Tricky radiation half-life question

In summary, the question is asking how long ago did the stars explode that released the elements that formed our Earth, assuming that the amounts of 235U and 238U were equal at the time of the explosion. The present ratio of 235U to 238U is 0.00725 and their respective half-lives are 0.704 x 10^9 years and 4.47 x 10^9 years. After an hour of research, the person calculated that the answer is 5,003,891,200 years using the formula n=n_oe^{-\lambda t}. However, this answer turned out to be wrong and they are looking for guidance in the right direction.
  • #1
lando45
84
0
Hey,

I have been set this question as an assignment and I spent about an hour researching it yesterday and came up with what I thought was the right answer, but it has turned out to be wrong.

"A theory of astrophysics proposes that all the elements heavier than iron are formed in supernova explosions ending the lives of massive stars. If we assume that at the time of the explosion the amounts of 235U and 238U were equal, how long ago did the star(s) explode that released the elements that formed our Earth? The present 235U / 238U ratio is 0.00725. The half-lives of 235U and 238U are 0.704 x 10^9 years and 4.47 x 10^9 years."

Here is what I did.

Reciprocal of 0.00725 = 137.93
Used log to find that 2^7.1078 = 137.93
Multiplied 7.1078 by 0.704 x 10^9 to get 5,003,891,200 years.

But this answer turned out to be wrong. Can anyone guide me in the right direction?
 
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  • #2
The exponential decay process is described by
[tex]n=n_oe^{-\lambda t}[/tex]
where [itex]n_o[/itex] is the initial amount of nuclei present (the same for both types) and [itex]\lambda[/itex] is the decay constant of the particular isotope. Its relationship with the halflife [itex]T_{\frac{1}{2}}[/itex] is
[tex]\lambda T_{\frac{1}{2}} = \ln(2)[/tex]
 
  • #3
lando45 said:
Hey,

I have been set this question as an assignment and I spent about an hour researching it yesterday and came up with what I thought was the right answer, but it has turned out to be wrong.

"A theory of astrophysics proposes that all the elements heavier than iron are formed in supernova explosions ending the lives of massive stars. If we assume that at the time of the explosion the amounts of 235U and 238U were equal, how long ago did the star(s) explode that released the elements that formed our Earth? The present 235U / 238U ratio is 0.00725. The half-lives of 235U and 238U are 0.704 x 10^9 years and 4.47 x 10^9 years."

Here is what I did.

Reciprocal of 0.00725 = 137.93
Used log to find that 2^7.1078 = 137.93
Multiplied 7.1078 by 0.704 x 10^9 to get 5,003,891,200 years.

But this answer turned out to be wrong. Can anyone guide me in the right direction?

Just telling us what arithmetic you did doesn't make it very clear WHY you did it. What equations did you have? What reason do you have for thing taking the reciprocal of 0.00725, etc. will give the correct answer?

We can take the "equal amounts" of U235 and U238 created to be 1. Since U235 has a half life of 0.2704 x 109 year, the amount after T years will be
[tex]U235= \left(\frac{1}{2}\right)^{\frac{T}{0.2704x10^9}}[/tex]
Since U238 has a half life of 4.47 x 109, the amount left after T years will be
[tex]U238= \left(\frac{1}{2}\right)^{\frac{T}{4.47x10^9}}[/tex]
The ratio of those is
[tex]\frac{U235}{U238}= \left(\frac{1}{2}\right)^{\frac{T}{0.2704x10^9}- \frac{T}{4.47x10^9}}= 0.00725[/tex]

Solve that for T.
 
  • #4
So could someone please tell me what the hell the answer is.

Thankso:)
 
  • #5
Nevermind... got names mixed up. sigh. lol
 
Last edited:

1. What is half-life?

Half-life is the amount of time it takes for half of a radioactive substance to decay into a stable form.

2. How is half-life calculated?

The half-life of a substance can be determined by measuring the rate of decay and using the equation t1/2 = 0.693/λ, where t1/2 is the half-life and λ is the decay constant.

3. What factors affect the half-life of a substance?

The half-life of a substance can be affected by its chemical properties, temperature, and external factors such as pressure or radiation exposure.

4. Can half-life be manipulated or changed?

No, the half-life of a substance is a fixed characteristic that cannot be altered or manipulated by any external factors.

5. How does half-life impact radiation exposure?

The longer the half-life of a radioactive substance, the longer it will take for the substance to become safe and non-hazardous. This means that substances with longer half-lives pose a greater risk for radiation exposure as they remain radioactive for longer periods of time.

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