Evidence for an Early Formation of Serenitatis Basin at 4.25 Ga Shifts Lunar Chronology

  • Evan Bjonnes
  • , Brandon C. Johnson
  • , Adrien Broquet
  • , Ian Garrick-Bethell
  • , Jeffrey C. Andrews-Hanna
  • , Shigeru Wakita
  • , Walter S. Kiefer

Research output: Contribution to journalArticlepeer-review

Abstract

Troctolite sample 76535, collected in Serenitatis basin during Apollo 17, formed at least 50 km deep, experienced maximum shock pressures of 6 GPa, and has a 40Ar/39Ar excavation age of 4.25 Ga. Previous work attributed 76535 to the South Pole-Aitken (SPA) basin, presumably dating the SPA-impact and constraining lunar bombardment history. Here we use the iSALE-2D shock-physics code and gravity inversion modeling to determine if instead the Serenitatis impact event excavated 76535. We find nearly 140,000 km3 of material (∼2% of near-surface ejecta) matching the depth and pressure constraints of 76535 is displaced to the surface during crater collapse of a Serenitatis-like impact event. We conclude that the Serenitatis impact event possibly excavated 76535, redefining its age to 4.25 Ga, 300 My older than the consensus age based on Apollo 17 samples. This finding would provide an important anchor point where lunar chronology where bombardment flux is especially uncertain.

Original languageEnglish (US)
Article numbere2025GL116654
JournalGeophysical Research Letters
Volume52
Issue number18
DOIs
StatePublished - Sep 28 2025

Keywords

  • geophysics
  • gravitational analysis
  • impact basin
  • impact processes
  • lunar basins
  • lunar chronology

ASJC Scopus subject areas

  • Geophysics
  • General Earth and Planetary Sciences

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