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N-body simulation of star forming regions

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Credit: Hubble

26Al and 60Fe, and other such Short-Lived Radioisotopes (SLRs) have a significant impact on the formation and evolution of planets. In particular, decay heating from these SLRs provide the bulk of energy for heating and desiccation of volatile-rich planetesimals in the early solar system. The source of these SLRs is contested, however.

The solar system has a significantly higher fraction of both 26Al and 60Fe than the interstellar medium.


© Joseph Eatson 1995-2025
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