Shown here is the crystal structure of molybdenite, MoS2. When hit with a burst of laser light, freed electrons and holes combine to form combinations called trions, consisting of two electrons and one hole, represented here by orange and green balls. (Credit: Jose-Luis Olivares/MIT)
via mit
A test version of NASA’s Orion capsule floats in the rear of the USS Anchorage during a recovery drill off the coast of California September 15, 2014. Orion is NASA’s next exploration spacecraft, designed to carry astronauts to destinations in deep space, including an asteroid and Mars. Picture taken September 15, 2014. (Credit: REUTERS/Mike Blake)
via reuters
A few major factors will drive exponential growth in the amount of terabytes falling on us from the skies over the next couple of decades: the increasing speed of commercial satellite deployment, implementation of faster communication technology, and the onset of interplanetary missions. (Credit: SKA Telescope, Golubovich)
via venturebeat
How many exoplanets have been discovered? According to the Extrasolar Planet Encyclopedia, a semi-official catalog based in Europe, there were as of the end of September last year 990 confirmed exoplanets and 2,321 candidate exoplanets. (Credit: Zina Deretsky, National Science Foundation)
via phys.org
A collaborative robot from Rethink Robotics, works on a mocked-up assembly line. Setting limits on the level of pain a robot may (accidentally) inflict on a human is a crucial goal of the first safety standards being drawn up for these “collaborative” robots. (Credit: Rethink Robotics, Simonite)
via technologyreview
The Tevatron, the particle accelerator used to find the oscillating Bs meson, has huge detectors surrounded by a cylindrical ‘tracking chamber’, shown here. (Credit: Fermilab)
via cornell
On Mercury a solar day is about 176 Earth days long. During its first Mercury solar day in orbit the MESSENGER spacecraft imaged nearly the entire surface of Mercury to generate a global monochrome map at 250 meters per pixel resolution and a 1 kilometer per pixel resolution color map. (Credit: NASA/JHU APL/CIW)
via phys.org
The researchers observed for the first time coherent oscillations between two spin states: |e↑,g↓〉⇔|e↓,g↑〉. From the oscillation frequency, they determine the spin-exchange interaction strength. (Credit: APS/Ana Maria Rey)
via physics.aps
NASA has found about 95 per cent of the largest and potentially most destructive asteroids, those measuring about one kilometre or larger in diameter, but only 10 per cent of those 140 metres or larger in diameter. (NASA/JPL-Caltech/Canadian Press)
via cbslocal
Rendering of the near–perfect crystal structure of the yttrium–iron–aluminum compound used in the study. The two–dimensional layers of the material allowed the scientists to isolate the magnetic ordering that emerged near absolute zero. (Credit:Brookhaven National Laboratory)
via azoquantum
Diamond anvils malformed during synthesis of ultrahard fullerite. Note the dent in the center. (Credit: Moscow Institute of Physics and Technology)
via nextbigfuture
Magnetic stripes of solar material – with alternating south and north polarity – march toward the sun’s equator. Such observations may change the way we think about what’s driving the sun’s 22-year solar cycle. (Credit: S. McIntosh)
This image illustrates Dawn’s spiral transfer from high altitude mapping orbit (HAMO) to low altitude mapping orbit (LAMO). The trajectory turns from blue to red as time progresses over two months. Red dashed sections are where ion thrusting is stopped so the spacecraft can point its main antenna toward Earth. (Credit: NASA/JPL-Caltech)
via nasa
The little mushroom cap between the two high-gain antennas is the X-band low-gain antenna. The little blue thing is DCAM3, a deployable camera that will hopefully take pictures of the explosion and impact of Hayabusa’s “Small Carry-on Impactor” while the mothership hides safely in the shadow of the asteroid. (Credit: Lakdawalla)
via gizmodo
Phase change materials can switch between two forms depending on how quickly they’re cooled. Cool them quickly and you get an amorphous form, which provides significant resistance to the flow of electrons. Cool them slowly and they will allow electrons to flow more readily. Once cooled, these two forms remain stable, locking the differences in conduction in place. (Credit: Columbia University, Timmer)
via arstechnica
The Yarkovsky Effect: The daylight side absorbs the solar radiation. As the object rotates, the dusk side cools down and hence emits more thermal photons than the dawn side. It may be possible to exploit this effect for planetary defense.
via thespacereview
An event in the IceCube neutrino telescope. Photomultipliers attached to strings buried deep in the Antarctic ice detect the bursts of light emitted when a neutrino collides with the ice and produces a muon. The event shown was generated by an upward moving muon, which was produced by an upward moving muon neutrino that passed through the Earth. APS/Joan Tycko;
via physics.aps
A 1974 photo of the part named Intersection 5 (I5) of the ISR of CERN’s old PS, clearly shows the layout of the magnets and the crossing of the two beams pipes. (Credit: Salem)
via onislam
Russian power engineering R&D institute NIKIET has completed the engineering design for the BREST-300 lead-cooled fast reactor. (NIKIET)
via world-nuclear-news
“This is a long-standing, really neat experimental idea,” says Paul Lett, of the National Institute of Standards and Technology in GaithersburgLett, “Now we have to see whether or not it will lead to something practical, or will remain just a clever demonstration of quantum mechanics.”(CreditBarreto-Lemos, Vergano)
via nationalgeographic
The Borexino neutrino detector uses a sphere filled with liquid scintillator that emits light when excited. This inner vessel is surrounded by layers of shielding and by about 2,000 photomultiplier tubes to detect the light flashes.(Credit: Borexino Collaboration)
via scientificamerican
MOLECULAR MODEL In the molecular model, quark-antiquark pairs form two color-neutral mesons that become weakly linked as a molecule.DIQUARK MODEL The particles form quark-quark and antiquark-antiquark pairs, which are forced to combine to balance their color charges.
via simonsfoundation
A computer model shows one scenario for how light is spread through the early universe on vast scales (more than 50 million light years across). Astronomers will soon know whether or not these kinds of computer models give an accurate portrayal of light in the real cosmos. (Credit: Andrew Pontzen/Fabio Governato)
via phys
Radio/optical composite of the Orion Molecular Cloud Complex showing the OMC-2/3 star-forming filament. GBT data is shown in orange. Uncommonly large dust grains there may kick-start planet formation. (Credit: S. Schnee, et al.; B. Saxton, B. Kent (NRAO/AUI/NSF)
via rdmag
In one potential method to realize superabsorption, a superabsorbing ring absorbs incident photons, giving rise to excitons. (Credit: Higgins, et al.)
via phys.org
An “air waveguide” has been used to enhance light signals collected from distant sources. A single waveguide could be used to send out a laser and collect a signal. (Credit: Howard Milchberg)
via theengineer
This image shows the stunning elliptical galaxy Centaurus A. Recently, astronomers have used the NASA/ESA Hubble Space Telescope to probe the outskirts of this galaxy to learn more about its dim halo of stars. (Credit: ESA/Hubble)/NASA/Digitized Sky Survey/MPG/ESO
via astronomy
Physicists long assumed a proton’s spin came from its three constituent quarks. New measurements suggest particles called gluons make a significant contribution (Credit: Brookhaven National Laboratory)
via scientificamerican
These artist’s renderings show one model of pulsar J1023 before (top) and after (bottom) its radio beacon (green) vanished. Normally, the pulsar’s wind staves off the companion’s gas stream. When the stream surges, an accretion disk forms and gamma-ray particle jets (magenta) obscure the radio beam. (Credit: NASA’s Goddard Space Flight Center)
via discovery
The research group demonstrates that adding such massive neutrinos to the standard model does not really explain all datasets. (Credit: The Milky Way, NASA.)
via phys.org
The Super Cryogenic Dark Matter Search is an international, multimillion dollar dark matter experiment currently based in Minnesota with plans to progress the project by building a more sensitive detector at SNOLAB. (Credit: SNOLAB)
via queensu
What is the view of time that Albert Einstein presents to us in special relativity? Einstein tells us that there is no separate ‘time’ or ‘space.’ ‘Time’ and ‘space’ cannot be separated; they are a united whole.
via davidreneke
