While the massive atmosphere of Jupiter consists mainly of hydrogen and helium, the key to understanding the gas giant’s formation and evolution lies in the distribution of the remaining (heavy) elements. Miguel et al. demonstrated that the heavy-element abundance is not homogeneous in Jupiter’s envelope. Image credit: NASA / ESA / NOIRLab / NSF / AURA / Wong et al. / de Pater et al. / M. Zamani. “When NASA’s Juno spacecraft arrived at Jupiter...