nPeace
Veteran Member
I'll just watch the debate, as it progresses over the years to come... that is, as long as I live.Yes, the expansion rate would be changed, clearly. The cooling time of the BB not so much, and by definition, the time of the BB. The formation of the solar system not so much.
There are several different methods for determining the age of the universe.
The most direct method is using the expansion rate and our models of gravity to 'work backwards'. This method is subject to a lot of measurement errors: first of all there are 'peculiar motions' of galaxies caused by their gravitational interaction in clusters. These peculiar motions are on the other of a couple hundred kilometers per second and are a significant effect for galaxies close to us.
The other problem with this direct method is that we have to get good estimates of the distances of galaxies. This has traditionally been done by looking for stars called Cephiad variables, which have the property that their brightness and the time for a cycle are correlated. Knowing their brightness and how bright they look in the sky will give their distance.
In any case, this direct method was the main one used until fairly recently (because it was the only one we had data for). When I was young, the range of possible ages consistent with this was 'between 10 and 20 billion years'. Toward the end of the last century, the age estimates had improved to 'between 11 and 15 billion years'.
The real breakthrough in precision cosmology came when we used satellites to measure the cosmic background radiation. The details in the fluctuation of that background give a lot of information about the early universe. it is because of the data from COBE and WMAP that we now have the 13.8 billion year estimate (actually, 13.77 with a possible error of .4%).
For lower estimates of the age of the universe, we look at very old stars (usually white dwarfs) and try to figure out their ages using models of how stars change over time. We know of stars over 10 billion years old. So that is the youngest the universe can be.
Of these, the data from the background radiation are the most likely to be accurate. There are just too many ways the other methods can go wrong.
In particular, the article in the OP used the traditional, expansion method. That method still has *huge* error bars compared to using the CBR. That is where the 2 billion year age difference came from. But, as has been pointed out, the results are still consistent with the CBR data (because of the size of the error bars on the expansion method).
Perhaps some day it will be settled permanently... or perhaps not.
I can't figure out what's the big deal.
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