Scientists have discovered mineral-rich structure on Mars that might be the evidence of niche environment on the planet’s subsurface that could support life. (NASA/JPL-Caltech/MSSS)
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In Einstein’s general theory of relativity, gravity is nothing more than the curvature of spacetime. A massive object, such as the sun, causes a deformation of the spacetime grid, while another object such as a planet or a light beam follows the shortest path (a “geodesic”) on this grid. To an observer, this looks like a deflection of the trajectory caused by gravity. (Bottom) A collapsing star can form a black hole so dense and massive that it creates a region of infinite curvature (a “singularity”) so that—inside the event horizon—light cannot escape. Current research in gravitation is attempting to modify general relativity to account for such objects consistent with quantum theory. (Credit: Carin Cain)
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European Space Agency astronaut Andre Kuipers, Expedition 30 flight engineer, prepares vials in the Columbus laboratory of the International Space Station for venous blood sample draws during an immune system investigation. (Credit: NASA)
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Shown above is part of one of the most imaged parts of the night sky, the Orion Nebula. Since the angular size of Orion’s Nebula is so large on the sky, only a portion is shown here. Located just below “Orion’s Belt” this star-forming region is dominated by four young, massive O stars (known as the Trapezium, not pictured here). The wispy blue, green gas seen above is composed mostly of hydrogen, the main element used in forming stars. The Orion Nebula is an astrophysical laboratory, providing an up-close view of the birth of stars. (Credit: Sloan Digital Sky Survey)
Greased Lighning (GL10) project 10 engine electric prototype remote control plane. Photo taken 8/14/14 (Credit: NASA Langley/David C. Bowman)
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The Kori nuclear power plant in Busan, southeast of Seoul, is seen in this picture released by the plant to Reuters. South Korea needs to quickly find additional space where it can store its spent nuclear fuel because some of its temporary storage capacity will be full by 2016, (Credit: Reuters/Kori Nuclear Power Plant/Handout)
via reuters
NASA’s Solar Dynamics Observatory captured this image of what the sun looked like on April 23, 2013, at 1:30 p.m. EDT when the EUNIS mission launched. EUNIS focused on an active region of the sun, seen as bright loops in the upper right in this picture. (Credit: NASA/SDO)
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The study, carried out at the Institute Laue-Langevin (ILL) and published in Nature Communications, showed that in an interferometer a neutron’s magnetic moment could be measured independently of the neutron itself, thereby marking the first experimental observation of a new quantum paradox known as the ‘Cheshire Cat’. Pictured are Yuji Hasegawa, Tobias Denkmayr, Stephan Sponar, Hartmut Lemmel, and Hermann Geppert. (Credit: Vienna University of Technology.)
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An artist’s concept of a rocky world orbiting a red dwarf star. (Credit: NASA/D. Aguilar/Harvard-Smithsonian center for Astrophysics)
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In this image from the Hubble Space Telescope, a giant elliptical galaxy 9.6 billion light-years away appears as a red patch. The bluish dot and tadpole-shaped smear are the distorted and magnified shapes of a more distant spiral galaxy 10.7 billion light-years away. (Credit: NASA, ESA, K.-V. Tran (Texas A&M University), and K. Wong)
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The Dundee tractor beam is not entirely dissimilar from those in “Star Wars” and “Star Trek,” in that it draws an object toward it without making physical contact. The device works by taking advantage of an acoustic wave’s natural push effect, called radiation pressure. (Photons also exert radiation pressure, which is part of the reason comet tails always point away from the sun.) What the Dundee team was able to demonstrate was an example of negative radiation pressure, otherwise known as pull. (Credit: iStock/360/Getty)
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The team says that during this 500 million year period the planet likely experienced three to seven impacts by objects more than 300 miles wide. There were also as many as four impacts by titanic space rocks more than 600 miles across. If there had been any life on the Earth, a 600 mile wide monster asteroid probably would have wiped it out. Surprisingly, these impacts are compatible with the existence of liquid water on the surface as early as 4.3 billion years ago. (D. A. Aguilar, Harvard-Smithsonian Center for Astrophysics)
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The European Space Agency’s Rosetta spacecraft saw the nucleus of comet 67P/Churyumov-Gerasimernko from a distance of 1,210 miles (1,950 kilometers). Image taken July 29, 2014. (Credit: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA)
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Three satellites fly in formation as part of the Synchronized Position Hold, Engage, Reorient, Experimental Satellites (SPHERES) investigation. This image was taken during Expedition 14 in the Destiny laboratory module. (Credit: NASA)
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In this computer simulation, light and dark purple highlight the cavities within the 3D pore structure of CC3. (Credit: Nature Materials 2014)
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According to Efimov’s prediction, bound states of three atoms can be universally described under certain conditions. The scientist found that infinitely many quantum mechanical bound states for the “ménage à trois” exist, even if two of the atoms cannot bind together. (Credit: Heidelberg Uni.)
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Delicate Arch and many other gigantic arches in the US are made of the stuff. It is a “locked sand”, whose angular grains can catch on each other.(Credit: Brad Goldpaint/Aurora Open/Corbis)
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An artistic view of the electron transfer inside an iodomethane molecule. After the interaction with an ultra fast X-ray laser, the electrons from the methyl group, on the right, jump to the iodine atom, on the left. (Credit: SLAC National Accelerator Laboratory)
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Candidate Higgs boson events from collisions between protons in the LHC. The top event in the CMS experiment shows a decay into two photons (dashed yellow lines and green towers). The lower event in the ATLAS experiment shows a decay into 4 muons (red tracks).(Credit: NASA)
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A time sequence of Hubble Space Telescope images, taken in the 15 years from 1994 to 2009, showing the collision of the expanding supernova remnant with a ring of dense material ejected by the progenitor star 20,000 years before the supernova. (Credit: NASA)
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Computational techniques developed by a team from NIST and IU could enable precise computation of atomic properties that are important for nuclear medicine, as well as astrophysics and other fields of atomic research. Image: Paco Ayala (Fotolia)
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The Perseus galaxy cluster is one of the most massive objects in the universe, containing thousands of galaxies immersed in a vast cloud of multimillion degree gas. (Credit: NASA)
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Two closely orbiting black holes in a galaxy about 4.2 billion light-years from Earth emit wavy jets, seen as a bluish spiral, while the third black hole in the trio is more distant, emitting linear jets off to the right.
via abc.net
More than 600 000 galaxies from the BOSS survey were utilized to measure the strength of gravitational interactions of galaxies extremely far away from each other. This is a visual representation of that measurement; the amount that the circles are distorted, or squashed from perfect concentric rings, indicates the velocity that galaxies are falling towards each other and hence the strength of the gravitational interactions. (Credit: BOSS/U. Portsmouth)
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This is a composite image of the lunar farside taken by the Lunar Reconnaissance Orbiter in June 2009, note the absence of dark areas. Credit: NASA
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Curiosity rover panorama of Mount Sharp captured on June 6, 2014 (Sol 651) during traverse inside Gale Crater. Note rover wheel tracks at left. She will eventually ascend the mountain at the ‘Murray Buttes’ at right later this year. Assembled from Mastcam color camera raw images and stitched by Marco Di Lorenzo and Ken Kremer. Credit: NASA/JPL/MSSS/Marco Di Lorenzo
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