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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