Wednesday, 28 February 2018

The Lunar X (V)


The Lunar X (V)
The striking X in this lunarscape is easily visible in binoculars or a small telescope, but not too many have seen it. The catch is, this lunar X is fleeting and only apparent in the hours before the Moon's first quarter phase. Along the shadow line between lunar day and night, the X illusion is produced by a configuration of craters seen here toward the left, Blanchinus, La Caille and Purbach.

Near the Moon's first quarter phase, an astronaut standing close to the craters' position would see the slowly rising Sun very near the horizon. Temporarily, crater walls would be in sunlight while crater floors would still be in darkness. Seen from planet Earth, contrasting sections of bright walls against the dark floors by chance look remarkably like an X. This sharp image of the Lunar X was captured on February 22nd. For extra credit, sweep your gaze along the lunar terminator and you can also spot the Lunar V.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Henrik Adamsson

#space #nasa #universe #moon #science

Remembering Joe Polchinski the modest physicist who conceived a multiverse


Remembering Joe Polchinski the modest physicist who conceived a multiverse
Creativity and modesty are two of the qualities that made Joe Polchinski an extraordinary theoretical physicist. The early pioneer of string theory died this month at age 63.

Polchinski was an early pioneer of string theory, the mathematical apparatus picturing the basic particles of matter and force as supertiny wriggling strands of energy known as superstrings. His contributions to the field were immense. As a young professor at the University of Texas at Austin in the 1980s, he developed a branch of superstring theory involving objects called supermembranes.

Superstrings are one-dimensional objects (like lines, hence “strings”) vibrating like rubber bands in multidimensional space. (String math presupposed more dimensions than the usual three.) Polchinski explored the possibility that those multiple dimensions could contain two-dimensional membranes, kind of like the film forming the surface of a soap bubble. He and his students derived the math describing such supermembranes living in 11 dimensions (10 of space, one of time).

Maybe, string/brane/M theory would explain the amount of that mysterious “dark” energy in space and all would be well. But no. Working with physicist Raphael Bousso, Polchinski found that string theory did not specify how much energy the vacuum of space contained. Instead the theory predicted a virtually countless number of vacuum states, with nearly any amount of repulsive energy you could imagine. In other words, string theory described a multiverse.

Polchinski’s modesty manifested itself in his reaction to this situation. He hated the idea of a multiverse, because it implied that some questions had no answers that physicists could calculate. No equation could specify the amount of dark energy; it would just be luck — determined by which universe had the right amount of dark energy to make it hospitable to life (an idea known as the anthropic principle).

Interesting Article:
https://www.sciencenews.org/blog/context/remembering-joe-polchinski-modest-physicist-who-conceived-multiverse

#physics #JoePolchinski #stringtheory

Why Your Stomach Hurts After You Get Hit In the Balls?


Why Your Stomach Hurts After You Get Hit In the Balls?
When you take a shot to your scrotum, your testicles aren’t the only ones that feel the pain: Your stomach often joins in on it, too.

But why would an organ situated above the belt reel from a blow felt below it?
Your testicles actually developed in your abdomen near your kidneys. From there, they descended toward the scrotum, pulling the sensory nerves with them.

That means you have sensitive nerves that stretch from your stomach to your scrotum.

So when the nuts are hit or squeezed, the nerve sends a signal to the upper part of the belly, which is why it hurts in the stomach when you get kicked down there.

In addition to feeling vengeful, you might also feel dizzy, nauseous, or even vomit—all of which is to be expected.

It’s due to the vagal reflex, in which a nerve signal from your testicles travels up your spinal cord and brain stem and activates the nausea and vomiting centers in your brain.

Info:
https://www.msdmanuals.com/home/men-s-health-issues/biology-of-the-male-reproductive-system/structure-of-the-male-reproductive-system
https://blogs.scientificamerican.com/bering-in-mind/why-do-human-testicles-hang-like-that/
https://www.menshealth.com/health/stomach-pain-hit-in-balls

#medicine #biology #scrotum #pain

“I don’t know anything with certainty, but seeing the stars makes me dream.”


“I don’t know anything with certainty, but seeing the stars makes me dream.”
― Vincent Van Gogh

#wordsofwisdom #space #universe

Tuesday, 27 February 2018

NASA’s SDO Reveals How Magnetic Cage on the Sun Stopped Solar Eruption


NASA’s SDO Reveals How Magnetic Cage on the Sun Stopped Solar Eruption
New research highlights the role of the Sun’s magnetic landscape in the development of solar eruptions that can trigger space weather events around Earth.

Using data from our Solar Dynamics Observatory, scientists examined an October 2014 Jupiter-sized sunspot group, an area of complex magnetic fields, often the site of solar activity. This was the biggest group in the past two solar cycles and a highly active region. Though conditions seemed ripe for an eruption, the region never produced a major coronal mass ejection (CME) - a massive, bubble-shaped eruption of solar material and magnetic field - on its journey across the Sun. It did, however, emit a powerful X-class flare, the most intense class of flares. What determines, the scientists wondered, whether a flare is associated with a CME?

The scientists found that a magnetic cage physically prevented a CME from erupting that day. Just hours before the flare, the sunspot’s natural rotation contorted the magnetic rope and it grew increasingly twisted and unstable, like a tightly coiled rubber band.

Credits: Tahar Amari et al./Center for Theoretical Physics/École Polytechnique/NASA Goddard/Joy Ng
https://www.nasa.gov/feature/goddard/2018/nasa-s-sdo-reveals-how-magnetic-cage-on-the-sun-stopped-solar-eruption

#space #sun #NASA #science #universe #solarflare #solarsystem

Sacred knowledge of the cosmos seems to be hidden within our souls and is shown within our artwork and creative...


Sacred knowledge of the cosmos seems to be hidden within our souls and is shown within our artwork and creative expressions.
N. Shiva

Work by bigblueboo
https://twitter.com/bigblueboo

#math #geometry #processing #science

Nutrition has benefits for brain network organization


Nutrition has benefits for brain network organization
Nutrition has been linked to cognitive performance, but researchers have not pinpointed what underlies the connection. A new study by University of Illinois researchers found that monounsaturated fatty acids – a class of nutrients found in olive oils, nuts and avocados – are linked to general intelligence, and that this relationship is driven by the correlation between MUFAs and the organization of the brain’s attention network.

The study of 99 healthy older adults, recruited through Carle Foundation Hospital in Urbana, compared patterns of fatty acid nutrients found in blood samples, functional MRI data that measured the efficiency of brain networks, and results of a general intelligence test. The study was published in the journal NeuroImage.

“Our goal is to understand how nutrition might be used to support cognitive performance and to study the ways in which nutrition may influence the functional organization of the human brain,” said study leader Aron Barbey, a professor of psychology. “This is important because if we want to develop nutritional interventions that are effective at enhancing cognitive performance, we need to understand the ways that these nutrients influence brain function.”

Source & further reading:
https://news.illinois.edu/view/6367/552515#image-1

Journal article:
https://www.ncbi.nlm.nih.gov/pubmed/28821393

#nutrition #fattyacids #functionalconnectivity #intelligence #brainfunction #neuroscience #research

Sunday, 25 February 2018

One small flare


One small flare
The sun's only visible active region sputtered and spurted and eventually unleashed a small (C-class) flare (Feb. 7, 2018). The flare appears as a brief, bright flash about mid-way through the half-day clip. These images were taken in a wavelength of extreme ultraviolet light.

Source:
https://sdo.gsfc.nasa.gov/gallery/potw/item/876
Credit: Solar Dynamics Observatory, NASA.

#universe #sun #SDO #NASA #science #space

Experiments support theory of cosmic magnetic field growth


Experiments support theory of cosmic magnetic field growth
Researchers have measured the amplification of a magnetic field in a turbulent laboratory plasma, providing the first physical demonstration of a mechanism that is thought to enhance fields in galaxies and galaxy clusters.

Source & further reading:
http://physicstoday.scitation.org/do/10.1063/PT.6.1.20180222a/full/

#physics #plasma #science #magneticfield #space

Wednesday, 21 February 2018

When roses aren't red


When roses aren't red
Not all roses are red of course, but they can still be very pretty. Likewise, the beautiful Rosette Nebula and other star forming regions are often shown in astronomical images with a predominately red hue, in part because the dominant emission in the nebula is from hydrogen atoms.

Hydrogen's strongest optical emission line, known as H-alpha, is in the red region of the spectrum, but the beauty of an emission nebula need not be appreciated in red light alone. Other atoms in the nebula are also excited by energetic starlight and produce narrow emission lines as well. In this gorgeous view of the Rosette Nebula, narrowband images are combined to show emission from sulfur atoms in red, hydrogen in blue, and oxygen in green.

In fact, the scheme of mapping these narrow atomic emission lines into broader colors is adopted in many Hubble images of stellar nurseries. The image spans about 100 light-years in the constellation Monoceros, at the 3,000 light-year estimated distance of the Rosette Nebula. To make the Rosette red, just follow this link or slide your cursor over the image.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Eric Coles and Mel Helm

#NASA #space #science #nebula

Tuesday, 20 February 2018

Jupiter in Infrared from Hubble


Jupiter in Infrared from Hubble
Jupiter looks a bit different in infrared light. To better understand Jupiter's cloud motions and to help NASA's robotic Juno spacecraft understand the Hubble Space Telescope is being directed to regularly image the entire Jovian giant. The colors of Jupiter being monitored go beyond the normal human visual range to include both ultraviolet and infrared light.

Featured here in 2016, three bands of near-infrared light have been digitally reassigned into a mapped color image. Jupiter appears different in infrared partly because the amount of sunlight reflected back is distinct, giving differing cloud heights and latitudes discrepant brightnesess. Nevertheless, many familiar features on Jupiter remain, including the light zones and dark belts that circle the planet near the equator, the Great Red Spot on the lower left, and the string-of-pearls storm systems south of the Great Red Spot.

The poles glow because high altitude haze there is energized by charged particles from Jupiter's magnetosphere. Juno has now completed 10 of 12 planned science orbits of Jupiter and continues to record data that are helping humanity to understand not only Jupiter's weather but what lies beneath Jupiter's thick clouds.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: NASA, ESA, Hubble;
Data: Michael Wong (UC Berkeley) et al.;
Processing & License: Judy Schmidt

#nasa #space #Jupiter #science #Juno #Hubble

King Tut's Sandals (gold and leather)


King Tut's Sandals (gold and leather)

Egyptian Museum, Cairo
http://www.aucegypt.edu/photo-gallery-shoes-ancient-egypt

#history #KingTut #Egypt

George Berkeley & Immaterialism


George Berkeley & Immaterialism
George Berkeley (1685-1753) is best known for his contention that the physical world is nothing but a compilation of ideas. This is represented by his famous aphorism esse est percipi (“to be is to be perceived”). His work predominantly includes idealism and immaterialism, but he also worked on visual perception, ethics, economics, and many other areas of academia.

Here are five facts you might not have known about Berkeley:
1.George Berkeley and his wife Anne donated their farm and almost a thousand books to Yale University upon leaving America in 1731 after the Bermuda Project didn’t go ahead.

2.Of the twelve years Berkeley had a fellowship at Trinity College, he only spent 3 years actually in Dublin.

3.Berkeley had a life-long friendship with Thomas Prior, an Irish author and founder of the Royal Dublin Society.

4.Berkeley’s three most important and famous works were all written and well established before he was 30 years old.

5.Whitehall, the house in Rhode Island which Berkeley built and inhabited with his family during his time in America, is still preserved and is now a museum on the philosopher.

References:
http://www.philosophypages.com/hy/4r.htm
https://plato.stanford.edu/entries/berkeley/

#history #GeorgeBerkeley #Immaterialism

Monday, 19 February 2018

A circle is the reflection of eternity.


A circle is the reflection of eternity. It has no beginning and it has no end and if you put several circles over each other, then you get a spiral.
~M.J. Keenan

Work by dvdp
https://www.instagram.com/dvdp/

#math #processing #animation

Thursday, 15 February 2018

Eating Triggers Endorphin Release in the Brain


Eating Triggers Endorphin Release in the Brain
The recent results obtained by researchers from Turku PET Centre have revealed that eating leads to widespread opioid release in the brain, likely signaling feelings of satiety and pleasure.

Eating a delicious pizza led to significant increase of pleasant feelings, whereas consumption of calorie-matched nutritional drink did not. However, both types of meals induced significant release of endogenous opioids in the brain.

Opioids are associated with pleasure and euphoria. The study revealed that a significant amount of endorphins is released in the entire brain after eating the pizza and, surprisingly, even more are released after the consumption of the tasteless nutritional drink. The magnitude of the opioid release was independent of the pleasure associated with eating. According to the researchers, it is likely that the endogenous opioid system regulates both feelings of pleasure and satiety.

– The opioid system regulates eating and appetite, and we have previously found that its dysfunctions are a hallmark of morbid obesity. The present results suggest that overeating may continuously overstimulate the opioid system, thus directly contributing to development of obesity. These findings open new opportunities for treating overeating and the development of obesity, says Professor Lauri Nummenmaa from Turku PET Centre.

– It was a surprise that endorphins are released in the entire brain and that the nutritional drink had a larger impact. This creates a basis for future research and hopefully we will find ways to study and describe the development and predictors of addiction, obesity and eating disorders, says Researcher, M.D., PhD. Jetro Tuulari.

The study was conducted using positron emission tomography (PET). The participants were injected with a radioactive compound binding to their brain’s opioid receptors. Radioactivity in the brain was measured three times with the PET camera: after a palatable meal (pizza), after a non-palatable meal (liquid meal) and after an overnight fast.

Source:
https://www.utu.fi/en/news/news/Pages/Eating-Triggers-Endorphin-Release-in-the-Brain.aspx

Journal article:
http://www.jneurosci.org/content/37/34/8284

Image: Feeding both bland (left panel) and delicious (right panel) meals triggered significant opioid release in the brain.

MR
Photos: StockSnap, Turku PET Centre

#opioids #eating #endorphins #appetite #obesity #neuroscience
#research

Comet PanSTARRS is near the Edge


Comet PanSTARRS is near the Edge
The comet PanSTARRS, also known as the blue comet (C/2016 R2), really is near the lower left edge of this stunning, wide field view recorded on January 13. Spanning nearly 20 degrees on the sky, the cosmic landscape is explored by well-exposed and processed frames from a sensitive digital camera. It consists of colorful clouds and dusty dark nebulae otherwise too faint for your eye to see, though.

At top right, the California Nebula (aka NGC 1499) does have a familiar shape. Its coastline is over 60 light-years long and lies some 1,500 light-years away. The nebula's pronounced reddish glow is from hydrogen atoms ionized by luminous blue star Xi Persei just below it. Near bottom center, the famous Pleiades star cluster is some 400 light-years distant and around 15 light-years across.

Its spectacular blue color is due to the reflection of starlight by interstellar dust. In between are hot stars of the Perseus OB2 association and dusty, dark nebulae along the edge of the nearby, massive Taurus and Perseus molecular clouds. Emission from unusually abundant ionized carbon monoxide (CO+) molecules fluorescing in sunlight is largely responsible for the telltale blue tint of the remarkable comet's tail. The comet was about 17 light minutes from Earth.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: JoAnn McDonald

#universe #space #NASA #comet

Tuesday, 13 February 2018

In the Heart of the Heart Nebula


In the Heart of the Heart Nebula
What's that inside the Heart Nebula? First, the large emission nebula dubbed IC 1805 looks, in whole, like a human heart. It's shape perhaps fitting of the Valentine's Day, this heart glows brightly in red light emitted by its most prominent element: hydrogen.

The red glow and the larger shape are all created by a small group of stars near the nebula's center. In the heart of the Heart Nebula are young stars from the open star cluster Melotte 15 that are eroding away several picturesque dust pillars with their energetic light and winds.

The open cluster of stars contains a few bright stars nearly 50 times the mass of our Sun, many dim stars only a fraction of the mass of our Sun, and an absent microquasar that was expelled millions of years ago. The Heart Nebula is located about 7,500 light years away toward the constellation of the mythological Queen of Aethiopia (Cassiopeia).

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Credit & Copyright: Alan Erickson

#space #NASA #nebula #science #universe

Research sheds new light on the link between gut bacteria and anxiety


Research sheds new light on the link between gut bacteria and anxiety
Research published in the open access journal Microbiome sheds new light on how gut bacteria may influence anxiety-like behaviors. Investigating the link between gut bacteria and biological molecules called microRNAs (miRNAs) in the brain; researchers at the APC Microbiome Institute at University College Cork, which is funded by Science Foundation Ireland, found that a significant number of miRNAs were changed in the brains of microbe-free mice. These mice are reared in a germ-free bubble and typically display abnormal anxiety, deficits in sociability and cognition, and increased depressive-like behaviors.

Dr Gerard Clarke, the corresponding author said: “Gut microbes seem to influence miRNAs in the amygdala and the prefrontal cortex. This is important because these miRNAs may affect physiological processes that are fundamental to the functioning of the central nervous system and in brain regions, such as the amygdala and prefrontal cortex, which are heavily implicated in anxiety and depression.”

miRNAs are short sequences of nucleotides (the building blocks of DNA and RNA), which can act to control how genes are expressed. miRNA dysregulation or dysfunction is believed to be an underlying factor contributing to stress-related psychiatric disorders, neurodegenerative diseases and neurodevelopmental abnormalities. miRNA changes in the brain have been implicated in anxiety-like behaviors.

Dr Clarke said: “It may be possible to modulate miRNAs in the brain for the treatment of psychiatric disorders but research in this area has faced several challenges, for example, finding safe and biologically stable compounds that are able to cross the blood-brain barrier and then act at the desired location in the brain. Our study suggests that some of the hurdles that stand in the way of exploiting the therapeutic potential of miRNAs could be cleared by instead targeting the gut microbiome.”

The researchers found that levels of 103 miRNAs were different in the amygdala and 31 in the prefrontal cortex of mice reared without gut bacteria (GF mice) compared to conventional mice. Adding back the gut microbiome later in life normalized some of the changes to miRNAs in the brain.

The findings suggest that a healthy microbiome is necessary for appropriate regulation of miRNAs in these brain regions. Previous research demonstrated that manipulation of the gut microbiome affects anxiety-like behaviors but this is the first time that the gut microbiome has been linked to miRNAs in both the amygdala and prefrontal cortex, according to the authors.

The researchers used next-generation-sequencing (NGS) to find out which miRNAs were present in the amygdala and the prefrontal cortex of groups of 10-12 control mice with a normal gut microbiota, GF mice and ex-GF mice – which had been colonized with bacteria by housing them with the control mice – and adult rats whose normal microbiota had been depleted with antibiotics.

They found that depleting the microbiota of adult rats with antibiotics impacted some miRNAs in the brain in a similar way to the GF mice. This suggests that even if a healthy microbiota is present in early life, subsequent changes in adulthood can impact miRNAs in the brain relevant to anxiety-like behaviors, according to the authors.

The authors note that the exact mechanism by which the gut microbiota is able to influence the miRNAs in the brain remains unclear. Even though the study shows that effects of the microbiota on miRNAs are present in more than one species (mice and rats), further research into the possible connection between gut bacteria, miRNAs and anxiety-like behaviors is needed before the findings can be translated to a clinical setting.

Dr Clarke said: “This is early stage research but the possibility of achieving the desired impact on miRNAs in specific brain regions by targeting the gut microbiota – for example by using psychobiotics – is an appealing prospect.”

Source:
https://www.biomedcentral.com/about/press-centre/science-press-releases/25-08-17

Journal article:
https://microbiomejournal.biomedcentral.com/articles/10.1186/s40168-017-0321-3

#infopraphic via The Huffington Post

#gutbacteria #miRNAs #gutmicrobiota #anxiety #prefrontalcortex #amygdala #neuroscience

Thursday, 8 February 2018

Total Solar Lunar Eclipse


Total Solar Lunar Eclipse
This digitally processed and composited picture creatively compares two famous eclipses in one; the total lunar eclipse (left) of January 31, and the total solar eclipse of August 21, 2017. The Moon appears near mid-totality in both the back-to-back total eclipses. In the lunar eclipse, its surface remains faintly illuminated in Earth's dark reddened shadow. But in the solar eclipse the Moon is in silhouette against the Sun's bright disk, where the otherwise dark lunar surface is just visible due to earthshine.

Also seen in the lunar-aligned image pair are faint stars in the night sky surrounding the eclipsed Moon. Stunning details of prominences and coronal streamers surround the eclipsed Sun. The total phase of the Great American Eclipse of August 21 lasted about 2 minutes or less for locations along the Moon's shadow path. From planet Earth's night side, totality for the Super Blue Blood Moon of January 31 lasted well over an hour.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Composite Image Credit & Copyright: Wang Letian, Zhang Jiajie

#universe #space #NASA #lunareclipse #science

Tuesday, 6 February 2018

Elon Musk's Falcon Heavy rocket launches successfully


Elon Musk's Falcon Heavy rocket launches successfully
The launch of this turbocharged version of the workhorse Falcon 9 rocket, which has been carrying cargo to space for years, marks an important milestone in spaceflight, the first time a rocket this powerful has been sent into space by a private company rather than a government space agency.

The rocket carried a playful payload: Mr. Musk’s red Roadster, an electric sports car built by his other company, Tesla. Strapped inside the car is a mannequin wearing one of SpaceX’s spacesuits. They are expected to orbit the sun for hundreds of millions of years.

With the ability to lift into orbit nearly 64 metric tons (141,000 lb)---a mass greater than a 737 jetliner loaded with passengers, crew, luggage and fuel--Falcon Heavy can lift more than twice the payload of the next closest operational vehicle, the Delta IV Heavy, at one-third the cost. Falcon Heavy draws upon the proven heritage and reliability of Falcon 9.

Its first stage is composed of three Falcon 9 nine-engine cores whose 27 Merlin engines together generate more than 5 million pounds of thrust at liftoff, equal to approximately eighteen 747 aircraft. Only the Saturn V moon rocket, last flown in 1973, delivered more payload to orbit. Falcon Heavy was designed from the outset to carry humans into space and restores the possibility of flying missions with crew to the Moon or Mars.

Article:
https://www.nytimes.com/2018/02/06/science/falcon-heavy-spacex-launch.html

Reference:
http://www.spacex.com/falcon-heavy

#space #SPACEX #FalconHeavy #universe #science

NGC 7331 Close-Up


NGC 7331 Close-Up
Big, beautiful spiral galaxy NGC 7331 is often touted as an analog to our own Milky Way. About 50 million light-years distant in the northern constellation Pegasus, NGC 7331 was recognized early on as a spiral nebula and is actually one of the brighter galaxies not included in Charles Messier's famous 18th century catalog.

Since the galaxy's disk is inclined to our line-of-sight, long telescopic exposures often result in an image that evokes a strong sense of depth. In this Hubble Space Telescope close-up, the galaxy's magnificent spiral arms feature dark obscuring dust lanes, bright bluish clusters of massive young stars, and the telltale reddish glow of active star forming regions. The bright yellowish central regions harbor populations of older, cooler stars. Like the Milky Way, a supermassive black hole lies at the core of of spiral galaxy NGC 7331.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & License: ESA/Hubble & NASA/D. Milisavljevic (Purdue University)

#space #nasa #universe #galaxies #science

Magnetic coil springs accelerate particles on the Sun

Magnetic coil springs accelerate particles on the Sun
In April and July 2014, the Sun emitted three jets of energetic particles into space, that were quite exceptional: the particle flows contained such high amounts of iron and helium-3, a rare variety of helium, as have been observed only few times before.

Since these extraordinary events occurred on the backside of our star, they were not discovered immediately. A group of researchers headed by the Max Planck Institute for Solar System Research (MPS) and the Institute for Astrophysics of the University of Göttingen (Germany) present a comprehensive analysis now in the Astrophysical Journal.

Source & further reading:
https://www.mps.mpg.de/Magnetic-coil-springs-accelerate-particles-on-the-Sun

Journal article:
http://iopscience.iop.org/article/10.3847/1538-4357/aa9d8f

#heliophysics #sun #solarphysics #astrophysics #science #universe

Toronto women learning how to shoot at the Long Branch training camp, 1915.


Toronto women learning how to shoot at the Long Branch training camp, 1915.

Article:
http://nationalpost.com/news/canada/hundreds-of-toronto-women-learned-military-drills-to-defend-the-home-front-during-first-world-war

#history #women #WWI

Adult brains produce new cells in previously undiscovered area


Adult brains produce new cells in previously undiscovered area
A University of Queensland discovery may lead to new treatments for anxiety, depression and post-traumatic stress disorder (PTSD).

UQ Queensland Brain Institute scientists have discovered that new brain cells are produced in the adult amygdala, a region of the brain important for processing emotional memories.
Disrupted connections in the amygdala, an ancient part of the brain, are linked to anxiety disorders such as PTSD.

Queensland Brain Institute director Professor Pankaj Sah said the research marked a major shift in understanding the brain’s ability to adapt and regenerate.

“While it was previously known that new neurons are produced in the adult brain, excitingly this is the first time that new cells have been discovered in the amygdala,” Professor Sah said.

“Our discovery has enormous implications for understanding the amygdala’s role in regulating fear and fearful memories.”

Researcher Dr Dhanisha Jhaveri said the amygdala played a key role in fear learning – the process by which we associate a stimulus with a frightening event. “Fear learning leads to the classic flight or fight response – increased heart rate, dry mouth, sweaty palms – but the amygdala also plays a role in producing feelings of dread and despair, in the case of phobias or PTSD, for example,” Dr Jhaveri said.

“Finding ways of stimulating the production of new brain cells in the amygdala could give us new avenues for treating disorders of fear processing, which include anxiety, PTSD and depression.”

Previously new brain cells in adults were only known to be produced in the hippocampus, a brain region important for spatial learning and memory.
The discovery of that process, called neurogenesis, was made by Queensland Brain Institute founding director Professor Perry Bartlett, who was also involved in the latest research.

“Professor Bartlett’s discovery overturned the belief at the time that the adult brain was fixed and unable to change,” Professor Sah said.

“We have now found stem cells in the amygdala in adult mice, which suggests that neurogenesis occurs in both the hippocampus and the amygdala.

“The discovery deepens our understanding of brain plasticity and provides the framework for understanding the functional contribution of new neurons in the amygdala,” Professor Sah said.

The research, led by Professor Sah, Professor Bartlett and Dr Jhaveri, is published in Molecular Psychiatry.

Journal article:
http://www.nature.com/articles/mp2017134?WT.feed_name=subjects_biological-sciences

Source:
https://www.uq.edu.au/news/article/2017/08/adult-brains-produce-new-cells-previously-undiscovered-area

#anxiety #PTSD #amygdala #neurogenesis #interneurons #neuroscience

Sunday, 4 February 2018

The haboobs are giant walls of dust created from high winds rushing out of a collapsing thunderstorm.


The haboobs are giant walls of dust created from high winds rushing out of a collapsing thunderstorm. The name comes from the Arabic habb, meaning 'wind' or 'to blow'.

Cold air in front of the storm rushes down at an incredible rate, picking up massive amounts of dust and sand and blowing them into the air.
As the dust storm builds, it can completely block out the sun, making it nearly impossible to see just a few feet in front of you.

A haboob storm-front may transport and deposit large quantities of sand or dust material, which move as an extremely dense wall that can reach a height of 1000 metres (about 3,000 feet). Haboobs occur regularly in arid regions throughout the world.

Reference:
https://www.weatheronline.co.uk/reports/wind/Haboob.htm

#naturalphenomena #haboob #sandstorm

Friday, 2 February 2018

Circular RNA linked to brain function


Circular RNA linked to brain function
Last year, scientists have shown that circular RNA is linked to brain function. When a RNA molecule called Cdr1as was deleted from the genome of mice, the animals had problems filtering out unnecessary information – like patients suffering from neuropsychiatric disorders.

While hundreds of circular RNAs (circRNAs) are abundant in mammalian brains, one big question has remained unanswered: What are they actually good for? In the September issue of Science, Nikolaus Rajewsky and his team at the Berlin Institute of Medical Systems Biology (BIMSB) of the Max Delbrück Center for Molecular Medicine in the Helmholtz Association (MDC), as well as other collaborators within the MDC and Charité, present data that – for the first time – link a circular RNA to brain function.

RNA is much more than the mundane messenger between DNA and the protein it encodes. Indeed, there are several different kinds of non-coding RNA molecules. They can be long non-coding RNAs (lncRNAs) or short regulatory RNAs (miRs); they can interfere with protein production (siRNAs) or help make it possible (tRNAs). In the past 20 years, scientists have discovered some two dozen RNA varieties that form intricate networks within the molecular microcosm.

The most enigmatic among them are circRNAs, an unusual class of RNAs whose heads are connected to their tails to form a covalently closed ring. These structures had for decades been dismissed as a rare, exotic RNA species. In fact, the opposite is true. Current RNA-sequencing analyses have revealed that they are a large class of RNA, which is highly expressed in brain tissues.

Thousands of circular RNAs exist in nematode worms, mice and humans
In 2013, two pioneering studies that characterized circular RNAs appeared in the journal Nature, one of them by Nikolaus Rajewsky and his team. Intriguingly, most circular RNAs are unusually stable, floating in the cytoplasm for hours and even days on end. The systems biologists proposed that – at least sometimes – circRNAs serve gene regulation.

Cdr1as, a large single-stranded RNA loop that is 1,500 nucleotides around, might act as a “sponge” for microRNAs. For example, it offers more than 70 binding sites for a microRNA called miR-7. MicroRNAs are short RNA molecules that typically bind to complementary sequences in messenger RNAs, thereby controlling the amounts of specific proteins produced by cells.

Additionally, Rajewsky and his collaborators mined databases and discovered thousands of different circRNAs in nematode worms, mice and humans. Most of them were highly conserved throughout evolution. “We had found a parallel universe of unexplored RNAs,” says Rajewsky. “Since publication the field has exploded; hundreds of new studies have been carried out.”

Understanding a circle that is mostly present in excitatory neurons
For the current paper in Science, the systems biologists teamed up with Carmen Birchmeier’s lab at the MDC to reconsider Cdr1as. “This particular circle can be found in excitatory neurons but not in glial cells,” says Monika Piwecka, one of the first authors of the paper and coordinator of most of the experiments.

“In brain tissues of mice and humans, there are two microRNAs called miR-7 and miR-671 that bind to it.” In a next step, Rajewsky and his collaborators selectively deleted the circRNA Cdr1as in mice using the genome editing technology CRISPR/Cas9. In these animals, the expression of most microRNAs in four studied brain regions remained unperturbed. However, miR-7 was downregulated and miR-671 upregulated. These changes were post-transcriptional, consistent with the idea that Cdr1as usually interacts with these microRNAs in the cytoplasm.

“This indicates that Cdr1as usually stabilizes or transports miR-7 in neurons by sponging them up, while miR-167 might serve to regulate levels of this particular circular RNA,” says Rajewsky. If microRNA floated in the cytoplasm without binding anywhere, it would get broken down as waste. The circle would prevent that and also carry it to new places like the synapses. He adds: “Maybe we should think about Cdr1as not as a ‘sponge’ but as a ‘boat.’ It prevents its passengers from drowning and also moves on to new ports.”

The changes in microRNA concentration had dramatic effects on the mRNA and proteins produced by nerve cells, especially for a group called “immediate early genes.” They are part of the first wave of responses when stimuli are presented to neurons. Also affected were messenger RNAs that encode proteins involved in the maintenance of the animals’ sleep-wake cycles.

Cdr1as modulates synaptic responses
Using single-cell electrophysiology, Charité-researcher Christian Rosenmund observed that spontaneous vesicle release at the synapse happened twice as often. The synaptic responses to two consecutive stimuli were also altered. Additional behavioral analyses performed at the MDC mirrored these findings. Even though the mice appeared normal in many ways, they were unable to tune down their responses to external signals such as noises. Similar disruptions in pre-pulse inhibition have been noted in patients suffering from schizophrenia or other psychiatric diseases.

It is an everyday experience how much we depend on this filtering function: When a loud noise suddenly disturbs the quiet atmosphere of a library, you cannot avoid being alarmed. The same bang, however, will seem much less threatening next to a construction site. In this instance, the brain has had the chance to process previous noises and filter out unnecessary information. Therefore, the startle reflex is dampened (pre-pulse inhibition). This basic brain function that allows healthy animals and people to temporarily adapt to a strong stimulus and avoid information overload has now been linked to Cdr1as.

“Functionally, our data suggest that Cdr1as and its direct interactions with microRNAs are important for sensorimotor gating and synaptic transmission,” says Nikolaus Rajewsky. “More generally, since the brain is an organ with exceptionally high and diverse expression of circular RNAs, we believe that our data suggest the existence of a previously unknown layer of biological functions carried out by these circles.”

Source:
https://insights.mdc-berlin.de/en/2017/08/circular-rna-linked-brain-function/

Journal article:
http://science.sciencemag.org/content/early/2017/08/09/science.aam8526

#Cdr1as #circRNAs #brainfunction #microRNA #neuroscience #research

Folding...your mind


Folding...your mind

Work by Charlie Deck
http://bigblueboo.com/

#math #processing #digitalart #geometry #science

Jean-Jacques Rousseau (1712-1778)


Jean-Jacques Rousseau (1712-1778)
Rousseau was a Swiss writer and philosopher. He is considered one of the most important figures for his contribution to modern European intellectual history and political philosophy. He is best known for Social Contract (1762) with its famous opening line: ‘Man is born free, but is everywhere in chains’. His books have attracted both admiration and hostility during his lifetime and exerted profound influence on French revolutionaries, his contemporaries and later thinkers such as Kant, Hume, Wollstonecraft, Hegel, and Marx.

Here are 5 interesting facts about Jean-Jacques Rousseau you might not know:
1. After his father’s exile to avoid arrest for political reason, Rousseau left Geneva, the city of his birth at the age of sixteen and served as a domestic servant in a noble household of Madam de Warens in 1728. He later found a new home in Chambéry with Madame de Warens and remained with her throughout 1730s, during which time, he taught himself philosophy and literature. She became for him his mentor, surrogate mother and lover.

2. Whilst in Paris during 1744, before he was famous, Rousseau contributed various articles on music and political economy to the Encyclopédie of Denis Diderot and d’Alembert, an encyclopedia representing Enlightenment thoughts. He also composed the successful opera, Le Devin du Village for a court production in 1752.

3. In 1749 Rousseau came across a newspaper announcement of the Academy of Dijon’s essay competition. The question asked whether the development of arts and sciences had improved mankinds. Rousseau wrote Discourse on the Arts and Sciences in response and won the first prize with a counter thesis that civilization had fostered moral corruptions. He wrote the Second Discourse, continuing the theme of social inequality.

4. On their publications in France and Geneva in 1762, The Social Contract, Rousseau’s most famous work on political philosophy, and Emile, his treatise on education, were condemned as subversive and met with outrage. The Genevan authorities ordered the burning of his books on account of Emile’s blasphemous views on religions. For many years throughout 1760s, Rousseau had to flee to escape arrest, seeking refuge in Switzerland, and England, and French provinces under an assumed name.

5. Towards the end of his writing career, Rousseau composed more personal and introspective works. He wrote the extraordinary and candid autobiography Confessions while in exile. In 1770, he wrote Reveries of the Solitary Walker which became a seminal text in its development of Romantic sensibilities.

References:
https://www.iep.utm.edu/rousseau/
https://plato.stanford.edu/entries/rousseau/

#history #science #philosophy