Science Advances

Supplementary Materials

This PDF file includes:

  • Supplementary Text
  • Morphology and morphometry of impact basins
  • Maps of impact basins
  • Multiring basins
  • Peak-ring basins and other sizeable lunar impacts
  • Basins without measurable rings that are identifed by GRAIL Bouguer gravity anomaly
  • Fig. S1. Serenitatis, Serenitatis North, and Lamont.
  • Fig. S2. Fitzgerald-Jackson.
  • Fig. S3. Amundsen-Ganswindt and Schrödinger.
  • Fig. S4. Nectaris and Asperitatis.
  • Fig. S5. Lorentz and Bartels-Voskresenskiy.
  • Fig. S6. Copernicus-H and Aestuum.
  • Fig. S7. Orientale and Orientale Southwest.
  • Fig. S8. Mendel-Rydberg.
  • Fig. S9. Imbrium and Iridum.
  • Fig. S10. Crisium and Crisium East.
  • Fig. S11. Humorum.
  • Fig. S12. Hertzsprung.
  • Fig. S13. Humboldtianum and Bel’kovich.
  • Fig. S14. Coulomb-Sarton and Fowler-Charlier.
  • Fig. S15. Smythii and Balmer-Kapteyn.
  • Fig. S16. Moscoviense and Moscoviense North.
  • Fig. S17. TOPO-22.
  • Fig. S18. Australe North.
  • Table S1. Lunar craters <200 km in diameter suggested from LOLA data.
  • Table S2. Diameters of the rings and inner depressions of multiring basins measured from LOLA topography and GRAIL Bouguer anomaly data.
  • Table S3. Ring diameters and centroids for circles fit to the rings of multiring basins.
  • Table S4. Lunar peak-ring basins.
  • Table S5. Lunar impact structures ≥200 km in diameter with only one topographic ring and no interior peak ring or central peak structure.
  • Table S6. Lunar depressions suggested by GRAIL data to be degraded basins.
  • Table S7. Features in basin catalogs not meeting criteria for inclusion in this study.
  • References (42–65)

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