Thursday 28 January 2016

Monstrous cloud boomerangs back to our galaxy

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New Hubble telescope observations suggest that a high-velocity gas cloud was launched from the outer regions of our own galaxy around 70 million years ago. Now, the cloud is on a return collision course and is expected to plow into the Milky Way's disk in about 30 million years. Astronomers believe it will ignite a spectacular burst of star formation then.
via Science Daily
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Putting silicon 'sawdust' in a graphene cage boosts battery performance

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Scientists have been trying for years to make a practical lithium-ion battery anode out of silicon, which could store 10 times more energy per charge than today's commercial anodes and make high-performance batteries a lot smaller and lighter. But two major problems have stood in the way: Silicon particles swell, crack and shatter during battery charging, and they react with the battery electrolyte to form a coating that saps their performance.
via Science Daily

Signs of Modern Astronomy Seen in Ancient Babylon

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Scientists have found a small clay tablet with markings indicating that a sort of precalculus technique was used to track Jupiter’s motion in the night sky.










via New York Times

Bringing time and space together for universal symmetry

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New research is broadening perspectives on time and space. Scientists challenge the long-held presumption that time evolution -- the incessant unfolding of the universe over time -- is an elemental part of Nature.
via Science Daily
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Monstrous Cloud Boomerangs Back to Our Galaxy


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The old adage "what goes up must come down" even applies to an immense cloud of hydrogen gas outside our Milky Way galaxy. First discovered in the 1960s, the comet-shaped cloud is 11,000 light-years long and 2,500 light-years across. If the cloud could be seen in visible light, it would span the sky with an apparent diameter 30 times greater than the size of the full moon. The cloud, which is invisible at optical wavelengths, is plummeting toward our galaxy at nearly 700,000 miles per hour. Hubble was used to measure the chemical composition of the cloud as a means of assessing where it came from. Hubble astronomers were surprised to find that the cloud, which is largely composed of hydrogen, also has heavier elements that could only come from stars. This means the cloud came from the star-rich disk of our galaxy. The Smith Cloud is following a ballistic trajectory and will plow back into the Milky Way's disk in about 30 million years. When it does, astronomers believe it will ignite a spectacular burst of star formation, perhaps providing enough gas to make 2 million suns.

Please join the scientists in a live discussion about the origin and conclusions of this research during the Hubble Hangout at 3pm EST today (Thurs., Jan. 28, 2016): http://hbbl.us/Baq .


via HubbleSite NewsCenter -- Latest News Releases
http://hubblesite.org/newscenter/archive/releases/2016/04/

Antarctic fungi survive Martian conditions on the International Space Station

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Scientists have gathered tiny fungi that take shelter in Antarctic rocks and sent them to the International Space Station. After 18 months on board in conditions similar to those on Mars, more than 60 percent of their cells remained intact, with stable DNA. The results provide new information for the search for life on the red planet. Lichens from the Sierra de Gredos (Spain) and the Alps (Austria) also traveled into space for the same experiment.
via Science Daily
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Increasing oil's performance with crumpled graphene balls

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Crumpled graphene balls self-disperse in oil to reduce friction and protect engines better than commercial lubricants.
via Science Daily

Elliptical M60, Spiral NGC 4647

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Giant elliptical galaxy M60 and spiral galaxy NGC 4647 do look like an odd couple in this sharp cosmic portrait from the Hubble Space Telescope. But they are found in a region of space where galaxies tend to gather, on the eastern side of the nearby Virgo Galaxy Cluster. About 54 million light-years distant, bright M60's simpler egg-like shape is created by its randomly swarming older stars, while NGC 4647's young blue stars, gas and dust are organized into winding arms rotating in a flattened disk. Spiral NGC 4647 is estimated to be more distant than M60, some 63 million light-years away. Also known as Arp 116, the pair of galaxies may be on the verge of a significant gravitational encounter, though. M60 (aka NGC 4649) is about 120,000 light-years across. The smaller NGC 4647 spans around 90,000 light-years, about the size of our own Milky Way.

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Martian labyrinth

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This block of martian terrain, etched with an intricate pattern of landslides and wind-blown dunes, is a small segment of a vast labyrinth of valleys, fractures and plateaus.


via ESA Space Science
http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Martian_labyrinth