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| | #73 (permalink) |
| Science Boy ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | The Big Bang The Big Bang is the cosmological model of the universe that is best supported by all lines of scientific evidence and observation. The essential idea is that the universe has expanded from a primordial hot and dense initial condition at some finite time in the past and continues to expand to this day. Georges Lemaître proposed what became known as the Big Bang theory of the origin of the Universe, although he called it his 'hypothesis of the primeval atom'. The framework for the model relies on Albert Einstein's General Relativity as formulated by Alexander Friedmann. After Edwin Hubble discovered in 1929 that the distances to far away galaxies were generally proportional to their redshifts, this observation was taken to indicate that all very distant galaxies and clusters have an apparent velocity directly away from our vantage point. The farther away, the higher the apparent velocity. If the distance between galaxy clusters is increasing today, everything must have been closer together in the past. This idea has been considered in detail back in time to extreme densities and temperatures, and large particle accelerators have been built to experiment on and test such conditions, resulting in significant confirmation of the theory. But these accelerators can only probe so far into such high energy regimes. Without any evidence associated with the earliest instant of the expansion, the Big Bang theory cannot and does not provide any explanation for such an initial condition. The theory accurately explains the general evolution of the universe since that instant. A major success of the theory is its ability to account for the comparative abundance of the elements we find around us, which if you look beyond Earth is mostly hydrogen and helium. The observed abundances of the light elements throughout the cosmos closely match the calculated predictions for the formation of these elements from nuclear processes in the rapidly expanding and cooling first minutes of the universe, as logically and quantitatively detailed according to Big Bang nucleosynthesis and well described in Steven Weinberg's classic The First Three Minutes. The term 'Big Bang' was apparently first coined by Fred Hoyle in a derisory statement seeking to belittle the credibility of the theory that he did not believe to be true. Ironically, Hoyle helped considerably in the effort to figure out the nuclear pathway for building certain heavier elements from lighter ones. At any rate, after the discovery of the cosmic microwave background in 1964, and especially when its collective frequencies sketched out a blackbody curve, most scientists were fairly convinced by the evidence that some Big Bang scenario must have occurred. ![]() According to the Big Bang model, the universe expanded from an extremely dense and hot state and continues to expand today. A common and useful analogy explains that space itself is expanding, carrying galaxies with it, like raisins in a rising loaf of bread. General relativistic cosmologies, however, do not actually ascribe any 'physicality' to space. For more Information, see Wikipedia Hubble Deep Field Last edited by MSFixR : 07-21-2008 at 02:20 PM. Reason: Added Video |
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| | #75 (permalink) | |
| Science Boy ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | Quote:
The consensus right now is that the expansion of the universe will continue to slow down but not stop, ie., no big crunch. Eventually, billions and billions of year from now, each gravitationally bound galaxy will be isolated from each other and entropy will increase to the point where no organized form of energy could be extracted from it. This scenario is known as heat death. The universe is not expanding into anything. This is a frequent misconception. Space itself is expanding carrying all matter, light and dark, and all energy with it. Think of the balloon analogy. Nothing outside of the balloon exists but as the balloon fills with gas it expands. If we make marks on the balloon which represent galaxies, the galaxies move further and further apart as the balloon expands. Actually this is an imperfect analogy since the marks will grow larger as the balloon inflates. Gravitationally bound objects such as galaxies do not grow larger as space expands, it is the distance between them that is increasing. | |
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| | #78 (permalink) |
| Science Boy ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | This "Heat Death" means that there would be no thermodynamic free energy left to support any type of motion. No motion = no collisions of atomic particles = no radiation of any kind - heat, light, etc. Everything would be stone-cold dead. Entropy would be maximized. See Heat Death Last edited by MSFixR : 07-23-2008 at 02:15 PM. |
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Seriously, thanks for this MSFixR. Do you think there's a possibility of a 'Big Crunch'? Or will the universe just keep on expanding? Also how do we know what we're expanding into, looks like?