<p>Be careful when saying "nearby stars". The scales involved in "nearby" are beyond what most people imagine. If our Sun was the size of a soccer ball located in California, the nearest star would be another soccer ball located in Greenland.</p>

<p>Let's say the average distance between "nearby" stars is a few light years. Let's say an average supernova is like the recent one in the M82 galaxy. That supernova, at, say, 10 light years, would be less bright and less hot than the Sun as seen from Earth. To make that supernova appear as bright and as hot as the mid-day Sun, you'd have to be at 1/3 light years from it (the supernova would have to be in the middle of the Oort cloud).</p>

<p>Interstellar distances are stupendous. Even a supernova cannot do much to compensate for distance.</p>

<p>But what if the stars are very close to each other? They would pretty much have to orbit each other, forming a double star. Moreover, both would have to be on the verge of going supernova. That's a pretty unlikely situation.</p>

<p>Even then, there are many kinds of supernova. There's type Ia, where a dwarf orbiting a red giant leeches too much material from the giant and eventually explodes:</p>

<p><img src="https://i.sstatic.net/16ZQZ.png" alt="enter image description here"></p>

<p>Then there's the core collapse supernova, where a star is simply too bloated and too old to sustain enough pressure in the core; the core collapses into itself due to gravity and re-ignites fusion, effectively exploding like a bomb and ejecting the outer layers:</p>

<p><img src="https://i.sstatic.net/e2etE.png" alt="enter image description here"></p>

<p>Is a nearby stellar explosion going to increase instability in its about-to-blow-up companion, or is it going to reduce its chances of exploding? The answer is not trivial.</p>

<p>Bottom line: I wouldn't say it's mathematically impossible, but it's a combination of quite unlikely scenarios. In a "normal" galactic neighborhood like ours, it's never going to happen.</p>

CC BY-SA 3.0
2014-04-25T17:03:36.963Z
Awesome explanation, thank you! I did use "nearby stars" specifically to reference binary stars or (if they even exist) clusters of "near-enough" stars -- I know astronomical distances are mind-bogglingly huge and that your "typical" supernova would have virtually no effect on other stars due to the sheer distances involved. That said, I think you've more than adequately sated my curiosity!
Kromey
CC BY-SA 3.0
2014-04-26T01:23:37.107Z
"the core collapses into itself due to gravity and re-ignites fusion" Only in a type La. In a standard core collapse the energy comes from gravity.
Kevin Kostlan
CC BY-SA 3.0
2014-04-25T16:55:32.037Z
2014-04-25T16:55:32.037Z
Florin Andrei
<p>I know not all stars can "go nova", and that of those that do there are different types of novae, among which are some that aren't even explosions (at least not as we think of them), and that even the ones that <em>are</em> explosions are really not like what we do with TNT or C4 anyway.</p>

<p>Nonetheless, I can't shake the comparison from my head, and that got me thinking: Are there any circumstances under which one star going nova can trigger novae in other nearby stars, creating a chain reaction?</p>

<star><supernova>
"Chain reaction" supernovae?
Kromey
# "Chain reaction" supernovae?

(Asked by: username_0 on 2014-04-25)

I know not all stars can "go nova", and that of those that do there are different types of novae, among which are some that aren't even explosions (at least not as we think of them), and that even the ones that *are* explosions are really not like what we do with TNT or C4 anyway.

Nonetheless, I can't shake the comparison from my head, and that got me thinking: Are there any circumstances under which one star going nova can trigger novae in other nearby stars, creating a chain reaction?

**Tags:** star, supernova


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## 1 answers

### Answer by username_1 on 2014-04-25. Score: 2 | Accepted answer

Be careful when saying "nearby stars". The scales involved in "nearby" are beyond what most people imagine. If our Sun was the size of a soccer ball located in California, the nearest star would be another soccer ball located in Greenland.

Let's say the average distance between "nearby" stars is a few light years. Let's say an average supernova is like the recent one in the M82 galaxy. That supernova, at, say, 10 light years, would be less bright and less hot than the Sun as seen from Earth. To make that supernova appear as bright and as hot as the mid-day Sun, you'd have to be at 1/3 light years from it (the supernova would have to be in the middle of the Oort cloud).

Interstellar distances are stupendous. Even a supernova cannot do much to compensate for distance.

But what if the stars are very close to each other? They would pretty much have to orbit each other, forming a double star. Moreover, both would have to be on the verge of going supernova. That's a pretty unlikely situation.

Even then, there are many kinds of supernova. There's type Ia, where a dwarf orbiting a red giant leeches too much material from the giant and eventually explodes:

![enter image description here](https://i.sstatic.net/16ZQZ.png)

Then there's the core collapse supernova, where a star is simply too bloated and too old to sustain enough pressure in the core; the core collapses into itself due to gravity and re-ignites fusion, effectively exploding like a bomb and ejecting the outer layers:

![enter image description here](https://i.sstatic.net/e2etE.png)

Is a nearby stellar explosion going to increase instability in its about-to-blow-up companion, or is it going to reduce its chances of exploding? The answer is not trivial.

Bottom line: I wouldn't say it's mathematically impossible, but it's a combination of quite unlikely scenarios. In a "normal" galactic neighborhood like ours, it's never going to happen.

> **Comments:**
> **username_0**: Awesome explanation, thank you! I did use "nearby stars" specifically to reference binary stars or (if they even exist) clusters of "near-enough" stars -- I know astronomical distances are mind-bogglingly huge and that your "typical" supernova would have virtually no effect on other stars due to the sheer distances involved. That said, I think you've more than adequately sated my curiosity!  
> **username_2**: "the core collapses into itself due to gravity and re-ignites fusion" Only in a type La. In a standard core collapse the energy comes from gravity.  

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