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The most precise measurement ever made of the speed of the universe's expansion is in, thanks to NASA's Spitzer Space Telescope, and it's a doozy. Space itself is pulling apart at the seams, expanding at a rate of 74.3 plus or minus 2.1 kilometers (46.2 plus or minus 1.3 miles) per second per megaparsec (a megaparsec is roughly 3 million light-years).
“Just over a decade ago, using the words ‘precision’ and ‘cosmology’ in the same sentence was not possible, and the size and age of the universe was not known to better than a factor of two,” said Freedman. “Now we are talking about accuracies of a few percent. It is quite extraordinary.”
Originally posted by CLPrime
reply to post by fenceSitter
It's not just related to Hubble's Law...it is the numerical value of Hubble's Law.
And the speeds, themselves, don't actually translate into physical (that is, proper) velocities. They only appear to be traveling that fast relative to us. In reality, it's the space between us that's stretching, causing light from distant objects to become redshifted (velocity and the expansion of space both cause the same sort of redshift).
Originally posted by fenceSitter
reply to post by CLPrime
One day, when someone eventually figures it out, they will look back and laugh about how stupid we were
Originally posted by watchitburn
But I know that's stupid fast. It didn't occur to me that the edge would be traveling faster than the center. I guess I thought everything would be moving at a uniformly accelerating pace.
Originally posted by fenceSitter
One day, when someone eventually figures it out, they will look back and laugh about how stupid we were
Originally posted by ChaoticOrder
Beat me to it.
In physical cosmology and astronomy, dark energy is a hypothetical form of energy that permeates all of space and tends to accelerate the expansion of the universe.[1] Dark energy is the most accepted hypothesis to explain observations since the 1990s that indicate that the universe is expanding at an accelerating rate. In the standard model of cosmology, dark energy currently accounts for 73% of the total mass–energy of the universe.[2]
The simplest explanation for dark energy is that it is simply the "cost of having space": that is, a volume of space has some intrinsic, fundamental energy. This is the cosmological constant, sometimes called Lambda (hence Lambda-CDM model) after the Greek letter Λ, the symbol used to mathematically represent this quantity. Since energy and mass are related by E = mc2, Einstein's theory of general relativity predicts that this energy will have a gravitational effect. It is sometimes called a vacuum energy because it is the energy density of empty vacuum. In fact, most theories of particle physics predict vacuum fluctuations that would give the vacuum this sort of energy.
Dark Energy - Wikipedia
Vacuum energy is an underlying background energy that exists in space throughout the entire Universe. Since there is so much space, this background energy is currently estimated to make up about 73% of the total mass-energy content of the Universe. (Dark matter apparently makes up 23%, with all the atoms we know about coming in at 4%.) Current theory has it that the vacuum energy of "empty" space not only contributes to the mass-energy content, it carries the added quality of negative pressure, which provides a mechanism for the expansion to be accelerating.
Special relativity predicts that energy is equivalent to mass, and therefore, if the vacuum energy is "really there", it should exert a gravitational force. Essentially, a non-zero vacuum energy is expected to contribute to the cosmological constant, which affects the expansion of the universe. In the special case of vacuum energy, general relativity stipulates that the gravitational field is proportional to ρ-3p (where ρ is the mass-energy density, and p is the pressure). Quantum theory of the vacuum further stipulates that the pressure of the zero-state vacuum energy is always negative and equal to ρ. Thus, the total of ρ-3p becomes -2ρ: A negative value. This calculation implies a repulsive gravitational field, giving rise to expansion, if indeed the vacuum ground state has non-zero energy.
Vacuum Energy - Wikipedia
Originally posted by CLPrime
reply to post by nightbringr
That's essentially right, except it is the radius of the universe that we view expanding from the apparent center, not half the radius. We view 13.7 billion light-years expanding in every direction.
Originally posted by CLPrime
It's also misleading to say "edge" or "center". Galaxies at what we see as the "edge" see exactly the same sort of stuff that we see, and, to them, we appear to be at the edge while they appear to be at the center. It's all a matter of perspective.
Originally posted by ChaoticOrder
reply to post by nightbringr
I believe what CLPrime meant was "the edge of the observable Universe".
Originally posted by nightbringr
No. If the radius is 15 billion light years, and we are in the middle looking towards the "edge", we only are viewing half of the 15 billions, thus 7.5 billion.
Originally posted by CLPrime
Perhaps you can explain this more? This would only work in the "wrap around universe" theory. Since we are discussion the "expansion" theory, this is i believe incorrect. The would be a distinct "edge". After all, the galaxy closest to the edge would see nothing looking towards the edge, however would view 15 billions light years of universe looking towards the center.
Originally posted by CLPrime
I see your "No" and raise you a Nay-Nay. You're getting the radius and diameter confused. Radius is half the diameter, and it's the radial distance that we see in every direction.
Originally posted by CLPrime
Since the universe appears to be flat (not spherical or hyperbolic), it would be reasonable to assume that the universe is infinite.
Reasonable perhaps, but if we are discussing the "expanding universe" theory, is there not an edge?
Originally posted by nightbringr
Reasonable perhaps, but if we are discussing the "expanding universe" theory, is there not an edge?