Type 1a Supernovae and Dark Energy

In summary, the conversation discusses how Type 1a supernovae were the initial evidence for the accelerating expansion of the universe and how this adds to Hubble's observations. It also explains the concept of dark energy and its role in causing this acceleration. The conversation ends with a discussion about the accuracy of the Type 1a distance measuring technique and how it led to the discovery of the acceleration.
  • #1
chris1969
7
1
Hello everyone

I hope you don't mind me asking a real silly question about the original evidence for dark energy. I've been reading about how Type 1a supernovae provided the initial evidence that the expansion of the universe was accelerating. They are able to do this because they are standard candles i.e they all have the same intrinsic brightness - therefore the fainter they seem the further away they must be.

The part I don't get is what this information adds to the original observations made by Hubble. These showed that the velocity of objects (as measured by the redshift) increased with distance (as measured by some form of standard candle). If velocity is increasing with distance and time then this implies that the rate expansion of the Universe is increasing i.e accelerating. If this is the case, what is it that the Type 1a supernovae add to the story.

I'm conscious that I'm misunderstanding something at a very basic level, so an idiot's level
explanation would be appreciated!

And many thanks in advance.

Chris
 
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  • #2
chris1969 said:
The part I don't get is what this information adds to the original observations made by Hubble. These showed that the velocity of objects (as measured by the redshift) increased with distance (as measured by some form of standard candle).

Hubble's observations point to a constant expansion rate, not an accelerating one.

chris1969 said:
If velocity is increasing with distance and time then this implies that the rate expansion of the Universe is increasing i.e accelerating.

That's not right. There was no acceleration according to Hubble's observations.

Consider a very long stretchy nylon rope that you cannot see the end of that's being stretched by trucks over the horizon at the rate of 1% per minute. If you measure two points separated by one meter, you'll get a velocity of separation of 1cm per minute, if you measure two meters, you'll get a velocity of separation of 2cm per minute. If you measure two points 100 meters apart, you'll get 1m per minute velocity of separation. So the velocity increases linearly with the distance measured.

This is what happens with a uniformly expanding universe and this is what Hubble observed. The further away you look, the faster the object will be moving away from you when the universe is expanding at a constant rate. This was thought to be the case until the Type 1a supernova observations of 1998.

chris1969 said:
If this is the case, what is it that the Type 1a supernovae add to the story.

These observations showed that the expansion was not at a constant rate but was accelerating slightly. This was a very surprising finding because to this day no one knows why this acceleration occurs.

For there to be an acceleration there needs to be a source of energy causing that acceleration. This is why dark energy was proposed. It is a placeholder name for whatever is causing the acceleration in the expansion of space in the universe.
 
  • #3
Many thanks for this, the rope analogy is very helpful. I've got another couple of questions.

Firstly, am I right in thinking that the increase in velocity with distance is because the rope (ie space) is being stretched?

My second question is why we were able to identify the acceleration from the type 1s but not from the other standard candles?

Many thanks once again.

Chris
 
  • #4
chris1969 said:
Many thanks for this, the rope analogy is very helpful. I've got another couple of questions.

Firstly, am I right in thinking that the increase in velocity with distance is because the rope (ie space) is being stretched?

Not stretched exactly more like it is expanding from within. This only happens between galaxies and galaxy clusters. But it acts like space itself is expanding.

chris1969 said:
My second question is why we were able to identify the acceleration from the type 1s but not from the other standard candles?

I'm not qualified to discuss the particulars of the experiment but you can find the papers for the 1998 discovery by Riess et al. and subsequent confirmation by Perlmutter et al. here:

http://www.arxiv.org/abs/astro-ph/9805201
http://arxiv.org/abs/astro-ph/9812133

But the main thing is that these measurements were more accurate because the Type 1a distance measuring technique was more accurate than prior measurements. The new observations showed that rather than there being a straight-line relationship between distance and speed there was a curve. The curve indicates acceleration. In other words, they found that the speed difference between very old (which is the same as very far away) galaxies was less than the equivalent distance between newer galaxies.
 
  • #5



Hello Chris,

Thank you for your question. It is great to see people interested in understanding scientific concepts.

To answer your question, let me first clarify the concept of standard candles. As you mentioned, Type 1a supernovae are considered standard candles because they have a consistent intrinsic brightness. This means that no matter how far away they are, we can use their brightness to determine their distance from us. This is because the amount of light we receive from an object decreases with distance, so by knowing the intrinsic brightness of a Type 1a supernova, we can calculate its distance based on how bright it appears to us.

Now, to your question about what Type 1a supernovae add to the story of dark energy. The original observations made by Hubble showed that the velocity of objects increases with distance, which suggests an expanding universe. However, it was not clear whether this expansion was slowing down or speeding up. This is where Type 1a supernovae come in.

Using Type 1a supernovae as standard candles, scientists were able to measure the distances to very distant galaxies. They found that these distant galaxies were moving away from us at a faster rate than expected, indicating that the expansion of the universe is not slowing down, but in fact, accelerating. This was a groundbreaking discovery and provided the first evidence for the existence of dark energy.

In summary, Type 1a supernovae add to the story of dark energy by providing a way to measure the distances to very distant objects and showing that the expansion of the universe is accelerating. I hope this helps clarify your understanding. Please let me know if you have any further questions. Keep asking questions and exploring the wonders of science!
 

1. What is a Type 1a Supernova?

A Type 1a Supernova is a type of stellar explosion that occurs in binary star systems. It happens when a white dwarf star, which is the remnant of a star that has run out of fuel, pulls matter from its companion star until it reaches a critical mass and undergoes a rapid nuclear fusion reaction, resulting in a powerful explosion.

2. How bright are Type 1a Supernovae?

Type 1a Supernovae are incredibly bright, often reaching peak luminosities that are 5 billion times brighter than the sun. This makes them visible from extremely far distances, allowing scientists to study them and gather information about the universe.

3. What is the role of Type 1a Supernovae in measuring distances in the universe?

Type 1a Supernovae are considered "standard candles" in astronomy, meaning that they have a consistent and predictable brightness. This makes them extremely useful for measuring distances in the universe, as scientists can compare the observed brightness of a Type 1a Supernova to its known intrinsic brightness to determine its distance from Earth.

4. How do Type 1a Supernovae relate to Dark Energy?

In the late 1990s, scientists used Type 1a Supernovae to study the expansion rate of the universe and found that it was accelerating. This led to the discovery of Dark Energy, a mysterious force that is believed to be responsible for the universe's accelerated expansion. Type 1a Supernovae are still used today to study and gather data on Dark Energy.

5. What are the implications of understanding Type 1a Supernovae and Dark Energy?

Studying Type 1a Supernovae and Dark Energy can help scientists better understand the structure and evolution of the universe. It can also provide insight into the ultimate fate of the universe and the role that Dark Energy plays in its expansion. Additionally, understanding these phenomena can potentially lead to advancements in fields such as cosmology and astrophysics.

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