Friday, August 6, 2010

620 PS Porsche 911 GT2 RS released

620 PS Porsche 911 GT2 RS released

2010 Porsche 911 GT2 RS -
2010 Porsche 911 GT2 RS
Image courtesy of Porsche


A new, more powerful Porsche 911 GT2 variant has just been released. The 2010 Porsche 911 GT2 RS features more power, less weight and even better performance.

The 3600 cc engine remains at the same capacity, but power and torque have been increased. Power is up 90 PS to 620 PS at the same 6500 rpm as the Porsche 911 GT2. Torque is up 20 Nm to 700 Nm, achieved in a rev band from 2500 to 5500 rpm, which is wider than the standard 911 GT2 which pulled maximum torque from 2200 rpm to 4500 rpm. A new intercooler and increased turbocharger boost from 1.4 bar to 1.6 bar account for most of the improvements here. The power is transmitted through a six speed manual gearbox.

Weight has been pared wherever possible, and the resultant drop of 70 kg over the 911 GT2, in combination with the engine tweaks, delivers sublime performance figures. The 0-100 km/h benchmark is covered in 3.5 seconds and in 28.9 seconds the 300 km/h mark is achieved. A top speed of 330 km/h is claimed. Despite these improvements in performance, the Porsche 911 GT2 RS boasts CO2 emissions of just 284 g/km, which is actually 14 g/km lower than the less powerful standard Porsche 911 GT2.

The Porsche 911 GT2 RS comes with Porsche's composite ceramic disc brake (PCCB) system as standard. The wheels are fitter with slightly wider 245/35 profile tyres at the front, whilst the rears remain 325/30. Both front and rear are 19 inch rims.

Porsche is limiting production of this, their most powerful road-legal car ever, to just 500 units. Sales in the UK start in September 2010.

305 KM/H BMW M3 GTS

 305 KM/H BMW M3 GTS
2010 BMW M3 GTS -
2010 BMW M3 GTS
Image courtesy of BMW

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The most hardcore BMW M3 yet - the BMW M3 GTS - will be available on the market, BMW has confirmed. With a longer stroke (82.0 mm - up from 75.2 mm on the standard E90 BMW M3), the V8 engine now displaces 4361 cc (E90 M3: 3999 cc). Power and torque are both improved, with maximum power being 450 PS (331 kW) at 8300 rpm and torque up 40 Nm to 440 Nm (325 ft.lb) at 3750 rpm.

The body is 30 mm longer, at 4645 mm compared to 4615 mm for the standard BMW M3 Coupé. It is also 37 mm lower at 1387 mm. Due to the demand for downforce, the aerodynamics are slightly poorer, with a coefficient of drag of 0.34, up from the standard M3's 0.31. Frontal area remains 2.17 m2, giving a CdA of 0.738 m2.

A seven speed Drivelogic transmission is fitted, and the gearchange timing has been set to match the GTS' engine characteristics. The final drive ratio is 3.154:1 and 7th gear is a direct ratio.

With all these improvements and changes, the M3 GTS delivers monumental performance. The standing start kilometre is covered in a searing 22.5 seconds, the 0-100 km/h sprint is despatched in 4.4 seconds. The top speed is over the magical 300 km/h mark too, at 305 km/h. CO2 emissions are 295 g/km.

The suspension and brakes have also been fettled for a more racing orientated set-up. The dampers are independently variable, as is front and rear camber and ride height. The brakes are ventilated discs at each corner, 18 mm and 30 mm larger, front and rear respectively, than the standard BMW M3 Coupé.

All up, the BMW M3 GTS weighs in at 1605 kg (EU) (1530 kg DIN) - the normal M3 is slightly heavier. BMW have delivered an enthusiasts' machine, sticking to their traditional principles.

Audi's A1 Luxury Baby

Audi's A1 Luxury Baby

 2010 Audi A1 -
2010 Audi A1
Image courtesy of Audi AG

The long-awaited 2010 Audi A1 is about to hit the markets, Audi have recently released the specifications of the A1 range at launch date.

Sitting on a 2469 mm wheelbase and with an overall length of just 3954 mm, the Audi A1 is the smallest Audi models since the Audi A2. The Audi A1 features a coefficient of drag of between 0.329 and 0.333, depending on the model, and a frontal area of 2.04 m2. 3 engine options are available initially: 1.2 and 1.4 TFSI petrol units and a 1.6 TDI diesel.

The 1.2 TFSI engine is good for 85 PS (63 kW) at 4800 rpm and has a peak torque of 160 Nm (118 ft.lb) developed between 1500 and 3500 rpm. Driving the front wheels through a five speed manual gearbox, this is enough to thrust the 1040 kg hatchback Audi A1 1.2 TFSI from 0 to 100 km/h in a claimed 11.7 seconds and on to a top speed of 180 km/h (112 mph). CO2 emissions are a tidy 118 g/km.

The next petrol engined variant is the 1.4 TFSI, available with or without start & stop technology. The turbocharged 1390 cc engine produces 122 PS (90 kW) at 5000 rpm and achieves peak torque of 200 Nm from 1500 rpm to 4000 rpm. Driving through a 7 speed automatic gearbox, the 1125 kg Audi A1 1.4 TFSI is propelled to 100 km/h from rest in 8.9 seconds and has a claimed top speed of 203 km/h. 122 g/km of CO2 is claimed overall, with that figure dropping to 119 g/km with the start & stop technology.

The only diesel engine available at launch is the 1.6 TDI. This 1598 cc unit delivers 105 PS (77 kW) at 4400 rpm and 250 Nm of torque at 1500-2500 rpm. Unusually for a modern diesel, it has just a 5-speed manual gearbox. Claimed CO2 emissions for the Audi A1 1.6 TDI are 103 g/km. It weighs 1040 kg and has a 0-100 km/h sprint time of 10.5 seconds. The claimed top speed for this model is 195 km/h.

Fake Photography


1. Medical Kitchen

2. Long Run

3. Face Vs. Fist

4. Work at Sea

5. Fishy Island

6. Road Worker’s Coffee Break

7. Arms Break

8. Reflective Cubes

9. Tough

Quantum Networks Advance With Entanglement of Photons, Solid-State Qubits



Physicists have achieved the first-ever quantum entanglement of photons and solid-state materials -- a key advance toward practical quantum networks in which solid-state quantum bits, or "qubits," can communicate with one another over long distances. (Credit: iStockphoto/Andrey Prokhorov)
 
 
 A team of Harvard physicists led by Mikhail D. Lukin has achieved the first-ever quantum entanglement of photons and solid-state materials. The work marks a key advance toward practical quantum networks, as the first experimental demonstration of a means by which solid-state quantum bits, or "qubits," can communicate with one another over long distances.Quantum networking applications such as long-distance communication and distributed computing would require the nodes that process and store quantum data in qubits to be connected to one another by entanglement, a state where two different atoms become indelibly linked such that one inherits the properties of the other.
"In quantum computing and quantum communication, a big question has been whether or how it would be possible to actually connect qubits, separated by long distances, to one another," says Lukin, professor of physics at Harvard and co-author of a paper describing the work in the journal Nature.
"Demonstration of quantum entanglement between a solid-state material and photons is an important advance toward linking qubits together into a quantum network."
Quantum entanglement has previously been demonstrated only with photons and individual ions or atoms.
"Our work takes this one step further, showing how one can engineer and control the interaction between individual photons and matter in a solid-state material," says first author Emre Togan, a graduate student in physics at Harvard. "What's more, we show that the photons can be imprinted with the information stored in a qubit."
Quantum entanglement, famously termed "spooky action at a distance" by a skeptical Albert Einstein, is a fundamental property of quantum mechanics. It allows one to distribute quantum information over tens of thousands of kilometers, limited only by how fast and how far members of the entangled pair can propagate in space.
The new result builds upon earlier work by Lukin's group to use single atom impurities in diamonds as qubits. Lukin and colleagues have previously shown that these impurities can be controlled by focusing laser light on a diamond lattice flaw where nitrogen replaces an atom of carbon. That previous work showed that the so-called spin degrees of freedom of these impurities make excellent quantum memory.
Lukin and his co-authors now say that these impurities are also remarkable because, when excited with a sequence of finely tuned microwave and laser pulses, they can emit photons one at a time, such that photons are entangled with quantum memory. Such a stream of single photons can be used for secure transmission of information.
"Since photons are the fastest carriers of quantum information, and spin memory can robustly store quantum information for relatively long periods of time, entangled spin-photon pairs are ideal for the realization of quantum networks," Lukin says. "Such a network, a quantum analog to the conventional internet, could allow for absolutely secure communication over long distances."
Lukin and Togan's co-authors on the Nature paper are Yiwen Chu, Alexei Trifonov, Jeronimo Maze, and Alexander S. Zibrov, all at Harvard; Liang Jiang of Harvard and the California Institute of Technology; Lilian I. Childress of Harvard and Bates College; M.V. Gurudev Dutt of Harvard and the University of Pittsburgh; A.S. Sorensen at the University of Copenhagen; and Phillip R. Hemmer of Texas A&M University. The work was supported by the Defense Advanced Research Projects Agency, the Harvard-MIT Center for Ultracold Atoms, the National Science Foundation, the National Defense Science & Engineering Graduate Fellowship, and the Packard Foundation.
 

Lunar's interior is quite dry

                                               
Astronaut Charles Duke collected moon rocks during the Apollo 16 mission in 1972. A new analysis of some of the rocks from various Apollo missions suggests the lunar interior is quite dry.                                         
                                                The inside of the moon might not be all wet after all. A new study suggests that, contrary to recent work, the lunar interior is as bone-dry as scientists thought 40 years ago, when NASA astronauts lugged home the first moon rocks.
New analyses of chlorine in those rocks, published Aug. 5 in Science, indicate that the moon contains just one-10,000th to one-100,000th the water that the Earth’s interior does.
Studying the wateriness of different worlds can illuminate how they evolved, says geochemist Zachary Sharp of the University of New Mexico in Albuquerque, lead author of the new paper. “It’s a window into processes that shaped the solar system soon after it formed.”
Researchers have long argued over whether the moon contains water on its surface — frozen in shadowy craters, for instance. Such water would not be native to the moon, but instead delivered there over time by comet impacts. The new studies tackle a more fundamental question: How much water did the moon contain inside when it formed, 4.5 billion years ago?
Most scientists think the moon was born when a huge object roaming the inner solar system — something about the size of Mars — smashed into the embryonic Earth. Debris from the collision coalesced to form the moon. As it cooled, an ocean of magma covering its surface began to crystallize. Sharp and his colleagues studied what happened to two isotopes of the element chlorine during that process.
Chlorine-35 has two fewer neutrons in its nucleus than chlorine-37, and hence is lighter and was more prone to vaporizing out from the magma ocean. But if the magma also contained a lot of hydrogen — perhaps in the form of water, H2O — a competing process would also take place. Chlorine-37 likes to bond with hydrogen and vaporize out as hydrogen chloride. So if hydrogen were present, more chlorine-37 would escape the magma along with chlorine-35.
But that’s not what Sharp’s team saw when analyzing 11 samples of moon rocks and soil. Instead, they found a wide range in the ratios of chlorine-35 to chlorine-37. The best explanation, Sharp says, is that there was hardly any hydrogen in the moon’s magma ocean. No hydrogen means no water.
Lunar scientists reached the same conclusion 40 years ago, when they first cracked into the Apollo samples and found them full of metallic iron, with no sign of having been chemically altered by water. But in 2008, an analysis of a handful of lunar volcanic glass beads suggested they might have formed in a watery environment. Since then, several research groups have also looked at the mineral apatite, which can lock up water in its chemical structure, in lunar rocks. Using newly developed analytical techniques, some of these groups reported — including in a paper in the July 22 Nature — that the moon could have contained quite a bit of water, perhaps almost as much as Earth’s interior did.
Such estimates are hard to reconcile with the new chlorine work suggesting a bone-dry moon. One possible explanation: The research teams are all looking at separate parts of the same problem, and some parts of the moon may have been wetter than others. “I think we’re dealing with a case of three blind men and an elephant,” says James Greenwood, a planetary scientist at Wesleyan University in Connecticut who has worked on apatite studies.
Another apatite researcher, Francis McCubbin of the University of New Mexico, points out that one person’s “bone-dry” could be another person’s “relatively damp.” Many researchers now agree that the moon contains some water, he says, but it’s “still very dry in comparison to other planetary bodies, like Earth and Mars.”
More studies will be needed to pinpoint exactly how much water the moon might have contained, says Lindy Elkins-Tanton, a geologist at MIT. “I think the moon is a little wetter than we used to think it was,” she says. “But there are many questions about how much water there was, and where it was residing.”