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01-29-2017, 12:43 PM | #2581 | |
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But I've been reading about this stuff lately. Really interesting. Quantum mechanics are a Hella hard undsrstanding. |
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01-29-2017, 03:27 PM | #2582 |
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Son of a bitch. Some of these black holes are scaringly huge.
https://www.youtube.com/watch?v=QgND...ature=youtu.be |
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01-29-2017, 03:33 PM | #2583 | |
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I have a Trex deck that is about 11 years old. It will go away next year. Good luck with yours. We also were of the no maintenance opinion when we built it. Its a three level deck and beautiful from a distance. The first thing we learned is that they grow mildew like crazy, The slightly rough surface is ideal for things like pollen to adhere to and that feeds the mildew. So unless its changed a lot, be prepared to use a brush and a clorox/TSP mis at least once a year.
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01-30-2017, 05:16 PM | #2584 |
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Yea, the small portion that is besides our maple tree gets a bit of "moss". I think it makes it look rustic. I If the wife doesn't like it, I power wash with a fan blade. I did that 4 yrs ago. The rest 7/8ths is fine. Plenty of sunshine. Looks like new.
I didn't use a "system". I used them like boards and screwed them in with a nail space in between. It has been up for 15 yrs. I nailed up under neath the tin metal sheets of roofing colored white. So under the deck is dry. I love sitting out under the deck with thunder storms. |
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02-04-2017, 12:07 AM | #2585 |
Ain't no relax!
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02-04-2017, 12:09 AM | #2586 |
Ain't no relax!
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Why it feels like you're spinning when you go to bed drunk..
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02-04-2017, 12:09 AM | #2587 |
Ain't no relax!
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02-04-2017, 12:13 AM | #2588 |
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Go K-State! This could be a pretty big deal down the road...
Physicists patent detonation technique to mass-produce graphene MANHATTAN Forget chemicals, catalysts and expensive machinery a Kansas State University team of physicists has discovered a way to mass-produce graphene with three ingredients: hydrocarbon gas, oxygen and a spark plug. Their method is simple: Fill a chamber with acetylene or ethylene gas and oxygen. Use a vehicle spark plug to create a contained detonation. Collect the graphene that forms afterward. Chris Sorensen, Cortelyou-Rust university distinguished professor of physics, is the lead inventor of the recently issued patent, "Process for high-yield production of graphene via detonation of carbon-containing material." Other Kansas State University researchers involved include Arjun Nepal, postdoctoral researcher and instructor of physics, and Gajendra Prasad Singh, former visiting scientist. "We have discovered a viable process to make graphene," Sorensen said. "Our process has many positive properties, from the economic feasibility, the possibility for large-scale production and the lack of nasty chemicals. What might be the best property of all is that the energy required to make a gram of graphene through our process is much less than other processes because all it takes is a single spark." Graphene is a single atom-thick sheet of hexagonally coordinated carbon atoms, which makes it the world's thinnest material. Since graphene was isolated in 2004, scientists have found it has valuable physical and electronic properties with many possible applications, such as more efficient rechargeable batteries or better electronics. For Sorensen's research team, the serendipitous path to creating graphene started when they were developing and patenting carbon soot aerosol gels. They created the gels by filling a 17-liter aluminum chamber with acetylene gas and oxygen. Using a spark plug, they created a detonation in the chamber. The soot from the detonation formed aerosol gels that looked like "black angel food cake," Sorensen said. But after further analysis, the researchers found that the aerosol gel was more than lookalike dark angel food cake it was graphene. "We made graphene by serendipity," Sorensen said. "We didn't plan on making graphene. We planned on making the aerosol gel and we got lucky." But unlike other methods of creating graphene, Sorensen's method is simple, efficient, low-cost and scalable for industry. Other methods of creating graphene involve "cooking" the mineral graphite with chemicals such as sulfuric acid, sodium nitrate, potassium permanganate or hydrazine for a long time at precisely prescribed temperatures. Additional methods involve heating hydrocarbons to 1,000 degrees Celsius in the presence of catalysts. Such methods are energy intensive and even dangerous and have low yield, while Sorensen and his team's method makes larger quantities with minimal energy and no dangerous chemicals. "The real charm of our experiment is that we can produce graphene in the quantity of grams rather than milligrams," Nepal said. Now the research team including Justin Wright, doctoral student in physics, Camp Hill, Pennsylvania is working to improve the quality of the graphene and scale the laboratory process to an industrial level. They are upgrading some of the equipment to make it easier to get graphene from the chamber seconds rather than minutes after the detonation. Accessing the graphene more quickly could improve the quality of the material, Sorensen said. The patent was issued to the Kansas State University Research Foundation, a nonprofit corporation responsible for managing technology transfer activities at the university.
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02-04-2017, 12:15 AM | #2589 |
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Blazars!
NASA's Fermi Discovers the Most Extreme Blazars Yet NASA's Fermi Gamma-ray Space Telescope has identified the farthest gamma-ray blazars, a type of galaxy whose intense emissions are powered by supersized black holes. Light from the most distant object began its journey to us when the universe was 1.4 billion years old, or nearly 10 percent of its present age. "Despite their youth, these far-flung blazars host some of the most massive black holes known," said Roopesh Ojha, an astronomer at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "That they developed so early in cosmic history challenges current ideas of how supermassive black holes form and grow, and we want to find more of these objects to help us better understand the process." Ojha presented the findings Monday, Jan. 30, at the American Physical Society meeting in Washington, and a paper describing the results has been submitted to The Astrophysical Journal Letters. Blazars constitute roughly half of the gamma-ray sources detected by Fermi's Large Area Telescope (LAT). Astronomers think their high-energy emissions are powered by matter heated and torn apart as it falls from a storage, or accretion, disk toward a supermassive black hole with a million or more times the sun's mass. A small part of this infalling material becomes redirected into a pair of particle jets, which blast outward in opposite directions at nearly the speed of light. Blazars appear bright in all forms of light, including gamma rays, the highest-energy light, when one of the jets happens to point almost directly toward us. Previously, the most distant blazars detected by Fermi emitted their light when the universe was about 2.1 billion years old. Earlier observations showed that the most distant blazars produce most of their light at energies right in between the range detected by the LAT and current X-ray satellites, which made finding them extremely difficult. Then, in 2015, the Fermi team released a full reprocessing of all LAT data, called Pass 8, that ushered in so many improvements astronomers said it was like having a brand new instrument. The LAT's boosted sensitivity at lower energies increased the chances of discovering more far-off blazars. The research team was led by Vaidehi Paliya and Marco Ajello at Clemson University in South Carolina and included Dario Gasparrini at the Italian Space Agency's Science Data Center in Rome as well as Ojha. They began by searching for the most distant sources in a catalog of 1.4 million quasars, a galaxy class closely related to blazars. Because only the brightest sources can be detected at great cosmic distances, they then eliminated all but the brightest objects at radio wavelengths from the list. With a final sample of about 1,100 objects, the scientists then examined LAT data for all of them, resulting in the detection of five new gamma-ray blazars. Expressed in terms of redshift, astronomers' preferred measure of the deep cosmos, the new blazars range from redshift 3.3 to 4.31, which means the light we now detect from them started on its way when the universe was between 1.9 and 1.4 billion years old, respectively. "Once we found these sources, we collected all the available multiwavelength data on them and derived properties like the black hole mass, the accretion disk luminosity, and the jet power," said Paliya. Two of the blazars boast black holes of a billion solar masses or more. All of the objects possess extremely luminous accretion disks that emit more than two trillion times the energy output of our sun. This means matter is continuously falling inward, corralled into a disk and heated before making the final plunge to the black hole. "The main question now is how these huge black holes could have formed in such a young universe," said Gasparrini. "We don't know what mechanisms triggered their rapid development." In the meantime, the team plans to continue a deep search for additional examples. "We think Fermi has detected just the tip of the iceberg, the first examples of a galaxy population that previously has not been detected in gamma rays," said Ajello. NASA's Fermi Gamma-ray Space Telescope is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy and with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden and the United States. For more information on Fermi, visit: https://www.nasa.gov/fermi
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02-07-2017, 10:00 AM | #2590 |
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Hubble takes a pic of the death of a star
Death of a star The Calabash Nebula, pictured here which has the technical name OH 231.8+04.2 is a spectacular example of the death of a low-mass star like the sun. This image taken by the NASA/ESA Hubble Space Telescope shows the star going through a rapid transformation from a red giant to a planetary nebula, during which it blows its outer layers of gas and dust out into the surrounding space. The recently ejected material is spat out in opposite directions with immense speed the gas shown in yellow is moving close to one million kilometers per hour (621,371 miles per hour). Astronomers rarely capture a star in this phase of its evolution because it occurs within the blink of an eye in astronomical terms. Over the next thousand years the nebula is expected to evolve into a fully-fledged planetary nebula. The nebula is also known as the Rotten Egg Nebula because it contains a lot of sulphur, an element that, when combined with other elements, smells like a rotten egg but luckily, it resides over 5,000 light-years away in the constellation of Puppis. |
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02-07-2017, 10:20 AM | #2591 |
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02-12-2017, 09:52 AM | #2592 |
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Discover reports scientists in Spain have figured out they can use ultrasound to create brandy that tastes like it's been aged for years in just three days.
http://www.newser.com/story/238178/n...urce=hedgrid_8
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02-12-2017, 11:01 AM | #2593 |
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I love this thread! Great posts everyone.
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02-12-2017, 12:20 PM | #2594 | |
Now you've pissed me off!
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"When the Know-Nothings get control, it will read 'all men are created equal, except negroes, and foreigners, and Catholics.' When it comes to this I should prefer emigrating to some country where they make no pretense of loving liberty to Russia, for instance, where despotism can be taken pure, and without the base alloy of hypocrisy.--Abraham Lincoln |
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02-12-2017, 08:20 PM | #2595 |
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