Sunday, April 28, 2013

Factbox: What is the chemical weapon sarin?

(Reuters) - Charges that Syria has used the chemical weapon sarin have raised questions about the nerve agent, how it kills and what level of evidence it will take to prove it was used on the Syrian people.

WHAT IS SARIN?

Sarin is a man-made nerve gas that was originally developed as a pesticide in Germany in 1938. It is chemically similar to a class of pesticides known as organophosphates.

Sarin, also known as GB, is part of a class of chemical weapons called G-series nerve agents that were developed during World War Two and were named for the German scientists who synthesized them. Other agents in the class include tabun, soman and cyclosarin.

At room temperature, G-series nerve agents are volatile liquids, with sarin being the most volatile.

Sarin is a clear, colorless and tasteless liquid that has no odor in its pure form. It is made up of four common chemical compounds: dimethyl methylphosphonate, phosphorus trichloride, sodium fluoride and alcohol.

Exposure usually occurs when the liquid form comes in contact with the skin or the agent is released as a vapor.

WHEN HAS IT BEEN USED?

Sarin and other nerve agents may have been used in chemical warfare during the Iran-Iraq war in the 1980s.

The Japanese cult Aum Shinrikyo used sarin in two attacks in Japan. In 1994, the group released sarin gas in Matsumoto in central Japan, in a failed attempt to kill three judges. In that attack, the group used a refrigerator truck to release the nerve agent and a wind dispersed the gas in a residential neighborhood. Eight people were killed and hundreds were hospitalized. The next year, the same group carried six newspaper-wrapped packages on to five subway trains, poked them with umbrella tips, releasing sarin. In that attack, 12 commuters were killed and more than 5,000 were injured.

HOW DOES IT KILL?

Sarin acts primarily by interfering with the neurotransmitter acetylcholine, which acts as an off switch for glands and muscles. Blocking that switch results in over-stimulation of muscles.

The extent of poisoning depends on how much chemical a person was exposed to and for how long. Exposure to sarin vapors can trigger symptoms within a few seconds; exposure to liquid sarin can take a few minutes to as much as 18 hours to cause symptoms.

Large doses of sarin can cause loss of consciousness, convulsions, paralysis and respiratory failure and death. Low doses can cause a range of symptoms, from a runny nose and watery eyes, to drooling, excessive sweating, nausea and vomiting.

Because sarin evaporates quickly, it presents an immediate but short-lived threat. According to biosecurity expert Sean Kaufman of Emory University's Center for Public Health Preparedness and Research, its ability to disperse quickly makes it hard to trace, but sarin does leave remnants in the area where it was used.

HIGH BAR FOR CONFIRMING SARIN USE

The use of sarin is extremely difficult to prove, said Charles Blair, a terrorism expert at the Federation of American Scientists and a columnist for the Bulletin of the Atomic Scientists. To get good evidence that sarin was used, investigators need soil, blood or hair samples directly from the area of attack or its victims, he said.

Weapons inspectors reinforce that view. According to the Organization for the Prohibition of Chemical Weapons, which works on inspections with the United Nations, inspectors will only determine whether banned chemical agents were used if they can gain access to sites and take soil, blood, urine or tissue samples and examine them in certified laboratories.

SYRIA'S TRACK RECORD WITH CHEMICAL WEAPONS

Syria in July acknowledged for the first time that it had chemical and biological weapons, saying they could be used if the country faced foreign intervention. It said this week it would not use chemical arms against its own citizens, or even against Israel.

Since the early 1980s, Syria has made efforts to acquire and maintain an arsenal of chemical weapons following defeats in wars against Israel in 1967, 1973 and 1982 and the Jewish state's development of nuclear weapons.

According to Global Security, which collects published intelligence reports and other data, there are four suspected chemical weapons sites in Syria - one just north of Damascus; the second near the industrial city of Homs; the third in Hama, believed to be producing VX agents in addition to sarin and tabun; and a fourth near the Mediterranean port of Latakia.

SOURCES: The U.S. Centers for Disease Control and Prevention; Center for Biosecurity at UPMC; www.medscape.com; Www.globalsecurity.org

(Reporting by Julie Steenhuysen; Editing by Mary Milliken and Peter Cooney)

Source: http://news.yahoo.com/factbox-chemical-weapon-sarin-235511462.html

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Saturday, April 27, 2013

Classic: Daily Show's John Oliver on Australia's Total Gun Control "Failure" (Little green footballs)

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Fired TV anchor who dropped f-bomb becomes Web star

A local news anchor?s disastrous first moments on the job have turned him into a Web sensation and an unlikely media star.

After being fired for dropping an f-bomb on his first seconds out as the weekend co-anchor at the NBC station in Bismarck, N.D., A.J. Clemente was cooked.

The unfortunate rookie was looking down and missed the on-air light as he struggled to get the names of the London Marathon winners right, causing him to express his frustration with two cuss words, ?bleeping bleep.? That was the end of his short career.

Or was it?

The tape went viral, naturally, and pretty soon, Clemente was telling his tale of woe to the most sympathetic of people?other live TV hosts, from those at the ?Today? show to David Letterman.

Not bad for a guy from Bismarck who couldn?t make it through one night delivering the local news.

The wannabe TV anchor has been a good sport, and told ?Today? that it was "gut-wrenching" to watch the clip. He called the ?fireball shot? he uttered ?inexcusable.?

His newly minted media-star status has turned into a plea for a second chance at a TV job. As Savannah Guthrie on ?Today? put it, along with reporting, shooting and editing, he has ?a way with words.?

Continuing his apology tour, Clemente told Letterman that he held no grudge against the TV station that hired him, then fired him. The late-night host told him he?s ?better than? the "goons" back in North Dakota and that ?they should apologize to you.? He added, ?If you want to, you should be offered that job back.?

Meanwhile, the ex-anchor picked up some work from the ?Today? show, which asked him to work the red carpet for the movie premiere of Pierce Brosnan's "Love Is All You Need."

Source: http://news.yahoo.com/blogs/sideshow/fired-tv-anchor-dropped-f-bomb-becomes-star-171303940.html

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Jenelle Evans: Heroin Wasn't Mine, Assault Was Self-Defense!

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Congress: Obamacare For Thee, But Not For Me? (talking-points-memo)

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Friday, April 26, 2013

The Gods

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Einstein's theory of general relativity gets most extreme test yet

In their efforts to crack the mysteries of gravity, scientists continue to probe Albert Einstein's theory of general relativity. The latest test involved a curious binary star system.

By Pete Spotts,?Staff writer / April 25, 2013

Snow falls on the Albert Einstein Memorial Statue at the National Academy of Sciences in Washington D.C. during the early morning hours in February 2010. Scientists continue to probe Einstein's theory of general relativity, in their efforts to crack the mysteries of gravity.

Hyungwon Kang/Reuters/File

Enlarge

The most massive neutron star known and its tightly orbiting companion, a wimp of a white-dwarf, have provided one of the most extreme tests yet of Einstein's theory of general relativity.

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The theory has again passed with flying colors ? for now.

Although the theory has cleared test after test over the past century, researchers keep trying to find its limits. They don't think it's wrong, just incomplete.

The other basic forces of nature ? the strong force, which binds particles in an atom's nucleus, the weak force, which governs radioactive decay, and electromagnetism ? have found explanations in quantum physics. Gravity is the only force that so far has resisted assimilation.

Many physicists are convinced that resistance is futile and that at some point gravity will yield to a quantum-physics explanation. But that breakdown may only become apparent under the most extreme conditions ? conditions no human technology can establish.

So researchers turn to the cosmos for their extremes. And in the binary pair identified as PSR J0348+0432, they've found perhaps the most extreme conditions yet.

The pair is located some 7,000 light-years from Earth. The neutron star is all that remains of a star at least 10 times more massive than the sun that ended its luminous run in an explosion known as a supernova. Astronomers estimate that the neutron star is about 12 miles across. But it is so dense that a thimble full of the matter the explosion left behind would weigh about 1 billion tons.

It's white dwarf companion is the slowly cooling end state of a star like the sun.

White dwarfs are dense as well, typically packing roughly half of the sun's mass into an object slightly larger than Earth. This one, however is a lightweight, tipping the scales at about 17 percent of the sun's mass into an object roughly seven times larger than Earth.

Follow-up observations at radio and visible wavelengths revealed a duo that orbits its combined center of mass once every 2.46 hours. Considering the two objects are about a 500,000 miles apart, that's a mighty brisk pace.

"What we were looking for were changes in the orbital period," Dr. Lynch explains, referring to the time it takes for the two objects to orbit each other.

Those changes arise because the act of orbiting dissipates energy. That energy leaves in the form of gravity waves ? ripples in space-time, the very fabric of the cosmos. These ripples travel through space almost as though some interstellar housekeeper was shaking out the sheets.

This loss of energy shortens the time it takes to complete an orbit, signaling that the two objects are slowing and inching closer to one another. Different theories of gravity offer up different predictions for the rate at which the orbits of objects as close and as massive as these decay.

The key issue: "Can we measure that number precisely enough that we can say this agrees with general relativity or disagrees?" Lynch says. After careful measurements using the Arecibo Radio Telescope in Puerto Rico to track the pulsar, and the Very Large Telescope in Chile to track the white dwarf, the answer is: Yes we can, and it agrees with general relativity.

Beyond the test of Einstein's theory of general relativity, the system also poses a challenge to ideas about how binary systems form, Lynch adds.

The neutron star was discovered in 2009 as researchers at the National Radio Astronomy Observatory's facility at Green Bank, W. Va., combed through data gathered two years earlier during a hunt for rapidly spinning neutron stars, dubbed pulsars.

Pulsars earned their name because they emit radio waves as they spin, acting like beacons in the cosmos. Researchers were able to detect this neutron star because it, too, is a pulsar, spinning once every 39 milliseconds.

The team, led by John Antoniadis, with the Max Planck Institute for Radio Astronomy in Bonn, Germany, also combed through data gathered by the Sloan Digital Sky Survey to see if anything showed up in the pulsar's vicinity at visible wavelengths. That's when they found the pulsar's companion.

Astronomers have found other pulsars that spin as fast as the pulsar in the PSR J0348+0432 system, he says. But when such pulsars appear in binary systems, their companions tend to have more mass.

It's the combination of a pulsar with a relatively long spin period in a tight orbit with a relatively low-mass white dwarf "that makes this a little strange," he says, adding that the combination suggests that the system had a unique evolutionary history,

So how fast is the orbital period decreasing? The pace is slowing by about 2.7 ten-trillionths of a second per second. At that rate, some 400 million years from now, the binary system will become an ultra-compact binary system with X-rays for a beacon, the team suggests.

If the neutron star ends up near the high end of the mass scale for such objects as it draws matter from its partner, an eventual merger with the white dwarf could lead to a catastrophic collapse into a black hole ? an object whose gravity is so strong that not even light, traveling at 186,000 miles a second, can escape. If the neutron star star ends up with a more middling mass, the white dwarf in essence would be considered a planet once it cools sufficiently.

A formal report of this test of Einstein's theory of general relativity was published Thursday in the journal Science.

Source: http://rss.csmonitor.com/~r/feeds/science/~3/WR6kqBKKYj0/Einstein-s-theory-of-general-relativity-gets-most-extreme-test-yet

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