Fluorine is one of the most interesting elements for nuclear and stellar astrophysics. Fluorine abundance was first measured for stars other than the Sun in 1992, then for a handful of metal-poor stars, which are likely to have formed in the early Universe. Now, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have detected fluorine — in the form of hydrogen fluoride — in the gravitationally lensed starburst galaxy...