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Imax said:OK, maybe I’m a fuzz brain (i.e full of dark matter), but I don’t understand why differences in photometric (i.e. brightness) and spectroscopic (i.e. red shift) measurements of type 1a supernovae imply an acceleration in the expansion of the Universe.
1a supernovae all put out the same amount of light. By measuring their brightness we can tell how far away they are. Red-shift tells us how fast they are receding. So if we plot brightness against red-shift we are plotting distance against recession. Also, since light travels at a set finite speed, we are looking at them as they were and not as they are. The further the supernova, the further in the past we are looking. It's like taking snapshots of the universe at different points of time.
If the universe were expanding at a constant speed, we would expect to see a one to one match of distance and recession. Double the distance and double the recession speed.
But we don't see this, instead, we see a pattern that indicates that, in the past, the universe did not expand as fast as it does now.
The initial study expected to find the opposite. They expected that the universe would slow its expansion over time due to gravitational attraction. What they were trying to determine if it was slowing fast enough to ever stop the expansion and cause the Universe to collapse back on itself. The results they got surprised them.