What Would Happen If We Nuked Jupiter?

The hypothetical detonation of a nuclear weapon on Jupiter immediately runs into the realities of space and physics. Jupiter is the solar system’s largest planet, a gas giant with a mass nearly 2.5 times greater than all the other planets combined. This immense scale dictates that any human-made explosion, no matter how powerful, would be a negligible event in the context of the Jovian system.

Jupiter’s Immense Scale and Composition

Jupiter’s composition is similar to the Sun, consisting primarily of hydrogen and helium. The atmosphere transitions from gaseous hydrogen and helium at the cloud tops to a super-pressurized liquid state deep within the planet. Under the crushing internal pressure, this liquid hydrogen eventually becomes liquid metallic hydrogen, a state where electrons are stripped from the atoms, allowing the material to conduct electricity.

The planet’s internal structure includes a core, which recent data from the Juno spacecraft suggests is not a compact, solid body but a large, diffuse region of rock and ice mixed with the metallic hydrogen. Estimates place the core mass between 7 and 25 times the mass of Earth. This sheer volume and mass create a powerful gravitational field that holds the entire system together with immense gravitational binding energy.

The Localized Effect of the Detonation

Detonating a nuclear device, even the 50-megaton Tsar Bomba, deep within Jupiter’s atmosphere would produce a localized effect. The energy release would create a superheated fireball and shockwave. However, this energy would be quickly absorbed and dissipated by the planet’s vast, dense layers of hydrogen and helium gas.

For context, the impact of Comet Shoemaker–Levy 9 in 1994 released an estimated 6 million megatons of energy in its largest explosion, 120,000 times more powerful than the Tsar Bomba. This natural event only left temporary dark scars that faded after a few months. The energy from a single nuclear weapon would simply create a temporary superheated bubble of gas that would rise, cool, and quickly collapse back into the surrounding atmosphere, leaving no lasting trace on the planet’s structure or dynamics.

Why Ignition Is Physically Impossible

The idea that a nuclear bomb could “ignite” Jupiter and turn it into a star is impossible due to the planet’s lack of sufficient mass. Stars sustain themselves through continuous nuclear fusion, a process requiring immense pressure and temperature to force atomic nuclei together. Jupiter does not have the mass required to generate the necessary internal pressure for self-sustaining fusion.

A nuclear bomb, even one utilizing fusion, only provides a momentary, localized spike of heat and pressure. It cannot replace the continuous, self-sustaining pressure generated by gravitational collapse that occurs in a true star. Jupiter would need to be approximately 13 times its current mass to begin the limited, short-lived fusion of deuterium, a heavy isotope of hydrogen, to become a brown dwarf. To achieve the sustained hydrogen fusion of a true star like the Sun, Jupiter would need 80 times its present mass. Since the detonation does not add the required mass, the reaction immediately extinguishes as the energy dissipates.

External Consequences for the Solar System

The vast distance between Jupiter and the inner solar system, combined with the planet’s colossal mass, ensures that the external consequences of the localized explosion would be nonexistent for Earth. The negligible energy input from the bomb would not cause any measurable change to Jupiter’s orbit, mass, or gravitational influence.

While the detonation would produce radioactive debris and a burst of radiation, Jupiter’s powerful gravity would ensure that most of the material either falls back into the planet or remains contained within its orbital region. The sheer distance means that any radiation or debris plume would dissipate across the vacuum of space long before reaching Earth or the inner solar system. The only observable effect would be a bright, brief flash visible through powerful telescopes, similar to the fleeting scars left by the comet impacts in 1994.