Curiosity NavigationCuriosity HomeMission OverviewWhere is Curiosity?Mission UpdatesScienceOverviewInstrumentsHighlightsExploration GoalsNews and FeaturesMultimediaCuriosity Raw ImagesImagesVideosAudioMosaicsMore ResourcesMars MissionsMars Perseverance RoverMars Curiosity RoverMars Reconnaissance OrbiterMars OdysseyMore Mars MissionsMars Home3 min readCuriosity Blog, Sols 4968-4974: Rock Climbing Towards the DiscontinuityNASA’s Mars rover Curiosity acquired this image, a frame of the “Longquimay” mosaic showing fine-scale sedimentary textures in a bedrock block near the supersurface, using its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm. Curiosity acquired the image on Aug. 1, 2026 — Sol 4972, or Martian day 4,972 of the Mars Science Laboratory mission — at 23:35:43 UTC.NASA/JPL-Caltech/MSSSWritten by Lucy Lim, Planetary Scientist at NASA’s Goddard Space Flight CenterEarth planning date: Friday, July 31, 2026As mentioned in the previous blog, Curiosity has been exploring a large-scale feature in Gale’s sedimentary record suspected to be an “erosional supersurface.” The “supersurface” represents a period in time when a net depositional environment changed to a net erosional one before returning to a depositional regime, thus producing a discontinuity in the rock record. The erosion can involve wind, water, or both. Sometimes there are clues about these environmental changes in the layers below and above the supersurface. So far we’ve been seeing some patterns that look like aeolian features and also some “lens” deposits that sometimes appear consistent with fluvial origins. We need higher-resolution imaging of these features.This week Curiosity came within detailed imaging range of a section of the “Cerro Paine Grande” vertical exposure just below the candidate supersurface before climbing on top of it. Mastcam was the star of the show on both planning days this week, capturing large stereo mosaics of the vertical face of the outcrop and a 360-degree panorama after the rover climbed on top of it.NASA’s Mars rover Curiosity acquired this image, showing the rover arm in action in the “Longquimay” workspace at the top of a steep climb. Curiosity captured the image using its Right Navigation Camera on Aug. 2, 2026 — Sol 4972, or Martian day 4,972 of the Mars Science Laboratory mission — at 00:49:52 UTC.NASA/JPL-CaltechRoving to the top took full advantage of Curiosity’s climbing capabilities, leaving the rover at an approximate 24-degree tilt in its final parking spot. The rover planners managed to reach the right posture for contact science at the same time — quite a feat, and one that approached the mission’s contact science tilt record of 27 degrees!Meanwhile, MAHLI and our geochemical instruments provided detailed characterization of the rock layers beneath the discontinuity. I was the Geology and Mineralogy Theme Lead for the Sol 4968 (Monday) planning cycle, during which “Puyehue” in the light-toned bedrock block of the workspace was co-targeted with APXS, MAHLI, and ChemCam LIBS. The other two targeted LIBS observations in the plan went to a similar-looking nearby bedrock block (“Lago Palena”) and an intriguing layered block off to the side of the workspace (“Piedras Juntas”). Another APXS measurement went to a sand target, “Cormudesi,” which will help us assess the consistency of sand compositions along the rover’s traverse. In the Sol 4972 workspace atop the slope, the bedrock was sharply divided between a smooth bedding-parallel surface on the local top of the outcrop and the darker-toned, rougher, angled exposure of the same rocks. The light-toned top surface was measured by MAHLI, APXS, and the LIBS at target “Sierra de Sangre,” whereas the darker-toned laminated face was targeted by APXS and MAHLI at “Laguna del Laja.” The fine-scale sedimentary structures in the textured material were also documented by a MAHLI mosaic (“Longquimay”) supported by Mastcam M100 imaging.Rounding out the week’s science observations were several long-distance ChemCam RMI mosaics on more distant targets such as sedimentary structures above the rover’s current stratigraphic position, and finally our regular cadence measurements of the modern Martian environment, including atmospheric opacity and a ChemCam passive-sky survey to monitor abundances of minor atmospheric gases.Want to read more posts from the Curiosity team?Visit Mission Updates Want to learn more about Curiosity’s science instruments?Visit the Science Instruments page NASA’s Curiosity rover at the base of Mount SharpNASA/JPL-Caltech/MSSSShareDetailsLast UpdatedAug 11, 2026Related TermsBlogsExplore More3 min readCuriosity Blog, Sols 4961-4967: Approaching a Break in the Rock Record?Article2 weeks ago3 min readCuriosity Blog, Sols 4954–4960: Celebrating Our Rover Engineers Past and PresentArticle3 weeks ago3 min readCuriosity Blog, Sols 4947-4953: Gale Crater Then and NowArticle4 weeks agoKeep ExploringDiscover More Topics From NASAMarsMars is the fourth planet from the Sun, and the seventh largest. 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