Carbon dating magnetic field changes
The photo above is not to make you feel insignificant, it is only for reference and scale. Depending on your field of view, you would have to be around 100,000 light years away to see this Galaxy using the naked human eye.
And as you got closer, it would almost disappear because of the tremendous amount of space there is between everything, like with atoms.
Since 8000 years is almost two half-lives for carbon-14, it's half-life being 5730 years (plus or minus 40 years), we have excellent observational evidence that the decay rate is constant.
We also have laboratory studies which support the constancy of all the decay rates used in radiometric dating.
A great many experiments have been done in attempts to change radioactive decay rates, but these experiments have invariably failed to produce any significant changes.
It has been found, for example, that decay constants are the same at a temperature of 2000 degrees C or at a temperature of 186 degrees C and are the same in a vacuum or under a pressure of several thousand atmospheres.
To unlock their secrets, David Pogue, technology columnist and lively host of NOVA's popular "Making Stuff" series, spins viewers through the world of weird, extreme chemistry: the strongest acids, the deadliest poisons, the universe's most abundant elements, and the rarest of the rare—substances cooked up in atom smashers that flicker into existence for only fractions of a second. Yet everything we know, the stars, the planets and life, itself, comes from about 90 basic building blocks,… …all right here, on this remarkable chart: the periodic table of the elements. And we're made, almost entirely, of just a handful of ingredients, including one that burns with secret fire inside us all. The sample, mixed with a lead oxide powder, goes into a furnace heated to 2,000 degrees. Using extreme heat, gold atoms are gradually coaxed away from the powdered rock. Turns out that an ounce per ton is pretty much optimal for the underground mine. The New York Mercantile Exchange is a vital hub in the global metals market, which is pretty good news for me. (Commodities Trader): Oh, this is an old, old business. It's so important that the rise and fall of copper prices provide a snapshot of the health of the entire world economy. Each atom gives up some of its electrons to create a kind of sea of these randomly moving charged particles.
It's a story that begins with the Big Bang and eventually leads to us. Join me as I explore the basic building blocks of the universe… …to the least—manmade elements that last only fractions of a second; strange metals with repellant powers;… So, after all that pulverizing and crushing and weighing and firing, what we're left with is this? Eighteen hundred dollars times…720,000 bucks a truck! The surface mine produces less, about half an ounce per ton. This goes back to the 1800s, the late 1800s, where farmers were looking, actually, for money to plant their next year's crops. We use it for infrastructure; we use it for electronic goods. When times are bad, copper prices tumble, and when times are good, they soar. It's these free-flowing electrons that make metals conductive.
This video stitches many together to make a flyby video that is breathtakingly beautiful. Here, at the Cortez Mine, in Nevada, high-tech prospectors are moving mountains, closing in from above and below. Which raises a question: if the gold is invisible to the naked eye, how do they even know if they're digging in the right place? Eight bars, million, sitting on this unassuming little table. Of all the elements that touch our lives, nothing drives humankind to acts of love or destruction like gold. Copper alone is impressive stuff, but when ancient metallurgists combined it with another element, they invented a much tougher material that went on to conquer the world. Tin; symbol Sn; atomic number 50—50 protons and 50 electrons.