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Phase III – Stealth Is.

“In the quietude, you may find solace in knowing.” “In knowing, you will find the solace of quietude.”

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Category: New Science

Humans have sent probes to planets and asteroids throughout our solar system. But we’ve never come close to propelling a manmade object as far as another star.

But if NASA and DARPA – the agency responsible for some of the early innovations that led to the Internet – have their way, in the next 100 years, a spaceship would stand ready to visit another star.

The two agencies have teamed up on a 1 million-dollar project called the 100-Year Starship Study to begin contemplating technologies and organizational strategies to make the mission happen.

For three days, scientists from universities, NASA centers and private institutions will discuss the merits of fusion versus nuclear thermal propulsion, as well as the social and psychological implications of sending humans on a one-way mission to the stars.

Religious and philosophical aspects of interstellar travel will also be discussed.

“The 100-Year Starship is about more than building a spacecraft or any one specific technology,” Fox News quoted DARPA officials as writing in a statement.

“Through this effort, DARPA seeks to inspire several generations to commit to the research and development of breakthrough technologies and cross-cutting innovations across myriad disciplines,” they added.

But a note to would-be space travellers: It’s too soon to sign up for the trip.

“Neither DARPA nor NASA are actually building a 100-Year Starship,” DARPA officials wrote.

“We are planting seeds for an organization. Consequently we are not taking starship crew applications at the present time.”

The synaptic pruning that helps sculpt the adolescent brain into its adult form continues to weed out weak neural connections throughout our 20s. The surprise finding could have implications for our understanding of schizophrenia, a psychological disorder which often appears in early adulthood.

As children, we overproduce the connections – synapses – between brain cells. During puberty the body carries out a kind of topiary, snipping away some synapses while allowing others to strengthen. Over a few years, the number of synapses roughly halves, and the adult brain emerges.

Or so we thought. Pasko Rakic at Yale University and colleagues at the University of Zagreb, Croatia, and the VU University Medical Center in Amsterdam, the Netherlands, have now found that the brains of adults in their 20s are still subject to synaptic pruning.

Rakic’s team analysed post-mortem tissue from a brain region called the prefrontal cortex (PFC) in 32 people aged between 1 week old and 91 years. Specifically, they calculated the density of dendritic spines – the tiny projections that protrude from the neuron’s long dendrites, each of which facilitates communication with other neurons through a synapse.

As expected, Rakic’s team found that spine density increased rapidly during infancy, reaching a peak before the 9th birthday. It then began to fall away as pruning began. Intriguingly, though, spine density did not plateau after adolescence, as might have been expected, but continued to fall gradually until the late 20s.

Rakic says the result could be good news for those hoping to gain new skills in their third decade. The period of pruning is associated with a heightened ability to learn – whether that is in picking up language skills or understanding new concepts, he says. “You should not give up learning just because you’re in your 20s – it isn’t too late,” he says.

Article source: http://www.aleph9.com/Research/?p=187


On August 9, 2011 at 3:48 a.m. EDT, the sun emitted an Earth-directed X6.9 flare, as measured by the NOAA GOES satellite.

This was the largest flare of the current solar cycle, an R3 (Strong) Radio Blackout, alternatively classified as an X6, according to the U.S. NOAA Space Weather Prediction Center.

These gigantic bursts of radiation can disrupt GPS and communications signals. In this case, scientists say the eruption took place on the side of the sun that was not facing Earth, so there’ll be little impact to satellites and communication systems, AP reports.

Space scientist Joe Kunches at the U.S. Space Weather Prediction Center in Colorado says there were reports of brief short-wave radio disruptions in Asia, but little else.

Bookmark:


Related posts:

  1. Solar flare eruptions set to reach Earth
  2. Antiproton ring found around Earth
  3. DIY Recordings of Awakening Sun
  4. What does the sun sound like?

Article source: http://www.aleph9.com/Research/?p=178

James Bond may have to up his game. Cloaking materials can now hide tiny microphones placed on a wall – and they will do the job at all visible wavelengths.

Optical cloaks can hide a free-floating object by bending light all the way around it, but only at specific wavelengths. They are usually made of synthetic metamaterials, which have a structure on a scale smaller than the wavelength of light they are meant to deflect.

Bumps or objects on a floor or wall are relatively easy to hide, since merely changing the angle at which light bounces off them can make the surface look flat. Previously, such “carpet cloaking”Movie Camera had only been achieved at infrared and microwave wavelengths.

Now two different cloak designs have managed to conceal bumps over the full visible spectrum. Chris Gladden and Majid Gharghi of the University of California, Berkeley, etched holes into a thin layer of silicon nitride deposited on porous glass. Varying the diameter of the holes between 20 and 65 nanometres – smaller than the wavelengths of visible light – changed the way the layer refracted light, allowing its interaction with the porous glass substrate to cloak a small bump.

Earlier this year, Baile Zhang and colleagues at the Singapore-MIT Alliance for Research and Technology achieved a similar effect with polarised light, whose electric field is lined up in one direction. The team aligned calcite crystals, which have refractive properties that depend on the electric field’s direction, to hide a 2-millimetre-high bump.

Gladden and Gharghi also used polarised light in their test, “but it’s not required” for the design, says Gladden. He says the ability to use normal unpolarised visible light would allow their setup to be used for a wider variety of applications beyond cloaking. “We could use the same approach in solar energy devices to control sunlight and potentially increase efficiency,” says Gharghi. This could be done by focusing light to higher intensity or diverting light around obstructions such as current-collecting wires.

Article source: http://www.aleph9.com/Research/?p=188


Antiprotons appear to ring the Earth, confined by the planet’s magnetic field lines. The antimatter, which may persist for minutes or hours before annihilating with normal matter, could in theory be used to fuel ultra-efficient rockets of the future.

Charged particles called cosmic rays constantly rain in from space, creating a spray of new particles – including antiparticles – when they collide with particles in the atmosphere. Many of these become trapped inside the Van Allen radiation belts, two doughnut-shaped zones around the planet where charged particles spiral around the Earth’s magnetic field lines.

Satellites had already discovered positrons – the antimatter partners of electrons – in the radiation belts. Now a spacecraft has detected antiprotons, which are nearly 2000 times as massive.

Heavier particles take wider paths when they spiral around the planet’s magnetic lines, and weaker magnetic field lines also lead to wider spirals. So relatively heavy antiprotons travelling around the weak field lines in the outer radiation belt were expected to take loops so big they would quickly get pulled into the lower atmosphere, where they would annihilate with normal matter. The inner belt was thought to have fields strong enough to trap antiprotons, and indeed that is where they have been found.

Piergiorgio Picozza from the University of Rome Tor Vergata, Italy, and colleagues detected the antiprotons using PAMELA, a cosmic-ray detector attached to a Russian Earth-observation satellite. The spacecraft flies through the Earth’s inner radiation belt over the south Atlantic.

Between July 2006 and December 2008, PAMELA detected 28 antiprotons trapped in spiralling orbits around the magnetic field lines sprouting from the Earth’s south pole. PAMELA samples only a small part of the inner radiation belt, but antiprotons are probably trapped throughout it. “We are talking about of billions of particles,” says team member Francesco Cafagna from the University of Bari in Italy.

Article source: http://www.aleph9.com/Research/?p=168

About a year and a half after her stroke, a 36-year-old professor started to feel sounds. A radio announcer’s voice made her tingle. Background noise in a plane felt physically uncomfortable.

Now Tony Ro, a neuroscientist at the City College of New York and the Graduate Center of the City University of New York, might have figured out the cause of this synesthesia. Sophisticated imaging of the woman’s brain revealed that new links had grown between its auditory part, which processes sound, and the somatosensory region, which handles touch.

“The auditory area of her brain started taking over the somatosensory area,” says Ro, who used diffusion tensor imaging, which focuses on the brain’s white matter connections, to spot the change.

This connection between sound and touch may run deep in the rest of us as well, Ro and colleagues said during presentations May 25 at a meeting of the Acoustical Society of America. Both hearing and touch, the scientists pointed out, rely on nerves set atwitter by vibration. A cellphone set to vibrate can be sensed by the skin of the hand, and the phone’s ringtone generates sound waves — vibrations of air — that move the eardrum.

Elizabeth Courtenay Wilson, a neuroscientist who did not attend the Seattle meeting, has also seen strong connections between areas of the brain that process hearing and touch. “We’re suggesting that the ear evolved out of the skin in order to do more finely tuned frequency analysis,” adds Wilson, of Beth Israel Deaconess Medical Center in Boston.

Wilson earned her Ph.D. in an MIT laboratory focused on studying whether vibrations could boost hearing aid performance. She published a series of papers showing that people with normal hearing were much better at detecting the combination of an extremely weak sound and an extremely weak vibration applied to the skin than either stimulus on its own.

Other researchers have shown that hearing a sound can boost touch sensitivity. Ro calls this the mosquito effect: The bug’s buzz makes our skin prickle. The frequency of the sound and the frequency of the vibrations our hands feel must match for this to work, according to a 2009 paper he published in Experimental Brain Research.

Frequency may be a two-way street in the brain that unites these two senses, says Jeffrey Yau, a neuroscientist at the Johns Hopkins University School of Medicine in Baltimore. A vibration that has a higher or lower frequency than a sound, he found, tends to skew pitch perception up or down. Sounds can also bias whether a vibration is perceived.

Article source: http://www.aleph9.com/Research/?p=165

Scientists at the University of Glasgow have, for the first time, been able to drag light by slowing it down to the speed of sound and sending it through a rotating crystal.
Most people may think the speed of light is constant, but this is only the case in a vacuum, such as space, where it travels at 671million mph.
However, when it travels through different substances, such as water or solids, its speed is reduced, with different wavelengths (colours) travelling at different speeds.
In addition, it has also been observed, but is not widely appreciated, that light can be dragged when it travels through a moving substance, such as glass, air or water – a phenomenon first predicted by Augustin-Jean Fresnel in 1818 and observed a hundred years later.
Prof. Miles Padgett in the Optics Group in the School of Physics Astronomy, said: “The speed of light is a constant only in vacuum . When light travels through glass, movement of the glass drags the light with it too.

“Spinning a window as fast as you could is predicted to rotate the image of the world behind it ever so slightly. This rotation would be about a millionth of a degree and imperceptible to the human eye.”

In research detailed in the latest edition of the journal Science (“Rotary Photon Drag Enhanced by a Slow-Light Medium”), researchers Dr Sonja Franke-Arnold, Dr Graham Gibson and Prof Padgett, in collaboration with their colleague Professor Robert Boyd at the Universities of Ottowa and Rochester, took a different approach and set up an experiment: shining a primitive image made up of the elliptical profile of a green laser through a ruby rod spinning on its axis at up to 3,000 rpm.

Once the light enters the ruby, its speed is slowed down to around the speed of sound (approximately 741mph) and the spinning motion of the rod drags the light with it, resulting in the image being rotated by almost five degrees: large enough to see with the naked eye.

Dr Franke-Arnold, who came up with the idea of using slow light in ruby to observe the photon drag, said: “We mainly wanted to demonstrate a fundamental optical principle, but this work has possible applications too.
“Images are information and the ability to store their intensity and phase is an important step to the optical storage and processing of quantum information, potentially achieving what no classical computer can ever match.
“The option to rotate an image by a set arbitrary angle presents a new way to code information, a possibility not accessed by any image coding protocol so far.”

Article source: http://www.aleph9.com/Research/?p=167


The Laboratory of Applied Bioacoustics (LAB), a unit of the Universitat Politècnica de Catalunya (UPC), directed by Professor Michel André, has recorded the sound of the earthquake that shook Japan on Friday, March 11. The recording, now available online, was provided by a network of underwater observatories belonging to the Japan Agency for Marine-Earth Science and Technology (JAMSTEC) and located on either side of the earthquake epicenter, close to the Japanese island of Hatsushima.

More on “Listening to the Deep Ocean Environment”:

The sea environment is filled with natural sounds, although increasingly many anthropogenic sources have contributed to the general noise budget of the oceans. The extent to which sound in the sea impacts and affects marine life is a topic of considerable current interest both to the scientific community and to the general public. Scientific interest arises from a need to understand more about the role of sound production and reception in the behaviour, physiology, and ecology of marine organisms and how anthropogenic sound, including sound necessary to study the marine environment, can interfere with the natural use of sound by marine organisms. Public interest concerns primarily the potential effects of anthropogenic sound on marine mammals, given the broad recognition of the importance of sound in the lives of these species. For acoustical oceanographers, marine seismologists, and minerals explorers, sound is the most powerful remote-sensing tool available to determine the geological structure of the seabed and to discover oil and gas reserves deep below the seafloor.

The scientific as well as the public’s interest in the impact of human-generated ocean noise on marine animals has greatly increased. Concerns include whether human-generated sounds may interfere with the normal use of sound by the marine animals or whether the human-generated sounds may cause the animals physical harm.

Many aquatic animals use sound for communication between members of their species. But equally important is the fact that all of these species probably also use sound to learn about their environment and to survive. Therefore, there should be concern not only about the effects of anthropogenic sounds on communication but also about the impact on general extraction of information from the environment. A fundamental question is whether the impact of anthropogenic sounds on marine mammals and the marine ecosystem is sufficiently important to warrant concern by both the scientific community and the public. The data currently available suggest that such interest is indeed justified.

Article source: http://www.aleph9.com/Research/?p=164

The two sides of the Moon look nothing like each other: the near side is flat and low, while the far side is incredibly mountainous. We may now be able to solve this topographical mystery…and it involves a second moon.

The current best theory for the origin of the Moon is the “giant impact” model. This holds that a Mars-sized object, sometimes called Theia, once shared Earth’s orbit and collided with it over four billion years ago, and the remains of this cataclysm ultimately formed into the Moon. Now it appears that that cosmic drama repeated itself in miniature with the Moon itself. Scientists are rather awesomely calling this “The Big Splat.”

It’s not just that the far side of the Moon is mountainous whereas the near side is flat – it actually has a substantially thicker crust than its lowland counterpart. That’s hard to explain if the Moon formed all at once, as the formation processes tend to even out such substantial irregularities. But planetary scientists at UC Santa Cruz propose a novel solution: what if the giant impact between Earth and Theia created not one, but two moons?

This second satellite would have been considerably smaller than the Moon we know today. It probably would have only been about 1/30 the mass of the Moon, which is still decently sized by the satellite standards (that’s a lot bigger than Mars’s moons, for instance). Both satellites would likely have shared the same orbit around Earth, with the second moon situated at one of the two Trojan points of stability relative to our Moon.

So how did the two collide? The second moon was able to remain stable in the early days of the Earth-Moon system, because the still forming larger Moon was initially much closer to Earth. As the initial chaos passed, the primary Moon moved out further into its current orbit. The second moon was no longer able to remain in a stable orbit, and it began a slow, gentle (collision?) with its larger companion – well, slow and gentle by the standards of two moons smashing into each other, that is.

Because the colliding object was moving at a relatively low velocity, crater formation and melting of the lunar surface was minimal. Instead, the entire second moon simple flattened and accumulated on one side of its former orbital partner, piling on tens of kilometers worth of new crust. This piling would not have been totally even, however, and that’s where you get the lunar highlands.

And it’s not just the elevation differences that this hypothesis accounts for. It also explains why the two sides of the Moon have such radically different compositions. The near side is rich in potassium, phosphorus, thorium, uranium, and various rare-earth elements, all of which were deposited on that side by the Moon’s primordial magma ocean. Now we know why they all ended up on side – the collision flattened the far side and pushed the resource-rich magma around to the other side of the satellite.

Indeed, the collision explains why there’s a far and near side at all. It made the Moon lopsided, causing the entire satellite to reorient itself so that the lighter side faced the Earth while the heavier side pointed away. All that said, there are still other possibilities to account for why the Moon is shaped the way it is. It’s possible that tidal forces could account for the Moon’s composition without invoking a second satellite.

Despite eons of mingling inside our cells, gene networks we’ve inherited from primitive, singled-celled ancestors have stayed separate. Our cells remain chimeras, a hybrid fusion of unrelated creatures.

The genes date from an event 1.5 billion years ago, when two kinds of simple cells, neither having a nucleus or cellular membrane, shacked up and created an entirely new form of life: eukaryotes.

While the two distinct communities of genes work together to keep cell machinery ticking, they otherwise stay out of each other’s hair, report biologists from the National University of Ireland.

“We humans, as part of the eukaryotes, we’re still a community of two prokaryotes,” said James McInerney, co-author of a study published in Genome Biology and Evolution, July 27.

While some scientists think prokaryotes evolved directly into eukaryotes, others think it required a merger, with two cells — one archaebacteria and one eubacteria — joining at some prehistoric point to make a cell capable of complex internal structures.

The merger led to an explosion of innovation. Suddenly cells could divide labor into ministructures, known as organelles, letting them specialize and grow larger. The extra biochemical whiz-bangery in eukaryotic cells makes lifeforms like orchids and dolphins possible.

“This idea is a hundred years old,” said McInerney. “But we wanted to ask, ‘If you have two types of organisms coming together to form a new kind of cell, do their metabolisms become completely blended together? What happens when genomes fuse?’”

To find out, McInerney and his colleague David Alvarez-Ponce surveyed the human genome and separated the genes into three groups based on taxonomic molecular signatures. One set contained genes inherited from our eubacterial ancestor, one from the archaebacterial ancestor and one held genes unique to eukaryotes. (Fingernail protein, for example, has no ancient doppelganger.)

Molecular tests showed that proteins coded by ancient parent cells still interact mostly with each other.

“They’ve found an imprint of this original symbiosis remaining after 1.5 billion years,” said Bill Martin, an endosymbiosis researcher at Heinrich-Heine-Universität Düsseldorf, in Germany and editor of the journal publishing the study. “This is a brilliant discovery. You would have thought someone would have noticed this, but nobody ever did.”

Beyond that, McInerney and Alvarez-Ponce found gene communities hold different functions. Archaebacterial genes are usually responsible for information processing, and appear to be especially important. They’ve accumulated fewer DNA mutations than eubacterial genes, suggesting that changes are more likely to have major consequences.

Eubacterial genes tended to be involved in biochemical processes. They were also more likely to be implicated in heritable human disease risk.

That more-important archaebacterial genes are found less frequently in disease might seem counterintuitive, but McInerney thinks the imbalance might exist because archaebacterial gene mutations often prevent organisms from developing at all.

Mutations to eubacterial biochemical process genes may cause problems, but organisms at least live long enough for disease to occur.

McInerney expects the study will cause a stir in the evolutionary biology community.

Jupiter is, quite literally, the biggest mystery in the solar system. But that will hopefully change after the launch of NASA’s Juno mission on Friday.

About 15 years ago, NASA’s Galileo mission revealed curious inconsistencies in the planet’s atmosphere. Models of the solar system suggest Jupiter formed near its current location, just outside the solar system’s “frost line”, a boundary beyond which water vapour condenses. Yet when Galileo launched a probe into the planet’s atmosphere in 1995, the probe found surprisingly little water.

Did the probe hit a rare dry spot on Jupiter? Or is all of Jupiter depleted in water? Juno will try to find out by searching the planet for water’s signature at six different microwave frequencies, which will reveal the molecule’s concentration from the top of the atmosphere to pressures of about 100 Earth-atmospheres. If the whole planet is dry, our very understanding of how and where objects came together in the solar system may need a rethink.

“Water is the key question that got this mission started,” says mission member Fran Bagenal of the University of Colorado, Boulder. “Not knowing where the water is in the solar system is a big deal. It puts a spanner in the works for solar system formation.”

The Juno spacecraft is a novel design. Three solar-panel wings, each about 9 metres long, will unfold after launch. The large panels are crucial because sunlight is only a few per cent as bright near Jupiter as it is on the Earth.

After its launch, Juno will travel for five years before slipping into an elongated, polar orbit around the planet that will dodge Jupiter’s deadly radiation belts. It will make 32 trips around Jupiter over a one-year period, skimming only 5000 kilometres above its cloud tops.

As it does so, it will glean data about the planet’s gravitational and magnetic fields, which could shed light on its internal structure, including whether it has a solid core. This is a mystery because no one knows what matter does at the extreme pressures inside such a massive body.

These pressures are estimated to be 50 million Earth atmospheres, says Bagenal: “Think of 100 elephants standing on top of each other with the bottom elephant standing on one foot – on a stiletto heel.”

See also: 6 Mysteries of Jupiter NASA’s New Spacecraft May Solve

The hybrids have been produced in secret over the past three years by researchers looking into possible cures for a wide range of diseases.

The revelation comes a day after a committee of scientists warned of a nightmare Planet of the Apes scenario in which work on human-animal creations goes too far.

Last night a campaigner against the excesses of medical research said he was disgusted that scientists were “dabbling in the grotesque”.

Figures seen by the Daily Mail show that 155 “admixed” embryos, containing both human and animal genetic material, have been created since the introduction of the 2008 Human Fertilisation Embryology Act.

This legalised the creation of a variety of hybrids, including an animal egg fertilised by a human sperm; “cybrids”, in which a human nucleus is implanted into an animal cell; and “chimeras”, in which human cells are mixed with animal embryos.

Scientists say the techniques can be used to develop embryonic stem cells which can be used to treat a range of incurable illnesses.

Wind is Japan’s strongest alternative to nuclear
Bye-bye electrons? Circuit made from flowing atoms
3D atomic imaging of nanoparticles — a new technique.
Liquid crystals could detect contaminated water
Deep inside the biggest storm we’ve ever seen on Saturn
‘Bizarre Bits’ Exhibition Took a Strange Turn When CDC arrived over Smallpox
Justices Ordered California To Reduce Amount Of Prisoners By 30,000
Milky Way Galaxy Has Mirrorlike Symmetry
Lockheed Martin buys first D-Wave quantum computing system
‘Nanowire’ Measurements Could Improve Computer Memory
World record in data transmission: 26 terabits per second on a single laser beam
First Cloned Cat Turns Ten Years Old
Scientists turn human skin cells directly into neurons
New battery design could give electric vehicles a jolt
The Rise of Predictive Policing: Police Using Statistics to Predict Crime
Toxin From Genetically Modified Crops Detected In Canadians’ Blood
Commuting is Making Us Fat and Miserable
Netizens speculate next target as hackers rule corporations world over
One in four US hackers ‘is an FBI informer’
Nazis Tried To Train Dogs To Read And Talk In Effort To Win WWII (See also: Operation Acoustic Kitty)
Milky Way faces midlife crisis
Who Owns the Advertising Space in an Augmented Reality World?
Tiny village is latest victim of the ‘The hum’
Wilhelm Reich comic.
Mulholland Drive inspires a Parisian club
Apollo 17 moon rocks are surprisingly wet
Scientists Create Tiny Artificial Brain That Exhibits 12 Seconds of Short Term Memory


A new survey is under way to search for signs of intelligent extraterrestrial life, but this one has a twist: Instead of listening for alien signals from anywhere in the sky, scientists are aiming radio telescopes at the alien planets most likely to be like our own Earth.

The new search, which began last week, is scanning 86 alien worlds for radio signals that could suggest the presence of an advanced civilization. The extrasolar planets are thought to be the most Earth-like of the 1,235 candidate planets discovered so far by NASA’s prolific Kepler space observatory.

“We’ve picked out the planets with nice temperatures — between zero and 100 degrees Celsius [32 and 212 degrees Fahrenheit] — because they are a lot more likely to harbor life,” said physicist Dan Werthimer of the University of California, Berkeley, in a statement.

This new SETI search is not part of the SETI Institute, which has long served as the Earth’s ears for any signals from intelligent aliens. Earlier this month, the Institute announced it was placing its primary listening station – a network of radio telescopes called the Allen Array — in hibernation due to funding problems.