That is a tough question because the universe is expanding. I do not know the value, however, we can certainly estimate it. Assume that the universe expands linearly with time (i.e., R[sub]Universe[/sub]=ct). From here, we can see that:
- 50 years = 1.58x10[sup]9[/sup] seconds
- using c=2.9979x10[sup]10[/sup] cm/s, then R[sub]50 years[/sub] = 4.76x10[sup]19[/sup] cm
- using V=4piR[sup]3[/sup]/3, then V[sub]50 years[/sub]=4.52x10[sup]59[/sup] cm[sup]3[/sup]
That is a pretty big number! However, we really need to compare this value to the linearly-interpolated volume of the universe.
- 13.7 billion years = 4.32x10[sup]17[/sup] s
- R[sub]Universe[/sub]=ct=1.30x10[sup]28[/sup] cm
- V[sub]Universe[/sub]=4piR[sup]3[/sup]/3=2.90x10[sup]84[/sup] cm[sup]3[/sup]
This is an even bigger number! The difference of 50 years seems like a lot, but compared to the entire universe, it is rather insignificant!
Also: the expansion rate was determined via observations and is independent of the existence/non-existence of dark matter and/or dark energy.