Mars Exploration News  
MARSDAILY
Sols 3401-3402: Sand, Boulders and Ridges, Oh My
by Lucy Thompson | Planetary Geologist - University of New Brunswick
Pasadena CA (JPL) Mar 02, 2022

3400 Right Navcam image of the drive direction. The rocks in the immediate foreground are the lowermost capping unit, with the pediment surface extending beyond. The large-scale layered ridge in the distance is the Gediz Vallis ridge, with Gale crater rim in the background.

Curiosity has been picking her way through sand, sharp boulders and ridges to find a way up onto the Greenheugh pediment. We briefly explored the pediment more than 600 sols ago, before resuming our traverse over the Mount Sharp group sedimentary rocks that we have been driving over since ~sol 750.

The science team is excited to drive up onto and investigate the very different looking rock that comprises the more resistant pediment again. As we have been driving along the side of the pediment cliffs, interesting textures have been observed, which we are hoping to examine in situ.

However, we are not quite there yet. Because of the tricky terrain, Curiosity's weekend drive stopped a little short of its intended location and she ended up perched on a rock, such that we were not able to safely deploy the arm and use either MAHLI or APXS. However, the rover engineers are confident that we can continue our drive in this plan to get us ever closer to the pediment surface.

Without the use of the arm in this plan, the science team set about planning how to utilize the remaining instruments to continue characterizing this important transitional area. ChemCam will analyze a small resistant ridge and associated bedrock ("Vert Knap of Howar") with its laser, acquire passive spectra on the bedrock target "River Oykell," and RMIs of the convoluted layering in the "Drumeizer" bedrock as well as of the blocky, Gediz Vallis ridge in the distance.

Mastcam will also image the Vert Knap of Howar target, as well as the "Lamington Sandstone" and "Broch of Gurness" targets to document textures and stratigraphy within the cap rock.

The environmental scientists planned several observations to continue monitoring changes in atmospheric conditions. These included: Mastcam basic and full tau observations and a dust devil movie, and a Navcam dust devil movie and images as well as a supra horizon movie.

After our hopefully successful drive, we will execute a ChemCam AEGIS analysis to autonomously measure the chemistry of a rock target in the new workspace. The terrain beneath the rover wheels will be imaged with MARDI. Standard REMS, DAN and RAD activities round out this plan.


Related Links
Curiosity Mars Science Laboratory
Mars News and Information at MarsDaily.com
Lunar Dreams and more


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MARSDAILY
Sols 3398-3400: The Road Ahead
Pasadena CA (JPL) Mar 01, 2022
The drive on Sol 3397 went well and gave us some good perspective on the road ahead, as seen in the above Navcam image. Curiosity is perched at the edge of the pediment, carefully planning our route to climb fully on top of the pediment capping unit, and the team is eager to investigate these rocks! This 3-sol plan was a typical weekend plan, with opportunities for contact science, remote sensing, and a drive. Although our workspace mostly consisted of loose sand, the team was able to plan MAHLI a ... read more

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