Calculation of the enrichment of the giant planet envelopes during the "late heavy bombardment"
Alexis Matter (MPIFR), Tristan Guillot (CASSIOPEE), Alessandro, Morbidelli (CASSIOPEE)

TL;DR
This study quantifies the heavy element accretion during the late heavy bombardment, revealing it is insufficient to explain the observed enrichments in giant planet envelopes, thus suggesting other processes contributed to their composition.
Contribution
It provides new estimates of heavy element accretion during the late heavy bombardment based on the Nice model, highlighting the limitations of bombardment alone in explaining planetary enrichments.
Findings
Jupiter's enrichment increase is about 0.033 ± 0.001.
Saturn's enrichment increase is about 0.074 ± 0.007.
Accreted masses are insufficient to explain observed enrichments.
Abstract
The giant planets of our solar system possess envelopes consisting mainly of hydrogen and helium but are also significantly enriched in heavier elements relatively to our Sun. In order to better constrain how these heavy elements have been delivered, we quantify the amount accreted during the so-called "late heavy bombardment", at a time when planets were fully formed and planetesimals could not sink deep into the planets. On the basis of the "Nice model", we obtain accreted masses (in terrestrial units) equal to for Jupiter, and for Saturn. For the two other giant planets, the results are found to depend mostly on whether they switched position during the instability phase. For Uranus, the accreted mass is with an inversion and without an inversion. Neptune accretes…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
