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Sunday, June 16, 2019

Transmissions for Sale

Transmissions for Sale


To learn a little about what other kinds of civilizations are possible, we can study history and cultural anthropology. But we are all of us - us whales, us apes, us people – too closely related. As long as our inquiries are limited to one or two evolutionary lines on a single planet, we will remain ignorant of the possible range and brilliance of other intelligences and other civilizations.

Thus we are looking for other intelligences using different means and methods. For example, we suppose that most of other civilization will use powerful sources to transmit their notions and ideas. Some of our most powerful sources are radar transmitters; a few are used for radar astronomy, to probe with radio fingers the surfaces of the nearby planets.

As the Earth rotates, our more powerful radio transmitters slowly sweep the sky. A radio astronomer on a planet of another star would be able to calculate the length of the day on Earth from the times of appearance and disappearance of our signals. The size of the radar beam projected against the sky is much larger than the size of the planets, and much of the signal wafts on, out of the solar system into the depths of interstellar space to any sensitive receivers that may be listening.

On Earth, most radar transmissions are for military purposes as they scan the skies in constant fear of a massive launch of missiles with nuclear warheads, and augury fifteen minutes early of the end of human civilization. The information content of these pulses is negligible: a succession of simple numerical patterns coded into beeps.

Overall, the most pervasive and noticeable source of radio transmissions from the Earth is our television programming. Because the Earth is turning, some television stations will appear at on horizon of the Earth while others disappear over the other. There will be a jumble of programs. These might be sorted out and pieced together by an advanced civilization on a planet of a nearby star.

Large-scale television transmission on the planet Earth began only in the late 1940’s. There is no calling those television programs back. There is no way of sending a faster message to overtake them and revise the previous transmission. Nothing can travel faster than light.

Thus, there is a spherical wave front centered on the Earth expanding at the speed of light.

Because these transmissions were broadcast a few decades ago, they are only a few tens of light-years away from Earth. Hum… the most frequently repeated messages will be and appeals to purchase detergents, headache tablets, deodorants, automobile and petroleum products.

The most noticeable messages will be those broadcast simultaneously by many transmitters in many time zones – for example, speeches in times of international crisis.

If the nearest civilization is about 100 years away, then we can continue to breathe easy for a while. In any case, we can hope that they will find these programs incomprehensible.

The mindless contents of commercial television and the integuments of international crisis and warfare within the human family are the principal messages about life on Earth that we choose to broadcast to the Cosmos. What must they think of us? Image : © Megan Jorgensen.

Theory of Clouds

The Theory of Clouds


Stéphane Audeguy, Harcourt, Inc. 2007. English translation by Timothy D. Bent

For quite a long time, Kumo told her, scientists never thought about why the sky was blue. It was of course the same then as now – apparently monochromatic yet consisting of a nearly infinite variety of shades. Thousands of poets wrote about it being azure or cerulean, but not a single scientist bothered to explain why this was so. The poets’ evocations were scarcely better than what the scholar-priests offered, for they were not truly interested in the sky’s blueness so much as in turning it into a symbol – the color of eternity from the palette of God. It was as if they couldn’t accept the idea that the blue was simply and sublimely of its own creation.

Centuries passed and as science became less a servant of the church the skies were emptied of angels and divinity, filled instead with men on balloons or planes. What came to be understood was that the sky only seemed blue. Explanations followed as to why this was so. The sun has no sense of color, the light it emits is of no color in particular or, rather, all of them. It bombards the Earth atmosphere with light of every wavelength, from red to violet and everything in between – orange, yellow, green, blue and indigo. But these colors never reach us; as soon as they reach the upper layers of the atmosphere they strike up against tiny air molecules. These air molecules diffract small quantities of light, though not in uniform fashion – they are better of diffusing shorter waves of light than longer ones. That’s why the air in the sky won’t diffuse red, orange or yellow light. But it is very good at diffusing blue, and better still at violet. Most of the colors emitted by the sun thus never reach our retina. That, say scientists, is why the sky is violet. So why does the sky look blue and not violet? Because the eyes of men, even the eyes of men of science, are unable to distinguish violet. We perceive the sky’s color as blue just as we sense that the earth is flat or that the sun rises and sets every day.

Little by little people learn how to survive. Photo by Elena.

Increasingly, people – ordinary observers, devoted amateurs, gentlemen farmers – began keeping weather journals as they were called, in which, day after day, they noted wind direction, the state of the sky in the morning and evening, rainfall amounts, and so forth. The more people shielded themselves from the weather the more they seemed to talk about it, perhaps to pass the time. Meteorologists were persuaded they were on the verge of wrestling from the rain and wind all of their innermost secrets. Meteorological societies were formed, congresses convened, and journals published.

These men of science advanced things. Little by little they learned how clouds formed – doing away with a number of even the venerable Luke Howard’s own hypotheses on the subject. They had no difficulty getting funding for their research, because their interests intersected perfectly with a seemingly infinite number of financial interests. Steel-hulled ships, very often British and growing in number, were plowing the seas of the world; large office buildings were going up in Geneva and Washington and Berlin and Paris, in which workers used rulers and ink pens to create rectilinear boundaries along what had previously been beautifully round.

Empires built to last a thousand years were founded and then disappeared in less than a hundred. More and more people went off to fight and die in distant corners of the world, in villages with strange-sounding names, villages whose existence they had not known of six months before – like Sebastopol or Falluja. The fate of the world depended upon what happened on the seas: It was a war of commerce, as much as war of the more traditional sort. England was in its Golden Age, dealing in spices and rare perfumes, amassing diamonds and opals, construction white-stoned temples to commerce in its enormous capital city.

Now that the island nation of sailors ruled the universe, weather became a serious matter. On Septembre 5, 1860, the Times of London published its first weather announcement. Five years later, on April 30, 1865, Admiral Robert Fitzroy, director of the Meteorological Department at the National Chamber of Commerce, committed suicide because his department had issued an egregiously inaccurate forecast and the press had hounded him for it. As the world was being circumnavigated more and more often, and more and more quickly, it was being learned that climatic phenomena did much the same thing. Simultaneously, it was being learned how high the costs of not understanding the sky and its movements could prove. The Agriculture Ministry had estimated that the total annual value of agricultural production worldwide, including horticulture and tree-farming, to be somewhere around 100 million pounds sterling, and, estimating that an annual 5 percent growth in productivity would result from more precise meteorological predictions and their communication to those concerned (farmers, for example), reliable forecasting had a potential value of 20 million pounds sterling. Simply identifying clouds would no longer do. One had to predict their movements, their behaviour. In 1879, the inhabitants of Dundee and the entire region were thrilled when a metal bridge was constructed to span the Bay of Tay, making it no longer necessary to go around this body of water, reducing travel time to Edinburgh by a three full hours. Britani’s finest engineers had designed the bridge.

Several times a day, heavy iron trains crossed the bridge without causing so much as a shake. A few journalists speculated about the danger of conveyance at such high speeds – close to thirty miles an hour – that would be unleashed upon the world. In the spring of 1879, after five months of reliable service, the magnificent new bridge tumbled into the river whose waters it spanned, taking with it the train that happened to be crossing it and all its passengers (Note of Univers.grandquebec.com: Actually the disaster took place on December 28, 1879, not in spring). The collapse was blamed on a series of strong wind gusts that none of the engineers had been imaginative enough to take into account. The newspapers were savage in their denunciations. Public opinion turned sour. A few elected officials tendered their resignations and, as always in cases such as this, someone took his life. Several amateur meteorologists wrote memoirs establishing that the architect had not considered wind speeds in the region. It was decided that a new bridge should be built in the same spot; this one, however, would not collapse.

Despite the occasional setbacks, British technology was unrivaled in the world; at the beginning of that same year, for example, it had permitted Her Majesty’s Army to slaughter eight thousand Zulu warriors during the course of several weeks in southern Africa. The Zulus had charged across a plain on foot, spears in their hands, using wooden shields covered with zebra skins, straight into professional soldiers equipped with the finest rifles available. On March 29, 1879, at the Battle of Rorke’s Drift, a regiment withstood a siege that endured for several days and killed a thousand native warriors in the process. Those who survived the siege were decorated.

The great and powerful nations of Europe were seeking a way of predicting storms. There were of course always storms, as well as farmers who feared them. But never before had these storms caused quite so many factories to be blown away, or house roofs to be carried off, or cattle and men sent to their doom. In short, never before had so much been at stake. On November 14, 1854, during the Crimean War, a number of warships and commercial vessels – a total of thirty-eight of them, all flying French colors – sank in the middle of Balaklava, in the North Sea. Four hundred souls were lost. Napoleon III summoned the Minister of War, to learn how he could have managed to lose so many lives and an entire fleet, including the mighty three-masted Henry IV. In an attempt to save face, the Minister of War in turn summoned the director of the Paris Observatory. The director’s name was Urbain Le Verrier. Le Verrier had no difficulty demonstrating to the minister that the evening before it had hit, the storm had been brewing over the Mediterranean, and that two days before this it had been attacking the inhabitants of Europe’s northwest regions. A telegram might have averted the whole disaster. Le Verrier was given an audience with the emperor, who wanted to know how such a thing might be accomplished. The director then wrote to every amateur astronomer and meteorologist he could find throughout Europe. Most scientists of the day spent most of their time writing each other about their discoveries anyway. The director’s request was straightforward: Could his honored colleagues relay to him their observations about the weather in their regions between November 12 and November 16? He received two hundred and fifty replies, which he posted on a map of Europe in order to track the storm’s path. Such a system had a fatal flaw of course. What good was predicting weather that had already happened? Le Verrier therefore was allocated funds to establish weather stations throughout his native land. The era of individual weather-watching had ended; the moment of the network had arrived. Before long, other countries – Holland, England, Sweden, and Russia – followed France’s example.

Clouds. Illustration by Elena.

Friday, June 14, 2019

Mind-Body Problem

The Easy and the Hard Mind-Body Problem


David Chalmers – one of the philosophers participating in the interdisciplinary field of “cognitive science” - argues that one aspect of the mind-body problem is “easy” and the other “hard.” (Chalmers, 1995). In this way, he divides the issue into two separate problems.

The easy problem is the one that mots neuroscientists are concerned with, and it is the one discussed by crick in his Scientific Search for the Soul. Crick attempts to solve the problem by neuroscientific means. His research strategy is to try to find the specific neural processes that are the correlates of our conscious awareness (he calls them the “neural correlates of consciousness,” or NCC for short). Finding the neural correlates of consciousness is a problem of the same general type as finding the neural correlates of anything – language or memory, for instance. Neuroscience has made great progress in solving such problems in the past. Finding the brain regions and processes that correlate with consciousness is simply a matter of directing an existing research strategy from areas of previous success (language, memory) onto a different aspect of mental functioning (consciousness).

We should not underestimate the difficulty of finding the neural correlates of consciousness, but Crick is only looking for which brain regions or processes correlate with consciousness and describing where they reside. He does not attempt to explain how that particular pattern of physiological events makes us conscious. This is the hard problem. The hard problem is a conundrum of a different magnitude – it raises the question of how consciousness (“you, your joys and your sorrow, your memories and your ambitions...”) actually emerges from matter. Modern neuroscience is well equipped to solve the easy problem, but it is less clear whether it is capable of solving the hard problem. Science has few precedents for solving a problem philosophers have deemed insoluble in principle.

A “thought experiment” is an imaginary experiment; the experiment is not really conducted. Photo by Elena. 

John Searle, another contemporary philosopher with a great interest in this problem, suggests the following thought experiment. Pinch yourself (hard) on your left hand. What happens? You feel pain, of course – it is sore. This is an expression of the mind-body problem : something physical happened to your hand, and yet you felt a pain in your mind. Let us see, in terms of the easy problem, how we fare in explaining this phenomenon.

We know exactly what the pain receptors embedded in your skin look like, and how they work. When pressure is applied yo these receptors, a very specific physical process excites the neurons connected with them. This sends a message down these neurons (causes them to fire), which in turn causes a chemical to cross the synaptic spaces at the ends of the axons – using the chemical-dependent neurotransmitter systems. The axons in question travel through a nerve coursing up the arm into the spinal cord and the brainstem, these axons terminate on a second set of neurons in the thalamus. From there the physiological message is relayed again, to a specific part of the primary sensory cortex of the right hemisphere. The pain receptors in the left hand are represented in a specific region of the somatosensory cortex in the parietal lobe, and that is where the nerve fibers we have been tracing terminate. (Pain receptors from other parts of the body map to different regions in the somatosensory cortex, as suggested by the dashed lines). Excitation of the cortical cells in this area causes you to feel pain. This solves (this particular instance of) the easy problem – these are the physiological processes that cause you to feel pain in your hand.

But it is not difficult to see that the hard problem remains entirely unsolved. What turned the physiology, anatomy, and chemistry just described into a feeling of pain? How did that happen?  We have just outlined a purely physiological process (and traced the anatomical pathways it traversed); we have not explained how the process started as something physical but somehow ended up as something mental. Searle used a memorable phrase to describe the hard problem we are left with: “How does the brain get over the hump from electrochemistry to feeling?”

This sort of question was traditionally considered to be a philosophical problem, but it is now being treated as a scientific one – one that might be addressed experimentally.

The Brain and the Inner World, Introduction to Basic Concepts. Mark Solms, Oliver Turnbull.

Do the trees have their own brains? Photo by Elena.

Autism

Autism and Case of Autism

Redesigning the brain


The mystery of autism – a human mind that cannot conceive of other minds – is one of the most baffling and poignant in psychiatry, and one of the most severe developmental disorders of childhood. It is called a “pervasive developmental disorder,” because so many aspects of development are disturbed: intelligence, perception, socializing skills, language, and emotion.

Most autistic children have an IQ of less than 70. They have major problems connecting socially to others and may, in severe cases, treat people like inanimate objects, neither greeting them nor acknowledging them as human beings. At times it seems that autistics don't have a sense that “other minds” exist in the world. They also have perceptual processing difficulties and are thus often hypersensitive to sound and touch, easily overloaded by stimulation. (That may be one reason autistic children often avoid eye contact: the stimulation from people, especially when coming from many senses at once, is too intense). Their neural networks appear to be overactive, and many of these children have epilepsy.

Because so many autistic children have language impairments, clinicians began to suggest  the Fast ForWord program for them. They never anticipated what might happen. Parents of autistic children who did Fast ForWord told Merzenich that their children became more connected socially. He began asking, were the children simply being trained to be more attentive listeners? And he was fascinated by the fact that with Fast ForWord both the language symptoms and the autistic symptoms seemed to be fading together. Could this mean that the language and autistic problems were different expressions of a common problem?

Two studies of autistic children confirmed what Merzenich had been hearing. One, a language study, showed that Fast ForWord quickly moved autistic children from severe language impairment to the normal range. But another pilot study of one hundred autistic children showed that Fast ForWord had a significant impact on their autistic symptoms as well. Their attention spans improved. Their sense of humor improved. They became more connected to people. They developed better eye contact, began greeting people and addressing them by name, spoke with them, and said good-bye at the end of their encounters. It seemed the children were beginning to experience the world as filled with other human minds.

The incidence of autism has been climbing at a staggering rate that can't be explained by genetics alone. Photo by Elena.

Case of Autism


Lauralee, an eight-year-old autistic girl, was diagnosed with moderate autism when she was three. Even as an eight-year-old she rarely used language. She didn't answer to her name, and to her parents, it seemed she was not hearing it. Sometimes she would speak, but when she did, “she had her own language,” says her mother, “which was often unintelligible.” If she wanted juice, she didn't ask for it.  She would make gestures and pull her parents over to the cabinets to get things for her.

She had other autistic symptoms, among them the repetitive movements that autistic children use to try to contain their sense of being overwhelmed. According to her mother, Lauralee had “the whole works – the flapping of the hands, toe-walking, a lot of energy, biting. And she couldn't tell me what she was feeling.”

She was very attached to trees. When her parents took her walking in the evening to burn off energy, she'd often stop, touch a tree, hug it, and speak to it.

Lauralee was unusually sensitive to sounds.  “She had bionic ears,” says her mother. “When she was little, she would often cover her hears. She couldn't tolerate certain music on the radio, like classical and slow music.” At her pediatrician's office she heard sounds from the floor upstairs that others didn't. At home she would go over to the sinks, fill them with water, then wrap herself around the pipes, hugging them, listening to the water drain through them.

Lauralee's father is in the navy and served in the Iraq war in 2003. When the family was transferred to California, Lauralee was enrolled in a public school with a special-ed class that used Fast ForWord. The program took her about two hours a day for eight weeks to complete.

When she finished it, “she had an explosion in language,” says her mother, “and began to speak more and use complete sentences. She could tell me about her days at school. Before I would just say, :Did you have a good day or a bad day?” Now she was able to say what she did, and she remembered details. If she got into a bad situation, she would be able to tell me, and I wouldn't have to prompt her to get it out of her. She also found it easier to remember things.” Lauralee has always loved to read, but now she is reading longer books, non-fiction and the encyclopedia. “She is listening to quieter sounds now and can tolerate different sounds from the radio,” says her mother. “It was an awakening for her. And with the better communication, there was an awakening for all of us. It was a big blessing.”

By Norman Doidge (excerpt from The Brain That Changes Itself).

Better communication can help to an awakening. Illustration by Elena.

Super Earth

Planet KOI-172.02 - Super Earth


KOI-172.02, which stands for Kepler Object of Interest, is a super Earth-size planet, meaning it has a radius 1.5-2 times the size of the Earth. While that may seem insignificant, it means that its mass is much more than that of the Earth, resulting in different properties such as a thicker gaseous atmosphere. It has been described as the most similar to our home planet yet.

The Kepler Mission, launched by NASA in March 2009, was specifically designed to survey a portion in our region of the Milky Way Galaxy to discover Earth-sized planets near the habitable zone, and to determine realistically how many of the billions of stars in our galaxy have such planets. The habitable zone is the region around a star where water might exist on the surface of a planet which provide favorable conditions for life.

The mission is designed to detect orbiting planets as they pass in front of their stars, causing a small decrease in the star’s brightness.

The Kepler Spacecraft and photometer, used to observe the stars, orbits the sun each year trailing behind the Earth. This spacecraft has found over 2,500 planets.

Kepler found planets by looking at just one large region of the Milky Way in the constellations Lyra and Cygnus. This region of space was picked due to certain limiting constraints; an environment rich in stars as well as one that can be continuously viewed and monitored throughout the mission “without obstruction of the Sun to the regions at any point of the spacecraft’s orbit”, say Dr. Howell, Deputy Project Scientist of the Kepler Mission at Ames.

Over the course of the mission, the Kepler spacecraft measures the variations in brightness, using the photometer, of 150.000 stars every 30 minutes, searching for tiny dips in the light output that occurs whenever a potential planet passes or “transits” in front of its star. Depending on the planet’s orbit and the type of star it orbits, this effect can last anywhere between an hour to about half a day.

Transits are only seen when a star’s planetary system is perfectly aligned with our line of sight, so if all the orbits are randomly distributed, as it should be, then Kepler – even if every star had a planet – would only see 1% of those stars having transits.

This is called “transit method” and is Kepler’s principal method in finding planets.

Regardless, the data received from the spacecraft is extensive in its own merit. Dozens of thousands of transit-like signals were analyzed and potential new planets were identified. Since not all variations in brightness necessarily represent a transit of a potential planet, there exist false positives. For example, there exist stars much like our Sun which can vary in brightness themselves. Such temporary phenomenon include “Sunspots” which create visible dark spots caused by intense magnetic activity. For that reason, the discovery of a planet is confirmed by observing a minimum of three transits.

Why three transits constitute a candidate planet? According to Dr. Alan Gould, co-investigator of the Kepler mission, the need for three transits explains as follows: Three transits are required for planet discovery by the transit method mainly because that is the minimum to assure that there is in fact a planet. One transit gives only the barest indication that a planet exists and an extremely rough idea at best of what the period of the planet might be. Two transits would pinpoint the period of the planet pretty pretty precisely, by virtue of the time between transits and allow accurate prediction of when the next transit is expected to occur. Actual observation of the third transit confirms the prediction and hence helps confirm the planet discovery”.

This would mean planets that are Earth-like and orbit around a star like our sun (every year) would take at least 3 years to get the three transits needed to be confirmed by Kepler to be a candidate planet. Once the planet candidate has been observed, it is then given the designation of KOI – Kepler Object of Interest). In terms of this new Super-Earth candidate KOI-172.02, it was the 172nd candidate in their running list of candidates to see if it really is a planet and has the right kind of star.

For the KOI-172.02 in particular, the 4 transit signals acquired by Kepler indicate that the planet orbits its star around every 243 days. We also know a lot about the star which KOI-172.02 orbits, which is very similar to our sum, but slightly smaller and colder.

The nominal mission of Kepler was 3.5 years, ending October 2012. Then it was in what NASA calls the extended mission. The next couple of years, Kepler started providing many more planets around stars like the sun that are much more like the Earth.

We have begun to contemplate our origins. Our loyalties are to the species and the planet. We speak for Earth. Image : © Megan Jorgensen.