Science Advances

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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