Code 580 Technologies and Products
Automatic Extraction of Planetary Features
Principal Investigator (PI)
- Jacqueline Le Moigne/Code 580
- Jacqueline.LeMoigne@nasa.gov
Description and Objectives
- New unsupervised method for extraction of spatial features of elliptical and geometrically compact shape from a planetary surface.
- Automatic processing of large amounts of data.
- Applicable to low contrast and uneven illumination characterized image data.
- Applicable to craters and rocks.
- Can be generalized to other spatial features, e.g., boulders and ridges.
Experimental Results Obtained by Applying the Proposed Method to High Resolution Imaging Science Experiment (HiRISE) Images (Top: Original; Bottom: Extracted object contours highlighted in red)
Technical Approach
- Combination of Image Processing Technique:
- Canny edge detection
- Watershed segmentation
- Generalized Hough transform
- Can be combined:
- With genetic algorithm or robust feature matching for image registration
- With Markov marked point process for more general shape detection
Main Innovation(s)
- Unsupervised technique that does not need a priori knowledge of the terrain
- Robust to low contrast and uneven illumination
- Can locate spatial features of interest and provide shape and size descriptions of the extracted objects
Infusion Potential
- Applicable to image registration as well as more general analysis of any planetary imagery