“At these altitudes, the ammonia acts like an antifreeze, lowering the melting point of water ice and allowing the formation of a cloud with ammonia-water liquid,” explained Becker in a NASA Jet Propulsion Laboratory press release. “In this new state, falling droplets of ammonia-water liquid can collide with the upgoing water-ice crystals and electrify the clouds. This was a big surprise, as ammonia-water clouds do not exist on Earth.”

Advertisement

Conveniently enough, this explanation appears to have solved another mystery having to do with Jupiter: uneven gaps of missing ammonia. Scientists previously figured that the absent ammonia was caused by rain, in which a wet mixture of ammonia and water precipitated down into the deeper levels. Calculations of this scenario didn’t work, however, as the hypothesized rain wouldn’t be capable of falling deep enough to match observations made by Juno’s Microwave Radiometer, which detected the depleted ammonia.

Graphic depicting the evolutionary process of shallow lightning and mushball hail on Jupiter.
Graphic depicting the evolutionary process of shallow lightning and mushball hail on Jupiter.
Image: NASA/JPL-Caltech/SwRI/CNRS
Advertisement

A new explanation, as described in the new Journal of Geophysical Research study, suggests scientists were on the right track. But rather than invoking rain as the cause, the new paper, also co-authored by Becker, posits a different type of precipitation: hailstones.

Referred to as “mushballs” by the researchers, these hailstones are made from water and ammonia. Similar to the way hailstones form in Earth’s atmosphere, the mushballs start as small seeds that grow in size as they’re kept aloft by violent winds. Eventually, these slushy orbs get too heavy and fall down to the deeper layers below, evaporating in the warmer temperatures.

Advertisement

“As it turned out, the ammonia isn’t actually missing; it is just transported down while in disguise, having cloaked itself by mixing with water,” explained Scott Bolton, a co-author of the study and Juno PI at the Southwest Research Institute in San Antonio, in the JPL press release.

Advertisement

So, in addition to showing where the missing ammonia had gone, the new theory also explains the uneven distribution of the missing ammonia in the Jovian atmosphere.

It’s so cool when one scientific discovery leads to another, which is what happened here. Some scientific endeavors might seem superfluous or indulgent, but as these two papers show, we don’t always know where they’re going to lead us.