This technology is extensible to Earth science and satellite monitoring and surveillance.
Science investigators need to quickly and effectively assess past observations of specific locations on a planetary surface. This innovation involves a location-based search technology that was adapted and applied to planetary science data to support a spatial query capability for mission operations software.
High-performance location-based searching requires the use of spatial data structures for database organization. Spatial data structures are designed to organize datasets based on their coordinates in a way that is optimized for location-based retrieval. The particular spatial data structure that was adapted for planetary data search is the R+ tree. The R+ tree arranges data as a set of nodes that represents bounding rectangles. Every leaf node in the tree is a particular datum with coordinates. The root node represents a bounding box containing the entire set of data. Each level of the tree subdivides the search space into smaller and smaller bounding rectangles, each containing a smaller subset of the data. A query on the R+ tree for a set of coordinates will follow one unique path from the root to the leaf, and return the data contained in the coordinates. The complexity of the search is bounded by the depth of the tree, so the R+ tree insertion algorithm maintains a balanced tree such that the depth is minimized.
A map view provides an intuitive way to specify a set of coordinates for a location-based query. The software will let the user select any location on the map of the rover’s traverse path to date and return all of the results in under a second. This was particularly useful during tactical activity planning when the question of “what data do we have of this location” is asked every day. The wrong answer to this question is very expensive: false negatives result in missed science opportunities that may never come again, while false positives results in a waste of spacecraft time and bandwidth resources.
This work was done by Khawaja S. Shams, Thomas M. Crockett, Mark W. Powell, Joseph C. Joswig, and Jason M. Fox of Caltech for NASA’s Jet Propulsion Laboratory.