On Sol 1385, our rover covered a distance of 66 meters as we continued our journey south between the “Baynes Mountains” and “Helgas Dune”. For Sol 1386, our plan includes conducting APXS and MAHLI observations of the target “Trekkopje”, followed by a brief science block.
Before taking any scientific measurements, Mastcam will begin the block by taking atmospheric measurements. ChemCam will then analyze Trekkopje to gather information about its composition. After these observations are complete, Mastcam will document them along with the AEGIS observation from Sol 1385. In addition to these activities, we will also capture small mosaics to study the rim of a nearby crater.
However, instead of driving on Sol 1386, we will be using MAHLI to conduct a check-up on our wheels. This is important for ensuring that our rover’s mobility system is functioning properly. Ryan Anderson, a planetary scientist at the USGS Astrogeology Science Center and a member of the ChemCam team on MSL, has provided insights into the planned activities for the rover. It is important to note that the dates of these planned activities may be subject to change due to various factors related to the Martian environment, communication relays, and the rover’s status.