Oxford Events, the new replacement for OxTalks, will launch on 16th March. The two-week OxTalks freeze period starts on Monday 2nd March. During this time, there will be no facility to publish or edit events. The existing OxTalks site will remain available to view during this period. Once Oxford Events launches, you will need a Halo login to submit events. Full details are available on the Staff Gateway.
Isotopes are useful probes of planet formation and evolution for at least two reasons. Some exhibit nucleosynthetic anomalies providing clues to their original location. Others undergo decay, providing age constraints. In this talk, I’ll discuss two applications of these ideas. The fact that the silicate Earth records different fractions of “carbonaceous” material in different elements implies that it experienced a change in the material it was accreting over time. The first ~95% was “non-carbonaceous”, while the last ~5% was “carbonaceous” and volatile-rich. Reconciling these constraints with existing planetary accretion scenarios is not easy. In the second part, I’ll discuss the idea that the pile-up of lunar ages around 4.35 Gyr is not the signature of magma ocean crystallization but is instead related to a tidal heating event. This story allows the Moon to be older (~4.45 Gyr or so), which is easier to reconcile with dynamical models.
