MathJakob said:
Why is Hubble's constant called a constant if it isn't constant?
As of 20 December 2012 the Hubble constant, as measured by NASA's Wilkinson Microwave Anisotropy Probe (WMAP) and reported in arxiv, is 69.32 ± 0.80 (km/s)/Mpc (or 21.25 ± 0.25 (km/s)/Mega-lightyear). [
Reference]
As of 21 March 2013, the Hubble constant, as measured by the Planck Mission, is 67.80 ± 0.77 (km/s)/Mpc. [
Reference]
It's the same number calculated from different sets of data. The actual Hubble expansion rate changes very very slowly. You would not notice a change over 100 years, it would be too small to measure even with much more advanced instruments.
I would encourage people to also know the Hubble rate as a PERCENTAGE rate of distance expansion per million years.
The Planck report figure of 67.8 km/s per Mpc corresponds to about 1/144 % growth per million years.
Everbody should know how to get this using google calculator: just type or paste this into the google window 67.8 km/s per Mpc in percent per million years
the google calculator can convert from one type of unit to another when you say IN. It can tell you x yards in feet or y yards in meters. you just paste that blue thing into the ordinary window that you use for searches, and press return to show you are done.
then it will say "0.00693384038 percent per (million years)"
and if you paste 1/0.00693384038 into the window it will say 144.220222...
So what it is really telling you is that the Planck figure of Hubble growth rate is actually
1/144 percent per million years.
The growth rate is declining very very slowly towards an estimated longterm level of 1/173 percent.
You can see that slow change reflected in the output of Jorrie's calculator, which is the "LightCone" link in my sig. Click on it for a condensed account of the past history and future of cosmic expansion. There are blue popup info buttons that explain stuff.
If you do that you should be able to spot the 1/144 I'm talking about in the row of the present (age 13.8 billion) and the 1/173 I mentioned in the row of a distant future (age 92 billion)
You will see the disguised as distances, e.g. 14.4 and 17.3, in the R column which gives the Hubble radius, a kind of "reciprocal" of the expansion rate. Try the blue dots if you need more explained.
That's how slow the Hubble rate is changing, you can see it in the table. so it's virtually constant in the short run.