This image shows observations of a newly discovered galaxy core dubbed GOODS-N-774, taken by the NASA/ESA Hubble Space Telescope’s Wide Field Camera 3 and Advanced Camera for Surveys. The core is marked by the box inset, overlaid on a section of the Hubble GOODS-N, or GOODS North, field (Great Observatories Origins Deep Survey). (Credit: NASA, ESA)
via phys.org
The moment of detonation of a Type 1a supernova is modeled. This situation arises when a white dwarf star has accreted mass from a binary partner to a point when gravitational forces overcome the outward electron degeneracy pressure. The star collapses and it is thought that carbon fusion is initiated in the core, creating a supernova. (Credit: Argonne National Laboratory)
White Dwarf No More – The Type 1a supernova proceeds in the simulation, ripping through the white dwarf star. The star is completely destroyed. Around 1-2 × 1044 Joules of energy is released from Type 1a supernovae, ejecting matter and shock waves traveling at velocities of 3-12,000 miles per second (approximately 2-7% the speed of light). (Credit: Argonne National Laboratory)
Complex Fluid Mechanics – Detailed visualizations of the nuclear combustion inside a supernova. The calculations are based on fluid mechanics, showing how the explosion rips through the star. (Credit: Argonne National Laboratory)
Cosmic rays can help scientists do something no one else can: safely image the interior of the nuclear reactors at the Fukushima Daiichi plant. In the Los Alamos National Laboratory, postdoc Elena Guardincerri, right, and undergraduate research assistant, Shelby Fellows, prepare a lead hemisphere inside a muon tomography machine. (Credit: Los Alamos National Laboratory, Tuttle)
via symmetrymagazine
This artist’s impression shows a possible mechanism for a Type Ia supernova. Astronomers have shown that dead stars known as white dwarfs can re-ignite and explode as supernovas. (Credit: NASA)via bbc
llustration of data from the Spitzer Space Telescope, showing the massive increase in dust around the star NGC 2547-ID8, thought to be the result of an asteroid collision. Image (Credit: NASA/JPL-Caltech/University of Arizona)
via americaspace
A plot showing a spin up, spin down, and the resulting spin polarized population of electrons. Inside a spin injector, the polarization is constant, while outside the injector, the polarization decays exponentially to zero as the spin up and down populations go to equilibrium. (Credit SA3.0)
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Natalie Hinkel gives a plenary talk at the Cool Stars 18 meeting in Flagstaff, Arizona, about her paper on the Hypatia Catalog. (Credit: Natalie Hinkel)
via asunews
The US Department of Energy has cancelled visits by Russian scientists to key US labs, including the Los Alamos National Laboratory. (Credit:NC-ND/Los Alamos National Laboratory)
via physicsworld
A star in a galaxy passes by a black hole closely enough to be destroyed once every 10,000 years. It is possible to detect the death of a star in a fairly distant galaxyas the destruction of a star generates a bright X-ray flare; it is only necessary to distinguish such a flare from other types of X-ray radiation. Because flares occur in a variety of astrophysical processes, the task of finding stars destroyed by black holes is quite complicated. (Credit: Sergei Sazonov)
via mipt
The recent finding of an intermediate-mass black hole provides evidence that could support some theories of how supermassive black holes form. (Credit: ESO/M. Kornmesser)
via discovery
Some of the best evidence for parallel worlds actually arrives courtesy of an enigmatic oddity within deep-space, careening toward the Milky Way at an incredible 200,000 miles per hour. Though it’s more than 2 million light years away, the Andromeda galaxy, appears to engage in anomalous behavior which suggests a strange gravitational phenomenon. Specifically, gravity that could be draining from another universe, as yet invisible to us, could be the impetus behind such anomalous phenomena. (Credit: Micah Hanks)
via mysteriousuniverse
Having a single point in contact with the ground lets a ballerina spin. In the same way, a quantum state is dynamic because it can turn about a point thanks to quantum uncertainty, say CQT and Oxford researchers. (Credit: Michael Garner, courtesy English National Ballet)
via quantumlah
A cross-section of the Earth’s ozone layer as measured by the limb profiler, part of the Ozone Mapper Profiler Suite that’s aboard the Suomi NPP satellite. (Credit: NASA/NOAA)
via ZeeNews
A simulation of two colliding black holes. Colors reflect the variation of gravitational waves. (Credit: Werner Benger/NASA Blueshift)
via physicscentral
