<p>Suppose you had a giant planet with a central temperature/density too low to sustain D fusion (i.e. below about 13 Jupiter masses). You then magically are able to increase the density by somehow driving the mass of the planet inwards (which will actually increase both the density and temperature).</p>
<p>It is the temperature rise that is important. The energy per unit volume generated by fusion is <span class="math-container">$\propto \rho T^n$</span>, where <span class="math-container">$n\gg 1$</span>.</p>
<p>All that would happen is that the fusion rate would become significant when <span class="math-container">$T\sim 3\times 10^5$</span> K, but the object is now completely out of equilibrium due to its higher central pressure. It will expand and the fusion reactions will be damped down.</p>
<p>The key to making an explosion happen is to get all the energy released from the fuel before that energy can be transported away from the burning site. In the case of planets/brown dwarfs, both conduction and convection are rather efficient energy transport mechanisms. Even so, <em>there is</em> a significant increase in luminosity and a <span class="math-container">$\sim 30\%$</span> increase in radius when D is ignited in a planetary mass object that accretes enough material to ignite D at its core (<a href="https://iopscience.iop.org/article/10.1088/0004-637X/770/2/120" rel="nofollow noreferrer">Bodenheimer et al. 2013</a>).
But this only happens because the weight of the object is sufficient to sustain a relatively <em>low</em> rate of D fusion - indeed the reaction proceed over <span class="math-container">$\sim 100$</span> million years.</p>
<p>So I think my answer is yes you could ignite D fusion, but to sustain it would mean sustaining whatever mechanism you had used to increase the density/temperature in the first place.</p>
<p><strong>Edit:</strong></p>
<p>I realise that there is an implicit piece to this argument that I really ought to make explicit. You might have thought that the density of an object could just increase without limit as it cooled and contracted. But no, the reason that there is a lower mass limit for fusion is that these low mass brown dwarfs and giant planets have electron-degenerate interiors. This means the central pressure becomes independent of temperature and that an object below the D-burning threshold can effectively cool at constant density. i.e. Their densities will not increase (much) further and they will simply cool at nearly constant radius. Fusion only occurs if the temperature/density combination reaches a threshold <em>before</em> electron-degeneracy pressure essentially fixes the internal density structure. And this only happens in balls of gas that are greater than 13 times the mass of Jupiter.</p>

CC BY-SA 4.0
2020-07-27T09:01:21.060Z
It's not like I gonna use some mechanism for it. The question is whether such objects could occur _naturally_. Obviously the answer seems to be No.
Ioannes
CC BY-SA 4.0
2020-07-27T21:37:54.907Z
I wonder if a collision between gas giants, for example, Saturn ramming into Jupiter,  could produce temperatures and pressures compatible with fusion, even if briefly.
ksousa
CC BY-SA 4.0
2020-07-27T08:27:10.470Z
2023-02-20T11:14:32.543Z
2023-02-20T11:14:32.543Z
ProfRob
<blockquote>
<p>Or did I miss something about hydrogen bombs?</p>
</blockquote>
<p>You missed something about hydrogen bombs.</p>
<p>The center of our Sun is the equivalent of a warm compost pile in terms of energy produced per unit volume. A multistage thermonuclear weapon briefly (very briefly) compresses and heats the fusible material in the bomb to conditions far beyond those found in our Sun, let alone Jupiter.</p>

CC BY-SA 4.0
2020-07-27T05:35:39.027Z
Obviously not, it is just impossible for a gaseous body to achieve enough density for nuclear fusion from themselves when their mass is too low.
Ioannes
CC BY-SA 4.0
2020-07-27T04:13:36.543Z
2020-07-27T04:18:39.153Z
2020-07-27T04:18:39.153Z
David Hammen
<p>I wonder whether the nuclear fusion of brown dwarfs and more massive stars really depends on their mass only or if it could also start nuclear fusion if it is dense enough but not as massive as brown dwarfs usually are (they need more than 12 Jupiter masses to ignite deuterium). It is like with a nuclear fusion bomb. Since hydrogen bombs explode because of their density and not only their mass, can this also happen to stars? Or did I miss something? Or is a density to ignite deuterium at lower masses simply impossible? If I'm right, what would be the critical density to ignite deuterium at 1 Jupiter mass?</p>

CC BY-SA 4.0
2020-07-26T13:53:48.443Z
It is the mass of the star that with creates enough density to start nuclear fusion. In a hydrogen bomb the density of hydrogen needed for fusion to start is achieved with a nuclear implosion – an atomic (uranium/plutonium) bomb explodes around a container with hydrogen pressing it inwards and creating the pressure needed to achieve the density.
Yellow Sky
CC BY-SA 4.0
2020-07-26T14:30:07.860Z
@YellowSky So it's simply impossible for a gas giant at 1 Jupiter mass to achieve the required density (in this case to fuse Deuterium, not hydrogen)?
Ioannes
CC BY-SA 4.0
2020-07-26T14:41:46.617Z
Interesting question. To get a high density with less mass the gas giant would need a *very* high proportion of heavy elements (which is unlikely to occur naturally). And that would give you an inert core with the deuterium outside it, which is not optimal for fusion. For a typical gas cloud composition, you need around 13× Jupiter's mass for deuterium fusion. BTW, deuterium fusion is *much* easier than plain hydrogen (protium) fusion.
PM 2Ring
CC BY-SA 4.0
2020-07-26T14:45:42.970Z
@Greenhorn - That's right, and that's the reason Jupiter is still a planet, not a star. Arthur C. Clarke's sci-fi novel [2010: Odyssey Two](https://en.wikipedia.org/wiki/2010:_Odyssey_Two) (1982) tells a story of how aliens increased the density of hydrogen on Jupiter and turned it into a star in order to stimulate life evolution on Europa. Both the novel and the film made after it in 1984 are sequels to the famous Stanley Kubrick's film [2001: A Space Odyssey](https://en.wikipedia.org/wiki/2001:_A_Space_Odyssey_(film)) (1968).
Yellow Sky
CC BY-SA 4.0
2020-07-26T15:21:04.473Z
Can we definitely exclude that Uranus/Neptune-like (and less massive) bodies exist that are fusing deuterium?
Ioannes
CC BY-SA 4.0
2020-07-26T15:38:57.777Z
fusion bombs are really fission bombs which create an explosion shell to compress the hydrogen contained in their core to a density reached within much larger objects than Jupiter. Pressure in celestial bodies is quasi static, thus no such process is possible
planetmaker
CC BY-SA 4.0
2020-07-26T16:00:12.070Z
@planetmaker But perhaps there is a body with Jupiter's or Neptune's mass, but much smaller and therefore much denser and thus might fuse deuterium. By the way, Jupiter _does_ become smaller, that's called the Kelvin–Helmholtz mechanism.
Ioannes
CC BY-SA 4.0
2020-07-26T16:44:38.893Z
@Greenhorn Equations of state don't allow for such object to exist.
planetmaker
CC BY-SA 4.0
2020-07-27T04:20:57.980Z
@PM2Ring - Re *For a typical gas cloud composition, you need around 13× Jupiter's mass for deuterium fusion* That is the mass needed for lithium fusion. Deuterium fusion requires even more mass, just a tiny bit less than that needed for hydrogen fusion.
David Hammen
CC BY-SA 4.0
2020-07-27T04:42:50.257Z
@David I thought it was the other way around. https://en.wikipedia.org/wiki/Brown_dwarf claims that deuterium burning can occur from around $13 M_J = 0.012 M_\odot$, and lithium burning kicks in around $65 M_J$. There similar info about the temperature required for Li burning on https://en.wikipedia.org/wiki/Lithium_burning Of course, Wikipedia isn't always reliable...
PM 2Ring
CC BY-SA 4.0
2020-07-27T09:53:51.293Z
@PM2Ring You are correct; I had it backwards.
David Hammen
<stellar-evolution><density><brown-dwarf><hydrogen>
Can a high enough density ignite a gas giant into a brown dwarf?
Ioannes
# Can a high enough density ignite a gas giant into a brown dwarf?

(Asked by: username_0 on 2020-07-26)

I wonder whether the nuclear fusion of brown dwarfs and more massive stars really depends on their mass only or if it could also start nuclear fusion if it is dense enough but not as massive as brown dwarfs usually are (they need more than 12 Jupiter masses to ignite deuterium). It is like with a nuclear fusion bomb. Since hydrogen bombs explode because of their density and not only their mass, can this also happen to stars? Or did I miss something? Or is a density to ignite deuterium at lower masses simply impossible? If I'm right, what would be the critical density to ignite deuterium at 1 Jupiter mass?

**Tags:** stellar-evolution, density, brown-dwarf, hydrogen
> **Comments:**
> **username_1**: It is the mass of the star that with creates enough density to start nuclear fusion. In a hydrogen bomb the density of hydrogen needed for fusion to start is achieved with a nuclear implosion – an atomic (uranium/plutonium) bomb explodes around a container with hydrogen pressing it inwards and creating the pressure needed to achieve the density.  
> **username_0**: @YellowSky So it's simply impossible for a gas giant at 1 Jupiter mass to achieve the required density (in this case to fuse Deuterium, not hydrogen)?  
> **username_2**: Interesting question. To get a high density with less mass the gas giant would need a *very* high proportion of heavy elements (which is unlikely to occur naturally). And that would give you an inert core with the deuterium outside it, which is not optimal for fusion. For a typical gas cloud composition, you need around 13× Jupiter's mass for deuterium fusion. BTW, deuterium fusion is *much* easier than plain hydrogen (protium) fusion.  
> **username_1**: @Greenhorn - That's right, and that's the reason Jupiter is still a planet, not a star. Arthur C. Clarke's sci-fi novel [2010: Odyssey Two](https://en.wikipedia.org/wiki/2010:_Odyssey_Two) (1982) tells a story of how aliens increased the density of hydrogen on Jupiter and turned it into a star in order to stimulate life evolution on Europa. Both the novel and the film made after it in 1984 are sequels to the famous Stanley Kubrick's film [2001: A Space Odyssey](https://en.wikipedia.org/wiki/2001:_A_Space_Odyssey_(film)) (1968).  
> **username_0**: Can we definitely exclude that Uranus/Neptune-like (and less massive) bodies exist that are fusing deuterium?  
> **username_3**: fusion bombs are really fission bombs which create an explosion shell to compress the hydrogen contained in their core to a density reached within much larger objects than Jupiter. Pressure in celestial bodies is quasi static, thus no such process is possible  
> **username_0**: @planetmaker But perhaps there is a body with Jupiter's or Neptune's mass, but much smaller and therefore much denser and thus might fuse deuterium. By the way, Jupiter _does_ become smaller, that's called the Kelvin–Helmholtz mechanism.  
> **username_3**: @Greenhorn Equations of state don't allow for such object to exist.  
> **username_4**: @PM2Ring - Re *For a typical gas cloud composition, you need around 13× Jupiter's mass for deuterium fusion* That is the mass needed for lithium fusion. Deuterium fusion requires even more mass, just a tiny bit less than that needed for hydrogen fusion.  
> **username_2**: @David I thought it was the other way around. https://en.wikipedia.org/wiki/Brown_dwarf claims that deuterium burning can occur from around $13 M_J = 0.012 M_\odot$, and lithium burning kicks in around $65 M_J$. There similar info about the temperature required for Li burning on https://en.wikipedia.org/wiki/Lithium_burning Of course, Wikipedia isn't always reliable...  
> **username_4**: @PM2Ring You are correct; I had it backwards.  

---

## 2 answers

### Answer by username_5 on 2020-07-27. Score: 3

Suppose you had a giant planet with a central temperature/density too low to sustain D fusion (i.e. below about 13 Jupiter masses). You then magically are able to increase the density by somehow driving the mass of the planet inwards (which will actually increase both the density and temperature).

It is the temperature rise that is important. The energy per unit volume generated by fusion is $\propto \rho T^n$, where $n\gg 1$.

All that would happen is that the fusion rate would become significant when $T\sim 3\times 10^5$ K, but the object is now completely out of equilibrium due to its higher central pressure. It will expand and the fusion reactions will be damped down.

The key to making an explosion happen is to get all the energy released from the fuel before that energy can be transported away from the burning site. In the case of planets/brown dwarfs, both conduction and convection are rather efficient energy transport mechanisms. Even so, *there is* a significant increase in luminosity and a $\sim 30\%$ increase in radius when D is ignited in a planetary mass object that accretes enough material to ignite D at its core ([Bodenheimer et al. 2013](https://iopscience.iop.org/article/10.1088/0004-637X/770/2/120)).
But this only happens because the weight of the object is sufficient to sustain a relatively *low* rate of D fusion - indeed the reaction proceed over $\sim 100$ million years.

So I think my answer is yes you could ignite D fusion, but to sustain it would mean sustaining whatever mechanism you had used to increase the density/temperature in the first place.

**Edit:**

I realise that there is an implicit piece to this argument that I really ought to make explicit. You might have thought that the density of an object could just increase without limit as it cooled and contracted. But no, the reason that there is a lower mass limit for fusion is that these low mass brown dwarfs and giant planets have electron-degenerate interiors. This means the central pressure becomes independent of temperature and that an object below the D-burning threshold can effectively cool at constant density. i.e. Their densities will not increase (much) further and they will simply cool at nearly constant radius. Fusion only occurs if the temperature/density combination reaches a threshold *before* electron-degeneracy pressure essentially fixes the internal density structure. And this only happens in balls of gas that are greater than 13 times the mass of Jupiter.

> **Comments:**
> **username_0**: It's not like I gonna use some mechanism for it. The question is whether such objects could occur _naturally_. Obviously the answer seems to be No.  
> **username_6**: I wonder if a collision between gas giants, for example, Saturn ramming into Jupiter,  could produce temperatures and pressures compatible with fusion, even if briefly.  

---

### Answer by username_4 on 2020-07-27. Score: 3

> Or did I miss something about hydrogen bombs?

You missed something about hydrogen bombs.

The center of our Sun is the equivalent of a warm compost pile in terms of energy produced per unit volume. A multistage thermonuclear weapon briefly (very briefly) compresses and heats the fusible material in the bomb to conditions far beyond those found in our Sun, let alone Jupiter.

> **Comments:**
> **username_0**: Obviously not, it is just impossible for a gaseous body to achieve enough density for nuclear fusion from themselves when their mass is too low.  

---

