Possible extinction event: nearby supernova

In summary, a popular science article on the end of the Devonian era examines the likelihood of an extinction event mediated by a nearby supernova. Samarium 146 and/or Plutonium 244 isotopes can be used to confirm or rule out the hypothesis that a nearby supernova caused the end of the Devonian era, and the decline in species diversity. Geologists are currently searching for signs of an extinction event in sedimentary rock near the surface of the Earth, and would need to sample the extinction horizon to confirm or rule out the hypothesis.
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jim mcnamara
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The extinction event 359 mya that ended Devonian times may have been caused by a nearby supernova.
A popular science article on the end of the Devonian era examines the likelihood of an extinction event mediated by a nearby supernova.
https://www.sciencedaily.com/releases/2020/08/200818142104.htm

Per the article -
A convincing argument can be made by finding Samarium 146 and/or Plutonium 244 isotopes in rock strata from that period.

The proposed model includes what the authors call a double whammy:
First a blast of ionizing radiation, then a massive radioactive cloud of ejecta that persists over a long period. Both which could alter the magnetosphere of Earth and allow the solar wind to damage extant flora and fauna. The latter cloud effect could persist over long periods. Which matches the known geologic record of a ~100000 year decline in species diversity at the end of the Devonian.

My takeaway is this looks like a great research project.

Gather rocks from several sites around the globe, test for those two isotopes that do not naturally occur on Earth. The most likely results will be either clearly negative or positive if the experiment is well designed. A positive result is sure to spark intense criticism of the experimental design. New findings are often generate that. The downside is Geology has a long and tortuous history of downright ugly debate.

Ruling out other causes for the presence of those two isotopes would be intense. Meteors.

Finding anomalous abundances of weird elements in rock layers often is the result of meteor impacts. They may need to be ruled out. Meteor impacts can create layers. Thin layers with odd isotopes or elements have been found and used to help prove other hypotheses. Example:

Iridium in the K-Pg (KT is the old name) boundary layer caused by the Chicxulub impact, which made life hard for the dinosaurs. This layer is high in Iridium, rare or non-existent in most Earth rock. It is sometimes called the Iridium Anomaly.

https://en.wikipedia.org/wiki/Cretaceous–Paleogene_boundary
https://en.wikipedia.org/wiki/Chicxulub_crater
https://en.wikipedia.org/wiki/Iridium_anomaly
 
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It is an interesting hypothesis, although it would be better to narrow it down to one particular event. In their paper, they are not distinguishing the Kellwasser event with the Hangenberg event (10 Myr separating them). Basically they are saying that their hypothesis could explain one of those events or even both. They should have stick with the Hangenberg event like it was suggested in previous papers.

Their paper: https://www.pnas.org/content/early/2020/08/17/2013774117
 
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jim mcnamara said:
My takeaway is this looks like a great research project.

Gather rocks from several sites around the globe, test for those two isotopes that do not naturally occur on Earth. The most likely results will be either clearly negative or positive if the experiment is well designed. A positive result is sure to spark intense criticism of the experimental design. New findings are often generate that.
There is a huge volume of sedimentary rock near the surface of the Earth. Checking it randomly for exotic isotopes would be a very expensive process. Instead, mapping the contacts of formations that show a reduction in palaeontology, and analysing those for changes in exotic isotopes is a tractable project. But that is exactly what is done now, for example the Chicxulub Iridium.
 
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Baluncore said:
There is a huge volume of sedimentary rock near the surface of the Earth. Checking it randomly for exotic isotopes would be a very expensive process. Instead, mapping the contacts of formations that show a reduction in palaeontology, and analysing those for changes in exotic isotopes is a tractable project. But that is exactly what is done now, for example the Chicxulub Iridium.
The problem is that this presupposes the conclusion.
You should check the sedimentary rocks for changes in exotic isotopes that show no accompanying extinctions, too.
 
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snorkack said:
The problem is that this presupposes the conclusion.
You should check the sedimentary rocks for changes in exotic isotopes that show no accompanying extinctions, too.
If you are trying to correlate exotic isotopes with extinction events, you should sample the extinction horizon, along with the profile immediately before and immediately after. That will provide the necessary control.

The extinction event in a sedimentary section can be identified using a binary search for the step change in palaeontology. That comes naturally to a geologist walking out a formation, or examining the core from a drill hole. The same is not true of exotic isotopes that appear as a pulse in the section. Exotics cannot be easily seen while walking up stream beds, ascending rocky ridges, or climbing cliff faces.

It is not feasible to sample and analyse all candidate sections for a pulse of exotics that will probably be less than one millimetre thick. A one kilometre thick stratigraphic section would require one million samples. Some of those samples may contain exotic isotopes from meteorites that are local, not regional or worldwide. It would be impossible to find the exact same age strata, in different rock types in different locations, without the help of fossil evidence. If there is no extinction, then you have no reliable calendar.

You could reduce the analysis processing cost by bulking the milli-samples into one metre mixed samples, but there is nothing to say the exotic layer would be present in any of the samples, or in the section. Random sampling will blow your budget long before you get any usable data.
 

1. What is a nearby supernova?

A nearby supernova refers to a type of explosion that occurs in a star, causing it to become extremely bright and release a large amount of energy. It is considered "nearby" if it occurs within our own galaxy, the Milky Way.

2. How could a nearby supernova cause an extinction event?

A nearby supernova could potentially cause an extinction event by releasing a large amount of radiation and debris into the surrounding space. This could have damaging effects on Earth's atmosphere, potentially leading to mass extinction of certain species.

3. How likely is a nearby supernova to occur?

The likelihood of a nearby supernova occurring is relatively low. Scientists estimate that a supernova event within our own galaxy happens about once every 50 years. However, it is difficult to predict when and where a supernova will occur.

4. How far away would a supernova need to be to not cause an extinction event?

The distance at which a supernova would not cause an extinction event is not certain. It would depend on the size and intensity of the explosion, as well as the distance of Earth from the supernova. However, scientists estimate that a supernova would need to be at least 50 light years away to not have a significant impact on Earth.

5. What precautions are being taken to prepare for a nearby supernova?

Currently, there are no specific precautions being taken to prepare for a nearby supernova. However, scientists continue to study and monitor nearby stars to better understand the likelihood and potential effects of a supernova event. In the future, advanced warning systems may be developed to notify us of a potential nearby supernova.

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