Vincent van Gogh
Three years ago, researchers fired whisky to the International Space Station as part of an experiment to see how the conditions in space change flavours. Next month, the whisky will return to Earth.http://www.sciencealert.com.au/news/20143108-26097-2.html
Spiral Galaxy NGC 3344
NGC 3344 is a glorious spiral galaxy around half the size of the Milky Way, which lies 25 million light-years distant. We are fortunate enough to see NGC 3344 face-on, allowing us to study its structure in detail.
The galaxy features an outer ring swirling around an inner ring with a subtle bar structure in the centre. The central regions of the galaxy are predominately populated by young stars, with the galactic fringes also featuring areas of active star formation.
Central bars are found in around two thirds of spiral galaxies. NGC 3344’s is clearly visible here, although it is not as dramatic as some (see for example heic1202).
Multnomah Falls, Oregon, USA by realronsummers
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Few things are capable of making a grown man scream in agony…a shotgun blast to the chest perhaps, a hammer that falls off of a high floor roof and hits you in the head, or an unlucky crossing of paths between yourself and the plastic death trap called a, “Lego”. It’s been a while since I’ve felt that pain, but it was worth it(sometimes). I kinda miss building random shit that pretty much made no sense. It looked cool though, that’s all that mattered back then!!
For the North Atlantic...Caribbean Sea and the Gulf of Mexico: 1. Satellite and surface data indicate that a broad area of low pressure has formed in association with a tropical wave moving across the Yucatan Peninsula. The low is forecast to move over the waters of the eastern Bay of Campeche early Monday, where environmental conditions are expected to be conducive for development. This system has the potential to become a tropical depression while it moves west-northwestward at about 10 mph across the southwestern Gulf of Mexico during the next two to three days. * Formation chance through 48 hours...medium...50 percent. * Formation chance through 5 days...high...60 percent.
Human trials of the surprisingly simple vaccine are now planned. If successful, it could be taken as a probiotic-like drink. via Science Alert/fb
A hoverbike currently being developed by British engineering company Malloy Aeronautics would bring drone technology to new heights.
The company is testing unmanned flights of the hoverbike, which, they say, will be able to reach an altitude of 9,000 feet when completed. Once they achieve aviation certifications for the unmanned model, they will be able to develop a manned prototype.
When finished, the quadcopter could be piloted by a person sitting on the bike or by remote control.
Videos of the test flights show just how high this bike can go. The drone used in the test is one-third the size the hoverbike will ultimately be.http://www.businessinsider.com.au/hoverbike-is-like-a-flying-motorcycle-2014-8
This new NASA/ESA Hubble Space Telescope image shows a variety of intriguing cosmic phenomena.
Surrounded by bright stars, towards the upper middle of the frame we see a small, young stellar object (YSO) known as SSTC2D J033038.2+303212. Located in the constellation of Perseus, this star is in the early stages of its life and is still forming into a fully grown star. In this view from Hubble’s Advanced Camera for Surveys (ACS) it appears to have a murky chimney of material emanating outwards and downwards, framed by bright bursts of gas flowing from the star itself. This fledgling star is actually surrounded by a bright disc of material swirling around it as it forms — a disc that we see edge-on from our perspective.
However, this small bright speck is dwarfed by its cosmic neighbour towards the bottom of the frame, a clump of bright, wispy gas swirling around as it appears to spew dark material out into space. The bright cloud is a reflection nebula known as [B77] 63, a cloud of interstellar gas that is reflecting light from the stars embedded within it. There are actually a number of bright stars within [B77] 63, most notably the emission-line star LkHA 326, and its very near neighbour LZK 18.
These stars are lighting up the surrounding gas and sculpting it into the wispy shape seen in this image. However, the most dramatic part of the image seems to be a dark stream of smoke piling outwards from [B77] 63 and its stars — a dark nebula called Dobashi 4173. Dark nebulae are incredibly dense clouds of pitch-dark material that obscure the patches of sky behind them, seemingly creating great rips and eerily empty chunks of sky. The stars speckled on top of this extreme blackness actually lie between us and Dobashi 4173.