We have modeled the nucleation and isothermal growth of bubbles in dacite from the 1912 Plinian eruption of Novarupta, Alaska. Bubble growth calculations account for the exsolution of H 2 O and CO 2 , beginning with bubble nucleation and ending when bubble sizes reproduced the observed size distribution of vesicles in Novarupta pumice clasts. Assuming classical nucleation theory, bubbles nucleated with a diameter of the order of 10 −8 m and grew to sizes ranging from 10 −6 m to greater than 10 −3 m, the typical range of vesicle sizes found in Novarupta pumice. The smallest vesicles in Novarupta pumices are also the most abundant and bubbles with radii of 10 −6 m to 10 −5 m comprise almost 90% of the entire bubble population. We find that these bubbles must have nucleated and grown to their final size within a few 100 milliseconds. Despite these extremely fast growth rates, the pressures of exsolved volatiles contained within the bubbles remained high, up to about 10 7 Pa in excess of ambient pressure. Assuming a closed‐system, the potential energy of these compressed volatiles was sufficient to cause magma fragmentation, even though only a fraction of the pre‐eruptive volatiles had exsolved. Unless the matrix glasses of Novarupta pyroclasts retains a large fraction of pre‐eruptive volatiles, the majority of magmatic volatiles (80–90%) was likely lost by open‐system degassing between magma fragmentation and quenching.
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B. F. Houghton (2012) studied this question.
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