Tuesday, 30 January 2018

The First Explorer


The First Explorer
Sixty years ago, on January 31, 1958, the First Explorer was successfully launched by the Army Ballistic Missile Agency on a Jupiter-C rocket. Inaugurating the era of space exploration for the United States, Explorer I was a thirty pound satellite that carried instruments to measure temperatures, and micrometeorite impacts, along with an experiment designed by James A. Van Allen to measure the density of electrons and ions in space.

The measurements made by Van Allen's experiment led to an unexpected and then startling discovery of two earth-encircling belts of high energy electrons and ions trapped in the magnetosphere. Now known as the Van Allen Radiation belts, the regions are located in the inner magnetosphere, beyond low Earth orbit. Explorer I ceased transmitting on February 28, 1958, but remained in orbit until March of 1970.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: NASA

#universe #space #science #ExplorerI #NASA

Kids & War


Kids & War
Lepa Svetozara Radić, was a Bosnian Serb member of the Yugoslav Partisans who was posthumously awarded the Order of the People’s Hero on 20 December 1951, for her role in the resistance movement against the Axis powers—becoming the youngest recipient at the time.

She was executed in February 1943 at the age of 17 for shooting at German troops during World War II. As her captors tied the noose around her neck, they offered her a way out of the gallows by revealing her comrades’ and leaders’ identities. She responded that she was not a traitor and that they would reveal themselves when they avenged her death.

https://ww2gravestone.com/lepa-svetozara-radic-young-hero/

#history #warkids #WWII #LepaRadic

Brain Scan Study Adds to Evidence That Lower Brain Serotonin Levels are Linked to Dementia


Brain Scan Study Adds to Evidence That Lower Brain Serotonin Levels are Linked to Dementia
In a study looking at brain scans of people with mild loss of thought and memory ability, Johns Hopkins researchers report evidence of lower levels of the serotonin transporter — a natural brain chemical that regulates mood, sleep and appetite.

Previous studies from Johns Hopkins and other centers have shown that people with Alzheimer’s disease and severe cognitive decline have severe loss of serotonin neurons, but the studies did not show whether those reductions were a cause or effect of the disease. Results of the new study of people with very early signs of memory decline, the researchers say, suggest that lower serotonin transporters may be drivers of the disease rather than a byproduct.

A report on the study, published in the September issue of Neurobiology of Disease, also suggest that finding ways to prevent the loss of serotonin or introducing a substitute neurotransmitter could slow or stop the progression of Alzheimer’s disease and perhaps other dementias.

“Now that we have more evidence that serotonin is a chemical that appears affected early in cognitive decline, we suspect that increasing serotonin function in the brain could prevent memory loss from getting worse and slow disease progression,” says Gwenn Smith, Ph.D., professor of psychiatry and behavioral sciences at the Johns Hopkins University School of Medicine and director of geriatric psychiatry and neuropsychiatry at Johns Hopkins University School of Medicine.

Serotonin levels that are lower and out of balance with other brain chemicals such as dopamine are well known to significantly impact mood, particularly depression, and drugs that block the brain’s “reuptake” of serotonin (known as SSRIs) are specific treatments for some major forms of depression and anxiety.

Smith notes that researchers have tried with limited success to treat Alzheimer’s disease and cognitive impairment with antidepressants such as SSRIs, which bind to the serotonin transporters. But, since these transporters are at much lower levels in people with Alzheimer’s, she speculates that the drugs can’t serve their purpose without their target.

The idea for Smith’s study was inspired by the work of co-author Alena Savonenko, M.D., Ph.D., associate professor of pathology, and her colleagues who showed that loss of serotonin neurons was associated with more protein clumps, or amyloid, in mouse brain.

To further study serotonin’s role in cognition and neurodegenerative disease, the Johns Hopkins research team used brain positron emission tomography (PET) scans to look at levels of serotonin in the brains of people with mild cognitive problems, which may be early harbingers of Alzheimer’s disease or other dementias.

For the study, the researchers recruited participants with community newspaper ads and flyers, as well as from the Johns Hopkins Memory and Alzheimer’s Treatment Center. They paired 28 participants with mild cognitive impairment to 28 healthy matched controls. Participants were an average age of 66 and about 45 percent were women.

People with mild cognitive impairment were defined as those who have a slight decline in cognition, mainly in memory in terms of remembering sequences or organization, and who score lower on tests such as the California Verbal Learning Test, which requires participants to recall a list of related words, such as a shopping list. According to Smith, the inability to do this test accurately reflects changes in memory and cognitive impairment indicative of Alzheimer’s disease.

Each participant underwent an MRI and PET scan to measure brain structures and levels of the serotonin transporter. During the PET scans, participants were given a chemical — similar in structure to an antidepressant but not a high enough dose to have a pharmacological effect — labeled with a radioactive carbon. The chemical binds to the serotonin transporter and the PET scanner detects the radioactivity.

When a neuron sends a message it releases the neurotransmitter serotonin, which is detected by the next neuron receiving the message. After this nerve impulse transaction completes, the serotonin transporter SERT grabs up the serotonin and carts it back into the message-sending cell, a metabolic process marked by the ebb and flow of the chemical.

Normally, as people age, the serotonin neurons are especially vulnerable to neurodegeneration, so the transporters are lost when these neurons die and serotonin levels go down. The older they are, the more likely a person is to have lower serotonin levels. That being said, the researchers found that people with mild cognitive impairment had up to 38 percent less SERT detected in their brains compared to each of their age-matched healthy controls. And not a single person with mild cognitive impairment had higher levels of SERT compared to their healthy control.

Each participant also underwent learning and memory tests. In the California Verbal Learning Test, on a scale of 0 to 80, with 80 reflecting the best memory, the healthy participants had an average score of 55.8, whereas those with mild cognitive impairment scored an average of 40.5.

With the Brief Visuospatial Memory Test, participants were shown a series of shapes to remember and draw later. From a scale of 0 to 36, with 36 being the top score, healthy people scored an average of 20.0 and those with mild cognitive problems scored an average of 12.6.

The researchers then compared the results from the brain imaging tests for the serotonin transporter to those two memory tests, and found that the lower serotonin transporters correlated with lower scores. For example, those people with mild cognitive impairment had 37 percent lower verbal memory scores and 18 percent lower levels of SERT in the brain’s hippocampus compared to healthy controls.

Smith says her group is investigating whether PET imaging of serotonin could be a marker to detect progression of disease, whether alone or in conjunction with scans that detect the clumping protein known as amyloid that accumulates in the brains of those with Alzheimer’s disease.

When it comes to targeting the disease, because of reduced levels of the serotonin transporters, Smith says, the receptors that detect serotonin on message-receiving cells might be a better option. There are 14 types of serotonin receptors that could be used as possible targets. She says a number of experimental drugs now in clinical trials are designed to target serotonin in other ways in the brain, and may have better success than the SSRIs.

Journal article:
https://www.sciencedirect.com/science/article/pii/S0969996117301109?via%3Dihub

Source:
https://www.hopkinsmedicine.org/news/media/releases/brain_scan_study_adds_to_evidence_that_lower_brain_serotonin_levels_are_linked_to_dementia_

Image caption:
A brain showing decreases of serotonin transporters (blue) in the whole mild cognitive impairment group compared to the whole healthy control group.
Credit: Gwenn Smith lab

#alzheimersdisease #serotonin #SSRIs #cognitivedecline #aging #neuroscience #research

Heads Up!


Heads Up!
A cosmic trifecta will occur this Wednesday, January 31, when some parts of the planet will see not just a super moon, a blue moon or a blood moon, but a super blue blood moon. A combination of events that last occurred 152 years ago, it will be best seen in the early hours before dawn across North America and the Pacific Ocean region.

The Jan. 31 full moon is special for three reasons: it’s the third in a series of “supermoons,” when the Moon is closer to Earth in its orbit -- known as perigee -- and about 14 percent brighter than usual. It’s also the second full moon of the month, commonly known as a “blue moon.” The super blue moon will pass through Earth’s shadow to give viewers in the right location a total lunar eclipse. While the Moon is in the Earth’s shadow it will take on a reddish tint, known as a “blood moon.”

Get informed:
https://www.nasa.gov/feature/super-blue-blood-moon-coming-jan-31

Beginning at 5:30 a.m. EST on Jan. 31, a live feed of the Moon will be offered on NASA TV and NASA.gov/live.
https://www.nasa.gov/multimedia/nasatv/index.html#public
https://www.nasa.gov/nasalive

#space #NASA #cosmictrifecta2018 #universe #science

Sunday, 28 January 2018

The Spider and The Fly


The Spider and The Fly
Will the spider ever catch the fly? Not if both are large emission nebulas toward the constellation of the Charioteer (Auriga). The spider-shaped gas cloud on the left is actually an emission nebula labelled IC 417, while the smaller fly-shaped cloud on the right is dubbed NGC 1931 and is both an emission nebula and a reflection nebula. About 10,000 light-years distant, both nebulas harbor young, open star clusters. For scale, the more compact NGC 1931 (Fly) is about 10 light-years across.

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

#universe #space #science #nebula #universe

Physicists create Star Wars-style 3D projections — just don’t call them holograms

Physicists create Star Wars-style 3D projections — just don’t call them holograms
They may not technically be holograms, but they're pretty impressive: Researchers have created moving 3D images that are viewable from any angle. The technique, called volumetric display, comes from the lab of Daniel Smalley at Brigham Young University. Smalley's team uses two sets of lasers—one traps and moves a particle around, while the other projects color onto the particle. The particle moves so quickly that our eyes perceive the projection as a solid-line image.
So...May The Force be with you! ;)

Source & further reading:
https://www.nature.com/articles/d41586-018-01125-y

#scitech #innovation #volumetricdisplay #3Dprojections #physics

Beatrice Tinsley


Beatrice Tinsley
Born on 27 January in 1941, Beatrice Tinsley was an astronomer and cosmologist who made fundamental contributions to our understanding of galaxy formation and evolution. She was born in Chester, England, but grew up in New Zealand and studied math and physics at Canterbury University. She married fellow physics student Brian Tinsley in 1961, and the couple moved to the US in 1963 when Brian accepted an appointment at the University of Texas at Dallas.

As a married woman with career aspirations, Beatrice struggled against gender bias in the male-dominated field of astronomy. Despite earning a PhD in 1967 and performing groundbreaking astronomical research, Beatrice was never able to secure a professorship at UT Dallas. In 1975 Beatrice divorced Brian and took a position at Yale University, where she became the school’s first female astronomy professor in 1978.

Among Tinsley’s many achievements was her synthesis of vast amounts of newly generated space telescope data to model galaxies and chart how they evolve over time. Her work was cut short, however, when she died of cancer at age 40 on 23 March 1981. By that time, Tinsley had published more than 100 scientific papers and become one of the most distinguished astronomers in the US.

In 1986 the American Astronomical Society created the Beatrice M. Tinsley Prize for outstanding creative contributions to astronomy or astrophysics.

Photo credit: AIP Emilio Segrè Visual Archives, gift of Edward Hill
You can read the Physics Today obituary written by Sandra Faber:
http://physicstoday.scitation.org/doi/abs/10.1063/1.2914734

#history #womeninSTEM #science #BeatriceTinsley

Reversing Prominence


Reversing Prominence
A prominence rose up above the sun, sent an arch of plasma to link up magnetically with an active region over a one-day period (Jan, 9-10, 2018). Then the flow of plasma seemed to largely change direction and head back where it came from. Finally, amidst the confused patterns of movement, it dissipated and fell away. Prominences are cooler clouds of charged particles tenuously tethered to the sun by magnetic forces. Images were taken in a wavelength of extreme ultraviolet light.

Credit: Solar Dynamics Observatory, NASA.
https://sdo.gsfc.nasa.gov/

#space #NASA #universe #prominences #sun #science

Thursday, 25 January 2018

Early Language Development in Fast Motion: How Sounds Become Words during Sleep


Early Language Development in Fast Motion: How Sounds Become Words during Sleep
Babies are exposed to a large amount of stimulation. Since no two situations are exactly the same, for babies every moment is a completely new experience— until the infant brain organizes the flood of stimuli. It has to save new information in long-term memory, to aggregate similar experiences and to categorize them. For these processes, sleep seems to be crucial. Researchers at the Max Planck Institute for Human Cognitive and Brain Sciences (MPI CBS) in Leipzig together with colleagues from other institutions have now discovered that, during sleep, babies can even create word meanings—much earlier than previously supposed.

While babies sleep, fascinating processes take place in their brains. Scientists at the Max Planck Institute for Human Cognitive and Brain Sciences (MPI CBS) in Leipzig observed that six- to eight-month-old babies succeed in creating a meaning for a word—a capability that, until now, has been attributed only to older children and adults. During sleep, the memory for word meanings passes through the same stages as during typical lexical development: So-called protowords that initially associate simultaneously occurring visual and acoustic stimuli become real words that are already bound with meanings.

The scientists investigated these processes by exposing six- to eight-month-old infants to fantasy objects which they gave fantasy names such as “Bofel“ or “Zuser“. Objects that differed only slightly in form and color were given the same names—just as all cats are called “cats” although they differ in their specific features. The researchers chose these fictitious objects to make sure that the young study participants could not use already existing knowledge.

The infants’ brain responses revealed that the babies did not assign new objects of the same category to the corresponding name. That means they did not recognize a new Bofel as a “Bofel” although it was quite similar to the previously seen Bofel versions. For the babies, every new object–word pair was unknown and unique, they did not yet see the general relation between the similar pairs.

This changed after a midday nap. In babies who had napped after the learning phase, the brain differentiated between the right and wrong name for a new object in the subsequent test phase. These babies had generalized their knowledge while sleeping. Babies that had stayed awake could not manage to do so.

Interestingly, the babies developed two different types of knowledge depending on the duration of sleep. After a half-hour nap they showed a brain response that is known from three-month-olds, when these infants associate visual object stimuli with acoustic patterns of words. Thus, during their short nap the babies had filtered out similar features of the objects and had associated them with the sounds of the words. However, similar to the three-month-old babies, they perceived a word only as a sound without meaning.

In contrast, babies who slept for about 50 minutes showed a brain response that was previously known only from older children and adults. The so-called N400 component observed here signals that incongruous meanings are processed in the brain—whether it be in sentences, word pairs, picture stories or object–word pairs. On the basis of this component the researchers realized that the young participants had in fact created meanings of the words.

“Our results show that infants can form long-term memory for word meanings much earlier than previously thought. Even though the brain structures that are relevant for this type of memory are not fully matured, they can already be used to a certain extent”, explains Angela D. Friederici, director at MPI CBS and senior author of the underlying study which has been published in Current Biology.

Journal article:
http://www.cell.com/current-biology/fulltext/S0960-9822(17)30807-2

Source:
http://www.cbs.mpg.de/sleep-babies-first-associate-words-with-content

#languagedevelopment #infants #sleep #memoryconsolidation #neuroscience #research

Selfie at Vera Rubin Ridge


Selfie at Vera Rubin Ridge
On sol 1943 of its journey of exploration across the surface of Mars, the Curiosity Rover recorded this selfie at the south rim of Vera Rubin Ridge. Of course a sol is a Martian solar day, about 40 minutes longer than an Earth day.

Curiosity's sol 1943 corresponds to Earth date January 23, 2018. Also composed as an interactive 360 degree VR, the mosaicked panorama combines 61 exposures taken by the car-sized rover's Mars Hand Lens Imager (MAHLI).

Frames containing the imager's arm have been edited out while the extended background used was taken by the rover's Mastcam on sol 1903. At the top of the rover's mast, sitting above the Mastcam, the laser-firing ChemCam housing blocks out the distant peak of Mount Sharp.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: Image Credit: NASA, JPL-Caltech, MSSS - Panorama: Andrew Bodrov

#space #nasa #universe #science #Mars #CuriosityRover

Wednesday, 24 January 2018

Cartwheel of Fortune


Cartwheel of Fortune
By chance, a collision of two galaxies has created a surprisingly recognizable shape on a cosmic scale, The Cartwheel Galaxy. The Cartwheel is part of a group of galaxies about 500 million light years away in the constellation Sculptor. Two smaller galaxies in the group are visible on the right. The Cartwheel Galaxy's rim is an immense ring-like structure 150,000 light years in diameter composed of newly formed, extremely bright, massive stars.

When galaxies collide they pass through each other, their individual stars rarely coming into contact. Still, the galaxies' gravitational fields are seriously distorted by the collision. In fact, the ring-like shape is the result of the gravitational disruption caused by a small intruder galaxy passing through a large one, compressing the interstellar gas and dust and causing a a star formation wave to move out from the impact point like a ripple across the surface of a pond. In this case the large galaxy may have originally been a spiral, not unlike our own Milky Way, transformed into the wheel shape by the collision. But ... what happened to the small intruder galaxy?

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: ESA, NASA

#space #NASA #science #universe #galaxy

Tuesday, 23 January 2018

Blocking a key enzyme may reverse memory loss


Blocking a key enzyme may reverse memory loss
In the brains of Alzheimer’s patients, many of the genes required to form new memories are shut down by a genetic blockade, contributing to the cognitive decline seen in those patients.

MIT researchers have shown that they can reverse that memory loss in mice by interfering with the enzyme that forms the blockade. The enzyme, known as HDAC2, turns genes off by condensing them so tightly that they can’t be expressed.

For several years, scientists and pharmaceutical companies have been trying to develop drugs that block this enzyme, but most of these drugs also block other members of the HDAC family, which can lead to toxic side effects. The MIT team has now found a way to precisely target HDAC2, by blocking its interaction with a binding partner called Sp3.

“This is exciting because for the first time we have found a specific mechanism by which HDAC2 regulates synaptic gene expression,” says Li-Huei Tsai, director of MIT’s Picower Institute for Learning and Memory and the study’s senior author.

Blocking that mechanism could offer a new way to treat memory loss in Alzheimer’s patients. In this study, the researchers used a large protein fragment to interfere with HDAC-2, but they plan to seek smaller molecules that would be easier to deploy as drugs.

Source & further reading:
http://news.mit.edu/2017/blocking-key-enzyme-may-reverse-memory-loss-0808

Journal article:
http://www.cell.com/cell-reports/fulltext/S2211-1247(17)31023-9

#HDAC2 #alzheimersdisease #geneexpression #plasticity #memory #neuroscience

The Tadpoles of IC 410


The Tadpoles of IC 410
This telescopic close-up shows off the otherwise faint emission nebula IC 410. It also features two remarkable inhabitants of the cosmic pond of gas and dust below and left of center, the tadpoles of IC 410. Partly obscured by foreground dust, the nebula itself surrounds NGC 1893, a young galactic cluster of stars.

Formed in the interstellar cloud a mere 4 million years ago, the intensely hot, bright cluster stars energize the glowing gas. Composed of denser cooler gas and dust, the tadpoles are around 10 light-years long and are likely sites of ongoing star formation.

Sculpted by winds and radiation from the cluster stars, their heads are outlined by bright ridges of ionized gas while their tails trail away from the cluster's central region. IC 410 lies some 10,000 light-years away, toward the nebula-rich constellation Auriga.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: Juan Ignacio Jimenez

#space #NASA #science #galaxies #nebula #universe

Turn inverse


Turn inverse
Behind your amygdala there are things waiting to be discovered...understand the omnipotence of the underside of things.

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

#math #animation #processing #inverseyourthoughts

Monday, 22 January 2018

Ribbons and Pearls of Spiral Galaxy NGC 1398


Ribbons and Pearls of Spiral Galaxy NGC 1398
Why do some spiral galaxies have a ring around the center? Spiral galaxy NGC 1398 not only has a ring of pearly stars, gas and dust around its center, but a bar of stars and gas across its center, and spiral arms that appear like ribbons farther out.

The featured image was taken with ESO's Very Large Telescope at the Paranal Observatory in Chile and resolves this grand spiral in impressive detail. NGC 1398 lies about 65 million light years distant, meaning the light we see today left this galaxy when dinosaurs were disappearing from the Earth.

The photogenic galaxy is visible with a small telescope toward the constellation of the Furnace (Fornax). The ring near the center is likely an expanding density wave of star formation, caused either by a gravitational encounter with another galaxy, or by the galaxy's own gravitational asymmetries.

Image & Info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: European Southern Observatory

#space #NASA #galaxies #science #universe

Sunday, 21 January 2018

Don't hold your nose and close your mouth when you sneeze, doctors warn


Don't hold your nose and close your mouth when you sneeze, doctors warn
One young man managed to rupture the back of his throat during this manoeuvre, leaving him barely able to speak or swallow, and in considerable pain.

Spontaneous rupture of the back of the throat is rare, and usually caused by trauma, or sometimes by vomiting, retching or heavy coughing, so the 34 year old's symptoms initially surprised the emergency care doctors.

The young man explained that he had developed a popping sensation in his neck which immediately swelled up after he tried to contain a forceful sneeze by pinching his nose and keeping his mouth clamped shut at the same time.

A little later he found it extremely painful to swallow and all but lost his voice.

When the doctors examined him they heard popping and crackling sounds (crepitus), which extended from his neck all the way down to his ribcage -- a sure sign that air bubbles had found their way into the deep tissue and muscles of the chest, which was subsequently confirmed by a computed tomography scan.

Because of the risk of serious complications, the man was admitted to hospital, where he was fed by tube and given intravenous antibiotics until the swelling and pain had subsided.

After seven days he was well enough to be discharged with the advice not to block both nostrils when sneezing in future.

"Halting sneezing via blocking [the] nostrils and mouth is a dangerous manoeuvre, and should be avoided," caution the authors.

"It may lead to numerous complications, such as pseudomediastinum [air trapped in the chest between both lungs], perforation of the tympanic membrane [perforated eardrum], and even rupture of a cerebral aneurysm [ballooning blood vessel in the brain]," they explain.

Source:
http://www.bmj.com/company/newsroom/dont-hold-your-nose-and-close-your-mouth-when-you-sneeze-doctors-warn/

#sneezing #medicine #nostrils #science

Increased brain acidity in psychiatric disorders


Increased brain acidity in psychiatric disorders
Your body’s acid/alkaline homeostasis, or maintenance of an adequate pH balance in tissues and organs, is important for good health. An imbalance in pH, particularly a shift toward acidity, is associated with various clinical conditions, such as a decreased cardiovascular output, respiratory distress, and renal failure. But is pH also associated with psychiatric disorders?

Researchers at the Institute for Comprehensive Medical Science at Fujita Health University in Japan, along with colleagues from eight other institutions, have identified decreased pH levels in the brains of five different mouse models of mental disorders, including models of schizophrenia, bipolar disorder, and autism spectrum disorder. This decrease in pH likely reflects an underlying pathophysiology in the brain associated with these mental disorders, according to the study published August 4th in the journal Neuropsychopharmacology.

While post-mortem studies have shown that the brains of patients with the abovementioned mental disorders tend to have a lower pH than those of controls, this phenomenon has been considered to be the result of secondary factors associated with the diseases rather than a primary feature of the diseases themselves. Secondary factors that confound the observation of a decreased brain pH level include antipsychotic treatments and agonal experiences associated with these disorders.

Dr. Miyakawa and his colleagues performed a meta-analysis of existing datasets from ten studies to investigate the pH level of postmortem brains from patients with schizophrenia and bipolar disorder. They observed that patients with schizophrenia and bipolar disorder exhibited significantly lower brain pH levels than control participants, even when potential confounding factors were considered (i.e., postmortem interval, age at death, and history of antipsychotic use). “These factors may not be major factors causing a decrease in pH in the postmortem brains of patients with schizophrenia and bipolar disorder,” Miyakawa explains.

The researchers then conducted a systematic investigation of brain pH using five mouse models of psychiatric disorders, including models for schizophrenia, bipolar disorder, and autism spectrum disorders. All of the mice used in the study were drug-naive, with equivalent agonal states, postmortem intervals, and ages within each strain. The analyses revealed that in all five mouse models, brain pH was significantly lower than that in the corresponding controls. In addition, the levels of lactate were also elevated in the brains of the model mice, and a significant negative correlation was found between brain pH and lactate levels. The increase in lactate may explain the decreased brain pH levels, as lactate is known to act as a strong acid.

Miyakawa suggests that, “while it is technically impossible to completely exclude confounding factors in human studies, our findings in mouse models strongly support the notion that decreased pH associated with increased lactate levels reflects an underlying pathophysiology, rather than a mere artifact, in at least a subgroup of patients with these mental disorders.”

Changes in the brain pH level have been considered an artifact, therefore substantial effort has been made to match the tissue pH among study participants and to control the effect of pH on molecular changes in the postmortem brain. However, given that decreased brain pH is a pathophysiological trait of psychiatric disorders, these efforts could have unwittingly obscured the specific pathophysiological signatures that are potentially associated with changes in pH, such as neuronal hyper-excitation and inflammation, both of which have been implicated in the etiology of psychiatric disorders. Therefore, the present study highlighting that decreased brain pH is a shared endophenotype of psychiatric disorders has significant implications on the entire field of studies on the pathophysiology of mental disorders.

This research raises new questions about changes in brain pH. For example, what are the mechanisms through which lactate is increased and pH is decreased? Are specific brain regions responsible for the decrease in pH? Is there functional significance to the decrease in brain pH observed in psychiatric disorders, and if so, is it a cause or result of the onset of the disorder? Further studies are needed to address these issues.

Source:
https://www.eurekalert.org/pub_releases/2017-08/fhu-iba080717.php

Journal article:
https://www.nature.com/articles/npp2017167

#psychiatricdisorders #phbalance #schizophrenia #bipolardisorder #lactate #neuroscience #research

Wednesday, 17 January 2018

Blue Comet in the Hyades


Blue Comet in the Hyades
Stars of the Hyades cluster are scattered through this mosaic spanning over 5 degrees on the sky toward the constellation Taurus. Presently cruising through the Solar System, the remarkably blue comet C/2016 R2 PanSTARRS is placed in the wide field of view using image data from January 12.

With the apex of the V-shape in the Hyades cluster positioned near the top center, bright Aldebaran, alpha star of Taurus, anchors the frame at the lower right. A cool red giant, Aldebaran is seen in orange hues in the colorful starfield. While the stars of the Hyades are gathered 151 light-years away, Aldebaran lies only 65 light-years distant and so is separate from the cluster stars.

On January 12, C/2016 R2 was over 17 light-minutes from planet Earth and nearly 24 light-minutes from the Sun. Its blue tinted tail largely due to CO+ gas fluorescing in sunlight, the head or coma of the comet appears with a slightly greenish hue, likely emission from diatomic carbon.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Rogelio Bernal Andreo (Deep Sky Colors)

#space #NASA #science #universe #comet

January 15 is reserved to Martin Luther King Jr.


January 15 is reserved to Martin Luther King Jr.
Martin Luther King Jr. was a social activist and Baptist minister who played a key role in the American civil rights movement from the mid-1950s until his assassination in 1968. King sought equality and human rights for African Americans, the economically disadvantaged and all victims of injustice through peaceful protest.

I have a dream that one day this nation will rise up and live out the true meaning of its creed: "We hold these truths to be self-evident; that all men are created equal."
At the age of thirty-five, Martin Luther King, Jr., was the youngest man to have received the Nobel Peace Prize.

I have a dream speech:
https://www.archives.gov/files/press/exhibits/dream-speech.pdf

Bio:
https://www.nobelprize.org/nobel_prizes/peace/laureates/1964/king-bio.html

#history #MartinLutherKingJr #civilrights

Monday, 15 January 2018

Liquids that are less dense than an ideal gas


Liquids that are less dense than an ideal gas
A water droplet has structural integrity because of attractive forces between water molecules. If the molecules get close enough, however, the intermolecular forces are repulsive; water molecules can pack only so tightly. In quantum systems, intrinsically quantum fluctuations can stabilize a cluster of atoms against collapse. As a result, quantum droplets can have extraordinarily low densities.

Using Bose-Einstein condensates, researches created liquids that have extraordinarily low densities - five orders of magnitude below that of an ideal gas at room temperature and pressure.

Journal article:
http://science.sciencemag.org/content/early/2017/12/13/science.aao5686

Source:
http://physicstoday.scitation.org/do/10.1063/PT.6.1.20180111a/full/

#physics #science #research #quantumdroplets

An Elephant's Trunk in Cepheus


An Elephant's Trunk in Cepheus
With image data from telescopes large and small, this close-up features the dusty Elephant's Trunk Nebula. It winds through the emission nebula and young star cluster complex IC 1396, in the high and far off constellation of Cepheus.

Also known as vdB 142, the cosmic elephant's trunk is over 20 light-years long. The colorful view highlights bright, swept-back ridges that outline the region's pockets of cool interstellar dust and gas. Such embedded, dark, tendril-shaped clouds contain the raw material for star formation and hide protostars within.

Nearly 3,000 light-years distant, the relatively faint IC 1396 complex covers a large region on the sky, spanning over 5 degrees. This dramatic scene spans a 1 degree wide field, about the size of 2 Full Moons.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Processing - Robert Gendler, Roberto Colombari
Data - Subaru Telescope (NAOJ), Robert Gendler, Adam Block

#space #science #NASA #nebula #universe

Sunday, 14 January 2018

Talking to yourself in the third person can help you control stressful emotions


Talking to yourself in the third person can help you control stressful emotions
The simple act of silently talking to yourself in the third person during stressful times may help you control emotions without any additional mental effort than what you would use for first-person self-talk, the way people normally talk to themselves.

A first-of-its-kind study led by psychology researchers at Michigan State University and the University of Michigan indicates that such third-person self-talk may constitute a relatively effortless form of self-control. The findings are published online in Scientific Reports, a Nature journal.

Say a man named John is upset about recently being dumped. By simply reflecting on his feelings in the third person (“Why is John upset?”), John is less emotionally reactive than when he addresses himself in the first person (“Why am I upset?”).

“Essentially, we think referring to yourself in the third person leads people to think about themselves more similar to how they think about others, and you can see evidence for this in the brain,” said Jason Moser, MSU associate professor of psychology. “That helps people gain a tiny bit of psychological distance from their experiences, which can often be useful for regulating emotions.”

The study, partially funded by the National Institutes of Health and the John Temple Foundation, involved two experiments that both significantly reinforced this main conclusion.

In one experiment, at Moser’s Clinical Psychophysiology Lab, participants viewed neutral and disturbing images and reacted to the images in both the first and third person while their brain activity was monitored by an electroencephalograph. When reacting to the disturbing photos (such as a man holding a gun to their heads), participants’ emotional brain activity decreased very quickly (within 1 second) when they referred to themselves in the third person.

The MSU researchers also measured participants’ effort-related brain activity and found that using the third person was no more effortful than using first person self-talk. This bodes well for using third-person self-talk as an on-the-spot strategy for regulating one’s emotions, Moser said, as many other forms of emotion regulation, such as mindfulness and thinking on the bright side, require considerable thought and effort.

In the other experiment, led by U-M psychology professor Ethan Kross, who directs the Emotion and Self-Control Lab, participants reflected on painful experiences from their past using first and third person language while their brain activity was measured using functional magnetic resonance imaging, or FMRI.

Similar to the MSU study, participants’ displayed less activity in a brain region that is commonly implicated in reflecting on painful emotional experiences when using third person self-talk, suggesting better emotional regulation. Further, third person self-talk required no more effort-related brain activity than using first person.

“What’s really exciting here,” Kross said, “is that the brain data from these two complimentary experiments suggest that third-person self-talk may constitute a relatively effortless form of emotion regulation.

“If this ends up being true – we won’t know until more research is done – there are lots of important implications these findings have for our basic understanding of how self-control works, and for how to help people control their emotions in daily life.”

Moser and Kross said their teams are continuing to collaborate to explore how third-person self-talk compares to other emotion-regulation strategies.

Journal article:
https://www.nature.com/articles/s41598-017-04047-3

Source & further reading:
http://msutoday.msu.edu/news/2017/talking-to-yourself-in-the-third-person-can-help-you-control-stressful-emotions/

#neuroimaging #brainactivity #emotion #emotionregulation #neuroscience #research

Rigel and the Witch Head Nebula


Rigel and the Witch Head Nebula
By starlight this eerie visage shines in the dark, a crooked profile evoking its popular name, the Witch Head Nebula. In fact, this entrancing telescopic portrait gives the impression that the witch has fixed her gaze on Orion's bright supergiant star Rigel.

More formally known as IC 2118, the Witch Head Nebula spans about 50 light-years and is composed of interstellar dust grains reflecting Rigel's starlight. The blue color of the Witch Head Nebula and of the dust surrounding Rigel is caused not only by Rigel's intense blue starlight but because the dust grains scatter blue light more efficiently than red.

The same physical process causes Earth's daytime sky to appear blue, although the scatterers in Earth's atmosphere are molecules of nitrogen and oxygen. Rigel, the Witch Head Nebula, and gas and dust that surrounds them lie about 800 light-years away.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Mario Cogo (Galax Lux)

#space #universe #NASA #science #nebula

Thursday, 11 January 2018

Eye Test Could Help Diagnose Autism


Eye Test Could Help Diagnose Autism
A new study out in European Journal of Neuroscience could herald a new tool that helps physicians identify a sub-group of people with Autism spectrum disorders (ASD). The test, which consists of measuring rapid eye movements, may indicate deficits in an area of the brain that plays an important role in emotional and social development.

ASD is characterized by a wide range of symptoms that can vary in severity from person to person. This unpredictability not only presents a challenge for diagnosis, but also how best to devise a course of treatment. Identifying the specific phenotype of the disorder is, therefore, an essential first step to providing effective care.

Eye movements and the mechanisms by which the brain controls and processes what we choose to look at have been a major focus of neuroscience researchers for decades. The rapid eye movements we make when we shift our attention from one object to another, known as saccades, are essential to navigating, understanding, and interacting with the world around us. In healthy individuals, these saccades are rapid, precise, and accurate, redirecting the line of sight from one point of interest to another.

The potential relevance of eye movement in individuals with Autism is the area of the brain that controls these actions, a densely-packed structure of neurons known as the cerebellum. Traditionally considered to play a role in motor control, the cerebellum is now known to be essential to emotion and cognition via its connections to the rest of the brain. There is growing evidence that the structure of the cerebellum is altered in a sub-population of individuals with ASD.

In a series of experiments, the authors of the current study tracked the eye movements of individuals with ASD. The participants were asked to track a visual target that appeared in different locations on the screen. The experiment was designed in a manner that often caused the participant’s focus to “overshoot” the intended target. In healthy individuals, the brain would correctly adjust eye movements as the task is repeated. However, the eye movements of individuals with ASD continued to miss the target suggesting that the sensory motor controls in the cerebellum responsible for eye movement were impaired.

The inability of the brain to adjust the size of eye movement may not only be a marker for cerebellum dysfunction, but it may also help explain the communication and social interaction deficits that many individuals with ASD experience.

“These finding suggest that assessing the ability of people to adapt saccade amplitudes is one way to determine whether this function of the cerebellum is altered in ASD,” said Edward Freedman, Ph.D. an associate professor in the URMC Department of Neuroscience and co-author of the study. “If these deficits do turn out to be a consistent finding in a sub-group of children with ASD, this raises the possibility that saccade adaptation measures may have utility as a method that will allow early detection of this disorder.”

Journal article:
http://onlinelibrary.wiley.com/doi/10.1111/ejn.13625/abstract

Source and further reading:
https://www.urmc.rochester.edu/news/story/5102/eye-test-could-help-diagnose-autism.aspx

#autism #eyemovements #ASD #cerebellum #neuroscience

Blue Comet PanSTARRS


Blue Comet PanSTARRS
Discovered with the PanSTARRS telescope on September 7, 2016, this Comet PanSTARRS, C/2016 R2, is presently about 24 light minutes (3 AU) from the Sun, sweeping through planet Earth's skies across the background of stars in the constellation Taurus. An inbound visitor from our Solar System's distant Oort Cloud, its beautiful and complex ion tail is a remarkable shade of blue. Still relatively far from the Sun, the comet's already well-developed ion tail is very impressive.

Emission from unusually abundant ionized carbon monoxide (CO+) atoms fluorescing in the increasing sunlight is largely responsible for the pretty blue tint. This color image of the blue comet is a combination of data taken from two different telescopes during the night of January 7. Located at the apex of the V-shaped Hyades star cluster in Taurus, bright star Gamma Tauri is responsible for the glow at the bottom left corner of the frame.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Damian Peach, Jose J. Chambo

#space #NASA #universe #science

Wednesday, 10 January 2018

“There is a crack in everything. That's how the light gets in.”


“There is a crack in everything. That's how the light gets in.”
~ Leonard Cohen

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

#math #processing #animation

Small Twisting Prominence


Small Twisting Prominence
A small prominence rose up above the sun, appeared to twist around for several hours, and then began to send some streams of plasma back into the sun (Jan. 3-4, 2018). The action, observed in a wavelength of extreme ultraviolet light, lasted just about one day. Prominences like this one are quite common. In fact, there were several over the past few days. For a sense of scale, the prominence reached up more than several times the size of Earth.

Credit: Solar Dynamics Observatory, NASA.
https://sdo.gsfc.nasa.gov/

#sun #space #universe #NASA #prominences

Brain Cells Found to Control Aging


Brain Cells Found to Control Aging
Scientists at Albert Einstein College of Medicine have found that stem cells in the brain’s hypothalamus govern how fast aging occurs in the body. The finding, made in mice, could lead to new strategies for warding off age-related diseases and extending lifespan. The paper was published online in Nature.

The hypothalamus was known to regulate important processes including growth, development, reproduction and metabolism. In a 2013 Nature paper, Einstein researchers made the surprising finding that the hypothalamus also regulates aging throughout the body. Now, the scientists have pinpointed the cells in the hypothalamus that control aging: a tiny population of adult neural stem cells, which were known to be responsible for forming new brain neurons.

“Our research shows that the number of hypothalamic neural stem cells naturally declines over the life of the animal, and this decline accelerates aging,” says senior author Dongsheng Cai, M.D., Ph.D., professor of molecular pharmacology at Einstein. “But we also found that the effects of this loss are not irreversible. By replenishing these stem cells or the molecules they produce, it’s possible to slow and even reverse various aspects of aging throughout the body.”

In studying whether stem cells in the hypothalamus held the key to aging, the researchers first looked at the fate of those cells as healthy mice got older. The number of hypothalamic stem cells began to diminish when the animals reached about 10 months, which is several months before the usual signs of aging start appearing. “By old age—about two years of age in mice—most of those cells were gone,” says Dr. Cai.

The researchers next wanted to learn whether this progressive loss of stem cells was actually causing aging and was not just associated with it. So they observed what happened when they selectively disrupted the hypothalamic stem cells in middle-aged mice. “This disruption greatly accelerated aging compared with control mice, and those animals with disrupted stem cells died earlier than normal,” says Dr. Cai.

Could adding stem cells to the hypothalamus counteract aging? To answer that question, the researchers injected hypothalamic stem cells into the brains of middle-aged mice whose stem cells had been destroyed as well as into the brains of normal old mice. In both groups of animals, the treatment slowed or reversed various measures of aging.

Dr. Cai and his colleagues found that the hypothalamic stem cells appear to exert their anti-aging effects by releasing molecules called microRNAs (miRNAs). They are not involved in protein synthesis but instead play key roles in regulating gene expression. miRNAs are packaged inside tiny particles called exosomes, which hypothalamic stem cells release into the cerebrospinal fluid of mice.

The researchers extracted miRNA-containing exosomes from hypothalamic stem cells and injected them into the cerebrospinal fluid of two groups of mice: middle-aged mice whose hypothalamic stem cells had been destroyed and normal middle-aged mice. This treatment significantly slowed aging in both groups of animals as measured by tissue analysis and behavioral testing that involved assessing changes in the animals’ muscle endurance, coordination, social behavior and cognitive ability.

The researchers are now trying to identify the particular populations of microRNAs and perhaps other factors secreted by these stem cells that are responsible for these anti-aging effects—a first step toward possibly slowing the aging process and treating age-related diseases.

Journal article:
https://www.nature.com/articles/nature23282

Source:
http://www.einstein.yu.edu/news/releases/1259/brain-cells-found-to-control-aging/

#aging #hypothalamus #stemcells #miRNAs #neuroscience #research

RCW 114: A Dragon's Heart in Ara


RCW 114: A Dragon's Heart in Ara
Large and dramatically shaped, this cosmic cloud spans nearly 7 degrees or 14 full moons across planet Earth's sky toward the southern constellation Ara. Difficult to image, the filamentary apparition is cataloged as RCW 114 and traced in this telescopic mosaic by the telltale reddish emission of ionized hydrogen atoms.

In fact, RCW 114 has been recognized as a supernova remnant. Its extensive filaments of emission are produced as the still expanding shockwave from the death explosion of a massive star sweeps up the surrounding interstellar medium.

Consistent estimates place its distance at over 600 light-years, indicating a diameter of about 100 light-years or so. Light from the supernova explosion that created RCW 114 would have reached Earth around 20,000 years ago. A neutron star or pulsar has recently been identified as the collapsed remains of the stellar core.

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

#space #NASA #science #cosmiccloud #universe

Tuesday, 9 January 2018

NGC 2623: Merging Galaxies from Hubble


NGC 2623: Merging Galaxies from Hubble
Where do stars form when galaxies collide? To help find out, astronomers imaged the nearby galaxy merger NGC 2623 in high resolution with the Hubble Space Telescope. Analysis of this and other Hubble images as well as images of NGC 2623 in infrared light by the Spitzer Space Telescope, in X-ray light by XMM-Newton, and in ultraviolet light by GALEX, indicate that two originally spiral galaxies appear now to be greatly convolved and that their cores have unified into one active galactic nucleus (AGN).

Star formation continues around this core near the featured image center, along the stretched out tidal tails visible on either side, and perhaps surprisingly, in an off-nuclear region on the upper left where clusters of bright blue stars appear. Galaxy collisions can take hundreds of millions of years and take several gravitationally destructive passes.

NGC 2623, also known as Arp 243, spans about 50,000 light years and lies about 250 million light years away toward the constellation of the Crab (Cancer). Reconstructing the original galaxies and how galaxy mergers happen is often challenging, sometimes impossible, but generally important to understanding how our universe evolved.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html

Image Credit: ESA/Hubble & NASA

#space #NASA #ESA #science #Hubble #galaxies #universe

Sunday, 7 January 2018

Depression changes brain structure


Depression changes brain structure
Changes in the brain’s structure that could be the result of depression have been identified in a major scanning study.

White matter
Alterations were found in parts of the brain known as white matter, which contains fibre tracts that enable brain cells to communicate with one another by electrical signals.
White matter is a key component of the brain’s wiring and its disruption has been linked to problems with emotion processing and thinking skills.

Brain Imaging
The study of more than 3000 people – the largest of its type to date – sheds light on the biology of depression and could help in the search for better diagnosis and treatment.

Scientists at the University of Edinburgh’s Division of Psychiatry used a cutting-edge technique known as diffusion tensor imaging to map the structure of white matter.

A quality of the matter – known as white matter integrity – was reduced in people who reported symptoms indicative of depression. The same changes were not seen in people who were unaffected.

Leading cause of disability
Depression is the world’s leading cause of disability, affecting around a fifth of UK adults over a lifetime. Symptoms include low mood, exhaustion and feelings of emptiness.
Experts say the large number of people included in the sample – 3461 – means that the study findings are very robust.

"This study uses data from the largest single sample published to date and shows that people with depression have changes in the white matter wiring of their brain. There is an urgent need to provide treatment for depression and an improved understanding of its mechanisms will give us a better chance of developing new and more effective methods of treatment.”
-Dr Heather Whalley Senior Research Fellow, Division of Psychiatry, University of Edinburgh

Participants were drawn from UK Biobank, a national research resource with health data available from 500,000 volunteers.

Wider research
The study forms part of a Wellcome Trust initiative called Stratifying Resilience and Depression Longitudinally (STRADL), which aims to classify subtypes of depression and identify risk factors.

The work – published in Scientific Reports – was carried out in collaboration with the University of Glasgow.

Our next steps will be to look at how the absence of changes in the brain relates to better protection from distress and low mood. -Dr Heather Whalley Senior Research Fellow, Division of Psychiatry, University of Edinburgh

Journal article:
https://www.nature.com/articles/s41598-017-05507-6

Source:
https://www.ed.ac.uk/news/2017/depression-structure-of-brain

Image: A PET scan can compare brain activity during periods of depression (left) with normal brain activity (right). An increase of blue and green colors, along with decreased white and yellow areas, shows decreased brain activity due to depression.
https://www.mayoclinic.org/tests-procedures/pet-scan/multimedia/-pet-scan-of-the-brain-for-depression/img-20007400

#depression #brainimaging #whitematter #diffusiontensorimaging #neuroscience #research

Clouds of Andromeda


Clouds of Andromeda
What are those red clouds surrounding the Andromeda galaxy? This galaxy, M31, is often imaged by planet Earth-based astronomers. As the nearest large spiral galaxy, it is a familiar sight with dark dust lanes, bright yellowish core, and spiral arms traced by clouds of bright blue stars.

A mosaic of well-exposed broad and narrow-band image data, this colorful portrait of our neighboring island universe offers strikingly unfamiliar features though, faint reddish clouds of glowing ionized hydrogen gas in the same wide field of view.

These ionized hydrogen clouds surely lie in the foreground of the scene, well within our Milky Way Galaxy. They are likely associated with the pervasive, dusty interstellar cirrus clouds scattered hundreds of light-years above our own galactic plane.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Daniel López / IAC

#space #NASA #science #universe #Andromeda

Saturday, 6 January 2018

January 7 is reserved to the discovery of the Galilean Moons


January 7 is reserved to the discovery of the Galilean Moons
Galileo first observed the moons of Jupiter on January 7, 1610 through a homemade telescope. He originally thought he saw three stars near Jupiter, strung out in a line through the planet. The next evening, these stars seemed to have moved the wrong way, which caught his attention. Galileo continued to observe the stars and Jupiter for the next week.

On January 11, a fourth star (which would later turn out to be Ganymede) appeared. After a week, Galileo had observed that the four stars never left the vicinity of Jupiter and appeared to be carried along with the planet, and that they changed their position with respect to each other and Jupiter.

Finally, Galileo determined that what he was observing were not stars, but planetary bodies that were in orbit around Jupiter. This discovery provided evidence in support of the Copernican system and showed that everything did not revolve around the Earth.
Galileo published his observations in Sidereus Nuncius in March 1610.

Jupiter, the largest planet in the solar system, has 67 moons and counting.
https://solarsystem.nasa.gov/planets/jupiter/moons

Read & learn:
http://solarviews.com/eng/galdisc.htm

#history #GalileanMoons #Jupiter #science #GalileoGalilei

A Tether in Space


A Tether in Space
One of the greatest unrequited legends of outer space is the tether. Tethers, long strands of material, hold the promise of stabilizing satellites, generating electricity, and allowing easy transportation. Possibly the most ambitious vision of the space tether is the space elevator popularized by Arthur C. Clarke, where a tether is constructed that connects the ground to geosynchronous orbit.

One problem is strength - it is difficult to make a long useful tether that does not snap. Pictured here is the deployment of the Tethered Satellite System 1 (TSS-1) by the space shuttle Altantis in 1992. Like other tested tethers, TSS-1 failed to live up to its promise, although many valuable lessons were learned.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: TSS-1, STS-46 Crew, NASA

#universe #space #NASA #science #TSS1

Stemonitis fusca fruits in clusters on dead wood, and has distinctive tall brown sporangia, supported on slender...

Stemonitis fusca fruits in clusters on dead wood, and has distinctive tall brown sporangia, supported on slender stalks with a total height of approximately 6–20 mm tall.

Slime molds have a pretty fascinating life cycle:

Slime molds begin life as amoeba-like cells. These unicellular amoebae are commonly haploid and multiply if they encounter their favorite food, bacteria. These amoebae can mate if they encounter the correct mating type and form zygotes that then grow into plasmodia. These contain many nuclei without cell membranes between them, which can grow to be meters in size. The species Fuligo septica is often seen as a slimy yellow network in and on rotting logs. The amoebae and the plasmodia engulf microorganisms. The plasmodium grows into an interconnected network of protoplasmic strands.

Within each protoplasmic strand the cytoplasmic contents rapidly stream. If one strand is carefully watched for about 50 seconds, the cytoplasm can be seen to slow, stop, and then reverse direction. The streaming protoplasm within a plasmodial strand can reach speeds of up to 1.35 mm per second which is the fastest rate recorded for any micro-organism. Migration of the plasmodium is accomplished when more protoplasm streams to advancing areas and protoplasm is withdrawn from rear areas. When the food supply wanes, the plasmodium will migrate to the surface of its substrate and transform into rigid fruiting bodies. The fruiting bodies or sporangia are what we commonly see; they superficially look like fungi or molds but are not related to the true fungi. These sporangia will then release spores which hatch into amoebae to begin the life cycle again.

Watch:
https://www.youtube.com/watch?v=PUXrx7Fw6sg

Know more:
https://www.inaturalist.org/taxa/126279-Stemonitis-fusca
https://www.gotmold.ca/2015/05/stemonitis-fusca-a-weird-but-amazing-species-of-slime-mold/

#biodiversity #stemonitisfusca #slimemold #science

Thursday, 4 January 2018

How Does Neuroplasticity Work?


How Does Neuroplasticity Work?
Neuroplasticity, is the process in which your brain's neural synapses and pathways are altered as an effect of environmental, behavioral, and neural changes.

The process of neuroplasticity isn't a quick or simple one; rather, it takes place throughout your lifetime and can involve many processes. Along with altering your neural synapses and pathways, it can involve changes to your neurons, vascular cells, and glial cells. Neuroplasticity also occurs hand-in-hand with synaptic pruning, which is the brain's way of deleting the neural connections that are no longer necessary or useful and strengthening the necessary ones. How your brain decides which connections to prune out depends on your life experiences and how recently connections have been used. In much the same way, neurons that grow weak from underuse die off through the process of apoptosis. In general, neuroplasticity is a way for your brain to fine-tune itself for efficiency.

Neuroplasticity happens continually as you learn and memorize new data, and as your brain develops; however, it can also be spurred by a physical trauma. In such cases, neuroplasticity serves as an adaptive mechanism that allows someone to compensate for function loss after suffering a bodily injury. For example, if someone suffers a brain injury, neuroplasticity allows the brain to 'rewire' itself in order to restore or maximize brain functioning by rebuilding neural circuits and allowing an uninjured part of the brain to take over the damaged part.

Read & Learn:
https://study.com/academy/lesson/what-is-neuroplasticity-definition-depression-quiz.html

#infographic via nicabm
http://www.nicabm.com/brain-how-does-neuroplasticity-work/

#neuroscience #medicine #neuroplasticity #brain

Wednesday, 3 January 2018

The Sun Forms a Question


The Sun Forms a Question
Oddly enough, an elongated coronal hole (the darker area near the center) seems to shape itself into a single, recognizable question mark over the period of one day (Dec. 21-22, 2017). Coronal holes are areas of open magnetic field that appear darker in extreme ultraviolet light, as is seen here.

These holes are the source of streaming plasma that we call solar wind. While this exercise is akin to seeing shapes in clouds, it is fun to consider what the sun might be asking? Perhaps what the new year will bring? Guess what I am going to do next?

Source: https://sdo.gsfc.nasa.gov/
Credit: Solar Dynamics Observatory, NASA.

#sun #NASA #space #universe #science #coronalhole

Individual insight into brain networks


Individual insight into brain networks
Harvard scientists have gained new insights into how the brain networks important for thought and remembering are organized in individual people, bringing the notion of using brain scans to help personalize medical treatments one step closer to reality.

Led by Randy Buckner, a Professor of Psychology and of Neuroscience, and Professor of Psychology in the Department of Psychiatry, and Rodrigo Braga, a post-doctoral fellow in Buckner’s lab, researchers identified two networks that lie side-by-side in the brain and may play key roles in planning, remembering and imagination. The networks are described in a July 19 paper published in Neuron.

“We’ve known for some time there is a network of brain regions that is involved in memory,” Braga said. “What we’ve done is look at the organization of this network in more detail than ever before by diving deeply into individuals as opposed to looking across groups of - sometimes - thousands of individuals…and by doing so we’ve been able to see a new level of detail.”

To understand this network, Braga and Buckner used MRI to intensively scan the brains of four individuals two dozen times over the course of several months.

What those scans revealed, they said, is that instead of one network there are actually two networks sitting side-by-side in numerous areas of the brain. The networks are, in fact, so intertwined that in some regions, one network is literally surrounded by the other.

Though the newly-discovered networks first appeared to be close copies of one another, closer examination reveals one key difference - one network is connected to memory structures while the other isn’t. The similarities suggest both might have originated in similar processes occurring during brain development and evolution. That critical difference, meanwhile, hints at how evolution has specialized the networks for different aspects of thought.

Source:
https://www.eurekalert.org/pub_releases/2017-07/hu-iii071917.php

Journal article:
http://www.cell.com/neuron/fulltext/S0896-6273(17)30562-7

#neuroscience #brainnetwork #research #memory #hippocampus #defaultmodenetwork #braincircuitry

New test shows when body is fighting a virus


New test shows when body is fighting a virus
Researchers at Yale University School of Medicine have shown that a nasal swab test can identify whether viral infections are causing a patient’s respiratory illness by measuring RNA or protein molecules in their cells.

“It’s a simpler test and more cost-effective for looking at viral infection,” says author Ellen Foxman, assistant professor of laboratory medicine at Yale University School of Medicine. “Instead of looking for individual viruses, our test asks the question: ‘Is the body fighting a virus?’ We found we can answer that question very well.”

Journal article:
https://academic.oup.com/jid/advance-article/doi/10.1093/infdis/jix648/4743270

Know more:
https://news.yale.edu/2017/12/21/new-test-shows-when-body-fighting-virus

#research #medicine #virus #infection #RNA #protein #medicaltest #bacteria #viralinfection #laboratorymedicine #illness #labtests #geneticsequencing

Monday, 1 January 2018

BepiColombo is Europe's first mission to Mercury.


BepiColombo is Europe's first mission to Mercury. It will set off in 2018 on a journey to the smallest and least explored terrestrial planet in our Solar System. When it arrives at Mercury in late 2025, it will endure temperatures in excess of 350 °C and gather data during its 1 year nominal mission, with a possible 1-year extension. The mission comprises two spacecraft: the Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (MMO). BepiColombo is a joint mission between ESA and the Japan Aerospace Exploration Agency (JAXA), executed under ESA leadership.

Know more:
http://sci.esa.int/bepicolombo/58591-bepicolombo-launch-rescheduled-for-october-2018/

Watch: https://www.youtube.com/watch?v=susMXnSuN_o

#infographic via Airbus
http://www.airbus.com/newsroom/topics-in-focus/BepiColombo-Mission-to-Mercury.html

#BepiColombo #ESA #JAXA #space #Mercury #exploration #science

Heads Up! A supermoon is coming!


Heads Up! A supermoon is coming!
On January 1, the full Moon will be at or near its closest point in its orbit around Earth, making it a supermoon. Bundle up, get outside and look up!

What's a Super Moon?
A supermoon is a Moon that is full when it is also at or near its closest point in its orbit around Earth. Since the Moon’s orbit is elliptical, one side (apogee) is about 30,000 miles (50,000 km) farther from Earth than the other (perigee). Nearby perigee full Moons appear about 14% bigger and 30% brighter than full Moons that occur near apogee in the Moon's orbit.

Source:
https://science.nasa.gov/science-news/news-articles/a-supermoon-trilogy

Watch: https://www.youtube.com/watch?time_continue=46&v=tARtQkWdZSM

#universe #space #science #NASA #supermoon

Caturday on the 1st Day


Caturday on the 1st Day
Well #caturday is not everyday ;)

Since it is January 1st 2018, I have two suggestions:
- live a life that gives your soul bliss.
- let all the failures of your past year be your best guide in the New Year.

#personalnonsense #NewYear2018