Luminosity & Stellar Lifetimes

In summary: If the efficiency is 20 times greater, then the energy output must be increased by the same factor, so the lifetime should be the same as before.
  • #1
Jimmy87
686
17

Homework Statement


Quasars have a luminosity on the order of 10^12 times more than our Sun. Our Sun is expected to last 5 billion years. Using this number estimate (in seconds) how long our Sun would last if it started using energy at the rate of a Quasar.

Homework Equations


None

The Attempt at a Solution


From the information given, there is no equation given so I did some research and it looks like you can roughly approximate that the luminosity of a star is inversely proportional to its lifetime therefore I did the following:

5 billion years = 1.58 x 10^17 seconds

I then simply divided this by 10^12 to give - 158,000 s or 44 hours

Does this sound right? Also, is it acceptable to approximate the age of a star to being inversely proportional to its luminosity. I see no other way of doing it based on the information given.

Thanks.
 
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  • #2
Looks reasonable. The underlying assumption is that there is a fixed amount of energy available and that the "burn" rate (power output) is constant over the lifetime of the object.
 
  • #3
gneill said:
Looks reasonable. The underlying assumption is that there is a fixed amount of energy available and that the "burn" rate (power output) is constant over the lifetime of the object.

Thanks. I just found out that nuclear fusion in a quasar can convert a set amount of mass into energy to an order of magnitude of 20 times more than mass into energy in a normal star. How would my answer change? Would it just be 20 times longer i.e. 880 hours?
 
  • #4
Jimmy87 said:
Thanks. I just found out that nuclear fusion in a quasar can convert a set amount of mass into energy to an order of magnitude of 20 times more than mass into energy in a normal star. How would my answer change? Would it just be 20 times longer i.e. 880 hours?
I don't see how your answer to the problem would change, because it doesn't depend upon the mass. You were given relative energy production rates only. There was nothing in your original problem statement to suggest that the total available energy should be modified.

On the other hand, if this is a new question where you are to consider that the total energy available changes due to different nuclear processes coming into play under different operating conditions, then yes, you'd have to take that into account.
 
  • #5
gneill said:
I don't see how your answer to the problem would change, because it doesn't depend upon the mass. You were given relative energy production rates only. There was nothing in your original problem statement to suggest that the total available energy should be modified.

On the other hand, if this is a new question where you are to consider that the total energy available changes due to different nuclear processes coming into play under different operating conditions, then yes, you'd have to take that into account.

Thanks for the answer. So if a new question was considered, e.g.

Quasars have a luminosity on the order of 10^12 times more than our Sun. Our Sun is expected to last 5 billion years. Using this number estimate (in seconds) how long our Sun would last if it started using energy at the rate of a Quasar. You need to take into account that the nuclear processes that operate inside Quasars are 20 times more efficient i.e. there is 20 times more energy converted per kg of mass compared to stars.

In this case would you simply multiply the previous answer by 20, therefore giving 880 hours. More logic is that the efficiency will slightly offset the reduced aging caused by the increased luminosity. For example, in a hypothetical situation you could have a star that is 20 times more luminous but 20 times more efficient which would result in no loss of lifetime. At least that's my interpretation of the situation?
 
  • #6
Jimmy87 said:
Thanks for the answer. So if a new question was considered, e.g.

Quasars have a luminosity on the order of 10^12 times more than our Sun. Our Sun is expected to last 5 billion years. Using this number estimate (in seconds) how long our Sun would last if it started using energy at the rate of a Quasar. You need to take into account that the nuclear processes that operate inside Quasars are 20 times more efficient i.e. there is 20 times more energy converted per kg of mass compared to stars.

In this case would you simply multiply the previous answer by 20, therefore giving 880 hours. More logic is that the efficiency will slightly offset the reduced aging caused by the increased luminosity. For example, in a hypothetical situation you could have a star that is 20 times more luminous but 20 times more efficient which would result in no loss of lifetime. At least that's my interpretation of the situation?
Sounds reasonable.
 

1. What is luminosity and how is it measured?

Luminosity is the total amount of energy that a star emits per unit time. It is measured in watts or solar luminosities. Solar luminosity is the amount of energy emitted by our Sun per unit time. Luminosity can be measured by observing the brightness of a star and its distance from Earth.

2. What is the relationship between luminosity and stellar lifetimes?

The relationship between luminosity and stellar lifetimes is that the more luminous a star is, the shorter its lifetime will be. This is because luminosity is directly related to a star's mass, and more massive stars have shorter lifetimes due to their higher rate of nuclear fusion and energy output.

3. How do scientists determine the lifetimes of stars?

Scientists determine the lifetimes of stars by studying their mass and luminosity. They use mathematical models and observations to estimate how long a star will remain on the main sequence, which is the stage in a star's life where it fuses hydrogen into helium in its core.

4. Can stellar lifetimes be affected by external factors?

Yes, external factors such as the presence of a companion star or a close encounter with another star can affect a star's lifetime. These interactions can alter a star's mass, which in turn changes its luminosity and can lead to a shorter or longer lifetime.

5. How does a star's luminosity change over its lifetime?

A star's luminosity changes over its lifetime depending on its stage of evolution. As a star ages, it uses up its hydrogen fuel and its core contracts, causing it to become more luminous. This leads to an increase in luminosity until the star leaves the main sequence and begins to fuse heavier elements, which can cause its luminosity to fluctuate before eventually decreasing as it evolves into a white dwarf or other end-of-life stage.

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