A team of astronomers used the ALMA radio array, located in the Atacama desert in Chile, to observe Jupiter in search of the two molecules. In the absence of motion, the signatures of the two molecules are centered around 354.5 GHz (HCN) and 345.8 GHz (CO). Just like a siren’s pitch of a moving vehicle changes upon passing a listener, so do the motions in Jupiter’s atmosphere shift the frequencies of the molecular lines. Most of the shift comes from the fast rotation of Jupiter itself. That can easily be accounted for, and any additional frequency shift is due to the winds.