Massive Jupiter storm churns ammonia deep into planet’s atmosphere

Massive Jupiter storm churns ammonia deep into planet’s atmosphere

Brightness temperature anomaly maps for each channel. The contours outline the difference between the mean background atmosphere (PJ1 to PJ12) and PJ4. The positive outlines indicate an atmosphere that is radio-warmer than the average atmosphere, whereas blue contours indicate a radio-colder atmosphere. All six maps are shown on the same color scale showing that the signal is strongest in the C6 and C5 channels, with sound pressures less than 3 bar. The signal strength decreases progressively from C4 (∼3 bar) to C1 (∼40 bar). Credit: Science Advances (2025). DOI: 10.1126/sciadv.ado9779

A pair of planetary scientists at the University of California, working with a colleague from the California Institute of Technology, has discovered that a massive amount of ammonia is churned up and down in Jupiter’s atmosphere during major storms. In their study published in Science Advances, Chris Moeckel, Imke de Pater, and Huazhi Ge analyzed data from multiple sources focused on a major storm that occurred on Jupiter starting in 2016.

Over the past several decades, as spaceborne observation technology has improved, astronomers have been studying the storms that occur on other planets. These studies have shown that storms tend to play a major role in the formation of atmospheric conditions. In this new effort, the researchers focused on a major storm that began on Jupiter in 2016 and continued through 2017.

To learn more about the impact of the storm on Jupiter’s atmosphere, the researchers obtained data from the Atacama Large Millimeter/submillimeter Array, the Hubble Space Telescope and from the Juno space probe, which just happened to be making a flyby of the planet during the time when the storm was occurring.

By comparing data between sources, the researchers were able to follow the flow of ammonia as it was pushed during downdrafts from the outer reaches of the planet’s atmosphere to levels deep below the clouds. This movement, the researchers found, resulted in trapping ammonia gas deeply in lower parts of the atmosphere even after the storm had passed—leaving what the team describes as a “fingerprint” in the atmosphere.

The research team created a simulation to show the movement of the atmospheric storm components, including ammonia. The simulations showed the ammonia gas being pushed far below the clouds and pulled during updrafts into the higher parts of the planet’s atmosphere, leading to it “drying out,” as the team described.

That was followed by the formation of dark patches, which the team believes comprised a mix of ammonia and water forming into slush balls, which fell back, like hail on Earth, to lower parts of the atmosphere during an ensuing downdraft, until they eventually evaporated.

The net result, the researchers found, was patches of ammonia hanging low in the atmosphere even after the storm had died.

More information:
Chris Moeckel et al, Tempests in the troposphere: Mapping the impact of giant storms on Jupiter’s deep atmosphere, Science Advances (2025). DOI: 10.1126/sciadv.ado9779

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Massive Jupiter storm churns ammonia deep into planet’s atmosphere (2025, April 4)
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