3 and PAX1, both known to be involved in cartilage growth, were linked to the breadth of a person’s nostrils;DCHS2, also related to cartilage, controlled nose pointiness; RUNX2, which drives bone development, was associated with the width of the nose bridge, the upper area of the nose; and EDAR, which has previously been linked to ear and tooth shape and hair texture, affected chin protrusion. The results, published online today in Nature Communications, may help shed light on how the human face evolved and why different ethnicities have distinct facial features. Moreover, the research could help forensic scientists reconstruct faces based on genetic samples.
A new study by an international team of researchers, affiliated with Ulsan National Institute of Science and Technology (UNIST) has announced that they have succeeded for the first time in observing the structural change.
The breakthrough comes from a research, conducted by Professor Chae Un Kim (School of Natural Science) of UNIST in collaboration with researchers from Soongsil University, Cornell University, and University of Florida. Carbonic anhydrase, which is found within red blood cells, is a crucial enzyme that stabilizes carbon dioxide (CO2 ) concentrations. This enzyme catalyzes a reaction converting CO2 and water into carbonic acid, which associates into protons and bicarbonate ions.
Moreover, it is also known that carbonic anhydraseis is able to catalyze at a rate of 106 reactions per second. In the absence of this catalyst, the conversion from CO2 to bicarbonate, and vice versa, would be extremely slow and difficult.
One of the important functions of the enzyme in humans is to adjust the acidity of the chemical environment to prevent damage to the body, as well as to help transport carbon dioxide out from tissue cells to the lungs. Although carbonic anhydrase performs a lot of beneficial functions, defects in the enzyme are responsible for developing diseases, such as glaucoma, acidemia, or osteopetrosis.
Prof. Kim, the lead researcher of the study states, "The reaction rate of carbonic anhydrase is one of the fastest of all enzymes." He continues, "Due to the rapid movement of proteins, direct observation for such movement has been extremely difficult to obtain, protein scientists say."
In this study, Prof. Kim's team used their own method of "High-pressure Crycooling" and "X-ray Crystallography" to capture the gaseous carbon dioxide in crystals of carbonic anhydrase and follow the sequential structure changes as the carbon dioxide is released. The results of the study will not only greatly contribute to the future biomedical research and new drug development, but will also help make carbon capture more economic.
According to Prof. Kim of UNIST, "This study also shows technical methods that may be applicable to other enzymes that bind and react to low-molecular weight substrates, such as CO2 and NO2 ."
During the rainy season in the Orinoco Llanos of Columbia and Venezuela, an odd landscape feature appears in places: mounds of grassy plants, as big as five meters across and two meters tall, surrounded by water. Traversing this landscape, called surales, requires either hopping from mound to mound or trudging through the boggy bits in between.
Locals and scientists have generally agreed that some kind of earthworm creates the mounds, but what species and how it does so has been a mystery. Now Anne Zangerlé of the Braunschweig University of Technology in Germany and colleagues report that they’ve found the culprit — giant Andiorrhinus earthworms, which can grow to a meter in length as juveniles. And the mounds themselves, the team reports May 11 in PLOS ONE, are actually made mostly of earthworm poop.
Zangerlé and her colleagues used Google Earth images to locate surales landscapes, finding that they come in the shape of both mounds and labyrinths. Leaving the complex labyrinths for a future study, the team studied the mounds and the lands on which they were found in both the rainy and dry seasons. They characterized the soil and the plants and worms living in and on the mounds. And then they pieced all of that information together to come up with a scenario that they think explains the construction of the mounds.
Via YEC Geo
After nearly a half trillion tries, a rare event was seen that might solve an evolutionary puzzle about noncoding sequences of DNA in genomes and address speciation and the cause of diseases like cancer.
For a long time, scientists have known that much of the DNA within any given organism’s genome does not code for functional molecules or protein. However, recent research has found that these genetic sequences, misnamed “junk” DNA in the past, often do have functional significance. These introns are no exception. Now known to play a role in gene expression, introns are the portion of gene sequences that are removed or spliced out of RNA before genes are translated into protein. When eukaryotes first diverged from bacteria, there was a massive invasion of introns into the genome. All living eukaryotes — from yeast to mammals — share this common ancestor, and whereas simple organisms such as yeast have eliminated most of their introns, organisms such as mammals have considerably expanded their intron inventory. Humans have more than 200,000 introns that take up about 40 percent of the genome.
In a current paper, Stevens and co-author Sujin Lee, a former graduate student in cellular and molecular biology at UT Austin, used a new reporter assay to directly detect the loss and gain of introns in budding yeast (Saccharomyces cerevisiae). The team tested nearly a half trillion yeast and found only two instances in which an intron was added to a new gene. The proposed mechanism for this addition is a reversal of a splicing reaction.
Normally, to make proteins, RNA is read from the instructions in DNA, and the introns are spliced out. But in these two instances, the cell allowed the spliced out introns to make it back into a different RNA and was recombined back into the genome, thus creating a permanent genetic change. These are called intron gains, and if these accumulate over time, they can contribute to the development of new species as well as human disease.
“We showed in this project that introns continue to be gained, although infrequently at any point in time,” says Stevens. “But can introns drive evolution? If these sequences give organisms a selective advantage and become fixed in a population, others have shown that it can be a major factor in the creation of new species.”
These evolutionary advances come at a cost, however, because diseases such as cancer correlate with the improper removal of introns from RNA. Stevens adds, “We are continuing this work to further understand how this process impacts our genetic history, our future, and the prospects of curing disease.”
Via Integrated DNA Technologies
Our bodies are constantly and successfully fighting off the development of cells that lead to tumors - but when there is disruption to this process cancer is free to develop.
Walter and Eliza Hall Institute researchers, led by Dr Sandra Nicholson and Dr Nicholas Huntington, together with colleagues from the Queensland Institute of Medical Research, are investigating ways to 'switch on' our Natural Killer (NK) cells.
Natural Killer cells exist to detect and then destroy any deviant cells in our bodies before those cells go on to develop into tumors or before infection spreads, Dr Nicholson said. "Natural Killer cells are a key part of our immune system that locate other cells posing a danger to health either because they are infected or because they are becoming a cancer cell," she said. However, it is known that abnormal cells sometimes escape the immune system and develop into a cancer.
The researchers identified a protein 'brake' within Natural Killer cells that controls their ability to destroy their target tumor cells.
In their paper published today in Nature Immunology, they showed that when the brake was removed in an experimental model, the NK cells were better able to protect the body against metastatic melanoma.
Natural Killer cells rely on a growth factor called Interleukin 15 (IL15) to activate. Dr Nicholson and Dr Huntington's research has shown that an inhibitor protein made inside the Natural Killer cells limits the ability of the NK cell to respond to IL15 and therefore kill cancer cells. By identifying for the first time how this protein inhibits NK cell responses, they now hope that a drug can be developed that will improve the NK cells' response to this growth factor and help patients fight cancer with their own immune system. "This is about learning how to activate the NK cells of the individual patient and boost their immune system to tackle the disease," Dr Huntington said.
When a sperm and an egg cell merge a new life begins. This is the case in humans and in animals, but in principle also in plants. A German-Israeli team led by the biologists Professor Ralf Reski from Freiburg and Professor Nir Ohad from Tel-Aviv has discovered a gene trigger in the moss Physcomitrella patens which leads to offspring without fertilization. The researchers assume that this mechanism is conserved in evolution and holds the key to answer fundamental questions in biology. The study is published in the journal “Nature Plants”.
Clutter is a special challenge for robots, but new Carnegie Mellon University software is helping robots cope, whether they're beating a path across the Moon or grabbing a milk jug from the back of the refrigerator.
The software not only helped a robot deal efficiently with clutter, it surprisingly revealed the robot's creativity in solving problems.
"It was exploiting sort of superhuman capabilities," Siddhartha Srinivasa, associate professor of robotics, said of his lab's two-armed mobile robot, the Home Exploring Robot Butler, or HERB. "The robot's wrist has a 270-degree range, which led to behaviors we didn't expect. Sometimes, we're blinded by our own anthropomorphism." In one case, the robot used the crook of its arm to cradle an object to be moved. "We never taught it that," Srinivasa added.
The rearrangement planner software was developed in Srinivasa's lab by Jennifer King, a Ph.D. student in robotics, and Marco Cognetti, a Ph.D. student at Sapienza University of Rome who spent six months in Srinivasa's lab. They will present their findings May 19 at the IEEE International Conference on Robotics and Automation in Stockholm, Sweden. In addition to HERB, the software was tested on NASA's KRex robot, which is being designed to traverse the lunar surface. While HERB focused on clutter typical of a home, KRex used the software to find traversable paths across an obstacle-filled landscape while pushing an object.
Robots are adept at "pick-and-place" (P&P) processes, picking up an object in a specified place and putting it down at another specified place. Srinivasa said this has great applications in places where clutter isn't a problem, such as factory production lines. But that's not what robots encounter when they land on distant planets or, when "helpmate" robots eventually land in people's homes.
P&P simply doesn't scale up in a world full of clutter. When a person reaches for a milk carton in a refrigerator, he doesn't necessarily move every other item out of the way. Rather, a person might move an item or two, while shoving others out of the way as the carton is pulled out.
The rearrangement planner automatically finds a balance between the two strategies, Srinivasa said, based on the robot's progress on its task. The robot is programmed to understand the basic physics of its world, so it has some idea of what can be pushed, lifted or stepped on. And it can be taught to pay attention to items that might be valuable or delicate, in case it must extricate a bull from a china shop.
An international team of scientists, including two professors and three graduate students from UCLA, has detected and confirmed the faintest early-universe galaxy ever. Using the W. M. Keck Observatory on the summit on Mauna Kea in Hawaii, the researchers detected the galaxy as it was 13 billion years ago. The results were published in the Astrophysical Journal Letters.
Tommaso Treu, a professor of physics and astronomy in the UCLA College and a co-author of the research, said the discovery could be a step toward unraveling one of the biggest mysteries in astronomy: how a period known as the "cosmic dark ages" ended.
The researchers made the discovery using an effect called gravitational lensing to see the incredibly faint object, which was born just after the Big Bang. Gravitational lensing was first predicted by Albert Einstein almost a century ago; the effect is similar to that of an image behind a glass lens appearing distorted because of how the lens bends light. The detected galaxy was behind a galaxy cluster known as MACS2129.4-0741, which is massive enough to create three different images of the galaxy.
According to the Big Bang theory, the universe cooled as it expanded. As that happened, Treu said, protons captured electrons to form hydrogen atoms, which in turn made the universe opaque to radiation -- giving rise to the cosmic dark ages.
"At some point, a few hundred million years later, the first stars formed and they started to produce ultraviolet light capable of ionizing hydrogen," Treu said. "Eventually, when there were enough stars, they might have been able to ionize all of the intergalactic hydrogen and create the universe as we see it now."
That process, called cosmic reionization, happened about 13 billion years ago, but scientists have so far been unable to determine whether there were enough stars to do it or whether more exotic sources, like gas falling onto supermassive black holes, might have been responsible.
"Currently, the most likely suspect is stars within faint galaxies that are too faint to see with our telescopes without gravitational lensing magnification," Treu said. "This study exploits gravitational lensing to demonstrate that such galaxies exist, and is thus an important step toward solving this mystery."
The research team was led by Marusa Bradac, a professor at UC Davis. Co-authors include Matthew Malkan, a UCLA professor of physics and astronomy, and UCLA graduate students Charlotte Mason, Takahiro Morishita and Xin Wang.
The galaxy's magnified spectra were detected independently by both Keck Observatory and Hubble Space Telescope data.
What used to be dismissed by many as "junk DNA" is back with a vengeance as growing data points to the importance of non-coding RNAs (ncRNAs)—genome's messages that do not code for proteins—in development and disease formation. But our progress in understanding these molecules has been slow because of the lack of technologies that allow the systematic mapping of their functions.
Now, Professor Benjamin Blencowe's team at the University of Toronto's Donnelly Centre, including lead authors Eesha Sharma and Tim Sterne-Weiler, have developed a method, described in May 19, 2016 issue of Molecular Cell, that enables scientists to explore in depth what ncRNAs do in human cells. The study is published on the same day with two other papers in Molecular Cell and Cell, respectively, from Dr. Yue Wan's group at the Genome Institute of Singapore and Dr. Howard Chang's group at Stanford University in California, who developed similar methods to study RNAs in different organisms.
Of the 3 billion letters in the human genome, only two per cent make up the protein-coding genes. The genes are copied, or transcribed, into messenger RNA (mRNA) molecules, which provide templates for building proteins that do most of the work in the cell. Much of the remaining 98 per cent of the genome was initially considered by some as lacking in functional importance. However, large swaths of the non coding genome—between half and three quarters of it—are also copied into RNA.
What the resulting ncRNAs might do depends on whom you ask. Some researchers believe that most ncRNAs have no function, that they are just a by-product of the genome's powerful transcription machinery that makes mRNA. However, it is emerging that many ncRNAs have important roles in gene regulation. This view is supported in that some ncRNAs act as carriages for shuttling the mRNAs around the cell, or provide a scaffold for other proteins and RNAs to attach to and do their jobs.
But the majority of available data has trickled in piecemeal or through serendipitous discovery. And with emerging evidence that ncRNAs could drive disease progression, such as cancer metastasis, there was a great need for a technology that would allow a systematic functional analysis of ncRNAs.
"Up until now, with existing methods, you had to know what you are looking for because they all require you to have some information about the RNA of interest. The power of our method is that you don't need to preselect your candidates, you can see what's occurring globally in cells, and use that information to look at interesting things we have not seen before and how they are affecting biology," says Eesha Sharma, a PhD candidate in Blencowe's group who, along with postdoctoral fellow Tim Sterne-Weiler, co-developed the method.
The new tool, called 'LIGR-Seq', captures interactions between different RNA molecules. When two RNA molecules have matching sequences - strings of letters copied from the DNA blueprint - they will stick together like Velcro. The paired RNA structures are then removed from cells and analyzed by state-of-the-art sequencing methods to precisely identify the RNAs that are stuck together. "Most researchers in the life sciences agree that there's an urgent need to understand what ncRNAs do. This technology will open the door to developing a new understanding of ncRNA function," says Blencowe, who is also a professor in the Department of Molecular Genetics.
Not having to rely on pre-existing knowledge is one strength of the method that will boost the discovery of RNA pairs that have never been seen before. The other is that scientists can for the first time look at RNA interactions as they occur in living cells, in all their complexity, unlike in the juices of mashed up cells that they had to rely on before. This is a bit like moving on to explore marine biology from collecting shells on the beach to scuba-diving among the coral reefs where the scope for discovery is so much bigger.
ncRNAs come in multiple flavours: there's rRNA, tRNA, snRNA, snoRNA, piRNA, miRNA, and lncRNA, to name a few, where prefixes reflect the RNA's place in the cell or some aspect of its function. But the truth is that no one really knows the extent to which these ncRNAs control what goes on in the cell, nor how they do this. The new technology developed by Blencowe's group has been able to pick up new interactions involving all classes of RNAs and has already revealed some unexpected findings.
The effects of this sudden release of particles and energy have been observed throughout the solar system and beyond.
In a first, the US space agency has directly observed fundamental process of nature after sending four spacecraft through an invisible whirlpool in space called magnetic reconnection, like sending sensors up into a hurricane. The findings showed that magnetic reconnection is dominated by the physics of electrons - thus providing crucial information about what powers this fundamental process in nature.
Magnetic reconnection is one of the prime drivers of space radiation and a key factor in the quest to learn more about our space environment and protect our spacecraft and astronauts. The effects of this sudden release of particles and energy - such as giant eruptions on the sun or radiation storms in near-Earth space - have been observed throughout the solar system and beyond.
"We developed a mission called the Magnetospheric Multiscale mission (MMS) that for the first time would have the precision needed to gather observations in the heart of magnetic reconnection," said Jim Burch, principal investigator at the Southwest Research Institute in San Antonio, Texas.
"We received results faster than we could have expected. By seeing magnetic reconnection in action, we have observed one of the fundamental forces of nature," he added. MMS is made of four identical spacecraft that were launched in March 2015. They fly in a pyramid formation to create a full 3D map of any phenomena they observe.
On October 16, 2015, the spacecraft travelled straight through a magnetic reconnection event at the boundary where Earth's magnetic field bumps up against the sun's magnetic field.
In only a few seconds, the 25 sensors on each of the spacecraft collected thousands of observations. By watching these electrons, MMS made the first observation of the predicted breaking and interconnection of magnetic fields in space.
"The data showed the entire process of magnetic reconnection to be fairly orderly and elegant," said Michael Hesse, space scientist at Goddard, in a paper published in the journal Science. There does not seem to be much turbulence present, or at least not enough to disrupt or complicate the process.
This suggests that it is the physics of electrons that is at the heart of understanding how magnetic field lines accelerate the particles.
Since its launch, MMS has made more than 4,000 trips through the magnetic boundaries around Earth, each time gathering information about the way the magnetic fields and particles move.
The promise of short interfering RNA (siRNA) is that it can be harnessed to turn off harmful genes in the cell. The difficulty is getting siRNA into the cell in the first place. In a new approach, nanoengineers have driven siRNA into the cell on acoustically-propelled nanomotors, silencing genes faster and more completely than with current methods (ACS Nano2016, DOI: 10.1021/acsnano.6b01415).
To silence a gene, researchers tap the cell’s own gene suppression system, which quashes the RNA messengers that are produced when a DNA sequence is expressed. The messengers are knocked out by siRNA, complementary to a given messenger RNA, which binds the mRNA and prevents it from being translated into a protein. Scientists can mooch off the cell’s gene suppression infrastructure simply by inserting an engineered siRNA specific to a target into the cell.
But that’s easier said than done. The negatively charged siRNA has to cross a negatively-charged cell membrane, traverse the intracellular milieu, and bump into the cell’s silencing complex before degradation enzymes destroy it.
The delivery challenge has spawned a bounty of possible siRNA carriers: metal particles, lipid bubbles, hydrogels, and more. Most of these strategies rely on some form of chemical camouflage to enter the cell and on diffusion to do the rest. But Yi Chen and Joseph Wang of the University of California, San Diego, thought that ultrasound-propelled nanowires might produce an siRNA transporter with more oomph.
When bombarded with ultrasound, these tiny gold rods—about 4 μm long, 200 nm in diameter, and concave at one end—scurry into motion. They penetrate cells, bounce around like pinballs, and even spin.
Via Integrated DNA Technologies
It’s been over 340 years since Danish physicist Ole Rømer observed that the speed of light was finite. And, to this day, photons still manage to surprise us. Last year, scientists revealed a new fundamental property of light. This year, a team of physicists from by the Trinity College Dublin and the CRANN Institute have just discovered a new form of light that refuses to behave normally, and undermines what physicists know about angular momentum.
“Angular momentum measures how much something is rotating,” one of the study’s researchers, Kyle Ballantine, told Trinity News. “For a beam of light, although traveling in a straight line it can also be rotating around its own axis.” Up until this finding, physicists thought the angular momentum of all forms of light was a multiple of Planck’s constant. Apparently, that’s not so.
To uncover this information, the researchers began by searching for new behaviors of light by shining beams through crystals to create “screw-like structures.” They used the theory of quantum mechanics to analyze these beam structures and realized that the angular momentum of the photon would be a half-integer, not a multiple of Planck’s constant.
This discovery might not sound like much, but researchers suggest that it will influence our knowledge about the very essence of light. “Our discovery will have real impacts for the study of light waves in areas such as secure optical communications,” Professor John Donegan said.
Finding a new form of light is undoubtedly exciting. However, much of the physics community’s real joy comes from validating 30-year-old theoretical physics predictions. In the 1980s, physicists speculated ways in which quantum mechanics would open doors for strange new discoveries, such as particles with fractions of their expected quantum numbers. This research provides the first validation of those predictions. “This discovery is a breakthrough for the world of physics and science alike,” said CRANN Director, Stefano Santo.
Via SIN JONES
Earth’s continuously changing magnetic field is thought to be largely generated by superheated, swirling liquid iron in Earth’s outer core. Other sources of earthly magnetism include minerals in our world’s mantle and crust.
Earth’s ionosphere, magnetosphere and oceans also play a role. The European Space Agency (ESA) now has two years of data from a trio of satellites in Earth-orbit, designed to measure magnetism from these various sources. The mission is called Swarm. At last week’s Living Planet Symposium held in Prague in the Czech Republic (May 9-13, 2016), scientists presented new results from the Swarm satellite trio and provided some recent insights about how Earth’s magnetic field is changing at this time.
Among other things, they said that the field has weakened by about 3.5% at high latitudes over North America, while it has grown about 2% stronger over Asia. The region where the field is at its weakest field – the South Atlantic Anomaly – has moved steadily westward and further weakened by about 2%.
Meanwhile, the magnetic north pole has been wandering east, towards Asia. The animation shown in this article is based partly on results from ESA’s Swarm mission, and partly on information from the CHAMP and Ørsted satellites. It shows how the strength of Earth’s magnetic field changed between 1999 and mid-2016. Blue depicts where the field is weak and red shows regions where the field is strong. As you can see, the changes in field strength are relatively small.
The CRISPR/Cas9 system is currently the technique in genome editing. Thanks to recent developments in the CRISPR genome editing system, we are able to alter DNA with unprecedented precision and accuracy. Ultimately, this revolutionary genome editing technique allows us to modify any region of the genome of any species—without harming other genes. But more than that, we are able to edit these genes at just a fraction of the cost of previous methods.
It has utterly revolutionized gene editing. However, a team of researchers has just developed a new approach that just might prove to be as efficient and effective as the current standard.
According to the report, the method is based on the Natronobacterium gregoryi Argonaute (NgAgo), a DNA-guided endonuclease that’s similar to Cas9, the endonuclease of CRISPR. These are a specific type of protein, otherwise known as restriction enzymes, that are responsible for cutting DNA at specific locations. Remarkably, the study shows that NgAgo is suitable for genome editing in human cells.
The team asserts that their study has a number of key differences between NgAgo and Cas9, where the former is at the advantage. They claim that that the method appears to have a low tolerance to guide-target mismatches, leading to a high efficiency in editing:
Though there has yet to be an extensive side-by-side comparison of the two enzymes, NgAgo and Cas9 appear to have similar efficiencies. The authors report that their tests with 47 guides targeting 8 human genes, the results showed a 21% to 41% efficiency.
Old-fashioned breeding techniques are bearing more fruit than genetic engineering in developing hyper-efficient plants.
Big corporations such as DuPont Pioneer in Johnston, Iowa, have spent more than a decadedeveloping improved crops through genetic engineering, and some companies say that their transgenic varieties look promising in field trials. But there are still no fertilizer-frugal transgenic crops on the market, and several agricultural organizations around the globe are reviewing their biotechnology initiatives in this area.
Plant biologist Allen Good of the University of Alberta in Edmonton, Canada, spent years working with companies to develop genetically modified (GM) crops that require little fertilizer, but he says that this approach has not been as fruitful as conventional techniques. The problem is that there are so many genes involved in nutrient uptake and use — and environmental variations alter how they are expressed.
“Nutrient efficiency was supposed to be one of those traits with broad applicability that could make companies lots of money. But they haven't developed the way we thought,” says Good.
Despite the scientific and breeding challenges, some researchers say that all strategies must be explored to develop crops that are less nutrient needy. With the global population heading towards 10 billion people by 2050, frugal crops could be essential to feed the planet. “There is a huge worldwide potential for these traits to help increase food production and sustainable development,” says Matin Qaim, an agricultural economist at the University of Göttingen in Germany.
Is dark energy the reason time moves forward? For years, physicists have attempted to explain dark energy - a mysterious influence that pushes space apart faster than gravity can pull the things in it together. But physics isn’t always about figuring out what things are. A lot of it is figuring out what things cause. In a recent paper, a group of physicists asked this very question about dark energy, and found that in some cases, it might cause time to go forward.
Via Kim Frye, Tania Gammage, The Planetary Archives / San Francisco, California, CineversityTV
A team of scientists from the Moscow Institute of Physics and Technology (MIPT), the National Research University of Electronic Technology (MIET), and the Prokhorov General Physics Institute have proposed a theoretical model that explains the unexpectedly high values of the linear magnetoelectric effect in BiFeO3 (bismuth ferrite) that have been observed in a number of experiments. The team also suggested a way of further enhancing the effect. The results of the study have been published in the journal Physical Review B.
One particular feature of bismuth ferrite is that in bulk samples, spins of Fe3+ iron ions are arranged in the form of a cycloid. This spin structure can be destroyed by a strong magnetic field or mechanical stress. Without a spin cycloid, bismuth ferrite exhibits a large linear magnetoelectric effect, and this effect was the focal point of the study.
"The theoretical description presented in the paper may be applicable to other multiferroics similar to BiFeO3. This will help in predicting the value of their magnetoelectric effect, which, in turn, will make it easier to find new and promising materials for industrial applications," says the head of MIPT's Laboratory of physics of magnetic heterostructures and spintronics for energy-saving information technologies, Prof. Anatoly Zvezdin.
Multiferroics are materials that simultaneously exhibit different ferroic orders, including magnetic, ferroelectric and/or ferroelastic. If there is an interaction between electric and magnetic subsystems in a material, a magnetoelectric (ME) effect may occur.
The magnetoelectric effect is when electric polarization occurs under the influence of an external magnetic field and magnetization occurs under the influence of an electric field. This allows an electric field to be used to control the magnetic properties of a material and a magnetic field to be used to control the electric properties. If the value of the ME effect is high (dozens or hundreds of times higher than normal), it is called a giant ME effect.
The main use of the magnetoelectric effect is in variable and static magnetic field sensors. These sensors are used in navigation systems, electric motors, and also in vehicle ignition systems. Compared to similar devices based on the Hall effect or magnetoresistance, sensors based on the ME effect are more sensitive (according to research, up to one million times more sensitive) and they are also relatively cheap to manufacture.
The ME effect offers exciting possibilities for the use of multiferroics in new types of magnetic memory, e.g. ROM -- read only memory. The ME effect could also potentially be used to create high-precision equipment for working with radiation in the microwave range, and to wirelessly transmit power to miniaturized electronic devices.
The subject of the study was bismuth ferrite (BiFeO3) -- a highly promising multiferroic that is very promising in terms of its practical applications. It is planned to be used to create ultra energy-efficient magnetoelectric memory. In addition, bismuth ferrite exhibits a magnetoelectric effect at room temperature, while in most other magnetoelectrics an ME effect of this magnitude is only observed at extremely low temperatures (below -160 degrees Celsius).
Bismuth ferrite is an antiferromagnetic, which means that the magnetic moments of its magnetic sublattices (structures formed by atoms with the same parallel spins) cancel each other out, and the total magnetization of the material is close to zero. However, the spatial arrangement of the spins forms the same cycloidal spin structure.
New system extends the lives of flying microrobots.
Call them the RoboBats. In a recent article in Science, Harvard roboticists demonstrate that their flying microrobots, nicknamed the RoboBees, can now perch during flight to save energy -- like bats, birds or butterflies.
"Many applications for small drones require them to stay in the air for extended periods," said Moritz Graule, first author of the paper who conducted this research as a student at the Harvard John A. Paulson School of Engineering and Applied Sciences (SEAS) and Wyss Institute for Biologically Inspired Engineering at Harvard University. "Unfortunately, smaller drones run out of energy quickly. We want to keep them aloft longer without requiring too much additional energy." The team found inspiration in nature and simple science.
"A lot of different animals use perching to conserve energy," said Kevin Ma, a post-doc at SEAS and the Wyss Institute and coauthor. "But the methods they use to perch, like sticky adhesives or latching with talons, are inappropriate for a paperclip-size microrobot, as they either require intricate systems with moving parts or high forces for detachment."
Instead, the team turned to electrostatic adhesion -- the same basic science that causes a static-charged sock to cling to a pants leg or a balloon to stick to a wall.
When you rub a balloon on a wool sweater, the balloon becomes negatively charged. If the charged balloon is brought close to a wall, that negative charge forces some of the wall's electrons away, leaving the surface positively charged. The attraction between opposite charges then causes the balloon to stick to the wall.
"In the case of the balloon, however, the charges dissipate over time, and the balloon will eventually fall down," said Graule. "In our system, a small amount of energy is constantly supplied to maintain the attraction."
The RoboBee, pioneered at the Harvard Microrobotics Lab, uses an electrode patch and a foam mount that absorbs shock. The entire mechanism weighs 13.4 mg, bringing the total weight of the robot to about 100mg -- similar to the weight of a real bee. The robot takes off and flies normally. When the electrode patch is supplied with a charge, it can stick to almost any surface, from glass to wood to a leaf. To detach, the power supply is simply switched off.
"One of the biggest advantages of this system is that it doesn't cause destabilizing forces during disengagement, which is crucial for a robot as small and delicate as ours," said Graule.
Icy objects in our solar system have large oceans under their surfaces and here life could evolve and flourish. So says a new thesis by Jesper Lindkvist, PhD student at the Swedish Institute of Space Physics and Umeå University. The thesis will be defended on Tuesday 31 May at the Swedish Institute of Space Physics in Kiruna, Sweden.
There has long been speculation as to whether Jupiter's large, icy moon Callisto has an ocean beneath its surface. Observations of Callisto's near-space environment by instruments on board the spacecraft Galileo, which is orbiting Jupiter, lead us to believe that there is such a sub-surface ocean. Computer simulations of the space plasma interactions support this belief. "If you find an ocean beneath the surface of one moon, perhaps the same is true of other icy objects in space," says Jesper Lindkvist.
Outflow of water vapor has been detected from the surface of the dwarf planet Ceres, which is in the asteroid belt between Mars and Jupiter. This could indicate a reservoir of water, also related to a large sea beneath the surface. The spacecraft Dawn is at Ceres right now, trying to answer this question. "If someone was planning to build a future space base on one of these Solar System objects, for example to seek after signs of life, I would suggest they take an extra long ice bore and their fishing equipment," jokes Jesper Lindkvist.
The outflow of water vapor from moons and dwarf planets is similar to that we see from comets. The icy comet 67/Churyumov-Gerasimenko which rounded the sun in the summer of 2015 has been followed closely by the European spacecraft Rosetta. Measurements of the space environment round it show that the water flowing out from the comet's nucleus forms a prominent atmosphere which interacts with the constant flow of ionized particles from the sun, the so-called solar wind.
"Understanding their origin and how icy bodies evolve is one more piece of the puzzle we need to lay in order to explain the origin of our Solar System and its eventual fate," says Jesper Lindkvist.
Jesper Lindkvist comes from the town of Vidsel in Northern Sweden. He has a Masters degree in engineering physics from Luleå University of Technology.
A team of scientists working at the U.S. Department of Energy's (DOE) Argonne National Laboratory and led by Northern Illinois University physicist and Argonne materials scientist Zhili Xiao has created a new material, called "rewritable magnetic charge ice," that permits an unprecedented degree of control over local magnetic fields and could pave the way for new computing technologies.
The scientists' research report on development of magnetic charge ice is published in the May 20, 2016 issue of the journal Science. With potential applications involving data storage, memory and logic devices, magnetic charge ice could someday lead to smaller and more powerful computers or even play a role in quantum computing, Xiao said. Current magnetic storage and recording devices, such as computer hard disks, contain nanomagnets with two polarities, each of which is used to represent either 0 or 1 -- the binary digits, or bits, used in computers. A magnetic charge ice system could have eight possible configurations instead of two, resulting in denser storage capabilities or added functionality unavailable in current technologies.
"Our work is the first success achieving an artificial ice of magnetic charges with controllable energy states," said Xiao, who holds a joint appointment between Argonne and NIU. "Our realization of tunable artificial magnetic charge ices is similar to the synthesis of a dreamed material. It provides versatile platforms to advance our knowledge about artificial spin ices, to discover new physics phenomena and to achieve desired functionalities for applications."
Over the past decade, scientists have been highly interested in creating, investigating and attempting to manipulate the unusual properties of "artificial spin ices," so-called because the spins have a lattice structure that follows the proton positioning ordering found in water ice.
Scientists consider artificial spin ices to be scientific playgrounds, where the mysteries of magnetism might be explored and revealed. However, in the past, researchers have been frustrated in their attempts to achieve global and local control of spin-ice magnetic charges.
To overcome this challenge, Xiao and his colleagues decoupled the lattice structure of magnetic spins and the magnetic charges. The scientists used a bi-axis vector magnet to precisely and conveniently tune the magnetic charge ice to any of eight possible charge configurations. They then used a magnetic force microscope to demonstrate the material's local write-read-erase multi-functionality at room temperature. For example, using a specially developed patterning technique, they wrote the word, "ICE," on the material in a physical space 10 times smaller than the diameter of a human hair.
Magnetic charge ice is two-dimensional, meaning it consists of a very thin layer of atoms, and could be applied to other thin materials, such as graphene. Xiao said the material also is environmentally friendly and relatively inexpensive to produce.
Although the technique presently works on just one virus, scientists say it could be adapted to detect a range of viruses that plague humans including Ebola, Zika and HIV.
"The ultimate goal is to build a cheap, easy-to-use device to take into the field and measure the presence of a virus like Ebola in people on the spot," says Jeffrey Dick, a chemistry graduate student and co-lead author of the study. "While we are still pretty far from this, this work is a leap in the right direction."
The new method is highly specific, meaning it is only sensitive to one type of virus, filtering out possible false negatives caused by other viruses or contaminants. There are two other commonly used methods for detecting viruses in biological samples, but they have drawbacks. One requires a much higher concentration of viruses, and the other requires samples to be purified to remove contaminants. The new method, however, can be used with urine straight from a person or animal.
The researchers demonstrated their new technique on a virus that belongs to the herpesvirus family, called murine cytomegalovirus (MCMV). To detect individual viruses, the team places an electrode — a wire that conducts electricity, in this case, one that is thinner than a human cell — in a sample of mouse urine. They then add to the urine some special molecules made up of enzymes and antibodies that naturally stick to the virus of interest. When all three stick together and then bump into the electrode, there's a spike in electric current that can be easily detected.
The researchers say their new method still needs refinement. For example, the electrodes become less sensitive over time because a host of other naturally occurring compounds stick to them, leaving less surface area for viruses to interact with them. To be practical, the process will also need to be engineered into a compact and rugged device that can operate in a range of real-world environments.
A key biochemical enables bacteria to repair otherwise fatal damage to their DNA, including that caused by antibiotics. That is the finding of a study.
Adjusting the action of a molecule called ppGpp (guanosine-3',5'-(bis)pyrophosphate), with future treatments may disable DNA repair in microbes to make them many times more vulnerable to existing antibiotics, say the study authors. Bacteria repeatedly exposed to the same drugs become resistant to treatment, according to the Centers for Disease Control and Prevention, with related infections linked to 23,000 deaths and 2 million illnesses each year in the United States.
"Most antibiotics have their effect, directly or indirectly, by causing damage to bacterial DNA, so finding ways to cripple DNA repair would represent a significant advance in the treatment of resistant infections," says senior study author Evgeny Nudler, PhD, the Julie Wilson Anderson Professor of Biochemistry, Department of Biochemistry and Molecular Pharmacology, NYU Langone.
"While reducing DNA repair in bacteria could help to overcome antibiotic resistance, we're also excited about the prospect of boosting DNA repair in human cells," says Nudler, also an investigator with the Howard Hughes Medical Institute. "DNA damage accumulates with age and creates risk for degenerative diseases from Alzheimer's to cancer."
The study results revolve around the delicacy of DNA molecules, the letters making up the genetic code. Experts estimate that DNA is damaged thousands of times an hour in each bacterial cell, and perhaps a million times a day in a human cell with larger, more complicated DNA chains. Sunlight and toxins do much of the damage, but the biggest culprit may be highly reactive byproducts created as cells use oxygen to turn sugar into energy.
Given that damaged DNA can result in lethal mistakes in the building of proteins that comprise vital structures and messages, cells evolved early on to have overlapping, split-second DNA repair mechanisms.
In both humans and the bacteria, a key protein complex called RNA polymerase clamps onto and ticks down the DNA chain, reading the code of DNA "letters" as it translates genetic instructions into intermediary RNA molecules on the way to building proteins. Studies in recent years have revealed that the RNA polymerase in bacteria also inspects the DNA chain for damage as it reads.
In 1997, Nudler and colleagues published a paper in Cell that found bacterial RNA polymerase, which moves down the DNA chain in one direction during normal reading, instead stops and slips backward in some instances - a process Nudler called backtracking. If RNA polymerase encounters a lesion in DNA, the theory went, backtracking could make room for repair enzymes to fly in, cut out the damaged section, and rebuild a normal chain in a process called nucleotide excision DNA repair (NER).
Indeed, in 2014, Nudler's team published work in Nature that found the NER enzyme UvrD causes RNA polymerase to backtrack in the bacterial species E. coli. The newly published paper identifies ppGpp (guanosine-3',5'-(bis)pyrophosphate), a compound related in structure to the guanine building block of DNA, as the central controller of UvrD-driven backtracking in the NER pathway. Levels of ppGpp rise rapidly as bacterial RNA polymerase encounters damage and backtracks, then drop as soon as the chain is repaired to return RNA polymerase to normal transcription. The study authors conclude that ppGpp is the sensor that enables RNA polymerase to shift back and forth between DNA transcription and repair, coupling the two processes in bacteria.
Bacteria must be able to repair DNA and preserve their genomic integrity to survive, so targeting this ability is sound strategy for drug development, says Nudler. In seeking to translate this work into new treatments that defeat antibiotic resistance, he says, the field needs to determine whether or not RNA polymerase directly communicates with enzymes that produce ppGpp, and if they do, to design specific inhibitors against them.
Researchers also hope to soon confirm that RNA polymerase backtracking enables related forms of DNA repair in human cells as theorized, an important step toward boosting human DNA repair in the future.