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Thrust Faulting and the Late-stage Contraction of the Moon

  • Authors: T. R. Watters, M. E. Banks, C. A. Nypaver, M. S. Robinson

T. R. Watters et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 1.

Lobate thrust fault scarps in the lunar highlands. (A),(B) The Pitiscus scarp (51.109°S, 31.18°) has a maximum relief of ∼56 m: (A) NAC Stereo DTM and (B) NAC image M1149280834. (C),(D) The Fowler scarp (43.02°N, 212.87°) has a maximum relief of ∼45 m: (C) NAC DTM and (D) NAC image M143221393. (E),(F) The Morozov scarp has a maximum relief of ∼36 m (6.54°N, 129.94°): (E) NAC DTM and (F) NAC image M1113318442. (G),(H) The Mouchez scarp (78.59°N, 318.79°) has a maximum relief of ∼116 m: (G) ShadowCam DTM and (H) ShadowCam image M0421567855.

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