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4854 |
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Date: March 19, 2014 at 05:57:06
From: Akira, [DNS_Address]
Subject: accelerating expansion of space..corollary for time? |
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I'm wondering if space is expanding at an ever accelerated rate, is there a corollary for time or our perception of time? Since the expansion of space theoretically can/does exceed the speed of light, does this change the relationship of space and time?
Does anyone know of any scientific data or investigation?
Time is on my mind.
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4864 |
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Date: March 28, 2014 at 12:07:01
From: marc / berkeley, [DNS_Address]
Subject: Re: accelerating expansion of space..corollary for time? |
URL: Time/Expansion of Universe? Read more: http://www.physicsforums.com |
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Hubble's law is the name for the observation in physical cosmology that: (1) objects observed in deep space (extragalactic space, ~10 megaparsecs or more) are found to have a Doppler shift interpretable as relative velocity away from the Earth; and (2) that this Doppler-shift-measured velocity, of various galaxies receding from the Earth, is approximately proportional to their distance from the Earth for galaxies up to a few hundred megaparsecs away. This is normally interpreted as a direct, physical observation of the expansion of the spatial volume of the observable universe.
The motion of astronomical objects due solely to this expansion is known as the Hubble flow. Hubble's law is considered the first observational basis for the expanding space paradigm and today serves as one of the pieces of evidence most often cited in support of the Big Bang model.
Although widely attributed to Edwin Hubble, the law was first derived from the General Relativity equations by Georges Lemaître in a 1927 article where he proposed that the Universe is expanding and suggested an estimated value of the rate of expansion, now called the Hubble constant. Two years later Edwin Hubble confirmed the existence of that law and determined a more accurate value for the constant that now bears his name. The recession velocity of the objects was inferred from their redshifts, many measured earlier by Vesto Slipher (1917) and related to velocity by him.
The law is often expressed by the equation v = HoD, with Ho the constant of proportionality (the Hubble constant) between the "proper distance" D to a galaxy (which can change over time, unlike the comoving distance) and its velocity v (i.e. the derivative of proper distance with respect to cosmological time coordinate; see Uses of the proper distance for some discussion of the subtleties of this definition of 'velocity'). The SI unit of H0 is s−1 but it is most frequently quoted in (km/s)/Mpc, thus giving the speed in km/s of a galaxy 1 megaparsec (3.09×1019 km) away. The reciprocal of Ho is the Hubble time.
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