Modern birds retain the physical characteristics of baby dinosaurs, according to a new Nature study that found birds are even more closely related to dinos than previously thought.
Depending on the non-avian dinosaur and bird compared, that might be hard to believe. A toothy, angry reconstruction of Tyrannosaurus rex, for example, on first glance looks little like a common garden blue jay.
When researchers go beyond the surface to the tissue and skull levels, however, the similarities become more obvious.
Harvard University's Arkhat Abzhanov, associate professor of organismic and evolutionary biology, and Bhart-Anjan Bhullar, a Ph.D. student in Abzhanov laboratory and the first author of the study, did just that and found evidence that the evolution of birds is the result of a drastic change in how dinosaurs developed. Rather than take years to reach sexual maturity, as many dinosaurs did, birds sped up the clock (some species take as little as 12 weeks to mature), allowing them to lock into their baby dinosaur look.
"What is interesting about this research is the way it illustrates evolution as a developmental phenomenon," Abzhanov was quoted as saying in a press release. "By changing the developmental biology in early species, nature has produced the modern bird –- an entirely new creature –- and one that, with approximately 10,000 species, is today the most successful group of land vertebrates on the planet."
"The evolution of the many characteristics of birds –- things like feathers, flight, and wishbones -– has traditionally been a difficult problem for biologists," Mark Norell, chair of the division of paleontology at the American Museum of Natural History and one of the paper's co-authors, added.
"By analyzing fossil evidence from skeletons, eggs, and soft tissue of bird-like dinosaurs and primitive birds, we've learned that birds are living theropod dinosaurs, a group of carnivorous animals that include Velociraptor," Norell continued. "This new work advances our knowledge by providing a powerful example of how developmental changes played a major role in the origin and evolution of birds."
Read more at Discovery News
May 31, 2012
Milky Way Doomed to Crash with Andromeda
Four billion years from now, the Milky Way galaxy as we know it will cease to exist.
Our Milky Way is bound for a head-on collision with the similar-sized Andromeda galaxy, researchers announced today (May 31). Over time, the huge galactic smashup will create an entirely new hybrid galaxy, one likely bearing an elliptical shape rather than the Milky Way's trademark spiral-armed disk.
"We do know of other galaxies in the local universe around us that are in the process of colliding and merging," Roeland van der Marel, of the Space Telescope Science Institute in Baltimore, told reporters today. "However, what makes the future merger of the Andromeda galaxy and the Milky Way so special is that it will happen to us."
Astronomers have long known that the Milky Way and Andromeda, which is also known as M31, are barrelling toward one another at a speed of about 250,000 mph (400,000 kph). They have also long suspected that the two galaxies may slam into each other billions of years down the road.
However, such discussions of the future galactic crash have always remained somewhat speculative, because no one had managed to measure Andromeda's sideways motion — a key component of that galaxy's path through space.
But that's no longer the case.
Van der Marel and his colleagues used NASA's Hubble space telescope to repeatedly observe select regions of Andromeda over a seven-year period. They were able to measure the galaxy's sideways (or tangential) motion, and they found that Andromeda and the Milky Way are indeed bound for a direct hit.
"The Andromeda galaxy is heading straight in our direction," van der Marel said. "The galaxies will collide, and they will merge together to form one new galaxy." He and his colleagues also created a video simulation of the Milky Way crash into Andromeda.
That merger, van der Marel added, begins in 4 billion years and will be complete by about 6 billion years from now.
A future cosmic crash
Such a dramatic event has never occurred in the long history of our Milky Way, which likely began taking shape about 13.5 billion years ago.
"The Milky Way has had, probably, quite a lot of small, minor mergers," said Rosemary Wyse of Johns Hopkins University in Baltimore, who was not affiliated with the new study. "But this major merger will be unprecedented."
The merger poses no real danger of destroying Earth or our solar system, researchers said. The stretches of empty space separating the stars in the two galaxies will remain vast, making any collisions or serious perturbations unlikely.
However, our solar system will likely get booted out to a different position in the new galaxy, which some astronomers have dubbed the "Milkomeda galaxy." Simulations show that we'll probably occupy a spot much farther from the galactic core than we do today, researchers said.
A new night sky
And the collision will change our night sky dramatically. If any humans are still around 3.75 billion years from now, they'll see Andromeda fill their field of view as it sidles up next to our own Milky Way. For the next few billion years after that, stargazers will be spellbound by the merger, which will trigger intense bouts of star formation.
Finally, by about 7 billion years from now, the bright core of the elliptical Milkomeda galaxy will dominate the night sky, researchers said. (The odds of viewing this sight, at least from Earth, are pretty slim, since the sun is predicted to bloat into a huge red giant 5 or 6 billion years from now.)
Read more at Discovery News
Our Milky Way is bound for a head-on collision with the similar-sized Andromeda galaxy, researchers announced today (May 31). Over time, the huge galactic smashup will create an entirely new hybrid galaxy, one likely bearing an elliptical shape rather than the Milky Way's trademark spiral-armed disk.
"We do know of other galaxies in the local universe around us that are in the process of colliding and merging," Roeland van der Marel, of the Space Telescope Science Institute in Baltimore, told reporters today. "However, what makes the future merger of the Andromeda galaxy and the Milky Way so special is that it will happen to us."
Astronomers have long known that the Milky Way and Andromeda, which is also known as M31, are barrelling toward one another at a speed of about 250,000 mph (400,000 kph). They have also long suspected that the two galaxies may slam into each other billions of years down the road.
However, such discussions of the future galactic crash have always remained somewhat speculative, because no one had managed to measure Andromeda's sideways motion — a key component of that galaxy's path through space.
But that's no longer the case.
Van der Marel and his colleagues used NASA's Hubble space telescope to repeatedly observe select regions of Andromeda over a seven-year period. They were able to measure the galaxy's sideways (or tangential) motion, and they found that Andromeda and the Milky Way are indeed bound for a direct hit.
"The Andromeda galaxy is heading straight in our direction," van der Marel said. "The galaxies will collide, and they will merge together to form one new galaxy." He and his colleagues also created a video simulation of the Milky Way crash into Andromeda.
That merger, van der Marel added, begins in 4 billion years and will be complete by about 6 billion years from now.
A future cosmic crash
Such a dramatic event has never occurred in the long history of our Milky Way, which likely began taking shape about 13.5 billion years ago.
"The Milky Way has had, probably, quite a lot of small, minor mergers," said Rosemary Wyse of Johns Hopkins University in Baltimore, who was not affiliated with the new study. "But this major merger will be unprecedented."
The merger poses no real danger of destroying Earth or our solar system, researchers said. The stretches of empty space separating the stars in the two galaxies will remain vast, making any collisions or serious perturbations unlikely.
However, our solar system will likely get booted out to a different position in the new galaxy, which some astronomers have dubbed the "Milkomeda galaxy." Simulations show that we'll probably occupy a spot much farther from the galactic core than we do today, researchers said.
A new night sky
And the collision will change our night sky dramatically. If any humans are still around 3.75 billion years from now, they'll see Andromeda fill their field of view as it sidles up next to our own Milky Way. For the next few billion years after that, stargazers will be spellbound by the merger, which will trigger intense bouts of star formation.
Finally, by about 7 billion years from now, the bright core of the elliptical Milkomeda galaxy will dominate the night sky, researchers said. (The odds of viewing this sight, at least from Earth, are pretty slim, since the sun is predicted to bloat into a huge red giant 5 or 6 billion years from now.)
Read more at Discovery News
May 30, 2012
Tiny Genetic Variations Led to Big Changes in the Evolving Human Brain
Changes to just three genetic letters among billions contributed to the evolution and development of the mammalian motor sensory circuits and laid the groundwork for the defining characteristics of the human brain, Yale University researchers report.
In a study published in the May 31 issue of the journal Nature, Yale researchers found that a small, simple change in the mammalian genome was critical to the evolution of the corticospinal neural circuits. This circuitry directly connects the cerebral cortex, the conscious part of the human brain, with the brainstem and the spinal cord to make possible the fine, skilled movements necessary for functions such as tool use and speech. The evolutionary mechanisms that drive the formation of the corticospinal circuit, which is a mammalian-specific advance, had remained largely mysterious.
"What we found is a small genetic element that is part of the gene regulatory network directing neurons in the cerebral cortex to form the motor sensory circuits," said Nenad Sestan, professor of neurobiology, researcher for the Kavli Institute for Neuroscience, and senior author of the paper.
Most mammalian genomes contain approximately 22,000 protein-encoding genes. The critical drivers of evolution and development, however, are thought to reside in the non-coding portions of the genome that regulate when and where genes are active. These so-called cis-regulatory elements control the activation of genes that carry out the formation of basic body plans in all organisms.
Sungbo Shim, the first author, and other members of Sestan's lab identified one such regulatory DNA region they named E4, which specifically drives the development of the corticospinal system by controlling the dynamic activity of a gene called Fezf2 -- which, in turn, directs the formation of the corticospinal circuits. E4 is conserved in all mammals but divergent in other craniates, suggesting that it is important to both the emergence and survival of mammalian species. The species differences within E4 are tiny, but crucially drive the regulation of E4 activity by a group of regulatory proteins, or transcription factors, that include SOX4, SOX11, and SOX5. In cooperation, they control the dynamic activation and repression of E4 to shape the development of the corticospinal circuits in the developing embryo.
Read more at Science Daily
In a study published in the May 31 issue of the journal Nature, Yale researchers found that a small, simple change in the mammalian genome was critical to the evolution of the corticospinal neural circuits. This circuitry directly connects the cerebral cortex, the conscious part of the human brain, with the brainstem and the spinal cord to make possible the fine, skilled movements necessary for functions such as tool use and speech. The evolutionary mechanisms that drive the formation of the corticospinal circuit, which is a mammalian-specific advance, had remained largely mysterious.
"What we found is a small genetic element that is part of the gene regulatory network directing neurons in the cerebral cortex to form the motor sensory circuits," said Nenad Sestan, professor of neurobiology, researcher for the Kavli Institute for Neuroscience, and senior author of the paper.
Most mammalian genomes contain approximately 22,000 protein-encoding genes. The critical drivers of evolution and development, however, are thought to reside in the non-coding portions of the genome that regulate when and where genes are active. These so-called cis-regulatory elements control the activation of genes that carry out the formation of basic body plans in all organisms.
Sungbo Shim, the first author, and other members of Sestan's lab identified one such regulatory DNA region they named E4, which specifically drives the development of the corticospinal system by controlling the dynamic activity of a gene called Fezf2 -- which, in turn, directs the formation of the corticospinal circuits. E4 is conserved in all mammals but divergent in other craniates, suggesting that it is important to both the emergence and survival of mammalian species. The species differences within E4 are tiny, but crucially drive the regulation of E4 activity by a group of regulatory proteins, or transcription factors, that include SOX4, SOX11, and SOX5. In cooperation, they control the dynamic activation and repression of E4 to shape the development of the corticospinal circuits in the developing embryo.
Read more at Science Daily
Can a 16-year-old Be a Math Genius?
There's a story in math circles that a famous Hungarian mathematician, Paul Erdos, used to speak of the Riemann hypothesis, a famous unsolved problem, saying that all infants were probably born knowing how to prove it, but then forgot the proof by the time they learned to talk.
While babies working out mathematical proofs may be a bit of a stretch, the news that a 16-year-old may have solved a 350-year-old problem (whether true or not), poses the question of just how youth approach math differently than adults.
Edward Frenkel, a Professor of Mathematics at University of California, Berkeley, and currently Eilenberg Visiting Professor at Columbia University, is now 44. But by the age of 21, he had already been invited to be a visiting professor at Harvard.
"When you're young, you're fast and quick and able to solve things quickly ... but you may not be able to see how the different pieces of mathematics fit together," he said. "That comes with experience."
In the last few years, he's been working with the The Langlands Program (a system of advanced mathematical ideas developed by Robert Langlands in the late 1960s with the goal of tying together different areas of mathematics). When he was younger, he said, he couldn't possibly have seen the big picture in that way.
"Mathematics is not like running the 100-meter dash," Frenkel said. "It's more like a marathon."
Still, he says "there's something to be said for not being spoiled by the traditional educational system when you're young." What is essential, he believes, is the right mentorship. "Math is so abstract, you need guidance. You need someone to open the door."
Mathematics professors who work with teens say that they often see glimpses of brilliance in kids as young as 13, and that "often these long-standing problems are solved by a mathematician who takes a completely different approach," says Jonathan Rogness, assistant professor and director of the Mathematics Center for Educational Programs at the University of Minnesota.
Still, working on famous, unsolved problems is rare until later in a career.
"Usually these problems are unsuitable for study by very young researchers, since they are too hard, too well studied, and require too much background to do anything of value," said MIT mathematics professor Pavel Etingof, who also works with a high school research program at MIT.
Etingof, who was 24 when he received his Ph.D., says that success in math comes from a combination of brainpower and experience.
"Brainpower starts to decrease after a certain age, while experience accumulates over years," he said. "Experience is not as important in mathematics as in some other fields, but it is important. So the power of a mathematician often peaks in his/her 30s. Which means that young people do have an advantage. But not people who are 16. Certainly someone who is 32 has a lot of advantage over someone who is 16."
Read more at Discovery News
While babies working out mathematical proofs may be a bit of a stretch, the news that a 16-year-old may have solved a 350-year-old problem (whether true or not), poses the question of just how youth approach math differently than adults.
Edward Frenkel, a Professor of Mathematics at University of California, Berkeley, and currently Eilenberg Visiting Professor at Columbia University, is now 44. But by the age of 21, he had already been invited to be a visiting professor at Harvard.
"When you're young, you're fast and quick and able to solve things quickly ... but you may not be able to see how the different pieces of mathematics fit together," he said. "That comes with experience."
In the last few years, he's been working with the The Langlands Program (a system of advanced mathematical ideas developed by Robert Langlands in the late 1960s with the goal of tying together different areas of mathematics). When he was younger, he said, he couldn't possibly have seen the big picture in that way.
"Mathematics is not like running the 100-meter dash," Frenkel said. "It's more like a marathon."
Still, he says "there's something to be said for not being spoiled by the traditional educational system when you're young." What is essential, he believes, is the right mentorship. "Math is so abstract, you need guidance. You need someone to open the door."
Mathematics professors who work with teens say that they often see glimpses of brilliance in kids as young as 13, and that "often these long-standing problems are solved by a mathematician who takes a completely different approach," says Jonathan Rogness, assistant professor and director of the Mathematics Center for Educational Programs at the University of Minnesota.
Still, working on famous, unsolved problems is rare until later in a career.
"Usually these problems are unsuitable for study by very young researchers, since they are too hard, too well studied, and require too much background to do anything of value," said MIT mathematics professor Pavel Etingof, who also works with a high school research program at MIT.
Etingof, who was 24 when he received his Ph.D., says that success in math comes from a combination of brainpower and experience.
"Brainpower starts to decrease after a certain age, while experience accumulates over years," he said. "Experience is not as important in mathematics as in some other fields, but it is important. So the power of a mathematician often peaks in his/her 30s. Which means that young people do have an advantage. But not people who are 16. Certainly someone who is 32 has a lot of advantage over someone who is 16."
Read more at Discovery News
Earhart's Anti-Freckle Ointment Jar Possibly Recovered
A small cosmetic jar offers more circumstantial evidence that the legendary aviator, Amelia Earhart, died on an uninhabited island in the southwestern Pacific republic of Kiribati.
Found broken in five pieces, the ointment pot was collected on Nikumaroro Island by researchers of The International Group for Historic Aircraft Recovery (TIGHAR), which has long been investigating the last, fateful flight taken by Earhart 75 years ago.
When reassembled, the glass fragments make up a nearly complete jar identical in shape to the ones used by Dr. C. H Berry's Freckle Ointment. The ointment was marketed in the early 20th century as a concoction guaranteed to make freckles fade.
"It's well documented Amelia had freckles and disliked having them," Joe Cerniglia, the TIGHAR researcher who spotted the freckle ointment as a possible match, told Discovery News.
The jar fragments were found together with other artifacts during TIGHAR's nine archaeological expeditions to the tiny coral atoll believed to be Earhart's final resting place.
Analysis of the recovered artifacts will be presented at a three-day conference in Arlington, Va. A new study of post loss radio signals and the latest forensic analysis of a photograph believed to show the landing gear of Earhart's aircraft on Nikumaroro reef three months after her disappearance, will be also discussed.
Beginning on June 1st, the symposium will highlight TIGHAR's high-tech search next July to find pieces of Earhart's Lockheed Electra aircraft.
The pilot mysteriously vanished while flying over the Pacific Ocean on July 2, 1937 during a record attempt to fly around the world at the equator. The general consensus has been that Earhart's twin-engined plane ran out of fuel and crashed in the Pacific Ocean, somewhere near Howland Island.
But according to Ric Gillespie, executive director of TIGHAR, there is an alternative scenario.
"The navigation line Amelia described in her final in-flight radio transmission passed through not only Howland Island, her intended destination, but also Gardner Island, now called Nikumaroro," Gillespie said at a special press event on March 20 hosted by Secretary of State Hillary Clinton.
According to Gillespie, the possibility that Earhart and navigator Fred Noonan might have made an emergency landing on Nikumaroro's flat coral reef, some 300 miles southeast of their target destination, is supported by a number of artifacts which, combined with archival research, strongly point to a castaway presence on the remote island.
"Broken shards from several glass containers have been recovered from the Seven Site, the archaeological site on the southeast end of Nikumaroro that fits the description of where the partial skeleton of a castaway was discovered in 1940," Gillespie told Discovery News.
Found with the skeletal remains at that time were part of a man's shoe, part of a woman's shoe, a box that had once contained a sextant, remnants of a fire, bird bones and turtle bones -- all suggesting that the site had been the castaways' camp.
"Unfortunately, the bones and artifacts found in 1940 were subsequently lost," said Gillespie.
Like most archaeological sites, the Seven Site has yielded evidence of activity from several different periods in the island's history and not all of the glass recovered from the site is attributable to the castaway.
"For example, the top of a war-time Coke bottle and pieces of what was probably a large salt shaker of a style used by the U.S. military are almost certainly relics of one or more U.S. Coast Guard target shooting forays," Gillespie said.
Much of the glass, however, appears to be associated with a castaway presence.
Two of the bottles, both dating from the 1930s, were found in what had been a small campfire.
"The bottoms of both bottles are melted but the upper portions, although shattered, are not heat-damaged -- implying that the bottles once stood upright in the fire. A length of wire found in the same spot has been twisted in such a way as to serve as a handle for holding a bottleneck," said Gillespie.
Read more at Discovery News
Found broken in five pieces, the ointment pot was collected on Nikumaroro Island by researchers of The International Group for Historic Aircraft Recovery (TIGHAR), which has long been investigating the last, fateful flight taken by Earhart 75 years ago.
When reassembled, the glass fragments make up a nearly complete jar identical in shape to the ones used by Dr. C. H Berry's Freckle Ointment. The ointment was marketed in the early 20th century as a concoction guaranteed to make freckles fade.
"It's well documented Amelia had freckles and disliked having them," Joe Cerniglia, the TIGHAR researcher who spotted the freckle ointment as a possible match, told Discovery News.
The jar fragments were found together with other artifacts during TIGHAR's nine archaeological expeditions to the tiny coral atoll believed to be Earhart's final resting place.
Analysis of the recovered artifacts will be presented at a three-day conference in Arlington, Va. A new study of post loss radio signals and the latest forensic analysis of a photograph believed to show the landing gear of Earhart's aircraft on Nikumaroro reef three months after her disappearance, will be also discussed.
Beginning on June 1st, the symposium will highlight TIGHAR's high-tech search next July to find pieces of Earhart's Lockheed Electra aircraft.
The pilot mysteriously vanished while flying over the Pacific Ocean on July 2, 1937 during a record attempt to fly around the world at the equator. The general consensus has been that Earhart's twin-engined plane ran out of fuel and crashed in the Pacific Ocean, somewhere near Howland Island.
But according to Ric Gillespie, executive director of TIGHAR, there is an alternative scenario.
"The navigation line Amelia described in her final in-flight radio transmission passed through not only Howland Island, her intended destination, but also Gardner Island, now called Nikumaroro," Gillespie said at a special press event on March 20 hosted by Secretary of State Hillary Clinton.
According to Gillespie, the possibility that Earhart and navigator Fred Noonan might have made an emergency landing on Nikumaroro's flat coral reef, some 300 miles southeast of their target destination, is supported by a number of artifacts which, combined with archival research, strongly point to a castaway presence on the remote island.
"Broken shards from several glass containers have been recovered from the Seven Site, the archaeological site on the southeast end of Nikumaroro that fits the description of where the partial skeleton of a castaway was discovered in 1940," Gillespie told Discovery News.
Found with the skeletal remains at that time were part of a man's shoe, part of a woman's shoe, a box that had once contained a sextant, remnants of a fire, bird bones and turtle bones -- all suggesting that the site had been the castaways' camp.
"Unfortunately, the bones and artifacts found in 1940 were subsequently lost," said Gillespie.
Like most archaeological sites, the Seven Site has yielded evidence of activity from several different periods in the island's history and not all of the glass recovered from the site is attributable to the castaway.
"For example, the top of a war-time Coke bottle and pieces of what was probably a large salt shaker of a style used by the U.S. military are almost certainly relics of one or more U.S. Coast Guard target shooting forays," Gillespie said.
Much of the glass, however, appears to be associated with a castaway presence.
Two of the bottles, both dating from the 1930s, were found in what had been a small campfire.
"The bottoms of both bottles are melted but the upper portions, although shattered, are not heat-damaged -- implying that the bottles once stood upright in the fire. A length of wire found in the same spot has been twisted in such a way as to serve as a handle for holding a bottleneck," said Gillespie.
Read more at Discovery News
Setting the Galaxy's Age
Scientists trying to piece together the story of how the universe evolved from clumps of dark matter into the sparkling galaxies of today have had to work around a central problem -- no reliable technique to determine the age of small stars like the sun, which are the most common.
An astronomer at the Space Telescope Science Institute has taken a big step in resolving the puzzle. Jason Kalirai used fresh stellar corpses of sun-like stars to serve as a key to time.
“It’s like putting hands on a clock,” Timothy Beers, director of Kitt Peak National Observatory, told Discovery News.
By analyzing four of these newly dead stars, Kalirai determined that the inner halo of stars surrounding the Milky Way is 11.4 billion years old.
The halo is spherical cloud of objects that are not orderly rotating around the center of the galaxy, like the sun and other stars in the Milky Way’s disk do.
“You’re either rotating around the center in an organized fashion -- that’s the disk -- or you’re supported by rapid, random motions. That’s the halo,” Beers said.
Within the halo are at least two populations of stars, again characterized less by location and more by relative motion.
How the stars came to be part of the Milky Way remains a mystery, but Kalirai’s technique can be used to home in on when they arrived.
“When an object comes into the halo, it gets shredded from its parent galaxy and depending on what the orbit was of that parent galaxy it is going to be moving in that orientation. By knowing when those stars formed, we have a limit on when they were accreted into the Milky Way because they couldn’t have been accreted before they were formed,“ Kalirai told Discovery News.
“Until this came along there was really no good way to quantify the age of the stellar distribution,” Beers added.
“Jason takes a handful of a set of stars, believed to be part of the inner halo population, age them and assigns them to a population from which they were drawn,” said Beers, who called the approach “ingenious.”
Kalirai chose so-called white dwarf stars as his portholes because they are simple stars whose light can be broken down into composite wavelengths impregnated with features directly relating to the star’s properties, such as its mass and temperature.
“You can measure it in a straightforward way. You can’t do that for normal hydrogen-burning stars,” Kalirai said.
White dwarfs are what remain after sun-like stars burn through all their hydrogen and shed their outer layers. They are 1 million times more dense than anything on Earth.
“If you took a tablespoon of material from the surface of a white dwarf, it would weigh as much as a school bus here on Earth,” Kalirai said.
They are also terribly common in the Milky Way. About 98 percent of the stars in the galaxy will end their lives as white dwarfs.
Read more at Discovery News
An astronomer at the Space Telescope Science Institute has taken a big step in resolving the puzzle. Jason Kalirai used fresh stellar corpses of sun-like stars to serve as a key to time.
“It’s like putting hands on a clock,” Timothy Beers, director of Kitt Peak National Observatory, told Discovery News.
By analyzing four of these newly dead stars, Kalirai determined that the inner halo of stars surrounding the Milky Way is 11.4 billion years old.
The halo is spherical cloud of objects that are not orderly rotating around the center of the galaxy, like the sun and other stars in the Milky Way’s disk do.
“You’re either rotating around the center in an organized fashion -- that’s the disk -- or you’re supported by rapid, random motions. That’s the halo,” Beers said.
Within the halo are at least two populations of stars, again characterized less by location and more by relative motion.
How the stars came to be part of the Milky Way remains a mystery, but Kalirai’s technique can be used to home in on when they arrived.
“When an object comes into the halo, it gets shredded from its parent galaxy and depending on what the orbit was of that parent galaxy it is going to be moving in that orientation. By knowing when those stars formed, we have a limit on when they were accreted into the Milky Way because they couldn’t have been accreted before they were formed,“ Kalirai told Discovery News.
“Until this came along there was really no good way to quantify the age of the stellar distribution,” Beers added.
“Jason takes a handful of a set of stars, believed to be part of the inner halo population, age them and assigns them to a population from which they were drawn,” said Beers, who called the approach “ingenious.”
Kalirai chose so-called white dwarf stars as his portholes because they are simple stars whose light can be broken down into composite wavelengths impregnated with features directly relating to the star’s properties, such as its mass and temperature.
“You can measure it in a straightforward way. You can’t do that for normal hydrogen-burning stars,” Kalirai said.
White dwarfs are what remain after sun-like stars burn through all their hydrogen and shed their outer layers. They are 1 million times more dense than anything on Earth.
“If you took a tablespoon of material from the surface of a white dwarf, it would weigh as much as a school bus here on Earth,” Kalirai said.
They are also terribly common in the Milky Way. About 98 percent of the stars in the galaxy will end their lives as white dwarfs.
Read more at Discovery News
May 29, 2012
Why Swine Flu Virus Is Developing Drug Resistance
Computer chips of a type more commonly found in games consoles have been used by scientists at the University of Bristol to reveal how the flu virus resists anti-flu drugs such as Relenza and Tamiflu.
Professor Adrian Mulholland and Dr Christopher Woods from Bristol's School of Chemistry, together with colleagues in Thailand, used graphics processing units (GPUs) to simulate the molecular processes that take place when these drugs are used to treat the H1N1-2009 strain of influenza -- commonly known as 'swine flu'.
Their results, published May 29 in Biochemistry, provide new insight that could lead to the development of the next generation of antiviral treatments for flu.
H1N1-2009 is a new, highly adaptive virus derived from different gene segments of swine, avian, and human influenza. Within a few months of its appearance in early 2009, the H1N1-2009 strain caused the first flu pandemic of the 21st-century.
The antiviral drugs Relenza and Tamiflu, which target the neuraminidase (NA) enzyme, successfully treated the infection but widespread use of these drugs has led to a series of mutations in NA that reduce the drugs' effectiveness.
Clinical studies indicate that the double mutant of swine flu NA known as IRHY2 reduced the effectiveness of Relenza by 21 times and Tamiflu by 12,374 times -- that is, to the point where it has become an ineffective treatment.
To understand why the effectiveness of Relenza and Tamiflu is so seriously reduced by the occurrence of this mutation, the researchers performed long-timescale molecular dynamics (MD) simulations using GPUs.
Professor Mulholland said: "Our simulations showed that IRHY became resistant to Tamiflu due to the loss of key hydrogen bonds between the drug and residues in a part of the NA's structure known as the '150-loop'.
"This allowed NA to change from a closed to an open conformation. Tamiflu binds weakly with the open conformation due to poor electrostatic interactions between the drug and the active site, thus rendering the drug ineffective."
These findings suggest that drug resistance could be overcome by increasing hydrogen bond interactions between NA inhibitors and residues in the 150-loop, with the aim of maintaining the closed conformation.
Read more at Science Daily
Professor Adrian Mulholland and Dr Christopher Woods from Bristol's School of Chemistry, together with colleagues in Thailand, used graphics processing units (GPUs) to simulate the molecular processes that take place when these drugs are used to treat the H1N1-2009 strain of influenza -- commonly known as 'swine flu'.
Their results, published May 29 in Biochemistry, provide new insight that could lead to the development of the next generation of antiviral treatments for flu.
H1N1-2009 is a new, highly adaptive virus derived from different gene segments of swine, avian, and human influenza. Within a few months of its appearance in early 2009, the H1N1-2009 strain caused the first flu pandemic of the 21st-century.
The antiviral drugs Relenza and Tamiflu, which target the neuraminidase (NA) enzyme, successfully treated the infection but widespread use of these drugs has led to a series of mutations in NA that reduce the drugs' effectiveness.
Clinical studies indicate that the double mutant of swine flu NA known as IRHY2 reduced the effectiveness of Relenza by 21 times and Tamiflu by 12,374 times -- that is, to the point where it has become an ineffective treatment.
To understand why the effectiveness of Relenza and Tamiflu is so seriously reduced by the occurrence of this mutation, the researchers performed long-timescale molecular dynamics (MD) simulations using GPUs.
Professor Mulholland said: "Our simulations showed that IRHY became resistant to Tamiflu due to the loss of key hydrogen bonds between the drug and residues in a part of the NA's structure known as the '150-loop'.
"This allowed NA to change from a closed to an open conformation. Tamiflu binds weakly with the open conformation due to poor electrostatic interactions between the drug and the active site, thus rendering the drug ineffective."
These findings suggest that drug resistance could be overcome by increasing hydrogen bond interactions between NA inhibitors and residues in the 150-loop, with the aim of maintaining the closed conformation.
Read more at Science Daily
16th-Century Korean Mummy Provides Clue to Hepatitis B Virus Genetic Code
The discovery of a mummified Korean child with relatively preserved organs enabled an Israeli-South Korean scientific team to conduct a genetic analysis on a liver biopsy which revealed a unique hepatitis B virus (HBV) genotype C2 sequence common in Southeast Asia.
Additional analysis of the ancient HBV genomes may be used as a model to study the evolution of chronic hepatitis B and help understand the spread of the virus, possibly from Africa to East-Asia. It also may shed further light on the migratory pathway of hepatitis B in the Far East from China and Japan to Korea as well as to other regions in Asia and Australia where it is a major cause of cirrhosis and liver cancer.
The reconstruction of the ancient hepatitis B virus genetic code is the oldest full viral genome described in the scientific literature to date. It was reported in the May 21 edition of the scientific journal Hepathology by a research team from the Hebrew University of Jerusalem's Koret School of Veterinary Medicine, the Robert H. Smith Faculty of Agriculture, Food and Environment; the Hebrew University's Faculty of Medicine, the Hadassah Medical Center's Liver Unit; Dankook University and Seoul National University in South Korea.
Carbon 14 tests of the clothing of the mummy suggests that the boy lived around the 16th century during the Korean Joseon Dynasty. The viral DNA sequences recovered from the liver biopsy enabled the scientists to map the entire ancient hepatitis B viral genome.
Using modern-day molecular genetic techniques, the researchers compared the ancient DNA sequences with contemporary viral genomes disclosing distinct differences. The changes in the genetic code are believed to result from spontaneous mutations and possibly environmental pressures during the virus evolutionary process. Based on the observed mutations rates over time, the analysis suggests that the reconstructed mummy's hepatitis B virus DNA had its origin between 3,000 to 100,000 years ago.
The hepatitis B virus is transmitted through the contact with infected body fluids , i.e. from carrier mothers to their babies, through sexual contact and intravenous drug abuse. According to the World Health Organization, there are over 400 million carriers of the virus worldwide, predominantly in Africa, China and South Korea, where up to 15 percent of the population are cariers of the virus. In recent years, universal immunization of newborns against hepatitis B in Israel and in South Korea has lead to a massive decline in the incidence of infection.
Read more at Science Daily
Additional analysis of the ancient HBV genomes may be used as a model to study the evolution of chronic hepatitis B and help understand the spread of the virus, possibly from Africa to East-Asia. It also may shed further light on the migratory pathway of hepatitis B in the Far East from China and Japan to Korea as well as to other regions in Asia and Australia where it is a major cause of cirrhosis and liver cancer.
The reconstruction of the ancient hepatitis B virus genetic code is the oldest full viral genome described in the scientific literature to date. It was reported in the May 21 edition of the scientific journal Hepathology by a research team from the Hebrew University of Jerusalem's Koret School of Veterinary Medicine, the Robert H. Smith Faculty of Agriculture, Food and Environment; the Hebrew University's Faculty of Medicine, the Hadassah Medical Center's Liver Unit; Dankook University and Seoul National University in South Korea.
Carbon 14 tests of the clothing of the mummy suggests that the boy lived around the 16th century during the Korean Joseon Dynasty. The viral DNA sequences recovered from the liver biopsy enabled the scientists to map the entire ancient hepatitis B viral genome.
Using modern-day molecular genetic techniques, the researchers compared the ancient DNA sequences with contemporary viral genomes disclosing distinct differences. The changes in the genetic code are believed to result from spontaneous mutations and possibly environmental pressures during the virus evolutionary process. Based on the observed mutations rates over time, the analysis suggests that the reconstructed mummy's hepatitis B virus DNA had its origin between 3,000 to 100,000 years ago.
The hepatitis B virus is transmitted through the contact with infected body fluids , i.e. from carrier mothers to their babies, through sexual contact and intravenous drug abuse. According to the World Health Organization, there are over 400 million carriers of the virus worldwide, predominantly in Africa, China and South Korea, where up to 15 percent of the population are cariers of the virus. In recent years, universal immunization of newborns against hepatitis B in Israel and in South Korea has lead to a massive decline in the incidence of infection.
Read more at Science Daily
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Occupy the Neolithic: Social Immobility in the Stone Age
Even the most democratic societies are rife with social and economic inequalities, as the current tension between the poorer “99 percent” and the richest “1 percent” vividly illustrates. But just how early in human events such social hierarchies became entrenched has been a matter of debate. A new study of skeletons from prehistoric farming communities across Europe suggests that hereditary inequality was an early feature, going back more than 7,000 years ago.
Most researchers agree that social hierarchies began with the advent of farming. The earliest known farming communities are found in the Near East, dating back almost 11,000 years. Archaeologists have looked for evidence of social stratification in these societies with mixed results. Some early farming societies show signs that people played different roles and that some were buried with greater ritual — shuffling off this mortal coil with a number of elaborate “grave goods,” including pottery and stone tools. However, there is little evidence that social inequality was hereditary or rigidly defined.
That seems to have changed sometime after farmers moved into Europe from the Near East, beginning about 8,500 years ago during a period known as the European Neolithic. One of the best studied farming cultures is the Linearbandkeramik (LBK), which arose in what is today Hungary about 7,500 years ago and spread as far as modern-day Paris within 500 years, after which it appears to have been superseded by other cultures.
Archaeologists have long noted signs that the LBK culture might have been socially stratified. For example, some, but not all, males were buried with stone tools called adzes, which were thought to be used to build the wooden houses in which the farmers lived. But a few researchers have argued that this stratification took place only gradually over the 500-year period of the LBK.
To get a better handle on the timing and nature of these social inequalities, a team led by Alexander Bentley, an archaeologist at the University of Bristol in the United Kingdom, analyzed the tooth enamel from more than 300 skeletons from seven LBK burial sites across Europe. These cemeteries, located in the Czech Republic, Slovakia, Austria, and France, ranged from 6,900 to 7,400 years in age, and covered most of the LBK’s territorial spread.
Specifically, the team looked for the element strontium in teeth and measured the ratio of two isotopes, or types of the atom with slightly different weights. Strontium atoms enter the body in the water that we drink and the food we eat, and the ratio of the heavier isotope strontium-87 to the lighter isotope strontium-86 reflects the kind of soil and geological formations a person lived on, particularly as a child, when the tooth enamel was laid down. The strontium isotopes are increasingly used by archaeologists to track movements of populations.
Previous studies have shown that the kind of soil favored by European farmers, lowland sediments known as loess, has a slightly lower strontium-87/strontium-86 ratio than less-fertile areas such as upland hills made from granite or sandstone. Yet because of Europe’s variable landscape, in which fertile and non-fertile areas can be as close as several kilometers apart, the team relied more heavily on the degree of variation of strontium ratios among the skeletons in a burial site than on their absolute values.
The results of the study, published online today in the Proceedings of the National Academy of Sciences, suggest that men who were buried with adzes — thought to be an indication of higher social status — were more likely to have grown up on loess soils than men who were buried without adzes. For example, among 310 burials the team analyzed, 62 featured adzes. But only one of the 62 skeletons from the adze burials had a strontium ratio in its teeth typical of a non-loess landscape, whereas all of the others were consistent with growing up on loess. Moreover, the variation in strontium ratios between adze skeletons was significantly lower than the variation between non-adze skeletons, suggesting to Bentley and his co-workers that the adze skeletons came from one kind of landscape, most likely loess, while the others came from a variety of other landscapes.
A similarly striking pattern was seen when the team looked at the female skeletons, which made up 153 of the total 311 individuals analyzed. The variation in strontium ratios for females was significantly greater than for males, suggesting that a greater number of females than males had grown up in non-fertile areas. Moreover, the patterns in the male and female burials appeared in both earlier and later LBK settlements, suggesting that the patterns of social inequality were established from the beginning of the LBK period and did not develop gradually over time.
The team came to two main conclusions: First, some males had greater access to fertile soils than others, probably because they were the sons of farmers who had inherited access to the best land. And second, LBK societies were “patrilocal,” meaning that males tended to stay put in one place while females moved in from other areas to mate with them. A number of recent genetic studies have shown similar patterns among early European farmers. “The signatures from these skeletons reinforce other indications of male-dominated descent and even land inheritance,” Bentley says, adding that such social inequalities “only grew in extent and scale” over the course of history.
Read more at Wired Science
Most researchers agree that social hierarchies began with the advent of farming. The earliest known farming communities are found in the Near East, dating back almost 11,000 years. Archaeologists have looked for evidence of social stratification in these societies with mixed results. Some early farming societies show signs that people played different roles and that some were buried with greater ritual — shuffling off this mortal coil with a number of elaborate “grave goods,” including pottery and stone tools. However, there is little evidence that social inequality was hereditary or rigidly defined.
That seems to have changed sometime after farmers moved into Europe from the Near East, beginning about 8,500 years ago during a period known as the European Neolithic. One of the best studied farming cultures is the Linearbandkeramik (LBK), which arose in what is today Hungary about 7,500 years ago and spread as far as modern-day Paris within 500 years, after which it appears to have been superseded by other cultures.
Archaeologists have long noted signs that the LBK culture might have been socially stratified. For example, some, but not all, males were buried with stone tools called adzes, which were thought to be used to build the wooden houses in which the farmers lived. But a few researchers have argued that this stratification took place only gradually over the 500-year period of the LBK.
To get a better handle on the timing and nature of these social inequalities, a team led by Alexander Bentley, an archaeologist at the University of Bristol in the United Kingdom, analyzed the tooth enamel from more than 300 skeletons from seven LBK burial sites across Europe. These cemeteries, located in the Czech Republic, Slovakia, Austria, and France, ranged from 6,900 to 7,400 years in age, and covered most of the LBK’s territorial spread.
Specifically, the team looked for the element strontium in teeth and measured the ratio of two isotopes, or types of the atom with slightly different weights. Strontium atoms enter the body in the water that we drink and the food we eat, and the ratio of the heavier isotope strontium-87 to the lighter isotope strontium-86 reflects the kind of soil and geological formations a person lived on, particularly as a child, when the tooth enamel was laid down. The strontium isotopes are increasingly used by archaeologists to track movements of populations.
Previous studies have shown that the kind of soil favored by European farmers, lowland sediments known as loess, has a slightly lower strontium-87/strontium-86 ratio than less-fertile areas such as upland hills made from granite or sandstone. Yet because of Europe’s variable landscape, in which fertile and non-fertile areas can be as close as several kilometers apart, the team relied more heavily on the degree of variation of strontium ratios among the skeletons in a burial site than on their absolute values.
The results of the study, published online today in the Proceedings of the National Academy of Sciences, suggest that men who were buried with adzes — thought to be an indication of higher social status — were more likely to have grown up on loess soils than men who were buried without adzes. For example, among 310 burials the team analyzed, 62 featured adzes. But only one of the 62 skeletons from the adze burials had a strontium ratio in its teeth typical of a non-loess landscape, whereas all of the others were consistent with growing up on loess. Moreover, the variation in strontium ratios between adze skeletons was significantly lower than the variation between non-adze skeletons, suggesting to Bentley and his co-workers that the adze skeletons came from one kind of landscape, most likely loess, while the others came from a variety of other landscapes.
A similarly striking pattern was seen when the team looked at the female skeletons, which made up 153 of the total 311 individuals analyzed. The variation in strontium ratios for females was significantly greater than for males, suggesting that a greater number of females than males had grown up in non-fertile areas. Moreover, the patterns in the male and female burials appeared in both earlier and later LBK settlements, suggesting that the patterns of social inequality were established from the beginning of the LBK period and did not develop gradually over time.
The team came to two main conclusions: First, some males had greater access to fertile soils than others, probably because they were the sons of farmers who had inherited access to the best land. And second, LBK societies were “patrilocal,” meaning that males tended to stay put in one place while females moved in from other areas to mate with them. A number of recent genetic studies have shown similar patterns among early European farmers. “The signatures from these skeletons reinforce other indications of male-dominated descent and even land inheritance,” Bentley says, adding that such social inequalities “only grew in extent and scale” over the course of history.
Read more at Wired Science
Huge Ancient Civilization's Collapse Explained
The mysterious fall of the largest of the world's earliest urban civilizations nearly 4,000 years ago in what is now India, Pakistan, Nepal and Bangladesh now appears to have a key culprit — ancient climate change, researchers say.
Ancient Egypt and Mesopotamia may be the best known of the first great urban cultures, but the largest was the Indus or Harappan civilization. This culture once extended over more than 386,000 square miles (1 million square kilometers) across the plains of the Indus River from the Arabian Sea to the Ganges, and at its peak may have accounted for 10 percent of the world population. The civilization developed about 5,200 years ago, and slowly disintegrated between 3,900 and 3,000 years ago — populations largely abandoned cities, migrating toward the east.
"Antiquity knew about Egypt and Mesopotamia, but the Indus civilization, which was bigger than these two, was completely forgotten until the 1920s," said researcher Liviu Giosan, a geologist at Woods Hole Oceanographic Institution in Massachusetts. "There are still many things we don't know about them."
Nearly a century ago, researchers began discovering numerous remains of Harappan settlements along the Indus River and its tributaries, as well as in a vast desert region at the border of India and Pakistan. Evidence was uncovered for sophisticated cities, sea links with Mesopotamia, internal trade routes, arts and crafts, and as-yet undeciphered writing.
"They had cities ordered into grids, with exquisite plumbing, which was not encountered again until the Romans," Giosan told LiveScience. "They seem to have been a more democratic society than Mesopotamia and Egypt — no large structures were built for important personalitiess like kings or pharaohs."
Like their contemporaries in Egypt and Mesopotamia, the Harappans, who were named after one of their largest cities, lived next to rivers.
"Until now, speculations abounded about the links between this mysterious ancient culture and its life-giving mighty rivers," Giosan said.
Now Giosan and his colleagues have reconstructed the landscape of the plain and rivers where this long-forgotten civilization developed. Their findings now shed light on the enigmatic fate of this culture.
"Our research provides one of the clearest examples of climate change leading to the collapse of an entire civilization," Giosan said.
The researchers first analyzed satellite data of the landscape influenced by the Indus and neighboring rivers. From 2003 to 2008, the researchers then collected samples of sediment from the coast of the Arabian Sea into the fertile irrigated valleys of Punjab and the northern Thar Desert to determine the origins and ages of those sediments and develop a timeline of landscape changes.
"It was challenging working in the desert — temperatures were over 110 degrees Fahrenheit all day long (43 degrees C)," Giosan recalled.
After collecting data on geological history, "we could reexamine what we know about settlements, what crops people were planting and when, and how both agriculture and settlement patterns changed," said researcher Dorian Fuller, an archaeologist with University College London. "This brought new insights into the process of eastward population shift, the change towards many more small farming communities, and the decline of cities during late Harappan times."
Some had suggested that the Harappan heartland received its waters from a large glacier-fed Himalayan river, thought by some to be the Sarasvati, a sacred river of Hindu mythology. However, the researchers found that only rivers fed by monsoon rains flowed through the region.
Previous studies suggest the Ghaggar, an intermittent river that flows only during strong monsoons, may best approximate the location of the Sarasvati. Archaeological evidence suggested the river, which dissipates into the desert along the dried course of Hakra valley, was home to intensive settlement during Harappan times.
"We think we settled a long controversy about the mythic Sarasvati River," Giosan said.
Initially, the monsoon-drenched rivers the researchers identified were prone to devastating floods. Over time, monsoons weakened, enabling agriculture and civilization to flourish along flood-fed riverbanks for nearly 2,000 years.
"The insolation — the solar energy received by the Earth from the sun — varies in cycles, which can impact monsoons," Giosan said. "In the last 10,000 years, the Northern Hemisphere had the highest insolation from 7,000 to 5,000 years ago, and since then insolation there decreased. All climate on Earth is driven by the sun, and so the monsoons were affected by the lower insolation, decreasing in force. This meant less rain got into continental regions affected by monsoons over time."
Eventually, these monsoon-based rivers held too little water and dried, making them unfavorable for civilization.
"The Harappans were an enterprising people taking advantage of a window of opportunity — a kind of "Goldilocks civilization," Giosan said.
Eventually, over the course of centuries, Harappans apparently fled along an escape route to the east toward the Ganges basin, where monsoon rains remained reliable.
"We can envision that this eastern shift involved a change to more localized forms of economy — smaller communities supported by local rain-fed farming and dwindling streams," Fuller said. "This may have produced smaller surpluses, and would not have supported large cities, but would have been reliable."
This change would have spelled disaster for the cities of the Indus, which were built on the large surpluses seen during the earlier, wetter era. The dispersal of the population to the east would have meant there was no longer a concentrated workforce to support urbanism.
Read more at Discovery News
Ancient Egypt and Mesopotamia may be the best known of the first great urban cultures, but the largest was the Indus or Harappan civilization. This culture once extended over more than 386,000 square miles (1 million square kilometers) across the plains of the Indus River from the Arabian Sea to the Ganges, and at its peak may have accounted for 10 percent of the world population. The civilization developed about 5,200 years ago, and slowly disintegrated between 3,900 and 3,000 years ago — populations largely abandoned cities, migrating toward the east.
"Antiquity knew about Egypt and Mesopotamia, but the Indus civilization, which was bigger than these two, was completely forgotten until the 1920s," said researcher Liviu Giosan, a geologist at Woods Hole Oceanographic Institution in Massachusetts. "There are still many things we don't know about them."
Nearly a century ago, researchers began discovering numerous remains of Harappan settlements along the Indus River and its tributaries, as well as in a vast desert region at the border of India and Pakistan. Evidence was uncovered for sophisticated cities, sea links with Mesopotamia, internal trade routes, arts and crafts, and as-yet undeciphered writing.
"They had cities ordered into grids, with exquisite plumbing, which was not encountered again until the Romans," Giosan told LiveScience. "They seem to have been a more democratic society than Mesopotamia and Egypt — no large structures were built for important personalitiess like kings or pharaohs."
Like their contemporaries in Egypt and Mesopotamia, the Harappans, who were named after one of their largest cities, lived next to rivers.
"Until now, speculations abounded about the links between this mysterious ancient culture and its life-giving mighty rivers," Giosan said.
Now Giosan and his colleagues have reconstructed the landscape of the plain and rivers where this long-forgotten civilization developed. Their findings now shed light on the enigmatic fate of this culture.
"Our research provides one of the clearest examples of climate change leading to the collapse of an entire civilization," Giosan said.
The researchers first analyzed satellite data of the landscape influenced by the Indus and neighboring rivers. From 2003 to 2008, the researchers then collected samples of sediment from the coast of the Arabian Sea into the fertile irrigated valleys of Punjab and the northern Thar Desert to determine the origins and ages of those sediments and develop a timeline of landscape changes.
"It was challenging working in the desert — temperatures were over 110 degrees Fahrenheit all day long (43 degrees C)," Giosan recalled.
After collecting data on geological history, "we could reexamine what we know about settlements, what crops people were planting and when, and how both agriculture and settlement patterns changed," said researcher Dorian Fuller, an archaeologist with University College London. "This brought new insights into the process of eastward population shift, the change towards many more small farming communities, and the decline of cities during late Harappan times."
Some had suggested that the Harappan heartland received its waters from a large glacier-fed Himalayan river, thought by some to be the Sarasvati, a sacred river of Hindu mythology. However, the researchers found that only rivers fed by monsoon rains flowed through the region.
Previous studies suggest the Ghaggar, an intermittent river that flows only during strong monsoons, may best approximate the location of the Sarasvati. Archaeological evidence suggested the river, which dissipates into the desert along the dried course of Hakra valley, was home to intensive settlement during Harappan times.
"We think we settled a long controversy about the mythic Sarasvati River," Giosan said.
Initially, the monsoon-drenched rivers the researchers identified were prone to devastating floods. Over time, monsoons weakened, enabling agriculture and civilization to flourish along flood-fed riverbanks for nearly 2,000 years.
"The insolation — the solar energy received by the Earth from the sun — varies in cycles, which can impact monsoons," Giosan said. "In the last 10,000 years, the Northern Hemisphere had the highest insolation from 7,000 to 5,000 years ago, and since then insolation there decreased. All climate on Earth is driven by the sun, and so the monsoons were affected by the lower insolation, decreasing in force. This meant less rain got into continental regions affected by monsoons over time."
Eventually, these monsoon-based rivers held too little water and dried, making them unfavorable for civilization.
"The Harappans were an enterprising people taking advantage of a window of opportunity — a kind of "Goldilocks civilization," Giosan said.
Eventually, over the course of centuries, Harappans apparently fled along an escape route to the east toward the Ganges basin, where monsoon rains remained reliable.
"We can envision that this eastern shift involved a change to more localized forms of economy — smaller communities supported by local rain-fed farming and dwindling streams," Fuller said. "This may have produced smaller surpluses, and would not have supported large cities, but would have been reliable."
This change would have spelled disaster for the cities of the Indus, which were built on the large surpluses seen during the earlier, wetter era. The dispersal of the population to the east would have meant there was no longer a concentrated workforce to support urbanism.
Read more at Discovery News
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