When space probes, such as Rosetta and Cassini, fly over certain planets and moons, in order to gain momentum and travel long distances, their speed changes slightly for an unknown reason. A researcher has now analyzed whether or not a hypothetical gravitomagnetic field could have an influence. However, other factors such as solar radiation, tides, or even relativistic effects or dark matter could be behind this mystery. An artist’s rendition of Rosetta probe during a flyby. (Credit: ESA/C.Carreau)
via sciencedaily
The starboard truss of the International Space Station while Space Shuttle Endeavour docked with the station. The newly installed Alpha Magnetic Spectrometer (AMS) is visible at center left. (Credit: NASA)
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The dome of the Blanco Telescope, which houses DECam, the 570-megapixel CCD camera used for the Dark Energy Survey, at the Cerro Tololo Inter-American Observatory in Chile. (Credit: Reidar Hahn)
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Mosaic of southern hemisphere of Miranda, the innermost regular satellite of Uranus, with radius of 236 km. Projection is orthographic, centered on the south pole. Visible from left to right are Elsinore, Inverness, and Arden coronae. (Credit: NASA/Jet Propulsion Laboratory/Ted Stryk)
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An international team of physicists has shown that the mass ratio between protons and electrons is the same in weak and in very strong gravitational fields. Pictured above is the laser system with which the hydrogen molecules were investigated on earth. (Credit: LaserLaB VU University Amsterdam/Wim Ubachs)
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The MIT BioSuit, a skintight spacesuit that offers improved mobility and reduced mass compared to modern gas-pressurized spacesuits. (Credit: Jose-Luis Olivares/MIT)
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Dark matter and dark energy continue to be cosmological conundrum for physicists worldwide. Nobel prize winner Brian Schmidt offers his perspective in an interview. The image shown here is of the ALMA antennas and the constellations of Carina (The Keel) and Vela (The Sails). The dark, wispy dust clouds of the Milky Way streak from middle top left to middle bottom right. (Credit: ESO, B. Tafreshi)
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“Our model predicts different fracture patterns on the surface of Charon depending on the thickness of its surface ice, the structure of the moon’s interior and how easily it deforms, and how its orbit evolved,” said Alyssa Rhoden of NASA’s Goddard Space Flight Center. (Credit: NASA)
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Open network environments have become essential in the sciences, enabling accelerated discovery and communication of knowledge. Yet, the real revolution began when open community databases allowed researchers to build on existing contributions and compare their results to established knowledge. (Credit: King, Uhlir)
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Indian physicists propose a tabletop experiment that will provide scientists their first opportunity to measure the probability that particles can move through slits in a twisted path, depicted by the purple ray. (Credit: Aninda Sinha and Urbasi Sinha)
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Physicists in the US have compressed a synthetic diamond to pressures of 50 million Earth atmospheres to recreate conditions in the cores of giant planets. (Credit: National Ignition Facility)
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. A novel class of electronic materials – the so-called transition-metal oxides – hold promise for exciting, new applications. Where layers of this novel class of electronic materials touch, often a unique, and unprecedented phenomenon occurs: for instance, the interface between two insulators can become superconducting, or a strong magnetic order can build up between two non-magnetic layers.
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Two atoms exchanging a virtual photon. Empty space around them is not as empty as one might think. (Credit: Vienna University of Technology, TU Vienna)
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New particles may yet be discovered, and even new laws. But it is almost taken for granted that everything from physics to biology, including the mind, ultimately comes down to four fundamental concepts: matter and energy interacting in an arena of space and time. (Credit: Carl Wiens)
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Kepler’s Supernova Remnant “On October 9, 1604, sky watchers — including astronomer Johannes Kepler, spotted a “new star” in the western sky, rivaling the brilliance of nearby planets. “Kepler’s supernova” was the last exploding supernova seen in our Milky Way galaxy. (Credit: NASA/ESA/JHU/R.Sankrit & W.Blair)
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A Diffusion Spectrum MRI (DSI) of the human brain obtained with the MGH-UCLA Human ‘Connectom’ Scanner. The fiber tracks are color-coded by direction: red=left-right, green=anterior-posterior, blue=through brain stem. (Credit: National Institutes of Biomedical Imaging and Bioengineering and National Institutes of Health)
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The interior of the target chamber at the National Ignition Facility at Lawrence Livermore National Laboratory. The object entering from the left is the target positioner, on which a millimeter-scale target is mounted. Researchers recently used NIF to study the interior state of giant planets. (Credit: Image by Damien Jemison/LLNL)
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Michael Slezak goes deep under the outback to find a home for the southern hemisphere’s first WIMP detector, which could confirm our best direct signal yet(Credit: Michael Slezak)
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Yes, you will certainly die from radiation poisoning if you are able to eat 10,000,000 bananas at once. You may also witness chronic symptoms if you eat 274 bananas a day for seven years. (Credit: Ping Zhu)
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The colored curves describe different velocity dependencies of the scattering strength; it is scaling as v to the nth power. The horizontal axis, k, is a measure of how separated two points in space might be; larger k corresponds to smaller physical separation. The vertical axis (technically known as a “power spectrum”) describes how correlated two points separated by a scale 1/k are; higher number mean more correlation. The one point with error bars shows that most of the models the authors consider are not very favored by the data. (Credit: C. Dvorkin, K. Blum, and M. Kamionkowski)
via astrobites
After a month surfing in and out of the atmosphere of Venus down to just 130 km from the planet’s surface, ESA’s Venus Express is about to embark on a 15 day climb up to the lofty heights of 460 km. (Credit: ESA – C. Carreau)
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Chao-Lin Kuo, who helped design the BICEP2 experiment, isn’t bothered by criticism that cosmic dust may account for his results. He just wants to know the truth. (Credit: Chao-Lin Kuo)
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This illustration depicts a main membrane out of which individual universes arise; they then expand in size through time. (Credit: Moonrunner Design)
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