http://www.scientificamerican.com/media/multimedia/periodic_table/periodic.html
Until the 1800s, when the technology was developed to separate it from rock, it was more expensive than gold; Napoleon III allegedly hosted a banquet in which the guests of honor ate on aluminum plates. Discovered in the 1960s, element 105 was officially named dubnium in 1996 when the International Union of Pure and Applied Chemistry (IUPAC) settled a bitter, decades-long dispute between teams of scientists at Dubna and at Lawrence Berkeley
http://www.pbs.org/wgbh/nova/physics/legacy-of-e-equals-mc2.html
Today we know radioactivity to be a property possessed by some unstable elements, such as uranium, or isotopes, such as carbon 14, of spontaneously emitting energetic particles as their atomic nuclei disintegrate. "Whenever you use a radioactive substance to illuminate processes in the human body, you're paying direct homage to Einstein's insight," says Sylvester James Gates, a physicist at the University of Maryland
http://www.physicscentral.com/explore/poster-stardust.cfm
But where did these little ingredients come from? And how were they made? The answer to these questions will take us back to a time long ago when the universe was much different than it is now. Now that we have established that every element in the periodic table aside from hydrogen is essentially stardust, we have to determine how much of our body is made up of this stardust
http://www.exploratorium.edu/origins/cern/ideas/bang.html
So how does this prove anything about the Big Bang? Scientists have shown, using theoretical calculations, that these abundances could only have been made in a universe that began in a very hot, dense state, and then quickly cooled and expanded. A Cooling, Expanding Universe photo: Space Telescope Science Institute As the early universe cooled, the matter produced in the Big Bang gathered into stars and galaxies
http://www.damninteresting.com/absolute-zero-is-0k/
About a billion years later all that hydrogen began to coalesce into stars pumping out the heavier elements that make up everything we are observing thirteen billion years later. Water seeps from these moistened acres and coalesces into the headwaters of a river which meanders through the countryside for nearly 22 miles until its terminus in Glasgow
http://www.pbs.org/wgbh/nova/physics/hunting-elements.html
DAVID POGUE: The military made only one uranium bomb, because separating rare U-235 from the more common U-238, which doesn't work in fission reactions, is a very difficult process. Dude, you just caught a shark with your bare hands! Then, flip the shark upside down, which induces a trance state called "tonic immobility." Once the shark is calm, we test its reaction to a piece of ordinary, non-magnetic lead
http://disease13.imascientist.org.au/2013/03/14/why-is-gold-under-the-ground-how-was-it-made-where-did-it-come-from/
Many big alluvial nuggets contain lumps of quartz, or show imprints of quartz crystals enclosed by the gold as it crystallised in cavities in the reefs. However, it has something to do with conditions in the surrounding rocks changing the solubility of gold in the warm water that had dissolved it in huge amounts and carried it up from deep in the crust
Helium, Chemical Element - Overview, Discovery and naming, Physical properties, Chemical properties, Occurrence in nature, Isotopes
http://www.chemistryexplained.com/elements/C-K/Helium.html
KEEP IT UP!3EDFDec 4, 2008 @ 7:19 pmWOW! That was an AMAZING article! It really helped me with my research for an essay! THANKS TO THE CREATOR!4EDFDec 18, 2008 @ 5:17 pmthat artical got me a WONDERFUL grade on my essay. helium comes from five large underground regions: the Hugoton Field that lies beneath Kansas, Oklahoma, and Texas; the Keyes Field in Oklahoma; the Panhandle and Cliffside Fields in Texas; and the Ridley Ridge area in Wyoming
http://www.nap.edu/openbook.php?record_id=13165&page=173
Only in the relatively recent past have people begun to recognize the dramatic role humans play as an essentially geological force on the surface of Earth, affecting large-scale conditions and processes. ESS1.A: THE UNIVERSE AND ITS STARS What is the universe, and what goes on in stars? The sun is but one of a vast number of stars in the Milky Way galaxy, which is one of a vast number of galaxies in the universe
Why Didn't The Big Bang Produce Heavy Elements? - Naked Science Forum
http://www.thenakedscientists.com/forum/index.php?topic=39430.0
As they die they run out of hydrogen fuel and start to fuse together heavier and heavier elements, with some really big stars in their death throes going super-nova exploding and throwing those elements far and wide. Information presented on this website is the opinion of the individual contributors and does not reflect the general views of the administrators, editors, moderators, sponsors, Cambridge University or the public at large
http://www.einstein-online.info/spotlights/BBN_obs
By systematic analysis of the light received from those outermost layers (more concretely, of the different emission and absorption lines), astronomers can determine the abundances of the layer's constituent elements. These are elements with nuclei that are produced by nuclear fusion reactions in stars, but that definitely could not have been produced during Big Bang Nucleosynthesis
http://startswithabang.com/?p=1762
But you also make a lot of heavier elements, like Carbon, Oxygen, and Nitrogen, and sometimes Silicon, Neon, and sometimes even Iron, Cobalt, and Nickel. Fortunately that people who sadly are overweight and also suffering from various diseases can help to eliminate the severity of the illnesses by simply losing weight
http://m.teachastronomy.com/astropedia/article/The-Creation-of-Heavy-Elements
Stellar iron is actually denser than terrestrial iron, but the electrons have been stripped from all the atoms and the nuclei are not held together in a lattice. Those of around 8 solar masses will have hot enough cores to further ignite the carbon and fuse it into heavier elements such as oxygen, neon, and magnesium
Case Study: The Natural Abundance of Elements - Chemwiki
http://chemwiki.ucdavis.edu/Inorganic_Chemistry/Case_Studies/Case_Study%3A_The_Natural_Abundance_of_Elements
Indeed, this process called the solar nebula theory has validity because we are able to see distantly forming solar systems with a dim central protostar surrounded by gas. Sign In Forgot Password Register username password If you like us, please share us on social media, tell your friends, tell your professor or consider building or adopting a Wikitext for your course
http://scienceblogs.com/startswithabang/2012/12/12/why-the-world-will-run-out-of-helium/
assuming we get fusion reactors working within the next decade or so we will be converting mass amounts of hydrogen into helium, every country every continent. It would be released to the atmosphere when the natural gas is burnt.So, not filling a balloon with helium would not slow down (or speed up) the depletion of helium from the underground reservoirs
http://www.wired.com/2011/05/where-does-the-carbon-come-from/
This excited state of the carbon-12 nucleus was postulated by Hoyle as a necessary ingredient for the fusion of three alpha particles to produce carbon at stellar temperatures. In this letter we report the first ab initio calculation of the low-lying states of carbon-12 using supercomputer lattice simulations and a theoretical framework known as effective field theory
physical chemistry - Where did all the elements come from? - Chemistry Stack Exchange
http://chemistry.stackexchange.com/questions/26479/where-did-all-the-elements-come-from
Big Bang According to the prevailing cosmological model for the early development of the Universe, known as the Big Bang theory, the Universe begun at about 14 billion years from a singularity that can be thought of a state of an infinite density and temperature, and since its creation the Universe began to expand and cool. Stellar nucleosynthesis But the gravitational attraction of the nearby matter by slightly denser regions and the subsequent growth of such regions resulted in formation of gas clouds, stars, galaxies, and other large structures
http://scienceblogs.com/startswithabang/2013/07/05/why-did-the-universe-start-off-with-hydrogen-helium-and-not-much-else/
It was once so hot that the Universe was filled with nearly equal amount of matter and antimatter: protons and antiprotons, neutrons and antineutrons, electrons and positrons, neutrinos and antineutrinos, and of course photons (which are their own antiparticle), among others. The brain just fills in a bunch of details because it decided that event took much longer than it really did, and therefore you should have been able to see a lot more than you normally would
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