Showing posts with label "Beast" Asteroid to Fly by Earth on Sunday. Show all posts
Showing posts with label "Beast" Asteroid to Fly by Earth on Sunday. Show all posts

Friday, October 10, 2014

Stimulated emission depletion (STED) microscopy

It is a process that provides super resolution by selectively deactivating fluorophores, so as to enhance the imaging in that area. It was developed by Stefan W. Hell in 1994, and was first experimentally shown in 1999. Hell was awarded the Nobel Prize in Chemistry in 2014 for its invention. This is one of several types of super resolution microscopy techniques that have recently been developed. Super resolution microscopy is a set of techniques to bypass the diffraction limit of microscopy to achieve better resolution.

Photoactivated localization microscopy (PALM) and stochastic optical reconstruction microscopy (STORM) are also super resolution microscopy techniques, although they use a different process than STED to achieve this resolution.


The techniques they developed enabled extremely high resolution images to be produced using optical microscopy. Their work circumvented the problem of the ‘diffraction limit’ – the inability of light microscopy to distinguish between structures smaller than half the wavelength of visible light or about 200nm. This advance allowed nanoscale structures – including individual molecules – to be visualised within cells while they are still alive, something that isn’t possible with techniques such as electron microscopy.

Diagram illustrating the principle behind Stimulated Emission Depletion microscopy
The basis of STED microscopy is the coupling of the excitation laser with the STED depletion laser, resulting in the doughnut-shaped depletion. The two perfectly aligned laser systems minimize the size of the fluorescence spot, overcoming the resolution-limiting effects of diffraction. 



The perhaps most straightforward way to sharpen the fluorescence focal spot is to selectively inhibit the fluorescence at its outer part. If this is applied to an otherwise diffraction-limited spot, one would expect that the diffraction barrier can be overcome since scanning with a smaller fluorescent spot signifies increased spatial resolution. A phenomenon that stops fluorescence (=spontaneous emission) is that of stimulated emission. This is one of the key ingredients of the Stimulated Emission Depletion (STED-) microscope. However, STED by itself could not really break the diffraction barrier since the beams with which STED is accomplished are diffraction-limited as well. Therefore the real physical ingredient for breaking the diffraction barrier is the saturation of the fluorescence inhibition by stimulated emission, as we will argue below.


The setup of STED Microscope 

The STED-microscope relies on pairs of synchronized laser pulses. To this end, excitation is performed by a subpicosecond laser pulse that is tuned to the absorption spectrum of the dye. The excitation pulse is focused into the sample, producing an ordinary diffraction limited spot of excited molecules. The excitation pulse is immediately followed by a depletion pulse, dubbed 'STED-pulse'. The STED pulse is red-shifted in frequency to the emission spectrum of the dye, so that its lower energy photons act ideally only on the excited dye molecules, quenching them to the ground state by stimulated emission. The net effect of the STED pulse is that the affected excited molecules cannot fluoresce because their energy is dumped and lost in the STED pulse. By spatially arranging the STED pulse in a doughnut mode, only the molecules at the periphery of the spot are ideally quenched . In the center of the doughnut, where the STED pulse is vanishing, fluorescence ideally remains unaffected.

No resolution limit For Microscopy

By increasing the STED pulse intensity, the depletion becomes complete at the spot's periphery and increasingly more effective towards the middle. At the doughnut hole, however, the fluorescence is ideally not affected at all. Therefore, by increasing the intensity of the doughnut-shaped STED-pulse, the fluorescent spot can be progressively narrowed down, in theory, even to the size of a molecule. This concept signifies a fundamental breaking of the diffraction barrier. The essential ingredient is the saturated reduction of the fluorescence (= depletion) at any coordinate but the focal point.

Comparison with confocal fluorescence microscopy

 This microscopy is in stark contrast to the presently known super resolution methods like the confocal, the multiphoton or related fluorescence microscopes, which can never surpass Abbe's barrier by more than a factor 2. In a way, confocal fluorescence and two-photon microscopes just cross the diffraction border, without breaking it. The resolution of these systems is still limited by diffraction, in contrast to the STED-microscope .

Depletion means saturation

The real physical reason for the breaking of the diffraction barrier is not the fact that fluorescence is inhibited, but the saturation (of the fluorescence reduction). Fluorescence reduction alone would not help since the focused STED-pulse is also diffraction-limited. What does saturation mean in this context? Whereas the fluorescence at the middle of the doughnut is unaffected, it is fully stopped at the closest proximity of the doughnut. Thus the fluorescent region is continuously narrowed down without limit! 

Fundamentally enlarged passband of the optical transfer function

It is clear that the decrease in spatial extent of the effective spot or point-spread-function in a STED-microscope is associated with a fundamental increase of the passband of the effective transfer function of the microscope. The STED-microscope is not a diffraction-limited system anymore. It is the first to provide conceptionally unlimited optical resolution, in spite of the fact that it relies on visible light and regular objective lenses .


To date an improvement beyond the diffraction barrier of 3 in the transverse direction and up to 6 along the optical axis has been experimentally demonstrated. The viability of the STED-concept has been exemplified in a number of simple experiments. Its practicability and the maximum spatial resolution depend very much on the level of saturation that can be obtained and on the deepness of the doughnut hole, which should be ideally zero. So far, experiments show that the level of saturation will be determined by the bleaching that is inflicted on the dye. Moreover, it will be interesting to see to which extent dyes can be switched off and if STED is applicable to all dyes, including those that are endogenous to the cell.

Ground-State-Depletion- (GSD) Microscopy, a cousin of STED

 An alternative to quenching the excited state is to deplete the ground state of the dye. This depletion could be achieved by shelving the dye into the triplet state or another long-lived state. As in the concept of STED, the real ingredient is the saturation of the depletion. Saturation entails a non-linear relationship between the (residual) fluorescence and the applied intensity

The New Era Of Light Microscopy-STED; Nobel Prize 2014

Saturday, June 7, 2014

"Beast" Asteroid to Fly by Earth on Sunday

What might be the effects if a large asteroid collided with Earth?


The orbit of near-Earth asteroid 2014 HQ124, first discovered on April 23, 2014, is shown in this NASA graphic. The asteroid will fly by Earth Sunday, June 8, at a safe distance of three times the Earth-moon distance.NASA/JPL-Caltech
 

Humanity should be thankful "The Beast" doesn't have Earth in its crosshairs.


This Sunday (June 8), the near-Earth asteroid 2014 HQ124—which some observers have nicknamed "The Beast"—will give the planet a relatively close shave, coming within 777,000 miles (1.25 million kilometers) at its closest approach, or about 3.25 times the distance from Earth to the moon.
There is no chance of an impact on this pass, researchers stress. But at 1,100 feet (335 meters) wide, 2014 HQ124 could do some serious damage if it slammed into us. [
Potentially Dangerous Asteroids (Images)]
"This one would definitely be catastrophic if it hit the Earth," asteroid impact expert Mark Boslough, of Sandia National Laboratories in New Mexico, said during a June 5 webcast produced by the online
Slooh community observatory that previewed 2014 HQ124's upcoming flyby.
"If it hit a city, it would definitely wipe out an entire metropolitan area," Boslough added.
Asteroid 2014 HQ124 is currently traveling about 31,000 mph (50,000 km/h) relative to Earth, Boslough said. But if the asteroid were on a collision course, our planet's gravity would boost its speed up to about 40,000 mph (64,000 km/h) at the time of impact.
If 2014 HQ124 is one solid piece of rock—its composition isn't known for certain—the strike would unleash an explosion with a yield of about 2,000 megatons, Boslough added. For comparison, the atomic bomb the United States dropped on the Japanese city of Hiroshima during World War II packed about 15 kilotons. (One megaton is equivalent to 1,000 kilotons.)
"You'd end up with a crater about 3 miles across," Boslough added. "An event like that would break windows over 100 kilometers away."
Asteroid 2014 HQ124 was discovered on April 23, just six weeks ago—not nearly enough time to deflect the asteroid if it were on a collision course with Earth. But that doesn't mean the
asteroid would kill millions of people if it struck New York City or Tokyo.
"Once it's within radar distance, the precision is remarkably good on its position and speed," Boslough said. "So the folks at JPL [NASA's Jet Propulsion Laboratory] would be able to predict its impact point to within the nearest kilometer and its time to within the nearest second."
There would thus probably be plenty of time to organize an effective evacuation campaign if 2014 HQ124 were headed straight for us. But that isn't always always the case, as some (smaller) space rocks slam into the planet without ever being detected.

In February 2013, for example, a 65-foot-wide (20 m) asteroid detonated without warning in the sky above the Russian city of Chelyabinsk, shattering thousands of windows and
injuring more than 1,200 people. And there are many more objects out there like the Chelyabinsk asteroid—small space rocks cruising unnamed through the dark depths of space.
Scientists estimates that they've found about 95 percent of the potential "civilization-enders" out there—mountain-size asteroids at least 0.6 miles (1 km) across. But there are probably more than 1 million near-Earth asteroids at least 100 feet (30 m) wide, and less than 1 percent of them have been discovered.
Originally published on Space.com.

"Beast" Asteroid to Fly by Earth on Sunday

 
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