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Yes ...somehow it didnt struck me at all.:(
koi nai......:-)
now don't be sad.....its just a gravity model...which has no use in general life....who cares for such modes anyway........
men only care for the models on ramp ..:lol::lol:
 
:disagree::disagree::disagree:

Professional trolling is a symptom.
(JOKINGGGGG:enjoy:)
Just that I see you guys are more interested in science and tech topics.:agree:
Okkkkk...
Sorry madamji....:(
no ramp modes...but only gravity model of earth...
 
:disagree::disagree::disagree:

Professional trolling is a symptom.
(JOKINGGGGG:enjoy:)
Just that I see you guys are more interested in science and tech topics.:agree:

I think Lawyers are the best Troll-pros....we engineers are sometimes constrained a bit by Logic and reasoning, and give up when we know we're sounding really absurd.:D
 
Its okay ...now I dont want to swing the other way.:D
Kidding :enjoy:
don't worry....I was also kidding.....
I know someone with whom talking is much more fun then watching those models.....:enjoy:
 
Ahem ahem ahem....why does this remind me of Japan?
You're doomed.:D
hhaha...
thats is cruel of you..saying like that.....:cry:
I am more interested in real world phenomenon than virtual...:D:D
 
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NASA aims to go to Europa on the cheap
The agency wants to send a robotic mission to Jupiter's moon for less than $1 billion.
14 March 2014


NASA/JPL/Ted Stryk

The recent discovery of geysers on Europa — photographed here by the Galileo probe during its mission from 1995 to 2003 — has rekindled interest in this icy moon of Jupiter.


For the last few year's NASA's planetary-science budget has seen a major crunch, and the lion's share of its remaining funds have gone to Mars missions. Despite the high priority given to Europa exploration in the US National Research Council’s last decadal survey, an overview of the most pressing goals in planetary science, NASA has not requested any money for planning a Europa mission in recent years. Nevertheless, Europa fans in Congress have allocated funding for it, granting $43 million in 2013 and $80 million in 2014. Proponents of the mission were therefore heartened last week to see the White House's 2015 NASA budget request include a line item of $15 million for Europa exploration planning, although the amount is far less than many would hope for. "If nothing else, we're excited to see NASA and the White House put it into budget lines and acknowledge it’s an important destination," says Casey Dreier, director of advocacy at the Planetary Society, a nonprofit organization devoted to solar system science and exploration. The size of the request — $15 million out of NASA's total budget request of $17.5 billion — is "a very small amount of money" but the symbolism of the move is significant, he says. "The fact that it's in there is a big, big shift, and I think a big part of that is the discovery of those plumes."


In December scientists announced that the Hubble Space Telescope had spotted geysers of water vapour shooting from Europa's surface, most likely originating from a liquid water ocean thought to exist under the moon's icy surface (see 'Hubble spots water spurting from Europa'). This theorized ocean has long been the focal point for hopes that Europa could host microbial life, but scientists assumed that a lander would be required to drill down into the ice to reach the liquid water for sampling. The geysers may make the water more accessible, however. "If that’s the case, maybe we don’t have to go to the ocean — the ocean will come to us," says astrobiologist Chris McKay of NASA Ames Research Center at Moffett Field, California.

The discovery of the geysers may have been the push that Europa needed to attain must-explore status. "The big question that ultimately drives us to study Europa is 'Does life exist there?'" says Kurt Retherford of the Southwest Research Institute (SwRI) in San Antonio, Texas, one of the co-discoverers of the water vapour plumes. "I think most of us had imagined that two or three large and expensive Europa missions would be needed before we find a clear answer to this compelling question, including future landers and deep-drilling devices."

Sending a probe to fly through the geysers would be cheaper but Retherford cautions against designing a Europa mission completely around the plumes. For one thing, the water vapour appears to be time-variable, and scientists cannot yet predict when the plumes will be active. "Until we are able to more firmly confirm our discovery of Europa’s water vapour plumes with additional observations in the next few years, it would seem inappropriate to focus a mission to exclusively study geysers at this time," Retherford says.

Europa presents other challenges as well: The moon is situated within Jupiter's intense radiation field, which would bombard spacecraft with radiation that could damage sensitive electronics. The best solution is to encase a Europa probe in thick shielding, which would increase its weight and thus the cost to launch it. The Jovian system is also far from Earth, probably at least a six-year journey, which adds to the time and expense of the total mission. "The Europa program is a complicated, expensive, step-by-step process because of these difficulties," McKay says.

Researchers have been working on Europa mission concepts for years. A proposed NASA mission called the Europa Orbiter, estimated to cost $4.7 billion, was canceled in 2002. Following that disappointment, scientists devised a reduced-cost plan for around $2 billion called the Europa Clipper, which would orbit Jupiter and make repeated low-altitude flybys of Europa. The Europa funding allocated to NASA in recent years has gone toward furthering that plan. "The Clipper concept is very mature," Dreier says. "They could basically start today on that mission."

After the NASA budget announcement last week, however, agency chief, Charles Bolden, said NASA was looking to spend less than $1 billion total on a Europa mission. That would put the spacecraft in a class of missions called "New Frontiers," a less expensive category than its bigger "Flagship missions." NASA plans to issue a "request for information" to solicit ideas from scientists on what type of Europa mission could be done for under $1 billion. But some worry that price point puts most major science goals out of reach. "No one has really thought much about what you can do with that minimal budget," Dreier adds.

Scientists' wish list for a Europa mission includes characterizing the chemistry of its subsurface ocean, learning how large the ocean is and determining the thickness of the ice shell that encloses it. "Measuring the composition of Europa's ice-water shell is important," says Lorenz Roth of the SwRI, lead author of the paper announcing the water geyser discovery. "Flying through plumes from active outgassing and measuring their composition" is another priority, Roth adds. Whether a New Frontiers mission can accomplish all those goals remains to be seen.

Europa has several champions in Congress. Texas Representative John Culberson, a Republican and a member of the House Appropriations Committee, has led the charge to insert Europa funding into the agency's budget. Culberson is next in line to become chairman of the subcommittee responsible for NASA's budget, where he could exert considerable influence to make the mission fly. That is comforting news to Europa proponents, who know it will take a cosmic alignment of political goodwill, money and technical know-how to reach Jupiter's enigmatic moon. If it happens, however, the payoff could be nothing less than finding life beyond Earth.

NASA aims to go to Europa on the cheap : Nature News & Comment
 

NIH rethinks psychiatry trials

Mental-health division will no longer fund research aiming to relieve symptoms without probing underlying causes.
14 March 2014
1.14877_Dr.-Tom-Insel-NYT-Eyevine-aack4966.jpg

Lexey Swall/New York Times/Redux/eyevine

Thomas Insel wants studies to identify the biological mechanisms that underlie psychiatric symptoms.

Thomas Insel, the director of the US National Institute of Mental Health (NIMH), has had enough of shooting in the dark. He thinks that if a clinical trial of a psychiatric therapy fails, scientists should at least learn something about the brain along the way.

Now Insel is translating that belief into action: the NIMH, based in Bethesda, Maryland, has decided to stop funding clinical trials that aim merely to ease patients’ symptoms. “Future trials will follow an experimental medicine approach in which interventions serve not only as potential treatments, but as probes to generate information about the mechanisms underlying a disorder”, he wrote in a 27 February blog post announcing the move. This funding switch, which will affect grants due to be made in a few months’ time, intensifies the NIMH’s apparent shift in emphasis from abstract psychiatry to the neurobiological roots of disease.

“It’s a totally new departure for us,” says Bruce Cuthbert, a clinical psychologist and director of the institute’s adult translational-research division. Insel notes that the NIMH spent about US$100 million on clinical trials in 2013, and says that more than half of recipient projects received funding without any requirement to examine the biological processes involved in a disease. In many cases, “if you get a negative result you have no idea why, and you have to try something else at random”, Cuthbert says. “It’s an incredible waste of money.”

The new rules, which will apply to the grant cycle that begins in June, also seek to increase transparency by requiring faster online registration of trials and stricter guidelines for reporting results. Insel acknowledges that researchers may have to rework their studies to satisfy the new guidelines. “I think this will be really unpopular,” he says.

History shows that Insel is not daunted by controversy. In April 2013, he raised eyebrows when he announced that the NIMH would stop using the Diagnostic and Statistical Manual of Mental Disorders 5 (DSM-5), the latest version of the American Psychiatric Association’s diagnostic guide, to classify mental disorders (see Nature http://doi.org/rvd; 2013). The book’s definitions tend to lump patients together by symptoms, which often do not precisely map to what is wrong with their brains, he says. With this haphazard approach to trials, even if symptoms are alleviated, researchers still may not understand what caused them. “We’ve studied drugs, not disorders — if you throw something at the wall, and P is less than 0.05, you win,” he says. Such thinking, he adds, wastes time and money.

Michael First, a psychiatrist at Columbia University in New York, says that targeting the wrong patient groups can also make therapies seem less effective than they really are. A treatment that helps a tiny fraction of people with a DSM diagnosis of depression, for example, might be highly effective for all people with a more specific trait, such as the inability to enjoy life. Beginning a trial with an idea about a treatment’s mechanism may allow researchers to quickly determine whether to expand or end the testing, First says. That could help to tempt drug companies to develop new classes of drugs for mental illnesses — an endeavour that many have abandoned after decades of failed research.

But Harold Pincus, a psychiatrist also at Columbia University, cautions that the data-driven approach is not a sure thing. Focusing trials on more specific biological targets will require researchers to think very carefully about how they recruit and classify their research subjects. Neuroscientist Michael Owen of Cardiff University, UK, concurs. “It’s a pretty scary prospect for everyone if you throw away the diagnostic rule book,” he says.

Others are strongly opposed to the NIMH’s new approach. Psychiatrist Allen Frances, an emeritus professor at Duke University in Durham, North Carolina, worries that an emphasis on brain science comes at patients’ expense. “Don’t bet everything you have on something so difficult,” he says. “We have a shameful problem of neglect of existing patients and an empty promissory note to the future that science will solve everything.” Understanding the workings of the brain is, of course, a fine goal, he says, but “it will be decades and decades before anyone will be helped by this research”.

Insel maintains that the NIMH wants the trials it funds to continue to ameliorate patients’ symptoms, but to probe how their brains work at the same time. His emphasis on biological mechanisms is not unique at the US National Institutes of Health, the NIMH’s parent agency: the National Institute of Neurological Disorders and Stroke in Bethesda is increasingly aiming therapies at specific targets in the brain rather than abstract constellations of symptoms. “We’ve all been burnt badly by treating the brain as a black box,” says that agency’s deputy director, neurologist Walter Koroshetz.

The difference, Koroshetz adds, is that a great deal is already known about how neurological disorders such as Parkinson’s disease work, and that allows scientists to focus on other challenges, such as adapting drugs that work in animals to work in humans. Psychiatry has a long way to go before it will have such accurate targets. “I feel bad for them,” Koroshetz says.

NIH rethinks psychiatry trials : Nature News & Comment
 
Toshiba, SanDisk Sue Hynix Over Flash Memory Use

Julien Happich
Toshiba Corp of Japan and SanDisk Corp of the United States have separately filed civil lawsuits against South Korea's SK Hynix Inc, reports Reuters.

Under Japan's Unfair Competition Prevention Act, the suit from Toshiba seeks damages for the wrongful acquisition and use of Toshiba's proprietary technical information related to NAND flash memory, the company says in a statement.

This technology was pioneered by Toshiba in 1987 and is now jointly developed and produced with SanDisk Corporation of the US.

Both companies seek damages over the suspected theft of data related to their flagship flash memory chip technology used in smartphones and tablet computers, reports Reuters.

Although Toshiba did not disclose how much it was seeking, the company estimates potential losses of at least 100 billion yen (US$980 million) as a result of the alleged leak. This allegation follows the arrest by Tokyo police on Thursday of a former SanDisk engineer suspected of improperly providing technical data to Hynix, where he later worked, according to Reuters.

In a previous case, Toshiba sued Hynix in 2004 seeking damages for the breach of its flash memory patents and an injunction against the sale of related products. The case was ultimately settled through a cross-licensing agreement with Hynix.

This story was originally published on EE Times Europe.
Toshiba, SanDisk Sue Hynix Over Flash Memory Use | EE Times
 
BBC News - Stephen Hawking 'wins inflation debate'
http://www.bbc.co.uk/emp/embed/smpE...ebates inflation with Neil Turok&product=news
Stephen Hawking 'wins inflation debate'
18 March 2014 Last updated at 09:34 GMT

Scientists say they have extraordinary new evidence to support a Big Bang Theory for the origin of the Universe.

Researchers believe they have found the signal left in the sky by the super-rapid expansion of space that must have occurred just fractions of a second after everything came into being.

The BBC's Tom Feilden discusses the significance of this new evidence, before Professor Stephen Hawking speaks to BBC Radio 4's Today programme, placing the latest discovery in the context of his previous work.

Professor Neil Turok also speaks to presenter Sarah Montague about a long-standing bet he has held with Mr Hawking, and how this latest discovery affects this.
 
New origin seen for Earth's tectonic plates : Nature News & Comment

New origin seen for Earth's tectonic plates
Continual diving of crust into mantle is sufficient to explain formation of plate boundaries.
06 April 2014
1.14993.jpg

Kevin Schafer/Alamy

The San Andreas fault in California marks the meeting of the Pacific and North American tectonic plates.

Earth's tectonic plates may have taken as long as 1 billion years to form, researchers report today in Nature1.


The plates — interlocking slabs of crust that float on Earth's viscous upper mantle — were created by a process similar to the subduction seen today when one plate dives below another, the report says.

Starting roughly 4 billion years ago, cooler parts of Earth's crust were pulled downwards into the warmer upper mantle, damaging and weakening the surrounding crust. The process happened again and again, the authors say, until the weak areas formed plate boundaries. Other researchers have estimated that a global tectonic plate system emerged around 3 billion years ago.

The finding offers a possible answer to an enduring puzzle in geology: how Earth's tectonic plates emerged. The subsequent movement of the plates has erased much of the evidence of their origin, says Paul Tackley, a geophysicist at Swiss Federal Institute of Technology (ETH) in Zurich, Switzerland.

Prior studies suggested the age of the plates, based on evidence of subduction gathered from minerals preserved in ancient rocks. The oldest such specimens are 4-billion-year-old zircons found in the Jack Hills of Australia, which appear to have formed at temperatures and pressures that areindicative of subduction.

Grains of time
To go a step further and investigate how the plates formed, the study's authors developed a computer model of Earth's crust as it may have existed billions of years ago, on the basis of mineral grains found in mantle rock. The model included a low-pressure zone at the base of the crust, which caused a piece of the crust to sink into the upper mantle — mimicking conditions thought to have occurred early in Earth's history.


As the process repeated over time, it created a large tectonic plate with an active subduction zone. Over a much longer period, the same process could have created many tectonic plates, says co-author David Bercovici, a geophysicist at Yale University in New Haven, Connecticut. “We’ve got a physical mechanism to explain how it could have happened,” he says.

This stands in contrast to conditions on Venus, where similar subduction occurs but has not produced tectonic plates. Conditions on Venus are much warmer, allowing the crust to better heal after a piece sinks down into the mantle. Bercovici's model suggests that early subduction created weak spots in Earth's crust that are now plate boundaries. Plate tectonics is defined by the idea that strong plates are separated by weak boundaries, and action at those boundaries creates geological phenomena such as volcanoes, mountains and earthquakes, he notes.

“They produce a model that plausibly explains what we see,” says Michael Brown, a petrologist at the University of Maryland in College Park. It shows how to start subduction and how that could have progressed to global tectonics, and it provides an amount of time between the two — 1 billion years — that is consistent with the rock record, he adds.

Robert Stern, a geologist at the University of Texas in Dallas, contends that there is no firm evidence of plate tectonics earlier than 1 billion years ago, but says that their theory of the mechanism behind plate formation is “the first interesting example of how it might have occurred”.

Nature

doi:10.1038/nature.2014.14993
 
Fossil galaxy may be one of first ever formed : Nature News & Comment

Fossil galaxy may be one of first ever formed

The stars in the nearby Segue 1 dwarf galaxy have low abundances of elements heavier than helium.

1.14997.jpg

Krzysztof Ulaczyk/Wikimedia/CC BY-SA 3.0

The Magellan Telescopes at Las Campanas Observatory in Chile targeted stars in the Segue 1 dwarf galaxy for 6 to 15 hours each to measure their content of 'metals', or elements heavier than helium.

A tiny galaxy circling the Milky Way may be a fossil left over from the early universe, astronomers say. A recent study found that the stars in the galaxy, called Segue 1, contain fewer heavy elements than those of any other galaxy known, implying that the object may have stopped evolving almost 13 billion years ago. If true, Segue 1 could offer a window into the conditions of the early universe and reveal how some of the first galaxies came to be.

Segue 1 is very, very tiny. It appears to contain only a few hundred stars, compared with the few hundred billion stars in the Milky Way Galaxy. Researchers led by Anna Frebel of the Massachusetts Institute of Technology in Cambridge collected detailed information on the elemental composition of six of the brightest of Segue 1’s stars using the Las Campanas Observatory’s Magellan Telescopes in Chile and the Keck Observatory in Hawaii. The measurements, reported in a paper accepted for Astrophysical Journal and posted on the arXiv repository, revealed that these stars are made almost entirely of hydrogen and helium, and contain just trace amounts of heavier elements such as iron. No other galaxy studied holds so few heavy elements, making Segue 1 the “least chemically evolved galaxy known.”

Complex elements are forged inside the cores of stars by the nuclear fusion of more basic elements such as hydrogen and helium atoms. When stars explode in supernovae, even heavier atoms are created. elements spew into space to infuse the gas that births the next generation of stars, so that each successive generation contains more and more heavy elements, known as metals. “Segue 1 is so ridiculously metal-poor that we suspect at least a couple of the stars are direct descendants of the first stars ever to blow up in the universe,” says study co-author Evan Kirby of the University of California, Irvine.

All supernovae are not created equal. When very massive stars blow up they form a mix of elements such as magnesium and calcium, whereas low-mass star explosions almost exclusively make iron. Frebel and her colleagues measured the content of each of these particular elements in Segue 1’s stars and found that they contained the products of high-mass stars but very few products of low-mass stars. Because high-mass stars die much younger than do low-mass ones, this evidence reveals how quickly star formation occurred in the dwarf galaxy. “Segue 1 is the only example that we know of now that was never enriched by these low-mass stars, meaning it formed stars really quickly, in the blink of an eye,” Kirby says. “If it had formed stars long enough those low-mass stars would have to contribute.”


The findings suggest Segue 1 went through one brief bout of star formation long ago, and then stopped forever. “The big question is, why did it stop?” says Irvine astrophysicist James Bullock, who was not involved in the study. “A galaxy like this should have been able to make a million more stars, but it didn’t.”

One possibility is the epoch of reionization. When the universe was born it was hot and dense, and all gas was ionized, meaning protons and electrons were isolated and could not band together to form atoms. Eventually the universe cooled enough to allow atoms to form in the gas and the first stars were born from this material. Those stars blasted out radiation, which energized the gas around them and reionized it sometime around 13.2 billion years ago. Because stars cannot form from ionized gas, reionization might have terminated star formation in the existing galaxies at the time. “Maybe Segue 1 was on its way to forming a bunch of stars but reionization turned on and killed all the star formation in the galaxy,” Kirby says. “That could also explain why the star formation lasted such a short time.”

The case is not closed, however. Bullock, one of the main authors of the reionization idea, says the latest theoretical simulations of galaxy formation suggest the shutdown caused by reionization looks to be less sudden than scientists previously thought. “It’s not obvious to me that reionization by itself could have done this,” he says. “Maybe, but I definitely think there are other possibilities.” For instance, perhaps some quirk has caused Segue 1 to be incredibly inefficient at forming stars compared with other galaxies.

Segue 1 may help reveal not just what halts galaxy evolution, but how it gets started as well. “This study is so interesting because I really want to know, can galaxies form this small?” says astronomer Beth Willman of Haverford College, who was not involved in the research. “Can galaxies form and look like Segue 1 when they form or do they have to form larger and then have some mass taken away?” It is possible, after all, that this dwarf was once a much larger galaxy and lost most of its stars, perhaps through disruptions from its close neighbor, the Milky Way. The extremely low metal counts in Segue 1’s stars, however, support the idea that it formed roughly the same size it is now, because disruptions would be unlikely to pull only the metal-rich stars from the galaxy, leaving behind the metal-poor.

If there is no barrier to such puny galaxies forming in the first place, then mini galaxies like Segue 1 could be plentiful, but unseen. Only Segue 1’s close proximity to the Milky Way makes such a small, dim galaxy detectable. “There could be 200 Segue 1-like galaxies around us,” Willman says. “My lifelong goal is trying to understand, are things like this the most abundant in the universe?”

Nature

doi:10.1038/nature.2014.14998
 
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