NASA's Mars rover Curiosity has successfully drilled its 44th hole on the Martian surface, a significant milestone in the investigation of the "boxwork unit," a region of resistant ridges surrounding pits or "hollows" of less-resistant rock.
The drilling took place over the weekend within the "Monte Grande" hollow at the "Valle de la Luna" target. The rover planning this week focused on ensuring that the granular drill tailings from Valle de la Luna were transferred to the SAM (Sample Analysis at Mars) and CheMin (X-ray diffraction) instruments, and analyzing the results.
These internal studies of the Valle de la Luna samples will provide critical information for determining how the boxwork features formed. However, subtle differences between the rocks making up the ridges and those making up the hollows have yet to be explained by chemistry from the APXS and ChemCam instruments and reflectance spectra from ChemCam.
While conducting internal studies, remote sensing data were collected by Mastcam of a series of targets, as well as atmospheric remote sensing. The rover is also analyzing images collected during a photometry study, which examines changes in the apparent reflected brightness of rocks and soils based on the illumination geometry.
The team plans to continue analyzing the drilled sample with more SAM experiments and analyze the tailings. They are also searching for a suitable drilling location on a ridge as the next drilling site to compare with the results from the Monte Grande hollow.
To learn more about Curiosity's science instruments, visit the Science Instruments page.
The drilling took place over the weekend within the "Monte Grande" hollow at the "Valle de la Luna" target. The rover planning this week focused on ensuring that the granular drill tailings from Valle de la Luna were transferred to the SAM (Sample Analysis at Mars) and CheMin (X-ray diffraction) instruments, and analyzing the results.
These internal studies of the Valle de la Luna samples will provide critical information for determining how the boxwork features formed. However, subtle differences between the rocks making up the ridges and those making up the hollows have yet to be explained by chemistry from the APXS and ChemCam instruments and reflectance spectra from ChemCam.
While conducting internal studies, remote sensing data were collected by Mastcam of a series of targets, as well as atmospheric remote sensing. The rover is also analyzing images collected during a photometry study, which examines changes in the apparent reflected brightness of rocks and soils based on the illumination geometry.
The team plans to continue analyzing the drilled sample with more SAM experiments and analyze the tailings. They are also searching for a suitable drilling location on a ridge as the next drilling site to compare with the results from the Monte Grande hollow.
To learn more about Curiosity's science instruments, visit the Science Instruments page.