Thursday, 30 November 2017

What's a calorimeter?


What's a calorimeter?
Calorimeters measure the energy a particle loses as it passes through the detector. It is usually designed to stop entire or “absorb” most of the particles coming from a collision, forcing them to deposit all of their energy within the detector. Calorimeters typically consist of layers of “passive” or “absorbing” high-density material – for example, lead – interleaved with layers of an “active” medium such as solid lead-glass or liquid argon.

Electromagnetic calorimeters measure the energy of electrons and photons as they interact with matter. Hadronic calorimeters sample the energy of hadrons (particles that contain quarks, such as protons and neutrons) as they interact with atomic nuclei. Calorimeters can stop most known particles except muons and neutrinos.

The components of the ATLAS calorimetry system are: the Liquid Argon (LAr) Calorimeter and the Tile Hadronic Calorimeter.

Info:
https://atlas.cern/discover/detector/calorimeter

Photo: portion of the Atlas Electromagnetic Calorimeter, CERN- I've seen at Museo Nazionale Scienza e Tecnologia Leonardo da Vinci in Milan.

#physics #calorimeter #Atlas #science #CERN

I like physics, but I love cartoons... or vice versa. :)


I like physics, but I love cartoons... or vice versa. :)

#personalnonsense #life #cartoon

What is secularism?


What is secularism?
Secularism is an increasingly hot topic in public, political, and religious debate across the globe. With discussions on secular schools, secular hospitals, and the move away from religion in modern society in the news, it’s important to know about secularism’s history and how it affects our lives.

Here are five facts about secularism:
1) The term was coined by George Holyoake in 1851. It originally denoted a system which sought to order and interpret life on principles taken solely from this world.

2) Some religious practices have been secularized and made so popular that the associations with religion are not always discussed. Yoga, meditation, and mindfulness are all promoted as secular programs despite their religious roots.

3) Usually secularism focuses on religion however it also demarcates the secular from other phenomena including superstition, the sacred, and the metaphysical.

4) Some perceive the religious decline of our modern world as religion’s role in society changing shape. More individualistic capitalist societies could just be changing the way we engage with belief systems, making them less recognizably religious.

5) Secularism is very different to atheism. A secular society is not necessarily a society in which there is little or no public manifestation of religious belief, it could in fact be the opposite. A secular society is simply one in which the state itself takes a neutral view with respect to religion, and protects the freedom of individuals to believe, or not to believe, to worship, or not to worship.

More on this topic:
http://www.oxfordreference.com/view/10.1093/acref/9780191816819.001.0001/acref-9780191816819-e-137

#secularism #history #thisthat

New Simple Test Could Help Cystic Fibrosis Patients Find Best Treatment


New Simple Test Could Help Cystic Fibrosis Patients Find Best Treatment
Researchers at the University of North Carolina have presented a simple test that aims to determine which treatment for cystic fibrosis (CF) will work best for a given patient.

The test uses nanospheroids, “fuzzy balls” that grow from cells taken from inside the noses of CF patients,as samples for drug testing.

“Any given drug may not be the drug that works best for a given patient, because there’s so much variation from person to person,” said Jennifer Guimbellot, MD, who conducted the research at UNC and is now assistant professor of pediatrics at the University of Alabama at Birmingham.

“We still have a long way to go to get a really optimized therapy for most cystic fibrosis patients, and the only way we can do that is to have a model like ours, where we can take cells from each individual patient and test them with each individual drug to find out which one is the best match.”

Source & further reading:
http://news.unchealthcare.org/news/2017/november/new-simple-test-could-help-cystic-fibrosis-patients-find-best-treatment

Image: These are nasospheroids that developed from a CF patient's nasal tissue in a dish. UNC researchers are using them to screen the effectiveness of CF treatments.

#research #medicine #cysticfibrosis #mucus #lungs #nanospheroids #treatment #CFTR #drugs #hydration #cells #rectal biopsy

Sun Magnetogram

Sun Magnetogram
There is currently a semi-circular quiescent filament suspended above the solar surface along the magnetic inversion line; between magnetic regions of opposite polarity. The magnetogram shows the surface distribution/polarity of the magnetic fields: the black areas are regions of ‘south’ magnetic polarity, and the white regions ‘north’ polarity.

The term magnetogram refers to a pictorial representation of the spatial variations in strength of the solar magnetic field. Magnetograms are often produced by exploiting the Zeeman effect (or, in some cases, the Hanle effect), which George Ellery Hale employed in the first demonstration that sunspots were magnetic in origin, in 1908.

References:
https://www.nasa.gov/content/goddard/sdo-hmi-magnetogram/
https://sdo.gsfc.nasa.gov/

#sun #NASA #magnetogram #science #space

November 30 is reserved to Jonathan Swift


November 30 is reserved to Jonathan Swift
It's Jonathan Swift's 350 B-day, how should we celebrate?
Eating babies, of course ;)

Jonathan Swift (30 November 1667 – 19 October 1745) was an Anglo-Irish satirist, essayist, political pamphleteer (first for the Whigs, then for the Tories), poet and cleric who became Dean of St Patrick's Cathedral, Dublin.

Swift is remembered for works such as A Tale of a Tub (1704), An Argument Against Abolishing Christianity (1712), Gulliver's Travels (1726), and A Modest Proposal (1729). He is regarded by the Encyclopædia Britannica as the foremost prose satirist in the English language, and is less well known for his poetry. He originally published all of his works under pseudonyms – such as Lemuel Gulliver, Isaac Bickerstaff, the Drapier – or anonymously. He was a master of two styles of satire, the Horatian and Juvenalian styles.

His deadpan, ironic writing style, particularly in A Modest Proposal, has led to such satire being subsequently termed "Swiftian".

Bio: https://www.britannica.com/biography/Jonathan-Swift
https://www.biography.com/people/jonathan-swift-9500342

#history #JonathanSwift

Tuesday, 28 November 2017

“Beyond the edge of the world there’s a space where emptiness and substance neatly overlap, where past and future...


“Beyond the edge of the world there’s a space where emptiness and substance neatly overlap, where past and future form a continuous, endless loop. And, hovering about, there are signs no one has ever read, chords no one has ever heard.”
~Kafka on the Shore

Work by bigblueboo

#math #animation #spirals #processing #coding

Acknowledge the power of your own self, you're an amazing creature and that alone should make you a confident driver...


Acknowledge the power of your own self, you're an amazing creature and that alone should make you a confident driver of your own life.

#wordsofwisdom #lickmythoughts

Neutron Stars Rip Each Other Apart to Form Black Hole


Neutron Stars Rip Each Other Apart to Form Black Hole
This supercomputer simulation shows one of the most violent events in the universe: a pair of neutron stars colliding, merging and forming a black hole.

A neutron star is the compressed core left behind when a star born with between eight and 30 times the sun's mass explodes as a supernova. Neutron stars pack about 1.5 times the mass of the sun — equivalent to about half a million Earths — into a ball just 12 miles (20 km) across.

As the simulation begins, we view an unequally matched pair of neutron stars weighing 1.4 and 1.7 solar masses. They are separated by only about 11 miles, slightly less distance than their own diameters. Redder colors show regions of progressively lower density.

As the stars spiral toward each other, intense tides begin to deform them, possibly cracking their crusts. Neutron stars possess incredible density, but their surfaces are comparatively thin, with densities about a million times greater than gold. Their interiors crush matter to a much greater degree densities rise by 100 million times in their centers. To begin to imagine such mind-boggling densities, consider that a cubic centimeter of neutron star matter outweighs Mount Everest.

By 7 milliseconds, tidal forces overwhelm and shatter the lesser star. Its superdense contents erupt into the system and curl a spiral arm of incredibly hot material. At 13 milliseconds, the more massive star has accumulated too much mass to support it against gravity and collapses, and a new black hole is born. The black hole's event horizon — its point of no return — is shown by the gray sphere. While most of the matter from both neutron stars will fall into the black hole, some of the less dense, faster moving matter manages to orbit around it, quickly forming a large and rapidly rotating torus. This torus extends for about 124 miles (200 km) and contains the equivalent of 1/5th the mass of our sun. The entire simulation covers only 20 milliseconds.

Watch & learn:
https://www.youtube.com/watch?v=vw2sLcyV7Vc
Credit: NASA Goddard

#space #NASA #neutrons #blackhole #science

Sunday, 26 November 2017

Flies' disease-carrying potential may be greater than thought, researchers say


Flies' disease-carrying potential may be greater than thought, researchers say
In a study of the microbiomes of 116 houseflies and blowflies from three different continents, researchers found, in some cases, these flies carried hundreds of different species of bacteria, many of which are harmful to humans. Because flies often live close to humans, scientists have long suspected they played a role in carrying and spreading diseases, but this study, which was originally initiated at Penn State's Eberly College of Science, adds further proof, as well as insights into the extent of that threat.

"We believe that this may show a mechanism for pathogen transmission that has been overlooked by public health officials, and flies may contribute to the rapid transmission of pathogens in outbreak situations," said Donald Bryant, Ernest C. Pollard Professor of Biotechnology and professor of biochemistry and molecular biology, Penn State.

Source & further reading:
https://phys.org/news/2017-11-flies-disease-carrying-potential-greater-thought.html#jCp

Image: Researchers used a scan electron microscope to find where bacterial cells and particles attach to the fly body. The electron microscope captures an up close look at the head of a blowfly in this picture.
Credit: Ana Junqueira and Stephan Schuster

#research #bacteria #flies #health

Barophene shines alone as 2D plasmonic material


Barophene shines alone as 2D plasmonic material
An atom-thick film of boron could be the first pure two-dimensional material able to emit visible and near-infrared light by activating its plasmons, according to Rice University scientists.

That would make the material known as borophene a candidate for plasmonic and photonic devices like biomolecule sensors, waveguides, nanoscale light harvesters and nanoantennas.

Plasmons are collective excitations of electrons that flow across the surface of metals when triggered by an input of energy, like laser light. Significantly, delivering light to a plasmonic material in one color (determined by the light's frequency) can prompt the emission of light in another color.

Models by Rice theoretical physicist Boris Yakobson and his colleagues predict that borophene would be the first known 2-D material to do so naturally, without modification.


Source: https://phys.org/news/2017-11-borophene-d-plasmonic-material.html#jCp

#nanotech #plasmons #science #research #scitech

Saturday, 25 November 2017

How to find a star cluster


How to find a star cluster
In the latter years of the 18th century, astronomers William and Caroline Herschel began to count stars. William called the technique "star gauging" and his aim was to determine the shape of our Galaxy.

With this simple technique the Herschels produced the first shape estimate for the Galaxy. Fast-forward to the 21st century and now researchers use star counts to search for hidden star clusters and satellite galaxies. They look for regions where the density of stars rises higher than expected. These patches are called stellar over-densities.

It's the perfect meeting of old and new. Astronomers have combined recent data from ESA's Gaia mission with a simple analysis technique from the 18th century to discover a massive star cluster that had previously escaped detection. Subsequent investigations are helping to reveal the star-forming history of our Galaxy, the Milky Way.

Source & further reading:
http://sci.esa.int/gaia/59741-how-do-you-find-a-star-cluster-easy-simply-count-the-stars/

Video credit: ESA

#stars #galaxy #Gaia #space #research #universe #science #ESA

Parkinson’s Is Partly An Autoimmune Disease, Study Finds


Parkinson’s Is Partly An Autoimmune Disease, Study Finds
Researchers have found the first direct evidence that autoimmunity — in which the immune system attacks the body’s own tissues — plays a role in Parkinson’s disease, the neurodegenerative movement disorder. The findings raise the possibility that the death of neurons in Parkinson’s could be prevented by therapies that dampen the immune response.

The study, led by scientists at Columbia University Medical Center (CUMC) and the La Jolla Institute for Allergy and Immunology, was published in Nature.

“The idea that a malfunctioning immune system contributes to Parkinson’s dates back almost 100 years,” said study co-leader David Sulzer, PhD, professor of neurobiology (in psychiatry, neurology, and pharmacology) at CUMC. “But until now, no one has been able to connect the dots. Our findings show that two fragments of alpha-synuclein, a protein that accumulates in the brain cells of people with Parkinson’s, can activate the T cells involved in autoimmune attacks.

“It remains to be seen whether the immune response to alpha-synuclein is an initial cause of Parkinson’s or if it contributes to neuronal death and worsening symptoms after the onset of the disease,” said study co-leader Alessandro Sette, Dr. Biol. Sci., professor in the Center for Infectious Disease at La Jolla Institute for Allergy and Immunology in La Jolla, Calif. “These findings, however, could provide a much-needed diagnostic test for Parkinson’s disease and could help us to identify individuals at risk or in the early stages of the disease.”

Source and further reading:
http://newsroom.cumc.columbia.edu/blog/2017/06/21/parkinsons-is-partly-an-autoimmune-disease-study-finds/

Journal article:
http://www.nature.com/articles/nature22815

#neuroscience #Parkinson's #alphasynuclein #immunesystem #dopaminergicneurons

Friday, 24 November 2017

24 November is reserved to Charles Darwin


24 November is reserved to Charles Darwin
24 November 1859: Charles Darwin publishes ‘On the Origin of Species’
The publication of Darwin’s letters and reports from South America and the Galapagos islands established his reputation as a geologist of real standing. Among his most important findings was that the finches found on different islands were fundamentally similar in shape, but displayed variations in size and claws – the result, he theorized, of ‘natural selection’.

Read the book online:
http://darwin-online.org.uk/converted/pdf/1861_OriginNY_F382.pdf

Bio:
https://www.biography.com/people/charles-darwin-9266433

#history #evolution #CharlesDarwin

Colored X-ray of the arteries(red) of a human neck and shoulder


Colored X-ray of the arteries(red) of a human neck and shoulder
The bones (purple) are also seen on the X-ray, aiding identification of the arteries. The ribs of the chest are seen from the front. The head has been turned to one side to expose the right-hand side of the neck and its carotid arteries (internal and external). These bring oxygenated blood to the head.

The right arm has been raised to show how the subclavian artery passes under the collar bone (clavicle) and into the arm. The arteries carry oxygenated blood from the heart (not seen). The arteries have been highlighted by arteriography: injecting them with a radio-opaque medium to absorb the X-rays.

Credits: CNRI/Science Photo Library

#medicine #arteries #anatomy #humanbody #science

Wednesday, 22 November 2017

Alnitak, Alnilam, Mintaka


Alnitak, Alnilam, Mintaka
Alnitak, Alnilam, and Mintaka, are the bright bluish stars from east to west (lower right to upper left) along the diagonal in this cosmic vista. Otherwise known as the Belt of Orion, these three blue supergiant stars are hotter and much more massive than the Sun.

They lie from 800 to 1,500 light-years away, born of Orion's well-studied interstellar clouds. In fact, clouds of gas and dust adrift in this region have some surprisingly familiar shapes, including the dark Horsehead Nebula and Flame Nebula near Alnitak at the lower right.

The famous Orion Nebula itself is off the right edge of this colorful starfield. This well-framed, 2-panel telescopic mosaic spans about 4 degrees on the sky.

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

#NASA #space #universe #science #stars #exploartion


“Long hair will send you to hell!” so I cut it to reach the limbo ;)

#personalnonsense

“Almost.


“Almost. It’s a big word for me. I feel it everywhere. Almost home. Almost happy. Almost changed. Almost, but not quite. Not yet. Soon, maybe.”
~ J.Bauer

#wordsofwisdom #almost

Tuesday, 21 November 2017

Life starts from a white hole and ends in a black hole.


Life starts from a white hole and ends in a black hole.
`S. Kalwar

Work by Bees & Bombs
https://beesandbombs.tumblr.com/

#math #processing #animation #coding #circle

Monday, 20 November 2017

"Colorless green ideas sleep furiously."


"Colorless green ideas sleep furiously."
~Noam Chomsky (1928)

Is this a sentence, you ask? In Chomsky's framework, yes it is. Chomsky pointed out that a sentence can be syntactically correct but semantically meaningless. To translate this quote into your daily life, remember that if you're not careful in your choice of language, you can also produce semantically meaningless sentences that have consequences other than what you intended. I remembered this quote when I saw Picasso's drawing...pinches my brain strings - numbing, intoxicating - and yet I find it fascinating. Like a sweet, bad grip of hell...wait...that's sexy! ;)

Photo: The Dream and Lie of Franco - Pablo Picasso (1881-1973)
Peggy Guggenheim Collection, Venice

#personalnonsense #Picasso #Chomsky #pinchmybrainstrings

Big Dipper over Pyramid Mountain


Big Dipper over Pyramid Mountain
When did you first learn to identify this group of stars? Although they are familiar to many people around the world, different cultures have associated this asterism with different icons and folklore. Known in the USA as the Big Dipper, the stars are part of a constellation designated by the International Astronomical Union in 1922 as the Great Bear (Ursa Major). The recognized star names of these stars are (left to right) Alkaid, Mizar/Alcor, Alioth, Megrez, Phecda, Merak, and Dubhe.

Of course, stars in any given constellation are unlikely to be physically related. But surprisingly, most of the Big Dipper stars do seem to be headed in the same direction as they plough through space, a property they share with other stars spread out over an even larger area across the sky.

Their measured common motion suggests that they all belong to a loose, nearby star cluster, thought to be on average only about 75 light-years away and up to 30 light-years across. The cluster is more properly known as the Ursa Major Moving Group. The featured image captured the iconic stars recently above Pyramid Mountain in Alberta, Canada.

What is an asterism?
In astronomy, an asterism is any pattern of stars recognized in the Earth's night sky. It may be part of an official constellation or it may be composed of stars from more than one constellation. Asterisms are composed of stars which, although visible in the same general area of the sky as viewed from Earth, are located at very different distances from Earth, at great distances from each other. Many asterisms are simple shapes composed of a few bright stars, making them easy to identify, and particularly useful to people who are familiarizing themselves with the night sky.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Steve Cullen
https://www.stevecullenmedia.com/about/

#universe #space #NASA #science #asterism #UrsaMajor

Saturday, 18 November 2017

Churning Filament

Churning Filament
A developing filament near the edge of the sun churned and twisted as the rotating sun brought it into clearer view over a day (Nov. 16-17, 2017). Filaments are cooler and often unstable clouds of particles floating above the sun's surface, which are tethered by magnetic forces. In extreme ultraviolet light, they appear darker than the sun's surface. The bright area to the right of the filament is an active region. The loop that appears behind the filament in the middle of the clip is made of charged particles tracing magnetic field lines.

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

#sun #space #SDO #NASA #science #filament #plasma

NGC 7822: Stars and Dust Pillars in Infrared


NGC 7822: Stars and Dust Pillars in Infrared
Young stars themselves are clearing out their nursery in NGC 7822. Within the nebula, bright edges and complex dust sculptures dominate this detailed skyscape taken in infrared light by NASA's Wide Field Infrared Survey Explorer (WISE) satellite. NGC 7822 lies at the edge of a giant molecular cloud toward the northern constellation Cepheus, a glowing star forming region that lies about 3,000 light-years away.

The atomic emission of light by the nebula's gas is powered by energetic radiation from the hot stars, whose powerful winds and light also sculpt and erode the denser pillar shapes. Stars could still be forming inside the pillars by gravitational collapse, but as the pillars are eroded away, any forming stars will ultimately be cut off from their reservoir of star stuff. This field spans around 40 light-years at the estimated distance of NGC 7822.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: WISE, IRSA, NASA; Processing & Copyright : Francesco Antonucci

#NASA #space #universe #nebula #stars #exploration

The Möbius strip — sometimes called the Möbius band — is named after mathematician and astronomer August Ferdinand...


The Möbius strip — sometimes called the Möbius band — is named after mathematician and astronomer August Ferdinand Möbius, who came up with the idea in September 1858. Curiously, German mathematician Johann Benedict Listing independently developed the same idea a few months earlier in July 1858. Unfortunately for Listing, one of the most famous surfaces in mathematics bears the name of Möbius, not Listing.

So what's the big deal with the Möbius strip? It's quite simple, actually. The Möbius strip is famous because it has only one side and one edge.

Read & learn:
http://mathworld.wolfram.com/MoebiusStrip.html
https://wonderopolis.org/wonder/what-is-a-mobius-strip

Animation by OmniDaily
http://omnidaily.tumblr.com/

#mathematics #animation #C4D #mobius #science

What is hyphema?


What is hyphema?
Hyphema is the term for a collection of blood inside the front part of the eye. This happens between the cornea (the clear covering of the eye) and the iris (the colored part of the eye). The blood may cover part or all of the iris and the pupil (the round, dark circle in the middle of your eye). If you have a hyphema, your vision might be partly or totally blocked in that eye.

A hyphema usually happens when an injury causes a tear to the iris or pupil of the eye. Sometimes people mistake a broken blood vessel in the front of the eye for a hyphema. A broken blood vessel in the eye is a common, harmless condition called subconjunctival hemorrhage. A subconjunctival hemorrhage does not hurt. A hyphema, though, is usually painful. A hyphema must be treated properly or it can cause permanent vision problems.

Get informed:
http://www.stanfordchildrens.org/en/topic/default?id=blood-in-the-eye-hyphema-90-P02825
https://www.aao.org/eye-health/diseases/hyphema-symptoms

#medicine #hyphema #health #ophthalmology #eyedisease

Egocentric hearing: Study clarifies how we can tell where a sound is coming from


Egocentric hearing: Study clarifies how we can tell where a sound is coming from
A new UCL and University of Nottingham study has found that most neurons in the brain’s auditory cortex detect where a sound is coming from relative to the head, but some are tuned to a sound source’s actual position in the world.

The study, published in PLOS Biology, looked at whether head movements change the responses of neurons that track sound location.

“Our brains can represent sound location in either an egocentric manner – for example, when I can tell that a phone is ringing to my left – or in an allocentric manner – hearing that the phone is on the table. If I move my head, neurons with an egocentric focus will respond differently, as the phone’s position relative to my ears has changed, while the allocentric neurons will maintain their response,” said the study’s first author, Dr Stephen Town (UCL Ear Institute).

The researchers monitored ferrets while they moved around a small arena surrounded by speakers that emitted clicking sounds. Electrodes monitored the firing rates of neurons in the ferrets’ auditory cortex, while LEDs were used to track the animals’ movement.

Among the neurons under investigation that picked up sound location, the study showed that most displayed egocentric orientations by tracking where a sound source was relative to the animal’s head, but approximately 20% of the spatially tuned neurons instead tracked a sound source’s actual location in the world, independent of the ferret’s head movements.

The researchers also found that neurons were more sensitive to sound location when the ferret’s head was moving quickly.

“Most previous research into how we determine where a sound is coming from used participants with fixed head positions, which failed to differentiate between egocentric and allocentric tuning. Here we found that both types coexist in the auditory cortex,” said the study’s senior author, Dr Jennifer Bizley (UCL Ear Institute).

The researchers say their findings could be helpful in the design of technologies involving augmented or virtual reality.

“We often hear sounds presented though earphones as being inside our heads, but our findings suggest sound sources could be created to appear externally, in the world, if designers incorporate information about body and head movements,” Dr Town said.

Source & further reading:
http://www.ucl.ac.uk/news/news-articles/0617/150617-egocentric-hearing

Journal article:
http://journals.plos.org/plosbiology/article?id=10.1371/journal.pbio.2001878

#neuroscience #hearing #auditorycortex #animalbehavior #neurons #soundlocalization #research

Friday, 17 November 2017

Coronal Hole All Spread Out


Coronal Hole All Spread Out
A broad coronal hole was the dominant feature on the sun (Nov. 7-9, 2017). It was easily recognizable as the dark expanse across the top of the sun and extending down in each side. Coronal holes are magnetically open areas on the sun that allow high-speed solar wind to gush out into space. They always appear darker in extreme ultraviolet. This one was likely the source of bright aurora that shimmered for numerous observers, with some reaching down even to Nebraska.

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

#sun #plasma #universe #science #space #NASA

Wednesday, 15 November 2017

The Tarantula Nebula is more than a thousand light-years in diameter, a giant star forming region within nearby...


The Tarantula Nebula is more than a thousand light-years in diameter, a giant star forming region within nearby satellite galaxy the Large Magellanic Cloud, about 180 thousand light-years away. The largest, most violent star forming region known in the whole Local Group of galaxies, the cosmic arachnid sprawls across this spectacular view composed with narrowband data centered on emission from ionized hydrogen and oxygen atoms.

Within the Tarantula (NGC 2070), intense radiation, stellar winds and supernova shocks from the central young cluster of massive stars, cataloged as R136, energize the nebular glow and shape the spidery filaments. Around the Tarantula are other star forming regions with young star clusters, filaments, and blown-out bubble-shaped clouds. In fact, the frame includes the site of the closest supernova in modern times, SN 1987A, right of center.

The rich field of view spans about 1 degree or 2 full moons, in the southern constellation Dorado. But were the Tarantula Nebula closer, say 1,500 light-years distant like the local star forming Orion Nebula, it would take up half the sky.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit & Copyright: Ignacio Diaz Bobillo

#universe #NASA #nebula #space #science

Insomnia genes found


Insomnia genes found
An international team of researchers has found, for the first time, seven risk genes for insomnia. With this finding the researchers have taken an important step towards the unraveling of the biological mechanisms that cause insomnia.
In addition, the finding proves that insomnia is not, as is often claimed, a purely psychological condition. Nature Genetics published the results of this research.

Insomnia is probably the most common health complaint. Even after treatment, poor sleep remains a persistent vulnerability for many people. By having determined the risk genes, professors Danielle Posthuma (VU and VUmc) and Eus Van Someren (Netherlands Institute for Neuroscience, VU and VUmc), the lead researchers of this international project, have come closer to unraveling the biological mechanisms that cause the predisposition for insomnia.

In a sample of 113,006 individuals, the researchers found 7 genes for insomnia. These genes play a role in the regulation of transcription, the process where DNA is read in order to make an RNA copy of it, and exocytosis, the release of molecules by cells in order to communicate with their environment. One of the identified genes, MEIS1, has previously been related to two other sleep disorders: Periodic Limb Movements of Sleep (PLMS) and Restless Legs Syndrome (RLS).

By collaborating with Konrad Oexle and colleagues from the Institute of Neurogenomics at the Helmholtz Zentrum, München, Germany, the researchers could conclude that the genetic variants in the gene seem to contribute to all three disorders. Strikingly, PLMS and RLS are characterized by restless movement and sensation, respectively, whereas insomnia is characterized mainly by a restless stream of consciousness.

Professor Van Someren, specialized in sleep and insomnia, believes that the findings are the start of a path towards an understanding of insomnia at the level of communication within and between neurons, and thus towards finding new ways of treatment.

Source & further reading:
https://www.vu.nl/en/news-agenda/news/2017/apr-jun/insomnia-genes-found.aspx

Journal article:
https://www.nature.com/articles/ng.3888

#neuroscience #insomnia #sleepdisorders #research

Sunday, 12 November 2017

Why does an anesthetic make us lose consciousness?


Why does an anesthetic make us lose consciousness?
To date, researchers assumed that anesthetics interrupt signal transmission between different areas of the brain and that is why we lose consciousness. Neuroscientists at Goethe University Frankfurt and the Max Planck Institute for Dynamics and Self-Organization in Göttingen have discovered that certain areas of the brain generate less information when under anesthesia. The drop in information transfer often measured when the brain is under anesthesia could be a consequence of this reduced local information generation and not – as was so far assumed – a result of disrupted signal transmission between brain areas.

If only a few telephone calls are made in a city then it could be the case that several telecommunication systems have broken down – or it is nighttime and most people are asleep. The situation is similar in an anesthetized brain: if there is remarkably little information transfer between various areas of the brain then either signal transmission in the nerve fibers is blocked or certain areas of the brain are less active as far as the generation of information is concerned.

Patricia Wollstadt, Favio Frohlich, their colleagues from the Brain Imaging Center at Goethe University Frankfurt and researchers at the MPI for Dynamics and Self-Organization have investigated this second hypothesis. Scientists used ferrets to examine “source” brain areas from which less information was transmitted under anesthesia than in a waking state.

They found that information generation under anesthesia was far more affected there than in the “target” brain areas to which the information was transferred. This indicates that it is the information available in the source area which determines information transfer and not a disruption in signal transmission. Were the latter the case, a far greater reduction could be expected in the target areas since less information “arrives” there.

“The relevance of this alternative explanation goes beyond anesthesia research, says Patricia Wollstadt, “since each and every examination of neuronal information transfer should categorically take into consideration how much information is available locally and is therefore also transferable.”

Journal article:
http://journals.plos.org/ploscompbiol/article?id=10.1371/journal.pcbi.1005511

Source & further reading:
http://www.goethe-university-frankfurt.de/66934196/019

#neuroscience #anesthesia #research #medicine #consciousness

Comet Machholz Approaches the Sun


Comet Machholz Approaches the Sun
Why is Comet Maccholz so depleted of carbon-containing chemicals? Comet 96P/Machholz's original fame derives from its getting closer to the Sun than any other short period comet -- half as close as Mercury -- and doing so every five years.

To better understand this unusual comet, NASA's Sun-monitoring SOHO spacecraft tracked the comet during its latest approach to the Sun in October. The featured image composite shows the tail-enhanced comet swooping past the Sun. The Sun's bright surface is hidden from view behind a dark occulter, although parts of the Sun's extended corona are visible.

Neighboring stars dot the background. One hypothesis holds that these close solar approaches somehow cause Comet Machholz to shed its carbon, while another hypothesis posits that the comet formed with this composition far away -- possibly even in another star system.

Image & info via APOD
https://apod.nasa.gov/apod/astropix.html
Image Credit: NASA, SOHO, LASCO, Barbara Thompson (NASA's GSFC)

#nasa #space #comet #science #SOHO #universe

Saturday, 11 November 2017

Scientists Are Close to Detecting the Elusive Tetraquark Particle


Scientists Are Close to Detecting the Elusive Tetraquark Particle
It’s been 100 years since scientists first split open the atom and realized it was not the smallest thing to exist. It’s been more than 50 years since they started to suspect that the atom’s components— protons, neutrons, and electrons—weren’t either. Protons and neutrons have components of their own, called quarks, which are particles so tiny they’re almost impossible to study.

Electrons and positrons are not made up of quarks. They are in a separate "family" of particles known as leptons. Leptons and quarks are "fundamental" (indivisible) particles. Leptons do not experience the "strong" or "hadronic" force that protons and neutrons do.

A combination of three quarks creates a hadron, which, when stable, we know as a proton or neutron. But a combination of four quarks is something scientists have never been able to prove exists. That would be the tetraquark, which scientists have been chasing without success since the 1960s.

Now, researchers are about to publish what they say is proof that the tetraquark exists, that it’s stable, and that they can generate it in the Large Hadron Collider at the CERN particle physics lab in Switzerland.

Story via live science
https://www.livescience.com/60900-tetraquark-particle-exists.html
http://www.newsweek.com/physics-breakthrough-50-year-search-holy-grail-particle-tetraquark-707569

#physics #tetraquark #research #science

Rare Encircling Filament


Rare Encircling Filament
We came across an oddity this week that our spacecraft has rarely observed before: a dark filament encircling an active region (Oct. 29-31, 2017). Solar filaments are clouds of charged particles that float above the sun, tethered to it by magnetic forces.

They are usually elongated and uneven strands. Only a handful of times before have we seen one shaped like a circle. (The black area to the left of the brighter active region is a coronal hole, a magnetically open region of the sun).

Credit: Solar Dynamics Observatory, NASA.
https://sdo.gsfc.nasa.gov/gallery/potw/item/854

#sun #solarfilament #nasa #space #universe

Distinct wiring mode found in chandelier cells


Distinct wiring mode found in chandelier cells
A basic tenet of neural development is that young neurons make far more connections than they will actually use, with very little specificity. They selectively maintain only the ones that they end up needing. Once many of these connections are made, the brain employs a use-it or lose-it strategy; if the organism’s subsequent experiences stimulate the synapse, it will strengthen and survive. If not, the synapse will weaken and eventually disappear.

Researchers from Hiroki Taniguchi’s lab at the Max Planck Florida Institute for Neuroscience (MPFI) published a study in eNeuro in May 2017 showing for the first time that a unique type of inhibitory interneuron called chandelier cells – which are implicated in several diseases affecting the brain such as schizophrenia and epilepsy – seem to develop their connections differently than other types of neurons.

Neurons have several dendrites – thin protrusions through which they receive input from many other cells, but only one axon, where all the information the cell receives is integrated and sent as a single outgoing signal. Most cells’ axons reach out and form synapses on other cells’ dendrites or cell bodies, but chandelier cells exclusively inhibitory synapse on other cells’ axon initial segments (AIS), right where the cell begins to send its own signal down the axon. At this location, the chandelier cells have a greater impact on other cell’s behavior. “Chandelier cells are the final gatekeeper of the action potential,” said Dr. Taniguchi. “We believe this role makes them an especially important factor in controlling epilepsy, where over-excitement spreads throughout the brain unchecked”.

Using their own recently-developed genetic labeling techniques for tracking these cells in early development in mice, Taniguchi and his team observed that, like most neurons, the cells remodeled their axonal organization through development. They also found excessive axonal varicosities that have been considered morphologically synaptic structures.
To investigate whether these varicosities actually contained synaptic molecules, the team expressed synaptic markers in the chandelier cells using transplantation techniques.

What they found was surprising. Only those varicosities that were associated with the AIS contained synapses – the rest appeared to be empty throughout development. This was also corroborated by their ultrastructures obtained with electron microscopy. These findings provide a big clue to understanding how this important cell type properly wires a unique circuit.

Source & further reading:
https://www.maxplanckflorida.org/news-and-media/news/distinct-wiring-mode-found-in-chandelier-cells/

Journal article:
http://www.eneuro.org/content/4/3/ENEURO.0057-17.2017

Gif: Brain biology by MIT

#neuroscience #medicine #neurons #brain #research #chandeliercells

Thursday, 9 November 2017

Elizabeth Stern is probably one of the most significant physician-scientists who worked at the interface of...


Elizabeth Stern is probably one of the most significant physician-scientists who worked at the interface of epidemiology and cancer in the mid-20th century, but it is unlikely you have ever heard her name. You won’t read about Stern’s research in medical textbooks, or find any symposiums or departments dedicated to her memory. But her groundbreaking research led the way to our modern understanding of the prevention, diagnosis and treatment of cervical cancer.

She found that patients diagnosed with dysplasia at the start of the study were at significantly higher risk for cervical cancer. Stern would go on to lead over a dozen epidemiological studies providing nearly irrefutable proof that dysplasia is an early marker of cervical cancer.

Of all of Stern’s achievements, perhaps her most lasting legacy is in the modern technology of the Pap test. She collaborated with the Jet Propulsion Laboratory (JPL) and Rosenthal, then the head cytopathologist at U.C.L.A, to apply NASA computer imaging technology to Pap screening.

Stern developed a liquid-based sampling system to isolate and enrich the cervical epithelium, and helped define cellular criteria for computer programs. The work she did at JPL revolutionized Pap screening for cervical cancer, and her liquid-based sampling technique is still used in hospitals, laboratories, and clinics around the world.

Story via Scientific American
https://blogs.scientificamerican.com/voices/one-more-pioneering-woman-in-science-youve-probably-never-heard-of/

Bio:
https://www.biography.com/people/elizabeth-stern-38623

#womeninstem #ElizabethStern #cervicalcancer #research #history #PAPsmear

Williamina Fleming's Triangular Wisp


Williamina Fleming's Triangular Wisp
Chaotic in appearance, these tangled filaments of shocked, glowing gas are spread across planet Earth's sky toward the constellation of Cygnus as part of the Veil Nebula. The Veil Nebula itself is a large supernova remnant, an expanding cloud born of the death explosion of a massive star. Light from the original supernova explosion likely reached Earth over 5,000 years ago.

Blasted out in the cataclysmic event, the interstellar shock waves plow through space sweeping up and exciting interstellar material. The glowing filaments are really more like long ripples in a sheet seen almost edge on, remarkably well separated into the glow of ionized hydrogen atoms shown in red and oxygen in blue hues. Also known as the Cygnus Loop, the Veil Nebula now spans nearly 3 degrees or about 6 times the diameter of the full Moon.

While that translates to over 70 light-years at its estimated distance of 1,500 light-years, this field of view spans less than one third that distance. Often identified as Pickering's Triangle for a director of Harvard College Observatory, the the complex of filaments is cataloged as NGC 6979. It is also known for its discoverer, astronomer Williamina Fleming, as Fleming's Triangular Wisp.

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

#space #NASA #science #nebula #universe

Wednesday, 8 November 2017

Immortalized human skin cells (HaCaT keratinocytes) expressing fluorescently tagged keratin


Immortalized human skin cells (HaCaT keratinocytes) expressing fluorescently tagged keratin
Dr. Bram van den Broek reveals an exceptional and microscopic view of something we see every day — our skin. The image depicts a cell expressing an excessive amount of keratin, seen here fluorescently labeled in yellow.

Keratin is an important structural protein in skin cells. The keratin fibrous network protects the cells against mechanical stress, and is involved in many other cellular functions, like cell migration and adhesion. Studying the structure, dynamics and regulation of the keratin network can reveal information about such processes. In certain types of cancer, for instance, reduced amounts of specific keratins are indicative for tumor aggressiveness.

This photo won 1st Place
2017 Photomicrography Competition

Credits: Dr. Bram van den Broek, Andriy Volkov, Dr. Kees Jalink, Dr. Reinhard Windoffer & Dr. Nicole Schwarz

The Netherlands Cancer Institute
BioImaging Facility & Department of Cell Biology
Amsterdam, The Netherlands

Magnification40x (objective lens magnification)
Technique:Confocal

#keratin #skin #biology #medicine #micrograph

“You are unstoppable


“You are unstoppable,
not because you do not
have failures or doubts,
but because you continue
on despite them.”
~B.Taplin

#wordsofwisdom #unstoppable

NGC 1055 Close-up


NGC 1055 Close-up
Big, beautiful spiral galaxy NGC 1055 is a dominant member of a small galaxy group a mere 60 million light-years away toward the aquatically intimidating constellation Cetus. Seen edge-on, the island universe spans over 100,000 light-years, a little larger than our own Milky Way.

The colorful stars in this cosmic close-up of NGC 1055 are in the foreground, well within the Milky Way. But the telltale pinkish star forming regions are scattered through winding dust lanes along the distant galaxy's thin disk.

With a smattering of even more distant background galaxies, the deep image also reveals a boxy halo that extends far above and below the central bluge and disk of NGC 1055. The halo itself is laced with faint, narrow structures, and could represent the mixed and spread out debris from a satellite galaxy disrupted by the larger spiral some 10 billion years ago.

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

#space #NASA #universe #science #NGC1055 #galaxies

Monday, 6 November 2017

Circles


Circles
Life is a circle. It spins you around.
~ L. Cvetanova

Work by bigblueboo

#math #animation #processing #coding

How to Turn Damaged Heart Tissue Back into Healthy Heart Muscle: New Details Emerge


How to Turn Damaged Heart Tissue Back into Healthy Heart Muscle: New Details Emerge
Researchers at the University of North Carolina School of Medicine report that they have used single cell RNA sequencing technology along with other techniques to sort out the details of how fibroblasts, scar tissue cells, can turn into cardiomyocytes, heart muscle cells, creating new healthy heart muscle.

“Some of what we found is clinically important,” Li Qian, PhD, assistant professor of pathology and laboratory medicine at the UNC School of Medicine, said, “For example, we know that after a heart attack, cardiac fibroblasts around the injured area are immediately activated and become highly proliferative but this proliferative capacity decreases over time. How to take advantage of the varied cell cycle status of fibroblasts over the progression of a heart attack and its aftermath would certainly broaden the application of cellular reprogramming for patients and optimize outcomes.”

Source & further reading:
http://news.unchealthcare.org/news/2017/october/how-to-turn-damaged-heart-tissue-back-into-healthy-heart-muscle-new-details-emerge

Image:
These are induced cardiomyocytes (iCMs) that Li Qian's lab produced in experiments turning scar tissue into healthy heart muscle.

#research #medicine #heartmuscle #fibroblasts #cardiomyocytes #pathology #laboratorymedicine #heartattack #cardiacfibroblasts #singlecellRNAsequencing #technology #science

Beacons of life could help researchers identify potentially habitable worlds


Beacons of life could help researchers identify potentially habitable worlds
Traditionally, researchers have sought potential biosignatures as ways of identifying inhabited worlds: byproducts from life as we know it such as oxygen or methane that over time accumulate in the atmosphere to detectable amounts. But with current technology, according to Vladimir Airapetian, lead author of a Nature Scientific Reports study published on Nov. 2, 2017, identifying these gases on distant terrestrial exoplanets is time-consuming, requiring days of observation time. The new study suggests hunting for cruder signatures of potentially habitable worlds instead, which would be easier to detect with current resources in less time.

“We’re in search of molecules formed from fundamental prerequisites to life — specifically molecular nitrogen, which is 78 percent of our atmosphere,” said Airapetian, who is a solar scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and at American University in Washington, D.C. “These are basic molecules that are biologically friendly and have strong infrared emitting power, increasing our chance of detecting them.”

Present life on Earth tells Airapetian and his team of researchers they should look for atmospheres rich with water vapor and nitrogen, and oxygen, the product of life. Oxygen and nitrogen free-float stably in their molecular form — that is, two atoms of either oxygen or nitrogen bound together in one molecule. But in the vicinity of an active dwarf star, extreme space weather sparks distinct chemical reactions, which researchers can use as indicators of atmospheric composition.

Source & further reading:
https://www.nasa.gov/feature/goddard/2017/atmospheric-beacons-guide-nasa-scientists-in-search-for-life

Journal article:
https://www.nature.com/articles/s41598-017-14192-4

Credits: NASA’s Goddard Space Flight Center/Mary Pat Hrybyk

#nasa #astrobiology #science #atmosphericbeacons #research #universe #space

Sunday, 5 November 2017

Reflection nebula NGC 1999


Reflection nebula NGC 1999
This spooky sight, imaged by the NASA/ESA Hubble Space Telescope, resembles fog lit by a streetlamp swirling around a curiously shaped hole – and there is some truth in that. While the ‘fog’ is dust and gas lit up by the star, the ‘hole’ really is an empty patch of sky.

When the dark patch was first imaged, it was assumed to be a very cold, dense cloud of gas and dust, so thick as to be totally opaque in visible light, and blocking all light behind it. In general, such globules are known to be small cocoons of forming stars, but thanks to ESA’s Herschel Space Observatory, which would have been able to see any hints of star formation at infrared wavelengths but did not, along with ground-based observations, it turned out to be a truly empty patch of sky.

Astronomers think that is was formed when jets of gas from some of the young stars in the wider region punctured the sheet of dust and gas that forms the surrounding nebula. The powerful radiation from a nearby mature star may also have helped to clear the hole.

The bright star seen here is V380 Orionis, a young star 3.5 times the mass of our own Sun. It appears white owing to its high surface temperature of about 10 000ºC – nearly twice that of the Sun. The star is so young that it is still surrounded by a cloud of material left over from its formation. This bright material in the area pictured here is only visible because of the light from the star; it does not emit any visible light of its own. This is the signature of a ‘reflection nebula’ – this one is known as NGC 1999.

Image & info via ESA
http://www.esa.int/spaceinimages/Images/2017/10/Reflection_nebula_NGC_1999

Credit: NASA and The Hubble Heritage Team (STScI)

#ESA #space #Hubble #nebula #science #NGC1999

Whale breaching


Whale breaching
When a humpback whale breaches, he essentially jumps out of the water and whirls around -- often numerous times in a row, but sometimes merely once.

The precise motives behind humpback whale breaching behavior are uncertain, according to the Whale Trust organization. However, a variety of different theories on the action do exist. One such theory is the transmission of messages. A humpback whale might, for example, want to convey to a fellow whale that he's planning on changing his course.

Breaching in humpback whales also could be a territorial action, suggests the Petersburg Marine Mammal Center. If a wary humpback whale senses an approaching intrusion or menace, he might attempt to intimidate them away from his personal turf by breaching.

Breaching could also be a standard cleanliness routine, nothing more and nothing less. By breaching, a humpback whale could simply be using motion to remove any pesky parasites that could be residing on his body.

More info:
http://animals.mom.me/meaning-humpback-whale-breaching-5781.html

#biodiversity #whalebreaching #coolcritters #marinelife

How neurons use crowdsourcing to make decisions


How neurons use crowdsourcing to make decisions
How do we make decisions? Or rather, how do our neurons make decisions for us? Do individual neurons have a strong say or is the voice in the neural collective?

One way to think about this question is to ask how many of my neurons you would have to observe to read my mind. If you can predict I am about to say the word “grandma” by watching one of my neurons then we could say our decisions can be attributed to single, perhaps “very vocal,” neurons. In neuroscience such neurons are called “grandmother” neurons after it was proposed in the 1960’s that there may be single neurons that uniquely respond to complex and important percepts like a grandmother’s face.

On the other hand, if you can only read my mind by polling many of my neurons then it would appear the decision a collective one, distributed across hundreds, thousands, or even millions of neurons. A big debate in neuroscience is whether single-neuron encoding or distributed encoding is most relevant for understanding how the brain functions.

In fact, both may be right. In research recently published in Frontiers in Neuroscience, Bryan Daniels, Jessica Flack, and David Krakauer tackle this problem using data recorded from the neurons of a macaque monkey tasked by the experimenter with making a simple decision.

In an area of the brain involved in the decision-making process, Daniels and colleagues find that as the monkey initially processes the data, polling many neurons is required to get a good prediction of the monkey’s decision. Then, as the time for committing to a decision approaches, this pattern shifts. The neurons start to agree and eventually each one on its own is maximally predictive. Hence at first the “neural voice” is heterogeneous and collective, but as the neurons get close to the decision point, the “neural voice” becomes homogenous and, in a sense, individualistic, as any neuron on its own is sufficient to read the monkey’s mind.

Daniels says a possible explanation for this odd behavior is that the system has two tasks to solve. It must gather good information from noisy data and it must use this information to produce a coherent decision. To find regularities in the input it polls many individual neurons, as the crowd’s answer is more reliable than any single neuron’s when the data are noisy. But, as Krakauer says, ultimately a decision has to be made. The neurons agree on an answer by sharing their information to come to a consensus.

This explanation echoes results in other collective systems, from animal societies to systems studied in statistical physics. Flack says this commonality suggests a general principle of collective computation: It has two phases — an information accumulation phase that uses crowdsourcing to collect reliable information and a consensus phase that allows the system to act.

Source & further reading:
https://www.santafe.edu/news-center/news/how-neurons-use-crowdsourcing-make-decisions

Journal article:
https://www.frontiersin.org/articles/10.3389/fnins.2017.00313/full

#decisionmaking #neurons #grandmothercell #neuroscience #research

Saturday, 4 November 2017

A Year of Full Moons


A Year of Full Moons
Do all full moons look the same? No. To see the slight differences, consider this grid of twelve full moons. From upper left to lower right, the images represent every lunation from 2016 November through 2017 October, as imaged from Pakistan.

The consecutive full moons are all shown at the same scale, so unlike the famous Moon Illusion, the change in apparent size seen here is real. The change is caused by the variation in lunar distance due to the Moon's significantly non-circular orbit. The dark notch at the bottom of the full moon of 2017 August is the shadow of the Earth -- making this a partial lunar eclipse.

Besides the sometimes exaggerated coloring, a subtler change in appearance can also be noticed on close examination, as the Moon seems to wobble slightly from one full moon to the next. This effect is known as libration.

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

#nasa #moon #space #universe #science #libration

From hot to hottest


From hot to hottest
This sequence of images shows the sun from its surface to its upper atmosphere all taken at about the same time (Oct. 27, 2017). The first shows the surface of the sun in filtered white light; the other seven images were taken in different wavelengths of extreme ultraviolet light. Note that each wavelength reveals somewhat different features.

They are shown in order of temperature from the first one at 6,000 degree C. surface out to about 10 million degrees C. in the upper atmosphere. Yes, the sun's outer atmosphere is much, much hotter than the surface. Scientists are getting closer to solving the processes that generate this phenomenon.

Credit: Solar Dynamics Observatory, NASA.
https://sdo.gsfc.nasa.gov/gallery/potw/item/852

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