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IN LINE: Emma Hayes, manager of Chelsea Ladies is being considered for the job of managing the men team. AFP Photo By Paul Kennedy I don know much about Emma Hayes other than what I read about her in recent weeks. For those of you as much in the dark as I was, she is the coach of Chelsea FC Women. And if you believe what you have read in the newspapers of late, she is in contention to take charge of the men team after the imminent departure of Maurizio Sarri. The 42 year old led Chelsea to third in the Women's Super League and to the semi finals of the Women's Champions League this season. In the previous season she won the double for Chelsea and during a spell coaching in America, won manager of the year. Not too shabby for sure, but in my mind, she has nowhere near the credentials required to take charge of the men first team and the reasons have got absolutely nothing to do with her sex.

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Determining the shapes of a rotating liquid droplet bound by surface tension is an archetypal problem in the study of the equilibrium shapes of a spinning and charged droplet, a problem that unites models of the stability of the atomic nucleus with the shapes of astronomical scale, gravitationally bound masses. The shapes of highly deformed droplets and their stability must be calculated numerically. Although the accuracy of such models has increased with the use of progressively more sophisticated computational techniques and increases in computing power, direct experimental verification is still lacking. Here we present an experimental technique for making wax models of these shapes using diamagnetic levitation. The wax models resemble splash form tektites, glassy stones formed from molten rock ejected from asteroid impacts. Many tektites have elongated or 'dumb bell' shapes due to their rotation mid flight before solidification, just as we observe here. Measurements of the dimensions of our wax 'artificial tektites' show good agreement with equilibrium shapes calculated by our numerical model, and with previous models. These wax models provide the first direct experimental validation for numerical models of the equilibrium shapes of spinning droplets, of importance to fundamental physics and also to studies of tektite formation.