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Simulated Effects of Radioactive Elements on Magnetic Evolution and Atmospheric Mass Loss of Earth-like Planets

  • Authors: Nathaniel Tanglin, Juliette Becker

Nathaniel Tanglin and Juliette Becker 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

Evolution of the planetary magnetic field and FAP fraction (Equation (2)) for Earth orbiting the Sun at 1 au, given differences in initial abundances of radioisotopes (40K in the core and mantle; 232Th, 235U, and 238U in the mantle only). The stellar magnetic field was held constant at B* = 5 Gauss.

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