How did scientists figure out the expansion is accelerating?

In summary, the discovery of the acceleration of the universe's expansion was made by observing distant Type 1a supernovae. To calculate the Hubble constant, scientists plotted distances derived from angular size and brightness against recession velocities, resulting in a non-linear graph. This unexpected shape showed decelerating expansion until a few billion years ago, followed by accelerating expansion, indicating an extra inflection point. Other evidence also supports the theory of accelerating expansion.
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resurgance2001
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I understand that the acceleration of the universe's expansion was discovered by looking at very far away Type 1a supernovae. My question is how was the data used exactly to calculate the Hubble constant in the past and then compare it with today's value? Did they simple plot the distances against recession velocities in the normal way but obtain a graph that was not a straight line? Thanks
 
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resurgance2001 said:
Did they simple plot the distances against recession velocities in the normal way but obtain a graph that was not a straight line?

More precisely, they plotted distances derived from two indirect measurements, angular size and brightness, against recession velocities and obtained a graph that was not a straight line. That in itself was not surprising; the graph would not be expected to be a straight line. But the particular shape of the curve indicated decelerating expansion until a few billion years ago, then accelerating expansion--in other words, it had an extra inflection point in it that wasn't expected.

A brief description is here:

https://en.wikipedia.org/wiki/Accelerating_expansion_of_the_universe#Evidence_for_acceleration

Note that other pieces of evidence for accelerating expansion are also given.
 
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1. How do scientists measure the expansion of the universe?

Scientists use a variety of methods to measure the expansion of the universe, including observing the redshift of distant galaxies, studying the cosmic microwave background radiation, and analyzing the brightness and distance of Type Ia supernovae.

2. What evidence supports the idea that the expansion of the universe is accelerating?

The primary evidence for accelerating expansion comes from observations of Type Ia supernovae, which are used as standard candles to measure the distance to faraway galaxies. These observations showed that the supernovae were fainter than expected, indicating that the expansion of the universe is accelerating.

3. How did scientists rule out other explanations for the accelerating expansion?

Scientists ruled out other explanations for accelerating expansion, such as the presence of dark matter or a cosmological constant, by carefully analyzing and comparing data from multiple sources, including observations of the cosmic microwave background and the large-scale structure of the universe.

4. What is the role of dark energy in the accelerating expansion of the universe?

Dark energy is believed to be the driving force behind the accelerating expansion of the universe. It is a mysterious, repulsive force that counteracts the gravitational pull of matter and causes the expansion of the universe to accelerate over time.

5. How does the discovery of accelerating expansion impact our understanding of the universe?

The discovery of accelerating expansion has revolutionized our understanding of the universe and its evolution. It has led to the development of the current model of the universe, known as the Lambda-CDM model, which includes dark energy and dark matter as key components. It also suggests that the universe will continue to expand at an increasing rate, eventually leading to a "big freeze" where all matter is too far apart to interact and the universe becomes a cold, dark place.

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