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Gordon E. Moore, the Intel Co-Founder Behind Moore’s Law, Dies at 94
His prediction in the 1960s about exponential advances in computer chip technology charted a course for the age of high tech.
Image
Gordon E. Moore in 1990 at the Silicon Valley headquarters of Intel, which he founded in 1968 with Robert Noyce.
Gordon E. Moore in 1990 at the Silicon Valley headquarters of Intel, which he founded in 1968 with Robert Noyce. Credit...Alamy
By Holcomb B. Noble and Katie Hafner
March 24, 2023, 9:36 p.m. ET
6 MIN READ
Gordon E. Moore, a co-founder and former chairman of Intel Corporation, the California semiconductor chip maker that helped give Silicon Valley its name, achieving the kind of industrial dominance once held by the giant American railroad or steel companies of another age, died on Friday at his home in Hawaii. He was 94.
His death was confirmed by Intel and the Gordon and Betty Moore Foundation. They did not provide a cause.
Along with a handful of colleagues, Mr. Moore could claim credit for bringing laptop computers to hundreds of millions of people and embedding microprocessors into everything from bathroom scales, toasters and toy fire engines to cellphones, cars and jets.
Mr. Moore, who had wanted to be a teacher but could not get a job in education and later called himself the Accidental Entrepreneur, became a billionaire as a result of an initial $500 investment in the fledgling microchip business, which turned electronics into one of the world’s largest industries.
Story continues below advertisement
And it was he, his colleagues said, who saw the future. In 1965, in what became known as Moore’s Law, he predicted that the number of transistors that could be placed on a silicon chip would double at regular intervals for the foreseeable future, thus increasing the data-processing power of computers exponentially.
He added two corollaries later: The evolving technology would make computers more and more expensive to build, yet consumers would be charged less and less for them because so many would be sold. Moore’s Law held up for decades.
Through a combination of Mr. Moore’s brilliance, leadership, charisma and contacts, as well as that of his partner and Intel co-founder, Robert Noyce, the two assembled a group widely regarded by many as among the boldest and most creative technicians of the high-tech age.
This was the group that advocated the use of the thumbnail-thin chips of silicon, a highly polished, chemically treated sandy substance — one of the most common natural resources on earth — because of what turned out to be silicon’s amazing hospitality in housing smaller and smaller electronic circuitry that could work at higher and higher speeds.
Story continues below advertisement
With its silicon microprocessors, the brains of a computer, Intel enabled American manufacturers in the mid-1980s to regain the lead in the vast computer data-processing field from their formidable Japanese competitors. By the ’90s, Intel had placed its microprocessors in 80 percent of the computers that were being made worldwide, becoming the most successful semiconductor company in history.
Much of his happened under Mr. Moore’s watch. He was chief executive from 1975 to 1987, when Andrew Grove succeeded him, and remained as chairman until 1997.
As his wealth grew, Mr. Moore also became a major figure in philanthropy. In 2001, he and his wife created the Gordon and Betty Moore Foundation with a donation of 175 million Intel shares. In 2001, they donated $600 million to the California Institute of Technology, the largest single gift to an institution of higher learning at the time. The foundation’s assets currently exceed $8 billion and it has given away more than $5 billion since its founding.
In interviews, Mr. Moore was characteristically humble about his achievements, particularly the technical advances that Moore’s Law made possible.
Story continues below advertisement
“What I could see was that semiconductor devices were the way electronics were going to become cheap. That was the message I was trying to get across,” he told the journalist Michael Malone in 2000. “It turned out to be an amazingly precise prediction — a lot more precise than I ever imagined it would be.”
Not only was Mr. Moore predicting that electronics would become much cheaper over time, as the industry shifted from away from discrete transistors and tubes to silicon microchips, but over the years his prediction proved so reliable that technology firms based their product strategy on the assumption that Moore’s Law would hold.
“Any business doing rational multiyear planning had to assume this rate of change or else get steamrolled,” said Harry Saal, a longtime Silicon Valley entrepreneur.
“That’s his legacy,” said Arthur Rock, an early investor in Intel and friend of Mr. Moore’s. “It’s not Intel. It’s not the Moore Foundation. It’s that phrase: Moore’s Law.”
Image
Mr. Moore during Intel’s early days. His prediction, a few years earlier, that the number of transistors that could be placed on a silicon chip would double at regular intervals became known as Moore’s Law.
Mr. Moore during Intel’s early days. His prediction, a few years earlier, that the number of transistors that could be placed on a silicon chip would double at regular intervals became known as Moore’s Law.Credit...Intel
Gordon Earl Moore was born on Jan. 3, 1929, in San Francisco. He grew up in Pescadero, a small coastal town south of San Francisco, where his father, Walter H. Moore, was deputy sheriff and the family of his mother, the former Florence Almira Williamson, ran the general store.
Mr. Moore enrolled at San Jose State College (now San José State University), where he met Betty Whitaker, a journalism student. They married in 1950. That year, he completed his undergraduate studies at the University of California, Berkeley, with a degree in chemistry. In 1954, he received his doctorate, also in chemistry, from the Caltech.
One of the first jobs he applied for was as a manager with Dow Chemical. “They sent me to a psychologist to see how this would fit,” Mr. Moore wrote in 1994. “The psychologist said I was OK technically but I’d never manage anything.”
So Mr. Moore took a position with the Applied Physics Laboratory at Johns Hopkins University in Maryland. Then, looking for a way back to California, he interviewed at Lawrence Livermore Laboratory in Livermore, Calif. He was offered a job, “but I decided I didn’t want to take spectra of exploding nuclear bombs, so I turned it down,” he wrote.
Instead, in 1956, Mr. Moore joined William Shockley, the inventor of the transistor, to work at a West Coast division of Bell Laboratories, a start-up unit whose aim was to make a cheap silicon transistor.
But the company, Shockley Semiconductor, foundered under Mr. Shockley, who had no experience running a company. In 1957, Mr. Moore and Mr. Noyce joined a group of defectors who came to be known as “the traitorous eight.” With each putting in $500, along with $1.3 million in backing from the aircraft pioneer Sherman Fairchild, the eight men left to form the Fairchild Semiconductor Corporation, which became a pioneer in manufacturing integrated circuits.
Bitten by the entrepreneurial bug, Mr. Moore and Mr. Noyce decided in 1968 to form their own company, focusing on semiconductor memory. They wrote what Mr. Moore described as a “very general” business plan.
“It said we were going to work with silicon … and make interesting products,” he said in an interview in 1994.
Their vague proposal notwithstanding, they had no trouble finding financial backing.
With $2.5 million in capital, Mr. Moore and Mr. Noyce called their start-up Integrated Electronics Corporation, and later shortened it to Intel. The third employee was Mr. Grove, a young Hungarian immigrant who had worked under Mr. Moore at Fairchild.
After some indecision around what technology to focus on, the three men settled on a new version of MOS — metal oxide semiconductor — technology called silicon-gate MOS. To improve a transistor’s speed and density, they used silicon instead of aluminum.
“Fortunately, very much by luck, we had hit on a technology that had just the right degree of difficulty for a successful start-up,” Mr. Moore wrote in 1994. “This was how Intel began.”
In the early 1970s, Intel’s 4000 series “computer on a chip” began the revolution in personal computers, although Intel itself missed the opportunity to manufacture a PC, which Mr. Moore blamed partly on his own shortsightedness.
“Long before Apple, one of our engineers came to me with the suggestion that Intel ought to build a computer for the home,” he wrote. “And I asked him, ‘What the heck would anyone want a computer for in his home?”
Image
Mr. Moore holding a silicon wafer in 2005. Silicon was a key to Intel’s success.
Mr. Moore holding a silicon wafer in 2005. Silicon was a key to Intel’s success.Credit...Paul Sakuma/Associated Press
Still, he saw the future. In 1963, while still at Fairchild as director of research and development, Mr. Moore contributed a book chapter describing what was to become the precursor to his eponymous law, without the explicit numerical prediction. Two years later, he published an article in Electronics, a widely circulated trade magazine, titled, “Cramming More Components Onto Integrated Circuits.”
“The article presented the same argument as the book chapter, with the addition of this explicitly numerical prediction,” said David Brock, a co-author of “Moore’s Law: The Life of Gordon Moore, Silicon Valley’s Quiet Revolutionary.”
There is little evidence that many people read the article when it was published, Mr. Brock said.
“He kept giving talks with these charts and plots, and people started using his slides and reproducing his graphs,” Mr. Brock said. “Then people saw the phenomenon happen. Silicon microchips got more complex, and their cost went down.”
In the 1960s, when Mr. Moore began in electronics, a single silicon transistor sold for $150. Later, $10 would buy more than 100 million transistors. Mr. Moore once wrote that if cars advanced as quickly as computers, “they would get 100,000 miles to the gallon and it would be cheaper to buy a Rolls-Royce than park it. (Cars would also be a half an inch long.)”
Mr. Moore’s survivors include his wife, and his sons Kenneth and Steven, as well as four grandchildren.
In 2014, Forbes estimated Mr. Moore’s net worth at $7 billion. Yet he remained unprepossessing throughout his life, preferring tattered shirts and khakis to tailored suits. He shopped at Costco and kept a collection of fly lures and fishing reels on his office desk.
Moore’s Law is bound to reach its end, as engineers encounter some basic physical limits, as well as the extreme cost of building factories to achieve the next level of miniaturization. And in recent years, the pace of miniaturization has slowed.
Mr. Moore himself commented from time to time on the inevitable end to Moore’s Law. “It can’t continue forever,” he said in a 2005 interview with Techworld magazine. “The nature of exponentials is that you push them out and eventually disaster happens.”
Holcomb B. Noble, a former science editor for The Times, died in 2017.
Katie Hafner, a former staff reporter for The New York Times, is a co-author of "Where Wizards Stay Up Late: The Origins of The Internet."
How The Times decides who gets an obituary. If you made news in life, chances are your death is news, too. There is no formula, scoring system or checklist. We investigate, research and ask around before settling on our subjects.
Learn more about our process.
Recommended Newsletters
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Times Journeys
(I'm sorry for not updating my photostream for a while. I almost spent a week thinking of an excuse, lol.)
Yeah, Spain won against Germany! :D WOOHOOO!
Have you heard of Paul the Octopus? I heard it was the one which can predict the results for the World Cup! Last time, Paul predicted that Spain will win... and he was right. Sounds crazy, I know, but try to find it on YouTube!
Gordon E. Moore, the Intel Co-Founder Behind Moore’s Law, Dies at 94
His prediction in the 1960s about exponential advances in computer chip technology charted a course for the age of high tech.
Image
Gordon E. Moore in 1990 at the Silicon Valley headquarters of Intel, which he founded in 1968 with Robert Noyce.
Gordon E. Moore in 1990 at the Silicon Valley headquarters of Intel, which he founded in 1968 with Robert Noyce. Credit...Alamy
By Holcomb B. Noble and Katie Hafner
March 24, 2023, 9:36 p.m. ET
6 MIN READ
Gordon E. Moore, a co-founder and former chairman of Intel Corporation, the California semiconductor chip maker that helped give Silicon Valley its name, achieving the kind of industrial dominance once held by the giant American railroad or steel companies of another age, died on Friday at his home in Hawaii. He was 94.
His death was confirmed by Intel and the Gordon and Betty Moore Foundation. They did not provide a cause.
Along with a handful of colleagues, Mr. Moore could claim credit for bringing laptop computers to hundreds of millions of people and embedding microprocessors into everything from bathroom scales, toasters and toy fire engines to cellphones, cars and jets.
Mr. Moore, who had wanted to be a teacher but could not get a job in education and later called himself the Accidental Entrepreneur, became a billionaire as a result of an initial $500 investment in the fledgling microchip business, which turned electronics into one of the world’s largest industries.
Story continues below advertisement
And it was he, his colleagues said, who saw the future. In 1965, in what became known as Moore’s Law, he predicted that the number of transistors that could be placed on a silicon chip would double at regular intervals for the foreseeable future, thus increasing the data-processing power of computers exponentially.
He added two corollaries later: The evolving technology would make computers more and more expensive to build, yet consumers would be charged less and less for them because so many would be sold. Moore’s Law held up for decades.
Through a combination of Mr. Moore’s brilliance, leadership, charisma and contacts, as well as that of his partner and Intel co-founder, Robert Noyce, the two assembled a group widely regarded by many as among the boldest and most creative technicians of the high-tech age.
This was the group that advocated the use of the thumbnail-thin chips of silicon, a highly polished, chemically treated sandy substance — one of the most common natural resources on earth — because of what turned out to be silicon’s amazing hospitality in housing smaller and smaller electronic circuitry that could work at higher and higher speeds.
Story continues below advertisement
With its silicon microprocessors, the brains of a computer, Intel enabled American manufacturers in the mid-1980s to regain the lead in the vast computer data-processing field from their formidable Japanese competitors. By the ’90s, Intel had placed its microprocessors in 80 percent of the computers that were being made worldwide, becoming the most successful semiconductor company in history.
Much of his happened under Mr. Moore’s watch. He was chief executive from 1975 to 1987, when Andrew Grove succeeded him, and remained as chairman until 1997.
As his wealth grew, Mr. Moore also became a major figure in philanthropy. In 2001, he and his wife created the Gordon and Betty Moore Foundation with a donation of 175 million Intel shares. In 2001, they donated $600 million to the California Institute of Technology, the largest single gift to an institution of higher learning at the time. The foundation’s assets currently exceed $8 billion and it has given away more than $5 billion since its founding.
In interviews, Mr. Moore was characteristically humble about his achievements, particularly the technical advances that Moore’s Law made possible.
Story continues below advertisement
“What I could see was that semiconductor devices were the way electronics were going to become cheap. That was the message I was trying to get across,” he told the journalist Michael Malone in 2000. “It turned out to be an amazingly precise prediction — a lot more precise than I ever imagined it would be.”
Not only was Mr. Moore predicting that electronics would become much cheaper over time, as the industry shifted from away from discrete transistors and tubes to silicon microchips, but over the years his prediction proved so reliable that technology firms based their product strategy on the assumption that Moore’s Law would hold.
“Any business doing rational multiyear planning had to assume this rate of change or else get steamrolled,” said Harry Saal, a longtime Silicon Valley entrepreneur.
“That’s his legacy,” said Arthur Rock, an early investor in Intel and friend of Mr. Moore’s. “It’s not Intel. It’s not the Moore Foundation. It’s that phrase: Moore’s Law.”
Image
Mr. Moore during Intel’s early days. His prediction, a few years earlier, that the number of transistors that could be placed on a silicon chip would double at regular intervals became known as Moore’s Law.
Mr. Moore during Intel’s early days. His prediction, a few years earlier, that the number of transistors that could be placed on a silicon chip would double at regular intervals became known as Moore’s Law.Credit...Intel
Gordon Earl Moore was born on Jan. 3, 1929, in San Francisco. He grew up in Pescadero, a small coastal town south of San Francisco, where his father, Walter H. Moore, was deputy sheriff and the family of his mother, the former Florence Almira Williamson, ran the general store.
Mr. Moore enrolled at San Jose State College (now San José State University), where he met Betty Whitaker, a journalism student. They married in 1950. That year, he completed his undergraduate studies at the University of California, Berkeley, with a degree in chemistry. In 1954, he received his doctorate, also in chemistry, from the Caltech.
One of the first jobs he applied for was as a manager with Dow Chemical. “They sent me to a psychologist to see how this would fit,” Mr. Moore wrote in 1994. “The psychologist said I was OK technically but I’d never manage anything.”
So Mr. Moore took a position with the Applied Physics Laboratory at Johns Hopkins University in Maryland. Then, looking for a way back to California, he interviewed at Lawrence Livermore Laboratory in Livermore, Calif. He was offered a job, “but I decided I didn’t want to take spectra of exploding nuclear bombs, so I turned it down,” he wrote.
Instead, in 1956, Mr. Moore joined William Shockley, the inventor of the transistor, to work at a West Coast division of Bell Laboratories, a start-up unit whose aim was to make a cheap silicon transistor.
But the company, Shockley Semiconductor, foundered under Mr. Shockley, who had no experience running a company. In 1957, Mr. Moore and Mr. Noyce joined a group of defectors who came to be known as “the traitorous eight.” With each putting in $500, along with $1.3 million in backing from the aircraft pioneer Sherman Fairchild, the eight men left to form the Fairchild Semiconductor Corporation, which became a pioneer in manufacturing integrated circuits.
Bitten by the entrepreneurial bug, Mr. Moore and Mr. Noyce decided in 1968 to form their own company, focusing on semiconductor memory. They wrote what Mr. Moore described as a “very general” business plan.
“It said we were going to work with silicon … and make interesting products,” he said in an interview in 1994.
Their vague proposal notwithstanding, they had no trouble finding financial backing.
With $2.5 million in capital, Mr. Moore and Mr. Noyce called their start-up Integrated Electronics Corporation, and later shortened it to Intel. The third employee was Mr. Grove, a young Hungarian immigrant who had worked under Mr. Moore at Fairchild.
After some indecision around what technology to focus on, the three men settled on a new version of MOS — metal oxide semiconductor — technology called silicon-gate MOS. To improve a transistor’s speed and density, they used silicon instead of aluminum.
“Fortunately, very much by luck, we had hit on a technology that had just the right degree of difficulty for a successful start-up,” Mr. Moore wrote in 1994. “This was how Intel began.”
In the early 1970s, Intel’s 4000 series “computer on a chip” began the revolution in personal computers, although Intel itself missed the opportunity to manufacture a PC, which Mr. Moore blamed partly on his own shortsightedness.
“Long before Apple, one of our engineers came to me with the suggestion that Intel ought to build a computer for the home,” he wrote. “And I asked him, ‘What the heck would anyone want a computer for in his home?”
Image
Mr. Moore holding a silicon wafer in 2005. Silicon was a key to Intel’s success.
Mr. Moore holding a silicon wafer in 2005. Silicon was a key to Intel’s success.Credit...Paul Sakuma/Associated Press
Still, he saw the future. In 1963, while still at Fairchild as director of research and development, Mr. Moore contributed a book chapter describing what was to become the precursor to his eponymous law, without the explicit numerical prediction. Two years later, he published an article in Electronics, a widely circulated trade magazine, titled, “Cramming More Components Onto Integrated Circuits.”
“The article presented the same argument as the book chapter, with the addition of this explicitly numerical prediction,” said David Brock, a co-author of “Moore’s Law: The Life of Gordon Moore, Silicon Valley’s Quiet Revolutionary.”
There is little evidence that many people read the article when it was published, Mr. Brock said.
“He kept giving talks with these charts and plots, and people started using his slides and reproducing his graphs,” Mr. Brock said. “Then people saw the phenomenon happen. Silicon microchips got more complex, and their cost went down.”
In the 1960s, when Mr. Moore began in electronics, a single silicon transistor sold for $150. Later, $10 would buy more than 100 million transistors. Mr. Moore once wrote that if cars advanced as quickly as computers, “they would get 100,000 miles to the gallon and it would be cheaper to buy a Rolls-Royce than park it. (Cars would also be a half an inch long.)”
Mr. Moore’s survivors include his wife, and his sons Kenneth and Steven, as well as four grandchildren.
In 2014, Forbes estimated Mr. Moore’s net worth at $7 billion. Yet he remained unprepossessing throughout his life, preferring tattered shirts and khakis to tailored suits. He shopped at Costco and kept a collection of fly lures and fishing reels on his office desk.
Moore’s Law is bound to reach its end, as engineers encounter some basic physical limits, as well as the extreme cost of building factories to achieve the next level of miniaturization. And in recent years, the pace of miniaturization has slowed.
Mr. Moore himself commented from time to time on the inevitable end to Moore’s Law. “It can’t continue forever,” he said in a 2005 interview with Techworld magazine. “The nature of exponentials is that you push them out and eventually disaster happens.”
Holcomb B. Noble, a former science editor for The Times, died in 2017.
Katie Hafner, a former staff reporter for The New York Times, is a co-author of "Where Wizards Stay Up Late: The Origins of The Internet."
How The Times decides who gets an obituary. If you made news in life, chances are your death is news, too. There is no formula, scoring system or checklist. We investigate, research and ask around before settling on our subjects.
Learn more about our process.
Recommended Newsletters
times journeys special offer
Times Journeys
Nostradamus was born in Saint Rémy de Provence, southern France, on December 14th of 1503, and he was a famous French physician, cabalist, and pharmacist, best known for his book Les Prophéties, its first edition published in 1555. Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece www.yearly-horoscope.org/nostradamus-2021-predictions. Nostradamus’ prophecies are expressed in verses, called quatrains. Many of his predictions, such as the rise to power of Adolf Hitler, and the Second World War, turned out to be accurate. Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece www.yearly-horoscope.org/nostradamus-2021-predictions
Nostradamus had written 6338 prophecies, many of them fulfilled. His prophecies cover a period reaching the year 3797. The secret of his predictions is not known. Nostradamus’ quatrains continue to fascinate the world, although they were written almost five centuries ago. Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece www.yearly-horoscope.org/nostradamus-2021-predictions..
Here are some of Nostradamus’ predictions for 2021: 1. Zombie Apocalypse A Russian scientist will create a biological weapon and produce a virus that can turn humankind into zombies, and we will all be extinct in the near future. “Few young people: half−dead to give a start. Dead through spite, he will cause the others to shine, And in an exalted place some great evils to occur: Sad concepts will come to harm each one, Temporal dignified, the Mass to succeed. Fathers and mothers dead of infinite sorrows, Women in mourning, the pestilent she−monster: The Great One to be no more, all the world to end.” 2. A Famine of Biblical Proportions Nostradamus predicted that the first signs of the end of the world would be famine, earthquakes, different illnesses, and epidemics, which are already happening more frequently. The Coronavirus pandemic from 2020 represents the beginning of a series of unfavorable events, which will affect the world’s population. The famine that lurks is one the world had never faced before. A catastrophe of huge proportions will throw us back in history, and a great part of the world population will not be able to overcome this curse. “After great trouble for humanity, a greater one is prepared, The Great Mover renews the ages: Rain, blood, milk, famine, steel, and plague, Is the heavens fire seen, a long spark running.” Starting from 2020, after 248 years, Saturn in Capricorn united its forces with Pluto, which is also in Capricorn, in the remarkable conjunction that will change the fate of the world. Saturn in Capricorn is responsible for social hierarchies, state power, authority, functions, and status, and this is what the conjunction with Pluto, the planet of death, destruction, and reconstruction triggered. 3. Solar Storms 2021 will be quite a significant year in terms of major global events. Great solar storms will take place, which could cause some major damages to the earth. Nostradamus supposedly warned: „We shall see the water rising and the earth falling under it”. The harmful effects of the climatic changes will then lead to many wars and conflicts, as the world will fight over resources, and mass migration will follow. 4. A Comet will hit the Earth or it will come very close to Terra This event will cause earthquakes and other natural disasters, which can be concluded from the quatrain: “In the sky, one sees fire and a long trail of sparks”. Other interpretations of this quatrain assert that it refers to a great asteroid that will hit the Earth. Once it enters the Earth’s atmosphere, the asteroid will heat up, appearing in the sky like a great fire. NASA announced that a huge asteroid is likely to hit the Earth in the next years after the American agency emits alerts daily, only this time, it is something more serious. An asteroid called 2009 KF1 has chances to hit the Earth on May 6th of 2021, the NASA coming to this conclusion, following analyzes regarding its trajectory. NASA claims that this asteroid has the power to hit the Earth with the equivalent of 230 kilotons of TNT explosive force, which means 15 times more than the nuclear bomb detonated by Americans over Hiroshima in 1945. 5. A Devastating Earthquake Will Destroy California According to the interpretation of a quatrain written by Nostradamus, an extremely powerful seism will destroy California in 2021. Nostradamus predicts that a great earthquake will hit the New World (“the western lands”), and California is the logical place where it might happen. According to the astrologers, “Mercury in Sagittarius, Saturn fading”, the following date when the planets Mars and Saturn will be in this position on the sky will be on November 25th of 2021. Nostradamus’ quatrain: “The sloping park, great calamity, Through the Lands of the West and Lombardy The fire in the ship, plague, and captivity; Mercury in Sagittarius, Saturn fading.” 6. The American Soldiers Will Have Brain Chip Implants The American soldiers will be turned into a kind of cyborgs, at least at the brain level, to save the human race. This chip should offer us the necessary digital intelligence to progress beyond the limits of biological intelligence. This could mean that we will incorporate artificial intelligence into our bodies and brains. The newly made one will lead the army, Almost cut off up to near the bank: Help from the Milanais elite straining, The Duke deprived of his eyes in Milan in an iron cage.
Conclusions: “A prophet is properly speaking one, who sees distant things through a natural knowledge of all creatures. And it can happen that the prophet bringing about the perfect light of prophecy may make manifest things both human and divine.” (Nostradamus in a letter to his son, Cesar) Nostradamus’ quatrains include many disturbing predictions. Based both on the knowledge of Nostradamus as a human being, and the dangerous era he lived, the eight prophecies of 2021 reveal fragments of what the alchemist predicted for our world.
Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece www.yearly-horoscope.org/nostradamus-2021-predictions/
By watching aspects such as climate changes, technological evolution, or inadequate governmental decisions, we might think that everything is against us, and humankind is on the verge of extinction. Here are just a few of Nostradamus’ predictions, outlining the idea of a terrifying future, far from what we would have imagined.
Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece wisehoroscope.org/nostradamus-2021/.ficial Intelligence – The Robots will rule the world From 2021, artificial intelligence will be equal or will even surpass human intelligence, which could lead to an apocalyptic scenario like those we see in movies. “The Moon in the full of night over the high mountain, The new sage with a lone brain sees it: By his disciples invited to be immortal, Eyes to the south. Hands in bosoms, bodies in the fire.” Mechanization Most previsions indicate that until 2023, the labor market will crash. The automated machines will replace the people in the work process, since they don’t demand higher salaries, and they don’t need breaks or other benefits. When employers choose robots instead of humans, the whole social model will crush. Unemployment, social disorders, and misery are just a few of the consequences of mechanization. A War between Two Allied Countries Two allied countries will get into a classic and open military conflict, with naval fleet fully engaged against each other. Unfortunately, this will only be the beginning because this conflict between these two seemingly “friendly” countries will degenerate into a global war, which will involve the most powerful countries in the world. “In the city of God there will be a great thunder Two brothers torn apart by Chaos while the fortress endures The great leader will succumb The third big war will begin when the big city is burning”. The Economic Collapse of 2021 Hundreds of closed hedge funds will go bankrupt, and the international exchange market will need to close in a short time – maybe even for a week, to stop the panic of selling shares, that will slowly envelop the stock markets. Nostradamus also predicted the 2008 crisis, and in 2021, things are not great: the exchange markets are in free fall and have reached panic levels the end of the crisis is still out of sight the United States is facing an economic stagnation for several years the economic fundamentals are no longer applying today. Space Flight will be Accessible to Common People In 2021, it will start a new era of space tourism. Common people will fly into space, being able to admire spectacular views of the Earth. Sea Level Rise There is no doubt: the climate is constantly changing. Out of all the apocalyptic scenarios which might come true, the sea level rise is the most dramatic. Presently, 50% of the world population lives in coastal areas. A prediction of a possible disaster can be seen by following the example of Newton City from Alaska, which, in less than five years, will be swallowed up by rising waters. The small community of 400 people will not be the only one affected. The current estimations suggest that Venice will be uninhabitable by 2100, and Los Angeles and Amsterdam will be abandoned five years later. “Peace and plenty for a long time the place will praise: Throughout his realm the fleur-de-lis deserted: Bodies dead by water, land one will bring there, Vainly awaiting the good fortune to be buried there.” Solar Eruptions The solar activity has been and still is a subject of interest for experts and not only. Because the sun will reach, in 2021, the peak of an 11-years cycle, known as the maximum solar, different theoreticians rushed to speculate in this regard. It is a fact that when a maximum solar occurs, much more intense solar explosions take place than the previous ones, but this does not translate into total chaos or natural catastrophe. Solar eruptions don’t just happen from yesterday but occur at regular intervals, and the event taking place in 2021 could mostly announce satellite communication interruptions. “Condom and Auch and around Mirande, I see fire from the sky which encompasses them. Sun and Mars conjoined in Leo, then at Marmande, lightning, great hail, a wall falls into the Garonne.” How many predictions did Nostradamus get right? A part of Nostradamus’s prophecies, the famous French doctor and alchemist from the 16th century, have come true. Nostradamus predicted the beginning of the Second World War, Hitler’s ascension, the fall of communism, President J. F. Kennedy’s assassination, India’s independence and the occurrence of Israel State on the world map, events confirmed by the passing of time, but also occurrences that go further in time. Read also: Horoscope 2021 for every zodiac sign. Things You Might Not Know About Nostradamus Nostradamus is certainly one of the most illustrious personalities in history. This notoriety is due to his famous prophecies and predictions. Beyond astrology, Nostradamus was a talented doctor, but also a controversial character, specialized in occultism. Everyone has heard of Nostradamus. He was a medieval character, renowned for his capacity to predict, through scientific methods, the events that will happen in the distant future. Nostradamus predictions, written around 500 years ago, are still going around the world today, and the French man is one of the most important figures of occult art. Besides astrology and his predictions regarding the future, Nostradamus had an adventurous love life, marked by long journeys, extrasensory experiences, the run from Inquisition, but also by an exceptional, yet unjustly less-mentioned medical career. Nostradamus aroused admiration, but also envy. Moreover, he was a controversial character. Nostradamus confessed that his predictions have a scientific fundament. He claimed that he managed to predict the future by calculating the position of the stars and planets towards the earth and other astral bodies. How Nostradamus died Nostradamus even predicted his death: ‘Next to the bench and bed, I will be found dead’. After he announced, one evening, that he will not survive the night, he died of a gout episode and was found dead the following morning, next to his worktable
Feel free to publish a summary of this article (in English or translated into another language) along with a link to the full piece wisehoroscope.org/nostradamus-2021/
I think this would make a great saying for a fortune cookie.
May good things come your way, and sooner than you think.
If predictions are anything to go by , the temperature in the city is set to soar further.
However, in all the rising delirium of heat and North Indian summer, there are loveable treats to be found. Like Kulfi, the Indian subcontinent's milk-based sweet dense creamy answer to frozen desserts as ice-cream.
The Kulfiwala outside Moet's In Defense Colony which is one of the best in the city and where i found this piece of Kulfi last summer, is said to source the Kulfis he sells from Sitaram Bazaar in Old Delhi. Around 80% of the city's Kulfi business, it is reported , is controlled by four families in this Bazaar area.
The Kulfis are frozen in small earthen pots(matkas) or on a tilli( a stick) frozen in moulds usually stored in a mix of ice and salt. They are either served in the same matka or demolded often over a bed of sweet vermicelli(rice noodles).
Cinema-Phono-Telegraphic Correspondence
This gallery depicts a series of futuristic pictures by the French painter Jean-Marc Côté and other artists issued in 1899, 1900, 1901 and 1910. Originally in the form of paper cards enclosed in cigarette/cigar boxes and, later, as postcards, the images described the world as it was imagined to be like in the then distant year of 2000.
At least 87 were produced, and I have managed to capture 73 of them 😊. While a few were on point (A version of Skype or Facetime), many were wildly off-tangent (underwater croquet, anyone?). And all are definitely worth a look!
Sources: All images are in the public domain; Most were obtained from gallica.bnf.fr/
, although I had to edit a few to render them in higher resolution.
It's that time of the year again where The Oscars is this Sunday! I've seen a lot of the nominated films this year, so I feel pretty confident in my predictions. So here are my predictions for best director, best score, best animated film, best visual effects, best adapted screenplay, and best original screenplay.
Best Director: Guillermo del Toro (The Shape of Water)
Best Score: Dunkirk
Best Animated Film: Coco
Best Visual Effects: War for the Planet of the Apes
Best Screenplay:
Adapted: Molly's Game
Original: Three Billboards
Make sure to check out part 1 for some other predictions: www.flickr.com/photos/antdude3001/25713366787/in/datepost...
Also, if you want to check out my predictions for all the Oscar categories, check out my Letterboxd list:
letterboxd.com/antman3000/list/2018-oscars-predictions/
What are your predictions? Leave them down in the comments below!
Scone, Upper Hunter Valley,
NSW, Australia.
I was up at Scone, a few hours drive north-west of Sydney, working for a week at the Scone Race Carnival which is one of the biggest in country Australia.
Scone is regarded as the horse capital of Australia and about 20,000 people attend the carnival over two days at Emirates Park.
I was there with my friend Russell Wilson helping install the power and lighting for the event.
One afternoon after work I decided to go for a drive to scout some locations for some astro photography.
Scone is out in country New South Wales so the night sky is quite dark with minimal light pollution.
The weather prediction was for a clear but cold night with a new moon, so ideal for what I had in mind.
I drove north on the New England Hwy for about 15-20kms and found a small lagoon that I thought would provide a nice foreground.
The nearby Barrington Tops range would also make for a nice silhouette at night.
I headed back to Scone for dinner & beers with the crew.
Later that night I grabbed my camera gear, a down jacket, gloves, and a beanie, and headed out into the night in my Subaru Forester.
I drove to roughly where I knew the lagoon was but as it was so dark at night I couldn’t find it.
I settled on using the mountains as a foreground, and also got an idea to use the highway as a lead-in line to a few of the nightscapes.
I brought a powerful LED Lenser torch to light-paint the road that would otherwise be pretty dark.
I was amazed at how many stars I could see in the sky and the Milky Way really stood out in all its grandeur.
I took a few shots from the side of the highway looking east toward Barrington Tops.
Amazingly, a treeline that was quite a way off the highway was lit at times by the powerful headlights of the large semi-trailers that thundered along the highway.
Next, it was time to ‘play chicken’ with these metal monsters on the highway.
I found a fairly straight stretch of road where I would set up my tripod along the white line right in the middle of the road.
I calculated a maximum shutter speed of 30secs before the stars would star to blur for my 16mm lens using the 500 rule .
I waited for a break in the traffic and set the tripod up facing south, lined up my composition, got the torch ready, and fired off the remote.
Then came the 30sec wait that seemed to take an eternity.
Several times during the photoshoot, a semitrailer would come roaring around the bend and light up the night with their headlights.
A couple of times I had to grab the tripod at the last second & run like hell to avoid being roadkill.
The New England Highway is a popular alternative to the Pacific Highway for truckies.
It was thrilling and a bit crazy, but worth it in the end as I got some good shots.
I was thankful to eventually get out of the freezing cold night, hop in the car and head back to the warmth of my hotel room.
en.wikipedia.org/wiki/Humpback_whale
The humpback whale (Megaptera novaeangliae) is a species of baleen whale. One of the larger rorqual species, adults range in length from 12–16 metres (39–52 ft) and weigh approximately 36,000 kilograms (79,000 lb). The humpback has a distinctive body shape, with unusually long pectoral fins and a knobbly head. An acrobatic animal known for breaching and slapping the water with its tail and pectorals, it is popular with whale watchers off Australia, New Zealand, South America, Canada, and the United States.
Males produce a complex song lasting 10 to 20 minutes, which they repeat for hours at a time. Its purpose is not clear, though it may have a role in mating.
Found in oceans and seas around the world, humpback whales typically migrate up to 25,000 kilometres (16,000 mi) each year. Humpbacks feed only in summer, in polar waters, and migrate to tropical or subtropical waters to breed and give birth in the winter. During the winter, humpbacks fast and live off their fat reserves. Their diet consists mostly of krill and small fish. Humpbacks have a diverse repertoire of feeding methods, including the bubble net feeding technique.
Like other large whales, the humpback was and is a target for the whaling industry. Once hunted to the brink of extinction, its population fell by an estimated 90% before a moratorium was introduced in 1966. While stocks have since partially recovered, entanglement in fishing gear, collisions with ships, and noise pollution continue to impact the 80,000 humpbacks worldwide.
Taxonomy
Humpback whales are rorquals (family Balaenopteridae), a family that includes the blue whale, the fin whale, the Bryde's whale, the sei whale and the minke whale. The rorquals are believed to have diverged from the other families of the suborder Mysticeti as long ago as the middle Miocene.[3] However, it is not known when the members of these families diverged from each other.
Though clearly related to the giant whales of the genus Balaenoptera, the humpback has been the sole member of its genus since Gray's work in 1846. More recently, though, DNA sequencing analysis has indicated the humpback is more closely related to certain rorquals, particularly the fin whale (Balaenoptera physalus), and possibly to the gray whale (Eschrichtius robustus), than it is to rorquals such as the minke whales.[4][5] If further research confirms these relationships, it will be necessary to reclassify the rorquals.
The humpback whale was first identified as baleine de la Nouvelle Angleterre by Mathurin Jacques Brisson in his Regnum Animale of 1756. In 1781, Georg Heinrich Borowski described the species, converting Brisson's name to its Latin equivalent, Balaena novaeangliae. In 1804, Lacépède shifted the humpback from the Balaenidae family, renaming it Balaenoptera jubartes. In 1846, John Edward Gray created the genus Megaptera, classifying the humpback as Megaptera longipinna, but in 1932, Remington Kellogg reverted the species names to use Borowski's novaeangliae.[6] The common name is derived from the curving of their backs when diving. The generic name Megaptera from the Greek mega-/μεγα- "giant" and ptera/πτερα "wing",[7] refers to their large front flippers. The specific name means "New Englander" and was probably given by Brisson due the regular sightings of humpbacks off the coast of New England.
Description
A humpback whale can easily be identified by its stocky body with an obvious hump and black dorsal coloring. The head and lower jaw are covered with knobs called tubercles, which are hair follicles, and are characteristic of the species. The fluked tail, which it lifts above the surface in some dive sequences, has wavy trailing edges.[8] The four global populations, all under study, are: North Pacific, Atlantic, and Southern Ocean humpbacks, which have distinct populations which complete a migratory round-trip each year, and the Indian Ocean population, which does not migrate, prevented by that ocean's northern coastline.
The long black and white tail fin, which can be up to a third of body length, and the pectoral fins have unique patterns, which make individual whales identifiable.[9][10] Several hypotheses attempt to explain the humpback's pectoral fins, which are proportionally the longest fins of any cetacean. The two most enduring mention the higher maneuverability afforded by long fins, and the usefulness of the increased surface area for temperature control when migrating between warm and cold climates.
Humpbacks have 270 to 400 darkly coloured baleen plates on each side of their mouths.[11] The plates measure from a mere 18 inches (46 cm) in the front to approximately 3 feet (0.91 m) long in the back, behind the hinge. Ventral grooves run from the lower jaw to the umbilicus about halfway along the underside of the whale. These grooves are less numerous (usually 14–22) than in other rorquals but are fairly wide.[11]
The stubby dorsal fin is visible soon after the blow when the whale surfaces, but disappears by the time the flukes emerge. Humpbacks have a 3 metres (9.8 ft), heart-shaped to bushy blow, or exhalation of water through the blowholes. Because humpback whales breathe voluntarily, the whales possibly shut off only half of their brains when sleeping.[12] Early whalers also noted blows from humpback adults to be 10–20 feet (3.0–6.1 m) high.
Newborn calves are roughly the length of their mother's head. At birth, calves measure 20 feet (6.1 m) at 2 short tons (1.8 t) The mother, by comparison, is about 50 feet (15 m). They nurse for approximately six months, then mix nursing and independent feeding for possibly six months more. Humpback milk is 50% fat and pink in color.
Females reach sexual maturity at the age of five, achieving full adult size a little later. Males reach sexual maturity at approximately seven years of age. Humpback whale lifespans range from 45–100 years.[13] Fully grown, the males average 13–14 m (43–46 ft). Females are slightly larger at 15–16 m (49–52 ft); the largest recorded specimen was 19 metres (62 ft) long and had pectoral fins measuring 6 metres (20 ft) each.[14] Body mass typically is in the range of 25–30 metric tons (28–33 short tons), with large specimens weighing over 40 metric tons (44 short tons).[15] The female has a hemispherical lobe about 15 centimetres (5.9 in) in diameter in its genital region. This visually distinguishes males and females.[11] The male's penis usually remains hidden in the genital slit.
Identifying individuals
The varying patterns on the tail flukes are sufficient to identify individuals. A study using data from 1973 to 1998 on whales in the North Atlantic gave researchers detailed information on gestation times, growth rates, and calving periods, as well as allowing more accurate population predictions by simulating the mark-release-recapture technique (Katona and Beard 1982). A photographic catalogue of all known North Atlantic whales was developed over this period and is currently maintained by College of the Atlantic.[16] Similar photographic identification projects have begun in the North Pacific by Structure of Populations, Levels of Abundance and Status of Humpbacks, and around the world.
Life history
Social structure
The humpback social structure is loose-knit. Typically, individuals live alone or in small, transient groups that disband after a few hours. These whales are not excessively social in most cases. Groups may stay together a little longer in summer to forage and feed cooperatively. Longer-term relationships between pairs or small groups, lasting months or even years, have rarely been observed. Some females possibly retain bonds created via cooperative feeding for a lifetime. The humpback's range overlaps considerably with other whale and dolphin species—for instance, the minke whale. However, humpbacks rarely interact socially with them, though one individual was observed playing with a bottlenose dolphin in Hawaiian waters.[17]
Courtship and reproduction
Courtship rituals take place during the winter months, following migration toward the equator from summer feeding grounds closer to the poles. Competition is usually fierce, and unrelated males, dubbed escorts by researcher Louis Herman, frequently trail females, as well as mother-calf dyads. Male gather into "competitive groups" and fight for females.[18] Group size ebbs and flows as unsuccessful males retreat and others arrive to try their luck. Behaviors include breaching, spyhopping, lob-tailing, tail-slapping, fin-slapping, peduncle throws, charging and parrying. Whale songs are assumed to have an important role in mate selection; however, they may also be used between males to establish dominance.[19]
Females typically breed every two or three years. The gestation period is 11.5 months, yet some individuals have been known to breed in two consecutive years. The peak months for birth are January, February, July, and August, with usually a one- to two–year period between humpback births. They can live up to 48 years. Recent research on humpback mitochondrial DNA reveals groups living in proximity to each other may represent distinct breeding pools.[20]
Song
Both male and female humpback whales vocalize, but only males produce the long, loud, complex "songs" for which the species is famous. Each song consists of several sounds in a low register, varying in amplitude and frequency, and typically lasting from 10 to 20 minutes.[21] Humpbacks may sing continuously for more than 24 hours. Cetaceans have no vocal cords, so whales generate their songs by forcing air through their massive nasal cavities.
Whales within a large area sing the same song. All North Atlantic humpbacks sing the same song, and those of the North Pacific sing a different song. Each population's song changes slowly over a period of years without repeating.[21]
Scientists are unsure of the purpose of whale songs. Only males sing, suggesting one purpose is to attract females. However, many of the whales observed to approach a singer are other males, often resulting in conflict. Singing may, therefore, be a challenge to other males.[22] Some scientists have hypothesized the song may serve an echolocative function.[23] During the feeding season, humpbacks make altogether different vocalizations for herding fish into their bubble nets.[24]
Humpback whales have also been found to make a range of other social sounds to communicate, such as "grunts", "groans", "thwops", "snorts" and "barks"
Ecology
Feeding and predation
Humpbacks feed primarily in summer and live off fat reserves during winter.[26] They feed only rarely and opportunistically in their wintering waters. The humpback is an energetic hunter, taking krill and small schooling fish such as Atlantic herring, Atlantic salmon, capelin, and American sand lance, as well as Atlantic mackerel, pollock, and haddock in the North Atlantic.[27][28][29] Krill and copepods have been recorded as prey species in Australian and Antarctic waters.[30] Humpbacks hunt by direct attack or by stunning prey by hitting the water with pectoral fins or flukes.
The humpback has the most diverse feeding repertoire of all baleen whales.[31] Its most inventive technique is known as bubble net feeding; a group of whales swims in a shrinking circle blowing bubbles below a school of prey. The shrinking ring of bubbles encircles the school and confines it in an ever-smaller cylinder. This ring can begin at up to 30 metres (98 ft) in diameter and involve the cooperation of a dozen animals. Using a crittercam attached to a whale's back, some whales were found to blow the bubbles, some dive deeper to drive fish toward the surface, and others herd prey into the net by vocalizing.[32] The whales then suddenly swim upward through the "net", mouths agape, swallowing thousands of fish in one gulp. Plated grooves in the whale's mouth allow the creature to easily drain all the water initially taken in.
Given scarring records, killer whales are thought to prey upon juvenile humpbacks, though this has never been witnessed. The result of these attacks is generally nothing more serious than some scarring of the skin, but young calves likely are sometimes killed.[33]
Range and habitat
Humpbacks inhabit all major oceans, in a wide band running from the Antarctic ice edge to 77° N latitude, though not in the eastern Mediterranean or the Baltic Sea.They are migratory, spending summers in cooler, high-latitude waters and mating and calving in tropical and subtropical waters.[21] An exception to this rule is a population in the Arabian Sea, which remains in these tropical waters year-round.[21] Annual migrations of up to 25,000 kilometres (16,000 mi) are typical, making it one of the mammals' best-traveled species.
A large population spreads across the Hawaiian Islands every winter, ranging from the island of Hawaii in the south to Kure Atoll in the north.[34] A 2007 study identified seven individuals wintering off the Pacific coast of Costa Rica as having traveled from the Antarctic—around 8,300 kilometres (5,200 mi). Identified by their unique tail patterns, these animals made the longest documented mammalian migration.[35] In Australia, two main migratory populations have been identified, off the west and east coasts, respectively. These two populations are distinct, with only a few females in each generation crossing between the two groups.[36]
Whaling
Humpback whales were hunted as early as the 18th century, but distinguished by whalers as early as the first decades of the 17th century. By the 19th century, many nations (the United States in particular), were hunting the animal heavily in the Atlantic Ocean, and to a lesser extent in the Indian and Pacific Oceans. The late-19th-century introduction of the explosive harpoon, though, allowed whalers to accelerate their take. This, along with hunting in the Antarctic Ocean beginning in 1904, sharply reduced whale populations. During the 20th century, over 200,000 humpbacks were estimated to have been taken, reducing the global population by over 90%, with North Atlantic populations estimated to have dropped to as low as 700 individuals.[37] In 1946, the International Whaling Commission was founded to oversee the whaling industry. They imposed rules and regulations for hunting whales and set open and closed hunting seasons. To prevent extinction, the International Whaling Commission banned commercial humpback whaling in 1966. By then, the population had been reduced to around 5,000.[38] That ban is still in force.
Prior to commercial whaling, populations could have reached 125,000. North Pacific kills alone are estimated at 28,000.[8] The full toll is much higher. It is now known that the Soviet Union was deliberately under-recording its catches; the Soviet catch was reported at 2,820, whereas the true number is now believed to be over 48,000.[39]
As of 2004, hunting of humpback whales was restricted to a few animals each year off the Caribbean island Bequia in the nation of St. Vincent and the Grenadines.[31] The take is not believed to threaten the local population. Japan had planned to kill 50 humpbacks in the 2007/08 season under its JARPA II research program, starting in November 2007. The announcement sparked global protests.[40] After a visit to Tokyo by the chairman of the IWC, asking the Japanese for their co-operation in sorting out the differences between pro- and antiwhaling nations on the Commission, the Japanese whaling fleet agreed no humpback whales would be caught for the two years it would take for the IWC to reach a formal agreement.[41]
In 2010, the International Whaling Commission authorized Greenland's native population to hunt a few humpback whales for the next three years.[42]
Conservation
The worldwide population is at least 80,000 humpback whales, with 18,000-20,000 in the North Pacific,[43] about 12,000 in the North Atlantic,[44] and over 50,000 in the Southern Hemisphere,[45] down from a prewhaling population of 125,000.[8]
This species is considered "least concern" from a conservation standpoint, as of 2008. This is an improvement from vulnerable in 1996 and endangered as recently as 1988. Most monitored stocks of humpback whales have rebounded well since the end of commercial whaling,[2][46] such as the North Atlantic, where stocks are now believed to be approaching levels similar to those before hunting began. However, the species is considered endangered in some countries, including the United States.[47][48] The United States initiated a status review of the species on August 12, 2009, and is seeking public comment on potential changes to the species listing under the Endangered Species Act.[49] Areas where population data are limited and the species may be at higher risk include the Arabian Sea, the western North Pacific Ocean, the west coast of Africa and parts of Oceania.[2]
Today, individuals are vulnerable to collisions with ships, entanglement in fishing gear, and noise pollution.[2] Like other cetaceans, humpbacks can be injured by excessive noise. In the 19th century, two humpback whales were found dead near sites of repeated oceanic sub-bottom blasting, with traumatic injuries and fractures in the ears.[50]
Once hunted to the brink of extinction, the humpback has made a dramatic comeback in the North Pacific. A 2008 study estimated the humpback population, which hit a low of 1,500 whales before hunting was banned worldwide, has made a comeback to a population of between 18,000 and 20,000.[51] Saxitoxin, a paralytic shellfish poisoning from contaminated mackerel has been implicated in humpback whale deaths.[52]
The United Kingdom, among other countries, designated the humpback as a priority species under the national Biodiversity Action Plan. The sanctuary provided by US National Parks, such as Glacier Bay National Park and Preserve and Cape Hatteras National Seashore, among others, have also become major factors in sustaining populations.[53]
Although much was learned about humpbacks from whaling, migratory patterns and social interactions were not well understood until two studies by R. Chittleborough and W. H. Dawbin in the 1960s.[54] Roger Payne and Scott McVay made further studies of the species in 1971.[55] Their analysis of whale songs led to worldwide media interest and convinced the public that whales were highly intelligent, aiding the antiwhaling advocates.
In August 2008, the IUCN changed humpback's status from Vulnerable to Least Concern, although two subpopulations remain endangered.[56] The United States is considering listing separate humpback populations, so smaller groups, such as North Pacific humpbacks, which are estimated to number 18,000-20,000 animals, might be delisted. This is made difficult by humpback's extraordinary migrations, which can extend the 5,157 miles (8,299 km) from Antarctica to Costa Rica.[20]
Whale-watching
Humpback whales are generally curious about objects in their environments. Some individuals, referred to as "friendlies", approach whale-watching boats closely, often staying under or near the boat for many minutes. Because humpbacks are often easily approachable, curious, easily identifiable as individuals, and display many behaviors, they have become the mainstay of whale-watching tourism in many locations around the world. Hawaii has used the concept of "ecotourism" to use the species without killing them. This whale-watching business brings in a revenue of $20 million per year for the state's economy
predictions for tomorrow in southern Wisconsin: 2 inches? 4 inches? 8 inches?
Might as well be 2 feet!!!!
It's that time of the year again where The Oscars is this Sunday! I've seen a lot of the nominated films this year, so I feel pretty confident in my predictions. So here are my predictions for best film, best lead actor, best lead actress, best supporting actor, and best supporting actress!
Best Film: The Shape of Water
Best Lead Actor: Gary Oldman (Darkest Hour)
Best Lead Actress: Frances McDormand (Three Billboards)
Best Supporting Actor: Sam Rockwell (Three Billboards)
Best Supporting Actress: Allison Janney (I, Tonya)
Make sure to check out part 2 for some other predictions: www.flickr.com/photos/antdude3001/39689489585/in/datepost...
Also, if you want to check out my predictions for all the Oscar categories, check out my Letterboxd list:
letterboxd.com/antman3000/list/2018-oscars-predictions/
What are your predictions? Leave them down in the comments below!
copyright © Genevieve Dietrich. All rights reserved.
We've gone biking every day since we got the bikes. It reminds me of when I started running. When you run enough to get to the point that you can just run and run forever at a reasonable pace, you notice this powerful feeling of being your own vehicle. You can get anywhere in your own body AND you are right there in the world. There is no barrier between you and the rest of the world. It is an unusual feeling, but honestly when we humans move with any speed we are usually in a vehicle. The bikes make me feel like this, like I'm running on human power and that I can go anywhere that way.
The slower pace of a bike compared to a machine puts me in the world around me rather than passing by it. I see and say hello to people I pass. I see the old people, sad people, lonely people, people playing, and the children. I notice the specifics of their condition. I can say something to them, I can smile. I see goldfinches clinging to the tops of grass seed heads watching me pass by. A woolly bear caterpillar with no black stripe at all desperately trying to cross a road caught my eye. If his weather prediction ability is good, we're in for a harsh winter. I picked him up and put him in the woods. A magnificent red-tailed hawk shot up in surprise at us. Swallowtails on six foot high thistle plants, hawks, crows, jays, cardinals and ravens are everywhere for us to see.
We headed home tonight near twilight because we'd stopped on the way home to get dinner. As we headed home I saw a bed of backlit cosmos flowers in the middle of suburbia shopping concrete land that looked like glowing splashes of pastel straight from Vincent Van Gogh's paint brush. We turned the corner and the same sun made the tall blooms of a landscape grass look like giant glowing feather dusters. My knees were weak and my eyes clouded with tears from the beauty of the most mundane things in the world. Our world is overwhelmingly beautiful, even the ugliest corners. It amazes me every time I get out in it and open my eyes. No matter how much of this earth we destroy, what remains still holds the beauty, mystery and promise, the seeds of hope and justification for faith of what came before.
Hear a Ruby-throated Hummingbird
The Hunt for Microbes
This gallery depicts a series of futuristic pictures by the French painter Jean-Marc Côté and other artists issued in 1899, 1900, 1901 and 1910. Originally in the form of paper cards enclosed in cigarette/cigar boxes and, later, as postcards, the images described the world as it was imagined to be like in the then distant year of 2000.
At least 87 were produced, and I have managed to capture 73 of them 😊. While a few were on point (A version of Skype or Facetime), many were wildly off-tangent (underwater croquet, anyone?). And all are definitely worth a look!
Sources: All images are in the public domain; Most were obtained from gallica.bnf.fr/
, although I had to edit a few to render them in higher resolution.
Predictions of 200-1000 per hour did not pan out. Oh well beautiful night anyway. Bonus points! Reddish glow Northern lights!
Newsweek Cover, July 3, 1978: TV of Tomorrow
www.facebook.com/photo/?fbid=1470218527709398&set=a.9...
Credit:
Computer Love Records
The construction of a new fire station to replace Gipton and Stanks fire stations and removal of 24 fulltime posts from the establishment by way of planned retirements.
Key Points:
Gipton is classed as a very high risk area and Stanks as medium risk area.
Stanks fire station is poorly located at the outer edge of the local community and access/egress from the site is problematic.
In the 5 year period between 2004/5 and 2009/10 operational demand in these areas reduced by 28% (there has been a reduction of 61% of serious fires) . 2
WYFRS has piloted a new type of vehicle (Fire Response Unit) to deal with smaller fires and incidents to free up fire appliances to respond to more serious emergencies.
The pilot has been successful and it is believed that a District based Fire Response Unit will handle in the region of 3,000 calls per year.
The new fire station would have lower running costs.
The two Killingbeck fire appliances would be supplemented by a Resilience Pump for use during spate conditions.
Targeted community safety and risk reduction work would continue.
1. Foreword
1.1 This proposal forms one of a number of similar initiatives developed by West Yorkshire Fire and Rescue Service (WYFRS) as part of its plans for the future provision of a highly effective and professional Fire and Rescue Service.
1.2 Each proposal is based on sound and comprehensive research, using real data from past performance and predictions of future demand and risk. Multiple sources of analysis have been used, allied to professional judgment and experience, to form the basis of robust business cases for change. The proposals are also reflective of the significant improvements in fire and community safety achieved over the past 10 years and represents a return on the investment made by the Authority on behalf of the public of West Yorkshire.
1.3 The proposals also incorporate a number of new and innovative approaches to addressing the challenge of maintaining high standards of performance for an emergency response service, within ever tightening financial constraints. The proposals have been developed as a package of inter related initiatives, representing major capital investment in local communities, whilst at the same time delivering annual recurring savings.
2. Introduction
2.1. Gipton fire station was constructed in 1937; it provides the initial emergency response cover for the residential and commercial areas of Gipton, Harehills, Burmantofts, Killingbeck, Halton Moor and Oakwood.
The fire station area covers approximately 8.45 square miles.
There is a population of 75,316.
There are approximately 2015 commercial properties within the area.
2.2. Stanks fire station was constructed 1973; it provides the initial emergency response cover for the mainly residential locations of Whinmoor, Swarcliffe, Whitkirk, Colton, Halton, Crossgates, Scarcroft, North Seacroft, Wellington Hill, Manston, Barwick-in-Elmet, Scholes and Thorner.
The station area covers approximately 14.39 square miles
There is a population of 42,452
There are approximately 663 commercial properties within the area.
2.3. Gipton has been classified as a very high risk area using the WYFRS Risk Matrix methodology. During 2009/10 there were 2196 operational incidents within this area including 86 dwelling fires and 33 Road Traffic Collisions. Stanks fire station area has been classified as medium risk and during the same period there were 688 operational incidents in the area including 34 dwelling fires and 12 Road Traffic Collisions. 1
2.4. Three fire appliances currently provide the initial fire and rescue coverage for Gipton and Stanks and are constantly crewed by 60 whole-time firefighters. The operational demand in these areas has reduced by 28% between 2004/5 and 2009/10 (there has been a reduction of 61% of serious fires) yet the provision of operational resources has remained the same over this period of time. 24
3. Community Impact Assessment
3.1. The following statement is taken from the 2011-2015 Community Risk Management Strategy and emphasises our commitment to deliver an efficient economic and effective range of services, “Every area within WYFRS will be considered in order to provide a better service at reduced cost”.
3.2. To enable WYFRS to deliver against this commitment a wide range of analysis and modelling tools have been used to determine the current and predicted levels of service delivery, together with their associated costs. These tools have also been used to undertake four separate impact assessments in regard to WYFRS proposals which will seek to:
Identify options which minimise reductions in service delivery standards and where there is scope for service delivery improvement.
Develop measures that will mitigate any negative impact upon service delivery and where possible maximise opportunities to achieve improvements.
3.3. WYFRS has developed a risk matrix which allocates a separate score/rating for hazards within communities. It is possible to use this risk rating in conjunction with the costs for providing services to each fire station to compare the cost of fire and rescue cover for each area. Gipton is one of the more cost effective stations in West Yorkshire but Stanks is almost 50% more expensive proportionate to the risk. 6
3.4. For most parts of the day the operational demand on resources based at the new station will be comparable to those of equally resourced fire stations. Figure 1 compares the predicted average operational activity levels for the new station with those of two other fire stations provided with two appliances. It indicates that although operational activity levels are generally comparable they are slightly higher during the evening hours due to the occurrence of smaller nuisance fires. 7
3.5. A Fire Response Unit has been piloted in Leeds District; this unit will attend small fires, car fires and certain fire alarms. These types of incident occur frequently in the East Leeds area. Figure 2 shows the level of activity in the new fire station area with the incidents the Fire response Unit attends taken out of the activity levels. The benefit of the Fire Response Unit can clearly be seen. The activity levels for the new station have been reduced considerably compared to other stations; it also shows that the new station will be less operationally active during the evening than the other local stations.
3.6. The new station in East Leeds will have a comparable level of activity to other fire stations provided with two appliances. 7
Figure 2 - Activity Timeline of Incidents Excluding Secondary Fires and Some False Alarms
Site Locations
3.7. An extensive review of emergency response cover has recently been completed and this has included the use of evaluation tools alongside local knowledge and professional judgment to identify optimum locations to build new WYFRS fire stations.
3.8. A site search mapping system has identified a number of appropriate areas across the County to build new fire stations and a number of sites have been identified within these areas which would provide the best solutions. A new fire station site must first be available for purchase and also provide access to road networks, it must not be located within flood plains and it must meet local planning permission requirements.
3.9. Analysis has been undertaken using the Fire Service Emergency Cover (FSEC – see also para 3.15) toolkit, together with the Phoenix/Active resource modelling toolkit.
3.10. The optimum area for a fire station between Gipton and Stanks has been identified as being situated on the A64 in the vicinity of Killingbeck police station. This proposed site is approximately 1.6 miles from Gipton Approach and 2.2 miles from Sherburn Road. The presence of a large site owned by West Yorkshire Police at this location may also present some potential to co-locate resources.
Determining where resources should be located
3.11. Independent research has assisted WYFRS to determine the potential impact that the implementation of each proposal would have on fire appliance attendance times to operational incidents. A simulation model has been used to identify the performance impact of moving resources to the new fire station. This modelling measures how the location of a new fire station would have performed if it had been in existence and responded to the actual incidents that did occurred in this area between 2007/8 and 2009/10. 4
3.12. Models have been run for locating a two fire appliances at Gipton and closing Stanks, and then run again for locating a two fire appliances at Stanks and closing Gipton, both these options provide a significantly lower level of response performance than would be achieved by locating
3.13. The proposals has a small reduction in performance in fire appliance attendance times against the Risk based Planning Assumptions for all incidents across the whole of West Yorkshire of approximately 0.3% for first appliance and 0.1% for the second appliance. 4
3.14. Local Impact – Figure 3 identifies that:
There is a reduction in response performance against the Risk Based Planning Assumptions in the Gipton station area. The main reason for this is simultaneous activity. This change will be greatly mitigated by the Fire Response Unit. The predicted response times still represent good performance and are appropriate for the. Further impact will be achieved by targeted risk reduction activities.
Fire Service Emergency Cover (FSEC) toolkit
3.15 The FSEC software toolkit has been developed by Central Government (Department for Communities and Local Government) for use by Fire and Rescue Authorities in determining appropriate fire and emergency cover. It enables the relationship between dwelling fire casualties and the social demographics of small areas in the county (super output areas) and the location of response resources (fire stations) to be determined. Four demographic benchmarks are used to demonstrate this relationship and to represent predicted risk associated with a range of appliance response times.
3.16 Analysis of the FSEC outputs (which is a cost benefit analysis in regard to property and life risk) predicts that the relocating the fire station to Killingbeck will:
Reduce the risk to the community.
Result in significant efficiencies. 9
3.17 The FSEC modelling suggests that the impact of the Killingbeck proposal would be less than other relocation options
3.18 The Phoenix/Active software tool is another analysis tool used to identify the impact of any changes of the Risk Based Planning Assumptions referred to above. It predicts that locally there is likely to be a small adverse impact on the performance against Risk Based Planning Assumptions. Across the Brigade the impact is negligible. 10
Predicted Risk Level
3.19. A new fire station located, within the Killingbeck area would attract the same risk classification as the Gipton fire station area therefore the new fire station would be classified as very high risk. Targeted risk reduction activity will help to reduce the risk, with the aim of reducing it sufficiently enough to re-categorise the area as high risk in the future. 1
3.20. Isochrones (travel distance) can be drawn around the proposed location of the new fire station (Section 8). These indicate the distance the appliance would be able to travel within the Risk Based Planning Assumption time of 7 minutes.
3.21. Section 8 also illustrates that for this area of West Yorkshire a single fire station in the new location provides fire appliance coverage which is more proportionate to risk than the current arrangements.
Risk Reduction
3.20 During 2010 a comprehensive and integrated framework for service delivery was developed, this is outlined in the Community Risk Management Strategy 2011-15. This was implemented in 2011 and is proving a very effective means for targeting resources and reducing risk and is an essential method for reducing any negative impact of change in fire cover. Fundamental to this approach is the introduction of District Risk Reduction Teams and Local Area Risk Reductions Teams.
3.21 The location of a fire station in the Killingbeck area will enable targeted community safety activities such as Home Fire Safety Checks to continue.
4 Firefighter Safety Impact Assessment
Risk and firefighters gathering risk information about premises.
4.1 One of WYFRS’s risk indicators is dedicated solely to “Firefighter safety” and has taken cognisance of the following statement within the 2009 WYFRS Firefighter Safety Strategy; “Effective gathering and analysis of information prior to operational incident attendance is of critical importance”.
4.2 The firefighter safety indicator captures the following information to reflect this statement:
The predominance of specified commercial properties within each fire station area.
The availability of associated risk information held for commercial properties.
The predominance of high-rise properties within each fire station area.
4.3 The swift arrival of supporting resources can have a beneficial impact upon the safe management of operational incidents and this is the rationale for this information being captured by the indicator.
4.4 Following the 2009/10 evaluation process the firefighter safety risk bandings for Gipton and Stanks have been determined as high and very low respectively. 1
8
4.5 The targets for operational risk information for the 2012/13 IRMP Action Plan will be set in a proportionate manner, with areas of higher risk levels receiving a greater number of operational risk information inspections. More inspections will take place in areas such as Gipton to increase the availability of risk information available to firefighters via the Mobile Data Terminals (MDT’s) and as more information is made available the corresponding risk level will be reduced.
4.6 The Premises Data-base currently indicates that there are a total of 1650 commercial properties within the Gipton and Stanks area that have not been made subject to an operational information inspection. A high priority has been placed on firefighters in Gipton visiting the premises where incidents could potentially occur. 11
4.7 It is therefore anticipated that the availability of risk information via the Mobile Data Terminals (MDT’s) for properties within all areas will be considerably improved by 2015, by which time the corresponding firefighter safety risk banding will have been reduced to Medium
The arrival times of the 2nd fire appliance
4.9. During 2009/10 there were a total of 333 operational incidents within the areas of Gipton and Stanks which required the attendance of more than one pumping appliance (one every 1.1 days). 12
4.10. Currently the North and East Leeds area has two fire appliances based at Gipton, Moortown and Leeds with one at Rothwell, Garforth, Stanks and Wetherby.
4.11. Increased second pump arrival times require the first attending crew to manage the initial stages of certain incidents in isolation; there is some potential for fires to become more developed in these initial stages.
4.12. The proposal improves the second appliance attendance times into Garforth station areas and there is little impact for the others local station areas.
5. Equality Impact Assessment
5.1 The new Public Sector Equality Duty places a requirement on the organisation to ensure where changes affect service delivery to the community or employees WYFRS assess those changes for any possible negative impact on equality. In this context equality refers to the protected characteristics in the Equality Act 2010, race, gender, disability, religion and belief, sexual orientation, age, gender-reassignment, maternity and pregnancy and marriage and civil partnerships.
5.2 This Equality Impact Assessment has been completed by using information drawn from the Office for National Statistics in regard to this area and has been used to determine whether the removal of a fire appliance from the area will lead to an adverse or disproportionate impact upon any sections of the population. 13
5.3 A 2008 report provided by the Communities and Local Government (CLG) department analysed the correlation between dwelling fires and socio demographics. This report has been used to provide an indication of whether any particular groups within the population are at heightened risk from fire. The report indicates that sick/disabled persons, lone pensioners and Black Caribbean/African groups were associated with a greater incidence of dwelling fires.
5.4 The Gipton and Harehills population was estimated as being 24,904 during 2001 with a fairly equal gender distribution. The predominant ethnic group within the population is White British with Asian/Asian British representing the next major group, followed by Pakistani, Black British/Caribbean and Asian/British Bangladeshi.
9
5.5 Approximately 49% of the resident Gipton and Harehills population are Christians, 23% are of Muslim faith and 25% declared no religious preference. In 2001 16% of the population was aged over 60 and 20% of the population had a limiting long-term illness.
5.6 The WYFRS Prevention strategy contained within the 2011-2015 Community Risk Management Strategy emphasises that risk reduction activities will be focussed toward areas of the county identified as being at higher risk from dwelling fires, deliberate fire setting and road traffic collisions and that an appropriate and proportionate allocation of resources will be made available for District Risk Reduction Teams (DRRT) to achieve this.
5.7 Although the Ward statistics indicate that the communities of Gipton and Harehills are very diverse the findings of the Equality Impact Assessment are that this proposal will not lead to any negative changes in the delivery of Prevention, Protection and Response services and consequently there will be no anticipated impact upon any under-represented groups. The Equality Impact Assessment also confirms that there is no negative impact on any employee group.
6. Organisational Impact Assessment
Efficiencies
6.1 This proposal will enable WYFRS to manage some of the financial deficit caused by reduced government funding.
6.2. The proposal has considered the less than optimal positioning of existing fire stations and appliances together with the reduced operational demand placed and associated costs. The most cost effective solution to these issues is to provide a new fire station and ensure that two fire appliances will be crewed by nine firefighters who will respond to emergencies in less than two minutes from being mobilised.
6.3. This can be achieved by reducing the staffing at Gipton and Stanks by 24 posts; this will be done by way of planned retirements. The staffing and duty system at the new fire station will remain the same.
6.4. The removal of posts that coincide with forecasted retirements will achieve significant revenue savings.
6.5. Although capital investment will be required to construct a new fire station, part of these costs will potentially be off-set by the sale of the two existing fire station sites.
6.6. There will be other associated savings delivered by this proposal, including:
Reduction of Personal Protective Equipment.
Reduction in consumables and station maintenance costs.
The new station will be more environmentally friendly and have energy efficiency technology.
6.7. The analysis undertaken for Gipton and Stanks has identified that there is considerable overlap in the existing Risk Based Planning Assumption isochrones (footprints) for these areas. This overlap represents a duplication of resource coverage and therefore one of the objectives for providing a more efficient service within these areas is to reduce this overlap. 14
10
Impact across West Yorkshire and Resilience
6.8 The reduction in pumping appliances in this area does have a small impact upon attendance times against the Risk Based Planning Assumptions across West Yorkshire for all incidents; performance is reduced by 0.3% for first appliances and 0.1% for second appliances. 4
6.9 In order to maintain WYFRS’s operational resilience, the fire appliance currently sited at Stanks will be relocated at the new fire station. This fire appliance will not be continually staff but will be activated during periods of anticipated or unanticipated high levels of operational activity and in response to significant events which could affect emergency response; such as wide area flooding, bonfire night, periods of bad weather or when attending very large incidents.
6.10 The use of Resilience Pumps supports WYFRS strategy of staffing the appropriate number of fire appliances for normal levels of activity and having the mechanisms to add further fire appliance when required. This strategy is important in maintaining an excellent fire and rescue service whilst meeting the efficiencies required by the reduction in public service budgets.
7. Conclusions
7.1 The existing fire stations at Gipton and Stanks are 3.7 miles apart and consolidating resources at a new fire station at a central location is an economic, effective and efficient way of providing fire and rescue services for these areas.
7.2 The provision of two front-line fire appliances constantly crewed by whole-time firefighters is still deemed appropriate for this area despite the success of previous year’s risk reduction activities.
7.3 Targeted risk reduction initiatives co-ordinated by the Leeds Outer North East, Inner North East and Outer East Local Area Risk Reduction Teams will be undertaken.
7.4 It is expected that the targets established for gathering safety critical risk information, will mitigate the impact upon the safety of WYFRS firefighters resulting from the removal of a pumping appliance from this area.
7.5 The introduction of a Resilience Pump will maintain three appliances in the area and support WYFRSs resilience arrangements
7.6 The consolidation of Gipton and Stanks resources at one central location together with the addition of a Resilience Pump will deliver significant efficiency savings whilst maintaining a high level of service delivery and providing employees with vastly improved accommodation facilities.
Tucker's predictions for Super Bowl 57 between
the Philadelphia Eagles and Kansas City Chiefs!
Tucker, Welsh Corgi brings down the stuffed bulldog
before he picks it up to run for a touchdown.
Tucker's prediction is the underdogs, Kansas City Chiefs,
to win!
Tucker picked the 2023 Super Bowl 57 Champions!
Yes, The Kansas City Chiefs win in a close, exciting game
down to the final seconds with a field goal.
Chiefs win 38 to 35!
Having just finished the book, I find myself “just thinking about the weather” (like 10,000 Maniacs).
Every decade, we have added one day to our forward weather forecast. So, today’s weekly forecast is as accurate as the 2-day forecast in the 70’s. In the first book on weather prediction — 100 years ago — Lewis Fry Richardson prophesied “perhaps someday in the dim future it will be possible to advance the computation faster than the weather advances, and at a cost less than the savings to mankind due to the information gained. But that is a dream.”
What a setup for Moore’s Law! More on that later.
Weather predictions started with telegraph networks in the 1860’s. News of a storm front could arrive by electrical signals faster than the wind itself. Those physical networks were interrupted by the civil war and the great wars. The observational stations drove short term forecasts driven by simple pattern matching; meteorologists flipped through maps of prior patterns to find one that looked similar, missing the nuances in the complex networks of interactions.
What was needed was a theory, a mathematics derived from first principles of the physics of atmospheric flows. Those equations, a collection of interlocking partial differential equations, across a matrix of pressure, temperature, air density, wind vectors and such, were first published in 1904 (and are the subject of the thick textbook below). They are practically unsolvable, but can be approximated with a variety of numerical / graphical methods and approximations (hydrostatic, anelastic, autobarotropic shallow fluid, etc.). New weather prediction models were then back tested on historical data, an iterative feedback cycle of learning from past to present.
The weather became important to ship traffic and battle planning, and forecasts were weaponized in wartime. The terminology of weather “fronts” traces to the martial vernacular of WW I. The Germans were at a distinct meteorological disadvantage, with storms coming from areas controlled by the Allied powers. Siemens developed automatic weather stations with NiCad batteries and radios that could be dropped off by plane in remote locations. With 200 submarines trying to maintain a blockade of England, the Germans desperately needed weather predictions for the North Atlantic. In 1943, they sent U-537 to an uninhabited part of North America, and set up a weather station on a local peak, with a long range 30-ft. diameter antenna to beam weather data back to Germany. To evade detection, they hand-painted “Canada Meteor Service” on the side and scattered American cigarette packs about. It remained there until discovered in 1981. Yes, the only known incursion by the Nazis onto North American soil was for the weather.
Then came the rockets. The first U.S. launch of a V-2 rocket brought back from Germany snapped a picture of the cloud cover as had never been seen before, with a quarter of the U.S. in a single frame. In 1954, an Aerobee rocket cam captured the first clear image of a tropical storm swirling in the Gulf of Mexico, and it became a full-page spread in Life magazine. (I have an Aerobee nose cone, fin can, and engine on display at work).
The first weather satellite, TIROS 1, launched in 1960, and in Kennedy’s famous speech that launched the Apollo program, he also beckoned “at the earliest possible time, a satellite system for worldwide weather observation.” It was overshadowed a bit by the whole man on the moon thing.
Today, the polar-orbiting LEO satellites raster scan the Earth (like Planet Labs) and “contribute the most quantitative data to the weather models. When it comes to meaningful impacts on forecasting, they are the champs.” (p.81). We have hundreds of LEO and GEO birds with a variety of weather instruments (optical, IR, radar) providing global coverage.
It’s a torrent of data, feeding supercomputers that are upgraded every two years. About half of the supercomputers on Earth are working on the weather. The European Center for Medium-Range Weather forecasts has two supercomputers the size of volleyball courts with 260,000 processor cores (in 2019). They maintain the current champion model for forecasting. They devote 50% of their compute cycles to iterating on model improvements (and the other 50% running the latest model for the world). They have improved their forecasts continuously for 40 years straight.
To build a global model, there are global sensors from many nations, all contributing to a public good. “WMO estimates put the economic value of weather services in excess of $100 billion annually, while the cost of providing them is a tenth of that.” (p.175) Still, a big number for a public good. “The weather machine is a last bastion of international cooperation.” (p.181)
P.S. The book is not nearly as gripping as the history of ammonia, and it ends abruptly without painting a picture of what’s next for Sim-Earth... with a proliferation of networked sensors and machine learning in the mix.
It's that time of the year again where The Oscars is tomorrow! I did this back in 2015 and I forgot to do this again last year, but I didn't forget this time! And like I did last time, I'm not going to make my predictions on all the awards, only the big ones. So here are my predictions for best director, best score, best animated film, best visual effects, best adapted screenplay, and best original screenplay.
Best Director: Denis Villeneuve (Arrival)
Best Score: La La Land
Best Animated Film: Moana (though I wouldn't be surprised if it's Zootopia, this one was kinda tough to call)
Best Visual Effects: The Jungle Book (But I'm holding out for Doctor Strange!)
Best Screenplay:
Adapted: Arrival
Original: Manchester by the Sea
Make sure to check out part 1 for some other predictions: www.flickr.com/photos/antdude3001/33076494876/in/datepost...
What are your predictions? Leave them down in the comments below!
His scientific works include a collaboration with Roger Penrose on gravitational singularity theorems in the framework of general relativity and the theoretical prediction that black holes emit radiation, often called Hawking radiation. Hawking was the first to set out a theory of cosmology explained by a union of the general theory of relativity and quantum mechanics. He is a vigorous supporter of the many-worlds interpretation of quantum mechanics.
Hawking is an Honorary Fellow of the Royal Society of Arts, a lifetime member of the Pontifical Academy of Sciences, and a recipient of the Presidential Medal of Freedom, the highest civilian award in the US. In 2002, Hawking was ranked number 25 in the BBC's poll of the 100 Greatest Britons. He was the Lucasian Professor of Mathematics at the University of Cambridge between 1979 and 2009 and has achieved commercial success with works of popular science in which he discusses his own theories and cosmology in general; his book A Brief History of Time appeared on the British Sunday Times best-seller list for a record-breaking 237 weeks.
Hawking has a rare early-onset, slow-progressing form of amyotrophic lateral sclerosis (ALS) that has gradually paralysed him over the decades. He now communicates using a single cheek muscle attached to a speech-generating device.
PRIMARY and SECONDARY SCHOOL YEARS
Hawking began his schooling at the Byron House School in Highgate, London. He later blamed its "progressive methods" for his failure to learn to read while at the school.In St Albans, the eight-year-old Hawking attended St Albans High School for Girls for a few months. At that time, younger boys could attend one of the houses.
Hawking attended Radlett School, an independent school in the village of Radlett in Hertfordshire, for a year, and from September 1952, St Albans School, an independent school in the city of St Albans in Hertfordshire. The family placed a high value on education. Hawking's father wanted his son to attend the well-regarded Westminster School, but the 13-year-old Hawking was ill on the day of the scholarship examination. His family could not afford the school fees without the financial aid of a scholarship, so Hawking remained at St Albans. A positive consequence was that Hawking remained with a close group of friends with whom he enjoyed board games, the manufacture of fireworks, model aeroplanes and boats, and long discussions about Christianity and extrasensory perception. From 1958 on, with the help of the mathematics teacher Dikran Tahta, they built a computer from clock parts, an old telephone switchboard and other recycled components.
Although known at school as "Einstein", Hawking was not initially successful academically. With time, he began to show considerable aptitude for scientific subjects and, inspired by Tahta, decided to read mathematics at university. Hawking's father advised him to study medicine, concerned that there were few jobs for mathematics graduates. He also wanted his son to attend University College, Oxford, his own alma mater. As it was not possible to read mathematics there at the time, Hawking decided to study physics and chemistry. Despite his headmaster's advice to wait until the next year, Hawking was awarded a scholarship after taking the examinations in March 1959.
UNDERGRADUATE YEARS
Hawking began his university education at University College, Oxford in October 1959 at the age of 17. For the first 18 months, he was bored and lonely – he was younger than many of the other students, and found the academic work "ridiculously easy". His physics tutor, Robert Berman, later said, "It was only necessary for him to know that something could be done, and he could do it without looking to see how other people did it." A change occurred during his second and third year when, according to Berman, Hawking made more of an effort "to be one of the boys". He developed into a popular, lively and witty college member, interested in classical music and science fiction. Part of the transformation resulted from his decision to join the college boat club, the University College Boat Club, where he coxed a rowing team. The rowing trainer at the time noted that Hawking cultivated a daredevil image, steering his crew on risky courses that led to damaged boats.
Hawking has estimated that he studied about a thousand hours during his three years at Oxford. These unimpressive study habits made sitting his finals a challenge, and he decided to answer only theoretical physics questions rather than those requiring factual knowledge. A first-class honours degree was a condition of acceptance for his planned graduate study in cosmology at the University of Cambridge. Anxious, he slept poorly the night before the examinations, and the final result was on the borderline between first- and second-class honours, making a viva (oral examination) necessary. Hawking was concerned that he was viewed as a lazy and difficult student. So, when asked at the oral to describe his future plans, he said, "If you award me a First, I will go to Cambridge. If I receive a Second, I shall stay in Oxford, so I expect you will give me a First." He was held in higher regard than he believed; as Berman commented, the examiners "were intelligent enough to realise they were talking to someone far cleverer than most of themselves". After receiving a first-class BA (Hons.) degree in natural science and completing a trip to Iran with a friend, he began his graduate work at Trinity Hall, Cambridge, in October 1962.
GRADUATE YEARS
Hawking's first year as a doctoral student was difficult. He was initially disappointed to find that he had been assigned Dennis William Sciama, one of the founders of modern cosmology, as a supervisor rather than noted astronomer Fred Hoyle, and he found his training in mathematics inadequate for work in general relativity and cosmology. After being diagnosed with motor neurone disease, Hawking fell into a depression – though his doctors advised that he continue with his studies, he felt there was little point. However, his disease progressed more slowly than doctors had predicted. Although Hawking had difficulty walking unsupported, and his speech was almost unintelligible, an initial diagnosis that he had only two years to live proved unfounded. With Sciama's encouragement, he returned to his work. Hawking started developing a reputation for brilliance and brashness when he publicly challenged the work of Fred Hoyle and his student Jayant Narlikar at a lecture in June 1964.
When Hawking began his graduate studies, there was much debate in the physics community about the prevailing theories of the creation of the universe: the Big Bang and Steady State theories. Inspired by Roger Penrose's theorem of a spacetime singularity in the centre of black holes, Hawking applied the same thinking to the entire universe; and, during 1965, he wrote his thesis on this topic. There were other positive developments: Hawking received a research fellowship at Gonville and Caius College; he obtained his PhD degree in applied mathematics and theoretical physics, specialising in general relativity and cosmology, in March 1966; and his essay entitled "Singularities and the Geometry of Space-Time" shared top honours with one by Penrose to win that year's prestigious Adams Prize.
CAREER
1966–1975
In his work, and in collaboration with Penrose, Hawking extended the singularity theorem concepts first explored in his doctoral thesis. This included not only the existence of singularities but also the theory that the universe might have started as a singularity. Their joint essay was the runner-up in the 1968 Gravity Research Foundation competition. In 1970 they published a proof that if the universe obeys the general theory of relativity and fits any of the models of physical cosmology developed by Alexander Friedmann, then it must have begun as a singularity. In 1969, Hawking accepted a specially created Fellowship for Distinction in Science to remain at Caius.
In 1970, Hawking postulated what became known as the second law of black hole dynamics, that the event horizon of a black hole can never get smaller.[83] With James M. Bardeen and Brandon Carter, he proposed the four laws of black hole mechanics, drawing an analogy with thermodynamics. To Hawking's irritation, Jacob Bekenstein, a graduate student of John Wheeler, went further—and ultimately correctly—to apply thermodynamic concepts literally.[85][86] In the early 1970s, Hawking's work with Carter, Werner Israel and David C. Robinson strongly supported Wheeler's no-hair theorem that no matter what the original material from which a black hole is created, it can be completely described by the properties of mass, electrical charge and rotation.[87][88] His essay titled "Black Holes" won the Gravity Research Foundation Award in January 1971.[89] Hawking's first book, The Large Scale Structure of Space-Time, written with George Ellis, was published in 1973.
Beginning in 1973, Hawking moved into the study of quantum gravity and quantum mechanics. His work in this area was spurred by a visit to Moscow and discussions with Yakov Borisovich Zel'dovich and Alexei Starobinsky, whose work showed that according to the uncertainty principle, rotating black holes emit particles. To Hawking's annoyance, his much-checked calculations produced findings that contradicted his second law, which claimed black holes could never get smaller,and supported Bekenstein's reasoning about their entropy.His results, which Hawking presented from 1974, showed that black holes emit radiation, known today as Hawking radiation, which may continue until they exhaust their energy and evaporate. Initially, Hawking radiation was controversial. However, by the late 1970s and following the publication of further research, the discovery was widely accepted as a significant breakthrough in theoretical physics. Hawking was elected a Fellow of the Royal Society (FRS) in 1974, a few weeks after the announcement of Hawking radiation. At the time, he was one of the youngest scientists to become a Fellow.
Hawking was appointed to the Sherman Fairchild Distinguished visiting professorship at the California Institute of Technology (Caltech) in 1970. He worked with a friend on the faculty, Kip Thorne, and engaged him in a scientific wager about whether the dark star Cygnus X-1 was a black hole. The wager was an "insurance policy" against the proposition that black holes did not exist. Hawking acknowledged that he had lost the bet in 1990, which was the first of several that he was to make with Thorne and others.Hawking has maintained ties to Caltech, spending a month there almost every year since this first visit.
1975–1990
Hawking returned to Cambridge in 1975 to a more academically senior post, as reader in gravitational physics. The mid to late 1970s were a period of growing public interest in black holes and of the physicists who were studying them. Hawking was regularly interviewed for print and television. He also received increasing academic recognition of his work. In 1975, he was awarded both the Eddington Medal and the Pius XI Gold Medal, and in 1976 the Dannie Heineman Prize, the Maxwell Prize and the Hughes Medal. He was appointed a professor with a chair in gravitational physics in 1977. The following year he received the Albert Einstein Medal and an honorary doctorate from the University of Oxford.
In the late 1970s, Hawking was elected Lucasian Professor of Mathematics at the University of Cambridge.His inaugural lecture as Lucasian Professor of Mathematics was titled: "Is the End in Sight for Theoretical Physics" and proposed N=8 Supergravity as the leading theory to solve many of the outstanding problems physicists were studying. His promotion coincided with a health crisis which led to his accepting, albeit reluctantly, some nursing services at home. At the same time, he was also making a transition in his approach to physics, becoming more intuitive and speculative rather than insisting on mathematical proofs. "I would rather be right than rigorous", he told Kip Thorne. In 1981, he proposed that information in a black hole is irretrievably lost when a black hole evaporates. This information paradox violates the fundamental tenet of quantum mechanics, and led to years of debate, including "the Black Hole War" with Leonard Susskind and Gerard 't Hooft.
Cosmological inflation – a theory proposing that following the Big Bang, the universe initially expanded incredibly rapidly before settling down to a slower expansion – was proposed by Alan Guth and also developed by Andrei Linde. Following a conference in Moscow in October 1981, Hawking and Gary Gibbons organized a three-week Nuffield Workshop in the summer of 1982 on "The Very Early Universe" at Cambridge University, which focused mainly on inflation theory. Hawking also began a new line of quantum theory research into the origin of the universe. In 1981 at a Vatican conference, he presented work suggesting that there might be no boundary – or beginning or ending – to the universe. He subsequently developed the research in collaboration with Jim Hartle, and in 1983 they published a model, known as the Hartle–Hawking state. It proposed that prior to the Planck epoch, the universe had no boundary in space-time; before the Big Bang, time did not exist and the concept of the beginning of the universe is meaningless. The initial singularity of the classical Big Bang models was replaced with a region akin to the North Pole. One cannot travel north of the North Pole, but there is no boundary there – it is simply the point where all north-running lines meet and end. Initially, the no-boundary proposal predicted a closed universe, which had implications about the existence of God. As Hawking explained, "If the universe has no boundaries but is self-contained... then God would not have had any freedom to choose how the universe began."
Hawking did not rule out the existence of a Creator, asking in A Brief History of Time "Is the unified theory so compelling that it brings about its own existence?" In his early work, Hawking spoke of God in a metaphorical sense. In A Brief History of Time he wrote: "If we discover a complete theory, it would be the ultimate triumph of human reason – for then we should know the mind of God." In the same book he suggested that the existence of God was not necessary to explain the origin of the universe. Later discussions with Neil Turok led to the realisation that the existence of God was also compatible with an open universe.
Further work by Hawking in the area of arrows of time led to the 1985 publication of a paper theorising that if the no-boundary proposition were correct, then when the universe stopped expanding and eventually collapsed, time would run backwards. A paper by Don Page and independent calculations by Raymond Laflamme led Hawking to withdraw this concept. Honours continued to be awarded: in 1981 he was awarded the American Franklin Medal, and in 1982 made a Commander of the Order of the British Empire (CBE). Awards do not pay the bills, however, and motivated by the need to finance the children's education and home expenses, in 1982 Hawking determined to write a popular book about the universe that would be accessible to the general public. Instead of publishing with an academic press, he signed a contract with Bantam Books, a mass market publisher, and received a large advance for his book. A first draft of the book, called A Brief History of Time, was completed in 1984.
One of the first messages Hawking produced with his speech-generating device was a request for his assistant to help him finish writing A Brief History of Time. Peter Guzzardi, his editor at Bantam, pushed him to explain his ideas clearly in non-technical language, a process that required many revisions from an increasingly irritated Hawking. The book was published in April 1988 in the US and in June in the UK, and it proved to be an extraordinary success, rising quickly to the top of bestseller lists in both countries and remaining there for months. The book was translated into many languages, and ultimately sold an estimated 9 million copies. Media attention was intense, and a Newsweek magazine cover and a television special both described him as "Master of the Universe". Success led to significant financial rewards, but also the challenges of celebrity status. Hawking travelled extensively to promote his work, and enjoyed partying and dancing into the small hours. He had difficulty refusing the invitations and visitors, which left limited time for work and his students. Some colleagues were resentful of the attention Hawking received, feeling it was due to his disability. He received further academic recognition, including five more honorary degrees,[149] the Gold Medal of the Royal Astronomical Society (1985), the Paul Dirac Medal (1987) and, jointly with Penrose, the prestigious Wolf Prize (1988). In 1989, he was appointed Member of the Order of the Companions of Honour (CH). He reportedly declined a knighthood.
1990–2000
Hawking pursued his work in physics: in 1993 he co-edited a book on Euclidean quantum gravity with Gary Gibbons and published a collected edition of his own articles on black holes and the Big Bang. In 1994, at Cambridge's Newton Institute, Hawking and Penrose delivered a series of six lectures that were published in 1996 as "The Nature of Space and Time". In 1997, he conceded a 1991 public scientific wager made with Kip Thorne and John Preskill of Caltech. Hawking had bet that Penrose's proposal of a "cosmic censorship conjecture" – that there could be no "naked singularities" unclothed within a horizon – was correct. After discovering his concession might have been premature, a new, more refined, wager was made. This one specified that such singularities would occur without extra conditions. The same year, Thorne, Hawking and Preskill made another bet, this time concerning the black hole information paradox. Thorne and Hawking argued that since general relativity made it impossible for black holes to radiate and lose information, the mass-energy and information carried by Hawking radiation must be "new", and not from inside the black hole event horizon. Since this contradicted the quantum mechanics of microcausality, quantum mechanics theory would need to be rewritten. Preskill argued the opposite, that since quantum mechanics suggests that the information emitted by a black hole relates to information that fell in at an earlier time, the concept of black holes given by general relativity must be modified in some way.
Hawking also maintained his public profile, including bringing science to a wider audience. A film version of A Brief History of Time, directed by Errol Morris and produced by Steven Spielberg, premiered in 1992. Hawking had wanted the film to be scientific rather than biographical, but he was persuaded otherwise. The film, while a critical success, was, however, not widely released. A popular-level collection of essays, interviews, and talks titled Black Holes and Baby Universes and Other Essays was published in 1993, and a six-part television series Stephen Hawking's Universe and a companion book appeared in 1997. As Hawking insisted, this time the focus was entirely on science.
2000–present
Hawking continued his writings for a popular audience, publishing The Universe in a Nutshell in 2001, and A Briefer History of Time, which he wrote in 2005 with Leonard Mlodinow to update his earlier works with the aim of making them accessible to a wider audience, and God Created the Integers, which appeared in 2006. Along with Thomas Hertog at CERN and Jim Hartle, from 2006 on Hawking developed a theory of "top-down cosmology", which says that the universe had not one unique initial state but many different ones, and therefore that it is inappropriate to formulate a theory that predicts the universe's current configuration from one particular initial state. Top-down cosmology posits that the present "selects" the past from a superposition of many possible histories. In doing so, the theory suggests a possible resolution of the fine-tuning question.
Hawking continued to travel widely, including trips to Chile, Easter Island, South Africa, Spain (to receive the Fonseca Prize in 2008),] Canada, and numerous trips to the United States. For practical reasons related to his disability, Hawking increasingly travelled by private jet, and by 2011 that had become his only mode of international travel. By 2003, consensus among physicists was growing that Hawking was wrong about the loss of information in a black hole. In a 2004 lecture in Dublin, he conceded his 1997 bet with Preskill, but described his own, somewhat controversial solution to the information paradox problem, involving the possibility that black holes have more than one topology. In the 2005 paper he published on the subject, he argued that the information paradox was explained by examining all the alternative histories of universes, with the information loss in those with black holes being cancelled out by those without such loss. In January 2014 he called the alleged loss of information in black holes his "biggest blunder".
As part of another longstanding scientific dispute, Hawking had emphatically argued, and bet, that the Higgs boson would never be found.[182] The particle was proposed to exist as part of the Higgs field theory by Peter Higgs in 1964. Hawking and Higgs engaged in a heated and public debate over the matter in 2002 and again in 2008, with Higgs criticising Hawking's work and complaining that Hawking's "celebrity status gives him instant credibility that others do not have." The particle was discovered in July 2012 at CERN following construction of the Large Hadron Collider. Hawking quickly conceded that he had lost his bet and said that Higgs should win the Nobel Prize for Physics, which he did in 2013.
In 2007, Hawking and his daughter Lucy published George's Secret Key to the Universe, a children's book designed to explain theoretical physics in an accessible fashion and featuring characters similar to those in the Hawking family.[188] The book was followed by sequels in 2009, 2011 and 2014.
In 2002, following a UK-wide vote, the BBC included Hawking in their list of the 100 Greatest Britons.[190] He was awarded the Copley Medal from the Royal Society (2006), the Presidential Medal of Freedom, which is America's highest civilian honour (2009), and the Russian Special Fundamental Physics Prize (2013).
Several buildings have been named after him, including the Stephen W. Hawking Science Museum in San Salvador, El Salvador, the Stephen Hawking Building in Cambridge, and the Stephen Hawking Centre at the Perimeter Institute in Canada.Appropriately, given Hawking's association with time, he unveiled the mechanical "Chronophage" (or time-eating) Corpus Clock at Corpus Christi College Cambridge in September 2008.
During his career, Hawking has supervised 39 successful PhD students. As required by Cambridge University regulations, Hawking retired as Lucasian Professor of Mathematics in 2009. Despite suggestions that he might leave the United Kingdom as a protest against public funding cuts to basic scientific research, Hawking has continued to work as director of research at the Cambridge University Department of Applied Mathematics and Theoretical Physics, and indicated in 2012 that he had no plans to retire.
On 28 June 2009, as a tongue-in-cheek test of his 1992 conjecture that travel into the past is effectively impossible, Hawking held a party open to all, complete with hors d'oeuvres and iced champagne, but only publicized the party after it was over so that only time-travellers would know to attend; as expected, nobody showed up to the party.
On 20 July 2015, Hawking helped launch Breakthrough Initiatives, an effort to search for extraterrestrial life. In 2015, Richard Branson offered Stephen Hawking a seat on the Virgin Galactic spaceship for free. While no hard date has been set for launch, Virgin Galactic's SpaceShipTwo is slated to launch at the end of 2017. At 75, Hawking will not be the oldest person ever to go to space (John Glenn returned to space at age 77), but he will be the first person to go to space with amyotrophic lateral sclerosis (ALS). While this will be Hawking's first time in space, it will not be the first time he will have experienced weightlessness: in 2007, he had flown into zero gravity aboard a specially-modified Boeing 727-200 aircraft. Hawking created Stephen Hawking: Expedition New Earth, a documentary on space colonization, as a summer 2017 episode of Tomorrow's World.
In August 2015, Hawking said that not all information is lost when something enters a black hole and there might be a possibility to retrieve information from a black hole according to his theory.