Categories: Exoplanets

How Large Can A Planet Be?

Jupiter is the largest planet in the solar system. In terms of mass, Jupiter towers over the other planets. If you were to gather all the other planets together into a single mass, Jupiter would still be 2.5 times more massive. It is hard to understate just how huge Jupiter is. But as we’ve discovered thousands of exoplanets in recent decades, it raises an interesting question about how Jupiter compares. Put another way, just how large can a planet be? The answer is more subtle than you might think.

The simple answer is that a large planet is anything too small to be a star. The usual definition for a star is that it must be large enough to fuse hydrogen into helium in its core. A main-sequence star is one where the heat and pressure generated by fusion are balanced by the gravitational weight of the star.

Stars are mostly made of hydrogen and helium, and it’s safe to assume that the largest planets would have a similar composition. The Sun is made of about 75% hydrogen and 24% helium, the other 1% being heavier elements. Jupiter is roughly 71% hydrogen, 24% helium, and 5% other. So let’s figure any large planet is 3 parts hydrogen to 1 part
helium.

As long as there’s no fusion going on, a large planet will be in a state of hydrostatic equilibrium. That means the weight of all that gas trying to collapse on itself is balanced by the pressure of the gas not wanting to be squeezed. The more mass you have, the more the interior is squeezed, and the hotter it gets. With enough mass, the interior gets hot enough for hydrogen to start fusing into helium. That critical mass is about 80 Jupiters. Anything with more mass than that must be a star.

But that’s not the best upper limit, because there are objects in the universe known as brown dwarfs. These objects are star-like because they aren’t in hydrostatic equilibrium. Their interiors generate heat like a star, and they can even fuse hydrogen into deuterium, just not helium. On the other hand, the smallest brown dwarfs have cool, cloudy surfaces, and would look like a planet. The lower limit of mass for a brown dwarf is about 13 Jupiter masses.

In terms of mass, 13 Jupiter masses is a good upper limit. But when it comes to large planets, the most massive ones aren’t actually the largest in size.

Estimated planet sizes by mass compared to observed exoplanets. Credit: Chen and Kipping

Unlike solids, which don’t compress much under pressure, gases can compress significantly. So as you add mass to a gas planet, its volume doesn’t increase by the same amount. For example, Jupiter is three times the mass of Saturn but is less than 20% larger by volume. Going back to our model of hydrostatic equilibrium, the most massive planets are actually smaller than Jupiter in size.

A few years ago Jingjing Chen and David Kipping looked at how the size of planets can vary depending on their mass.[^1] They found that there is a transition point between Neptune-type worlds where more mass tends to increase their size and Jupiter-type worlds where more mass tends to simply compress the gas more. That critical point is about half the mass of Jupiter, so the largest planets should have around that mass. This agrees with observation. The largest confirmed exoplanet is WASP-17b. It is roughly twice the size of Jupiter but has only 49% of Jupiter’s mass.

Some of the largest exoplanets compared. Credit: NASA/ESA/Hubble

Of course, there are other factors that come into play, such as composition and temperature. The largest known exoplanets tend to be hot Jupiters orbiting close to their star. This means they are much warmer and less dense than a cold jovian planet like Jupiter. Jupiter also has a dense rocky core, which means it is smaller than it would be if it were made only of hydrogen and helium.

But even taking these factors into account, jovian planets are clearly both the largest and most massive planets that can exist. Jupiter isn’t the largest planet in the universe, but it is one of the giants.

Source: Probabilistic forecasting of the masses and radii of other worlds, by Chen, Jingjing, and David Kipping.

Brian Koberlein

Brian Koberlein is an astrophysicist and science writer with the National Radio Astronomy Observatory. He writes about astronomy and astrophysics on his blog. You can follow him on YouTube, and on Twitter @BrianKoberlein.

View Comments

  • So when a hot Jupiter loses all it's gases to their star, is the rocky core left behind? If so, does it become a 'Mercury' size planet?
    Could Mercury be a former hot Jupiter?
    How can we determine if it is or isn't?

  • "Their interiors generate heat like a star, and they can even fuse hydrogen into deuterium, just not helium."

    That's not quite correct: they cannot fuse hydrogen, but can fuse deuterium to produce helium-3.

Recent Posts

How Squeezable are Neutron Stars?

Two neutron stars. One is 50% more massive than the other, yet they are almost…

3 hours ago

Following the Moon for Amazing May Astronomy

The May Moon Meets Venus and Mercury at dusk en route to eclipse season and…

4 hours ago

Astronomers see a Rare “Double Quasar” in a Pair of Merging Galaxies

What's better than a quasar? That's right, two quasars. Astronomers have spotted for the first…

9 hours ago

Blue Origin Will Finally Fly Passengers to the Edge of Space in July

Blue Origin has a charitable auction going and whoever makes the highest bid will win…

19 hours ago

Starlink and OneWeb Have Their First Avoidance Maneuver With Each Other’s Constellations

Two companies, OneWeb and SpaceX, are racing to put fleets of thousands of communication satellites…

1 day ago

How can White Dwarfs Produce Such Powerful Magnetic Fields?

White dwarfs have some surprisingly strong magnetic fields, and one team of astronomers may have…

1 day ago