Abstract
A new object-oriented method has been developed for the extraction of Mars rocks from Mars rover data. It is based on a combination of Mars rover imagery and 3D point cloud data. First, Navcam or Pancam images taken by the Mars rovers are segmented into homogeneous objects with a mean-shift algorithm. Then, the objects in the segmented images are classified into small rock candidates, rock shadows, and large objects. Rock shadows and large objects are considered as the regions within which large rocks may exist. In these regions, large rock candidates are extracted through ground-plane fitting with the 3D point cloud data. Small and large rock candidates are combined and postprocessed to obtain the final rock extraction results. The shape properties of the rocks (angularity, circularity, width, height, and width-height ratio) have been calculated for subsequent geological studies.
| Original language | English |
|---|---|
| Pages (from-to) | 125-135 |
| Number of pages | 11 |
| Journal | Journal of Earth Science |
| Volume | 24 |
| Issue number | 1 |
| DOIs | |
| Publication status | Published - Feb 2013 |
Keywords
- 3D point cloud data
- Mars rover
- rock extraction
- rover image