The X-ray image from the Swift X-ray Telescope of the gamma-ray burst GRB 130925. The white object in the center is the gamma-ray burst. The large diffuse region to the right is a cluster of galaxies. The other objects are X-ray-emitting celestial objects, most likely supermassive black holes at the centers of distant galaxies. The full image is approximately the size of the full moon. (Credit: Phil Evans/ University of Leicester)
via psu
The Borexino collaboration, which announced the detection of an elusive solar neutrino in August, involved several scientific contributions from Princeton over its 25-year history. The detector consists of two massive transparent nylon balloons filled with a petroleum-based liquid called “scintillator,” which emits a flash of light when it detects a neutrino. These flashes are picked up by an array of sensors embedded in a stainless steel sphere that surrounds the balloons. (Credit: Borexino collaboration)
via princeton
The experiment effectively measures the shift in the laser frequencies relative to what these transition frequencies are for ions at rest. The combination of two frequency shifts eliminates uncertain parameters and allows the team to validate the time dilation prediction to a few parts per billion, improving on previous limits. The result complements other Lorentz violation tests that use higher precision atomic clocks but much slower relative velocities. (Credit: Botermann, et al., Schirber)
via aps.org
The image above is a comparison of the radial density profiles of the galaxies which the researchers have created by displaying the soliton in the centre of each galaxy with a halo surrounding it. The solitons are broader but have less mass in the smaller galaxies. (Credit: /kipac.stanford.edu/kipac/media)
via dailygalaxy
The sky facing south at nightfall in late September from a dark, light-pollution-free site with stars visible to magnitude 6.5, the naked eye limit. (Credit: Stellarium)
via skyandtelescope
Artistic rendering of the generation of an entangled pair of photons by spontaneous parametric down-conversion as a laser beam passes through a nonlinear crystal. Inspired by an image in Dance of the Photons. (Credit: A. Zeilinger)
via newswise
“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
In 2013, huge active plumes containing water vapour being released from the surface of Jupiter’s moon Europa were discovered. This sensational find was made using the NASA/ESA Hubble Space Telescope. Europa has been a focus of extraterrestrial research for some time now, as there were clear indications that it harbors a liquid ocean beneath its icy crust. Now, it appears, the geysers have vanished. (Credit: K. Retherford, Southwest Research Institute, NASA/ESA/K.)
via dailygalaxy
A pulsar is the rapidly spinning and highly magnetized core left behind when a massive star explodes. Because only rotation powers their intense gamma-ray, radio and particle emissions, pulsars gradually slow as they age, and eventually cease their characteristic emissions. (Credit: F. Reddy of Goddard Space Flight Center, NASA)
via onislam
A weird theoretical cousin of the Higgs boson, one that inspired the decades-long hunt for the elusive particle, has been properly observed for the first time. The discovery bookends one of the most exciting eras in modern physics. The above is a simulation of the production and dec (Credit: Slezak)
via newscientist
MAVEN is NASA’s next Mars orbiter and launched on Nov. 18, 2014 from Cape Canaveral, Florida. It will study the evolution of the Red Planet’s atmosphere and climate. Universe Today visited MAVEN inside the clean room at the Kennedy Space Center. With solar panels unfurled, this is exactly how MAVEN looks when flying through space and circling Mars and observing Comet Siding Spring. (Credit: Ken Kremer)
via universetoday
“This is a time of very rapid advances in the field. You don’t know on any given day what new discovery you’re going to see posted that night on arXiv,” said Liam McAllister, associate professor of physics and a specialist in string theory. (Credit: Glaser)
via cornell
Diagram illustrating quasar observations. In 2010, a research team looked at light from distant quasars that had passed through large intergalactic clouds of gas. They found evidence of some slight variation of alpha depending on the direction we looked in the sky, which would imply a spatial variation of the physical constants. This made lots of news in the press, but the findings were not strong enough to be conclusive. (Credit: J. C. Berengut, Koberlein)
via phys
The ratios of various elements found in the sample of RSGs, where the dark gray line is the theoretical model for a RSG, the lighter grey shows a three sigma deviation from normal, and the black points show the observed ratios for the sampled stars. The red, however, are the ratios observed in the TZO candidate HV 2112- indicating some elements are present at ratios far from expected. (Credit: E.Levesque et al.)
via astrobites
Once every year or two, a comet appears in the sky that is bright enough to be seen with a small telescope or binoculars. Right now, observers anywhere in the Northern Hemisphere can see such a comet. (Credit: Starry Night Software)
via space
Sofie Carsten Nielsen, Danish science minister, and Swedish education minister Jan Björklund break ground for the €1.84bn European Spallation Source in Lund, Sweden. (Credit: ESS)
via physicsworld
Artist impression of the Square Kilometer Array. If all goes according to plan in the next decade, we could see these small perturbations on the moon—and begin to solve some of the mysteries of space. (Credit: SKA)
via gizmodo
Space travelers from around the world are headed to China this month for an international Planetary Congress, which will explore the possibilities for expanding human spaceflight cooperation among different countries. Pictured above is China’s first astronaut, Yang Liwei, is now vice director of the China Manned Space Engineering Office. (Credit: CMS)
via space
An animation of the quicksort algorithm sorting an array of randomized values. The red bars mark the pivot element; at the start of the animation, the element farthest to the right hand side is chosen as the pivot. (Credit: RonaldH)
via wired
Rather than keeping all its eggs in D-Wave’s basket, Google’s “Quantum A.I. Lab” announced that it is starting a collaboration with an academic quantum computing researcher, John Martinis of the University of California-Santa Barbara. (Credit: Wiki, Timmer)
via arstechnica
A new map places the Milky Way (black dot) within a large supercluster of galaxies (white dots) by tracing the gravitational pull of galaxies toward one another. White filaments reveal the paths of galaxies moving toward a gravitational center in the new supercluster, dubbed “Laniakea.” (Blue, low galaxy density; green, intermediate; red, high.) (Credit: DP at CEA/Saclay, France)
via nationalgeographic
This three-dimensional map offers a first look at the web-like large-scale distribution of dark matter, an invisible form of matter that accounts for most of the Universe’s imaginary mass. The map reveals a loose network of dark matter filaments, gradually collapsing under the relentless pull of gravity, and growing clumpier over time. The three axes of the box correspond to sky position, and distance from the Earth increasing from left to right. Note how the clumping of the dark matter becomes more pronounced, moving right to left across the volume map, from the early Universe to the more recent Universe. (Credit: NASA/ESA/Richard Massey)
via ku.edu
Cosmologists have revealed intruiging new ways to probe the mystery of whether dark energy exists and how it might be accelerating the universe’s growth. (Credit: Picturegarden/Getty)
via newscientist
As time ticks down to the restart of the Large Hadron Collider, scientists are making sure their detectors run like clockwork. (Credit: Antonio Saba, CERN)
via symmetrymagazine
Schematic representation of a spin-exchanging collision. Two atoms in different orbitals (blue and green) and different spin orientations (black arrows) collide. The two atoms exiting the collision have swapped their spins after interacting. Crucially, the process is independent of the two specific initial spin states. (Credit: LMU-München / MPQ, Quantum Many Body Systems Division)
via phys.org
The Giant Magellan Telescope (GMT) is a ground-based extremely large telescope planned for completion in 2020.[5] It will consist of seven 8.4 m (27.6 ft) diameter primary segments,[6] with the resolving power of a 24.5 m (80.4 ft) primary mirror and collecting area equivalent to a 22.0 m (72.2 ft) one,[7] (which is about 368 square meters) (Credit: wiki, Tarantola)
via gizmodo
A new analysis suggests that hot super-Earths might be the skeletal remnants of hot Jupiters stripped of their atmospheres. The above image is an artist’s depiction of an early stage in the destruction of a hot Jupiter by its star. (Credit: NASA / GSFC / Reddy, S. Hall)
via skyandtelescope
