# How do I give my planet a stronger magnetic field? Playing with variables

Let's say I have a terrestrial planet superficially like earth, except that it rotates much slower (about 10-15 days per rotation) and its atmosphere is ideally several times thicker. If I want this planet to have a substantial magnetic field (3/4 of Earth's as a minimum, though higher is better), what factors can I play with to plausibly provide it that field strength? What approximate values would I need to give these factors to accomplish this?

Here are some ideas I'm toying with (please vet for plausibility):

• Large metallic core
• Tidal Heating: Interactions with the planet's star can generate internal heat and keep a dynamo active. (Would that work?)
• Increase radius: The larger the radius, the faster (m/s) the spin for a given rotation period. The faster the spin the more potential for a strong magnetosphere?
• I read somewhere that Venus's small (non-core generated) magnetosphere can be attributed to some interesting physics happening within its dense atmosphere. Is there a way to take advantage of this phenomena? I presume my planet's atmosphere isn't dense enough nor the phenomena significant enough.

Giving the planet a bigger metal core (and hence making it denser) AND giving it a larger radius would seem to be a good recipe for increasing field strength. [Edit: Removed gravity considerations. Planet can be a Super Earth]

It's not clear to me what variables are the most critical. Is rotation rate more important than core size/composition, or vice-versa? Is internal heating (whether from tidal stress, radioactive decay, or leftover formation heat) as critical as the above two variables? I'm not versed enough in this domain to know.

My understanding is that the exact parameters behind terrestrial magnetic fields haven't 100% been worked out. From what I've read there are no 100% reliable models for taking in a set of variables (planet size, density, etc.) and spitting out a simple value for the strength of a magnetosphere. If this is the case, then all I need to aim for is plausibility. As long as it's credible I can use the wiggle room to our advantage.

Thanks!

• @StarfishPrime You misconstrue my statement. Venus's atmosphere is creating the small magnetic field. From what I've read, Venus has a minute magnetic field that is produce by the interaction of the atmosphere and the stellar wind. Of course Venus has no core magnetic field, which has nothing to do with the atmosphere. – n_bandit Jun 9 '19 at 18:30
• Ahh, that makes more sense now, thanks. – Starfish Prime Jun 9 '19 at 19:16

How does the Earth's core generate a magnetic field?

https://www.usgs.gov/faqs/how-does-earths-core-generate-a-magnetic-field?qt-news_science_products=0#qt-news_science_products

The Earth's outer core is in a state of turbulent convection as the result of radioactive heating and chemical differentiation. This sets up a process that is a bit like a naturally occurring electrical generator, where the convective kinetic energy is converted to electrical and magnetic energy. Basically, the motion of the electrically conducting iron in the presence of the Earth's magnetic field induces electric currents. Those electric currents generate their own magnetic field, and as the result of this internal feedback, the process is self-sustaining so long as there is an energy source sufficient to maintain convection.

Most of the energy from this is thought to come from radioactive decay of elements in the core: radioactive potassium, thorium and uranium. Increase the amounts of those elements and you increase heat production.

Resistance increases with temperature in metals. You might consider giving your planet a nonmetallic core, where temperature increases would improve conductivity or at least not reduce it. Maybe a planet with a supercritical saltwater core? Or a core of molten salt? Those would be big, hot and not as dense as metal. And also awesome.

Answering the comment with an ocean planet example - how about Ganymede?

Ganymede is a moon with planetary aspirations, a colossal saltwater ocean, and a nice magnetic field which I here assert is produced by electrical currents formed within its heated internal ocean.

And there is ice on top for your critters to skate on.

• There's also a little stirring, because the inner core and the mantle spin at slightly different rates. – Spencer May 9 '19 at 23:48
• An important problem to consider with a molten salt core, is that the mantle and crust would therefore need to be composed of materials less dense than molten salt. The core of a planet forms specifically because the most dense materials of the molten protoplanet migrate inward. – Arkenstein XII May 10 '19 at 0:46
• Sounds interesting, but I don't know how a planet would form with those types of non-earth-like features. I'd like to keep this planet as earth-like as possible and only play with the basic variables within reason. – n_bandit May 14 '19 at 15:45
• Ooo! Superionic ice! That is your core! wired.com/story/… – Willk May 15 '19 at 15:01
• A thinner mantle would help too, allowing heat to be lost more quickly through the surface of the planet. However, this would also mean the core cools faster and the planet wouldn't be able to maintain the field for as long. – Christopher James Huff Jun 11 '20 at 23:52

I think your ideas are mostly spot-on. Off the top of my head, you can increase the rotation rate, core density, core size or planet size.

At the edge of the core, the magnetic field has a magnitude of roughly $$B_{\text{core}}\sim\sqrt{\frac{\rho\Omega}{\sigma}}$$ where $$\rho$$ is the density, $$\Omega$$ is the rotation rate and $$\sigma$$ is the electrical conductivity. I find it unlikely that $$\sigma$$ could be changed much unless the composition of the core were to drastically change, but both the density and angular speed could be increased. Core density would presumably scale with the mass of the planet, as it would be under greater pressures, and the rotation rate could very easily be increased through a collision early on with another body. (This does assume that the rotation of the core is coupled to the rotation of the planet itself - not an unrealistic assumption.)

According to dynamo theory, a dipole magnetic field scales as an inverse cube; at a distance $$r$$ from the center of the core, we have $$B(r)\propto r^{-3}$$. The surface field is then (ignoring the angular dependence) $$B_{\text{surf}}=B_{\text{core}}\left(\frac{R_p}{R_c}\right)^{-3}$$ with $$R_p$$ and $$R_c$$ the radius of the planet and the core, respectively. We can turn this into a scaling relation: \begin{aligned} B_{\text{surf}}=&\;2.5\times10^{-5}\left(\frac{\rho}{10\text{ g cm}^{-3}}\right)^{1/2}\left(\frac{\Omega}{7.27\times10^{-5}\text{ rad s}^{-1}}\right)^{1/2}\\ &\times\left(\frac{\sigma}{10^7\text{ Ohm}^{-1}\;\text{m}^{-1}}\right)^{-1/2}\left(\frac{R_p}{6370\text{ km}}\right)^{-3}\left(\frac{R_c}{2890\text{ km}}\right)^{3}\;\text{Tesla} \end{aligned} Decreasing $$R_p$$ or increasing $$R_c$$would decrease the surface-core distance, thereby increasing the surface field. Unlike changing $$B_{\text{core}}$$, this won't change the intrinsic field strength, but for inhabitants on the surface, the two are effectively the same (while there would be a difference when it comes to things like the van Allen belts).

In your case, you want a (roughly) 15-day rotation period. This means that $$\Omega$$ will be lower than Earth's by a factor of 15. As $$B\propto\Omega^{1/2}R_c^{3}$$, we can reach a magnetic field 75% the strength of Earth's by increasing the core radius by a factor of about 1.4.

• Thanks! This is great. I love it when an answer includes calculations. Makes it so much easier to assess and utilize. – n_bandit Jun 11 '20 at 16:06
• @n_bandit I'm glad it was helpful! – HDE 226868 Jun 11 '20 at 17:26

Jupiter’s magnetosphere is immensely strong. Jupiter rotates much slower than earth, and has a much thicker atmosphere, like your requirements. What are the requirements for a similar powerful magnetosphere?

According to Dynamo Theory on Wikipedia, three things are needed.

1. An electrically conductive fluid medium
2. Kinetic energy provided by planetary rotation
3. An internal energy source to drive convective motions within the fluid
1. An electrically conductive fluid medium is pretty straightforward. Just fill the planet with a high concentration of molten iron or copper. (Earth’s mantle is 8% iron.)

2. The lack of kinetic energy can be compensated for, like Jupiter and like you proposed, making the planet bigger. The equation for kinetic energy is K=0.5mv^2, so increasing mass (m) compensates for low velocity (v).

3. Earth’s magnetic field’s heat source can be found on Wikipedia:

The heat is generated by potential energy released by heavier materials sinking toward the core (planetary differentiation, the iron catastrophe) as well as decay of radioactive elements in the interior.

Mix in a little extra U-238 and you’ve got a powerful magnetosphere.

• Umm, Jupiter actually rotates much faster then Earth (the Jovian sidereal day is a mere 9.925 hours, as opposed to Earth's 23.934 hours). – Vikki Mar 12 '20 at 22:48