The UW’s current fusion experiment, HIT-SI3. It is about one-tenth the size of the power-producing dynomak concept. (Credit: U of Washington)
via washington.edu
Gas column density 5 Myr after stars begin forming in the “real” Clouds (left panels) and corresponding Spheres (right panels). The Spheres begin forming stars 5-6 Myr after t=0, so the figure shows simulations at a similar stage of star formation. Clouds show more widespread star formation, and alignment of their major gas filaments along the larger-scale structures present in the galaxy. (Credit: Rey-Raposo, Dobbs & Duarte-Cabral 2014)
via astrobites
Larger galaxies are unable to create new stars at a rapid enough pace so they start to “eat” stars in neighboring galaxies. (Photo By Nasa/Getty Images)
via cbs
The SETI Institute’s Allen Telescope Array (ATA) is hunting for radio signals from hypothetical intelligent alien life in our galaxy. (Credit: SETI) Institute
via aninews
NASA has a new project underway called GEDI. The sole purpose of GEDI is to point a laser-based device at Earth from the International Space Station in order to map out forests in 3D, eventually determining the amount of carbon in Earth’s forests. (Credit: NASA’s Goddard Space)
via industrytap
A look through the open hatch of SpaceX’s Dragon V2 capsule, one of two designs chosen for NASA’s Commercial Crew Transportation Capability program. Both Boeing and SpaceX have been told to halt production of their space taxi designs until a protest filed by the Sierra Nevada Corporation has been resolved. (Credit: NASA)
via popsci
German winner of the Nobel Prize for chemistry Stefan Hell gestures at a small party with his colleagues in Goettingen, Germany, Wednesday, Oct. 8, 2014. Hell shares the prize with Americans Eric Betzig and William E. Moerner for developing ways to dramatically improve the resolution of optical microscopes. Hell developed the underlying technology for R&D 100 Awards-winning super-resolution microscopes from Leica. (Credit AP/dpa, Swen Pfoertner)
via rdmag
The Einstein Papers Project, a group of scholars devoted to collecting and transcribing Einstein’s works and publishing The Collected Papers of Albert Einstein both online and in printed format, have collected thousands of Einstein’s letters, both those from him and to him. But this exchange is new. (Credit: The Telegraph)
via inquisitr
Dust map of the Universe. The region studied by BICEP2 is indicated by the rectangle in the right circle. (Credit: Planck Collaboration)
via universetoday
n this illustration, the artificial atom on the right side of the image sends out sound waves that are picked up by the microphone on the left. (Credit: Philip Krantz)
via livescience
A serious challenge to the discovery of gravity waves by the BICEP2 2014 results has appeared: the researchers had underestimated the amount of interstellar dust that could be contaminating their data. (Credit: MacRobert, Andrei Linde)
via skyandtelescope
Scientists have found definitive traces of water on a relatively small exoplanet. HAT-P-11b is the size of Neptune and four times the size of Earth. The exoplanet has copious amounts of both water vapor and hydrogen in its atmosphere. (Credit: NASA)
via bbc
Our current model of the early inflationary period predicts that the universe should be flat, and so far that has held up. If the universe actually is curved, then the inflationary period must have been more complex than we have thought. (Credit: Koberlien)
via phys.org
Few scientists doubt that Einstein was right. But the mathematics describing the time-dilation effect are “fundamental to all physical theories”, says Thomas Udem, a physicist at the Max Planck Institute for Quantum Optics in Garching, Germany, who was not involved in the research. “It is of utmost importance to verify it with the best possible accuracy.” (Credit: A. Witze, Martin Poole/Getty)
via nature
Graphic representation of a seaborgium hexacarbonyl molecule on the silicon dioxide covered detectors of a COMPACT detector array. (Credit: Alexander Yakushev (GSI) / Christoph E. Düllmann)
via newscientist
A transmission electron microscopic image of titanium dioxide plates resting on a near-invisible sheet of graphene. (Credit: Rozhkova et. al.)
via anl.gov
There have been recent near misses – an explosion over Russia, a mysterious crater in Nicaragua. But what would we do in the event of an actual meteor strike? A simulated meteor strike at a training facility in Texas. (Credit: Nick Ballon)
via theguardian
ITTY BITTY LIVING SPACE The tiny galaxy M60-UCD1 (circled in white) harbors a black hole with the mass of around 21 million suns. M60-UCD1 may be a remnant of a larger galaxy torn apart by the massive galaxy M60 (center), which is also pulling in a nearby spiral galaxy (upper right). (Credit: NASA, ESA)
via sciencenews
The illustration shows how oscillating photons create an image of frozen light. At first, photons in the experiment flow easily between two superconducting sites, producing the large waves shown at left. After a time, the scientists cause the light to ‘freeze,’ trapping the photons in place. Fast oscillations on the right of the image are evidence of the new trapped behavior. (Credit: James Raftery et al.)
via princeton
Pakistan is a signing ceremony away from becoming the associate member of the European Organisation for Nuclear Research. Above photo is CERN Labs on the Swiss-French border. (Credit: CERN)
via dawn
The quasicrystals formed 4.5 billion years ago in a violent collision between two rocks, among the asteroids that coalesced into planets. The rock with the quasicrystals landed in Chukotka as a meteorite. “They’re part of the primal stuff that formed our solar system,” Dr. Steinhardt said. The above is A penteract (5-cube) pattern using 5D orthographic projection to 2D using Petrie polygon basis vectors overlaid on the diffractogram from an Icosahedral Ho-Mg-Zn quasicrystal. (Credit: NYTimes)
via nytimes
Upper plot shows the slope of positron fraction measured by AMS (red circles) and a straight line fit at the highest energies (blue line). The data show that at 275±32 GeV the slope crosses zero. Lower plot shows the measured positron fraction as function of energy as well as the location of the maximum. (Credit CERN)
via interactions
An organic light-emitting diode, or OLED, glows orange when electrical current flows through it. It is a step toward ‘spintronic’ devices such as faster computers, better data storage and more efficient OLEDs for TV, computer and cell phone displays. (Credit: Andy Brimhall, University of Utah)
via phys.org
This revolutionary work could open up new real estate in the phone by embedding the glass with layer upon layer of sensors, including ones that could take your temperature, assess your blood sugar levels if you’re diabetic or even analyze DNA. (Credit: Jerome Lapointe, Mathieu Gagné, Ming-Jun Li, and Raman Kashyap)
via mediacastermagazine
The NASA/ESA Hubble Space Telescope has produced this finely detailed image of the beautiful spiral galaxy NGC 6384. This galaxy lies in the constellation of Ophiuchus (The Serpent Bearer), not far from the centre of the Milky Way on the sky. The positioning of NGC 6384 means that we have to peer at it past many dazzling foreground Milky Way stars that are scattered across this image. (Credit NASA/ESA)
via nationalgeographic
he problem was first identified some time ago. Dubbed the “cosmological lithium discrepancy,” the issue is very simple: everything we know about the Big Bang, supernovae, and the dynamics of stars, tells us that we should find a very specific concentration of lithium in the universe at large — but the universe actually seems to contain far less than that amount. (Credit: NASA, HUbble)
European Space Agency’s Giotto probe returned 2333 images during the Comet Halley encounter of March 13-14, 1986. All were recorded before the closest approach of 596 km at 00:03:02 UTC on 14 March 1986; the last from a distance of 1180 km, 15 seconds before closest approach. (Credit: MPAE, Dr H.U. Keller.
An Atlas V rocket lifts off with the mysterious CLIO satellite. The rocket was carrying a satellite known only as CLIO, which it delivered into an unidentified (though probably geosynchronous) orbit. (Credit: ULA)
via forbes
Random number generator setup: a camera is fully and homogeneously illuminated by a LED. The raw binary representation of pixel values are concatenated and passed through a randomness extractor. This extractor outputs quantum random numbers. (Credit: arXiv:1405.0435 [quant-ph])
Science says the universe could be a hologram, a computer program, a black hole or a bubble—and there are ways to check. (Credit: NASA, ESA, SAO, CXC, JPL-Caltech, and STScI)
via smithsonianmag
“I confess that in my early in my career as a physicist I was rather cynical about sophisticated statistical tools, being of the opinion that “if any of this makes a difference, just get more data”. That is, if you do enough experiments, the confidence level will be so high that the exact statistical treatment you use to evaluate it is irrelevant.” (Credit: Jon Butterworth)
via theguardian
It was the daytime soap opera of particle physics. But the final episode of the first season ends in an anticlimax. The Higgs boson’s decay into pairs of photons – the strongest yet most confusing clue to the particle’s existence – is looking utterly normal after all. (Credit: D. Moir/Reurters, M. Slezak)
via newscientist
NIST chip containing a single-photon detector was made of superconducting nanowires. Four chips like this were used in the experiment that entangled three photons. (Credit: Verma/NIST)
via extremetech
The new plan, proposed by researchers at the University of Southampton in England, is to eavesdrop on the faint nanosecond radio signals sent our way when cosmic rays hit edges of the Moon at a near-tangent. (Credit J. Hewitt, astrobiology.aob.rs)
via extremetech
“The key question is whether a real quantum dynamics, of the general form suggested by de Broglie and the walking drops, might underlie quantum statistics,” Bush said. “While undoubtedly complex, it would replace the philosophical vagaries of quantum mechanics with a concrete dynamical theory,” said John Bush of MIT. (Credit: D. Harris/MIT, M. Byrne)
via motherboard
A composite photo of comet 67P/C-G showing gases escaping from the ‘neck’. The first jets of dust were detected spurting from the comet as Rosetta approached it in August but detailed photographs weren’t available until last week. (Credit: Emily Lakdawalla/ESA)
via forbes
The spacecraft captured the views between July 20 and July 22, 2014, as it departed Titan following a flyby. Cassini tracked the system of clouds as it developed and dissipated over Ligeia Mare during this two-day period. Measurements of the cloud motions indicate wind speeds of around 7 to 10 miles per hour (3 to 4.5 meters per second). (Credit: NASA, Cassini)
via smithsonianmag
Less than two months after it first began repeatedly scanning the sky, the ESA’s Gaia space observatory has discovered its first supernova – a powerful stellar explosion that had occurred in a distant galaxy located some 500 million light-years from Earth, the agency announced on Friday. The above is an artist’s impression of a Type Ia supernova – the explosion of a white dwarf locked in a binary system with a companion star. (Credit: ESA/ATG medialab/C. Carreau, Bednar)
via redorbit
Grain boundaries are rows of defects that disrupt the electronic properties of two-dimensional materials, like graphene, but a new theory by scientists at Rice University shows no such effects in atomically flat phosphorus. That may make the material ideal for nano-electronic applications. (Credit: Evgeni Penev/Rice University)
via energy-daily
To find out if the universe is a hologram, scientists at the U.S. Department of Energy’s Fermi National Accelerator Laboratory have powered up their exotic holographic inferometer, or Holometer. The results of the Fermilab E-990 experiment could indeed indicate that the nature of the universe is holographic. (Credit: Baskin, M. Freiberger)
via guardianlv
The ultimate fate of the universe depends on the nature of dark matter and dark energy, about which we know almost nothing. (Credit: NASA)
via mysteriousuniverse