Lunar Crater Identification using Triangle Reprojection

Author(s)
Thrasher, Ava C.
Molina, Giovanni
Hansen, Michael
Pelgrift, John Y.
Nelson, Derek S.
Advisor(s)
Editor(s)
Associated Organization(s)
Organizational Unit
Daniel Guggenheim School of Aerospace Engineering
The Daniel Guggenheim School of Aeronautics was established in 1931, with a name change in 1962 to the School of Aerospace Engineering
Series
Supplementary to:
Abstract
Image-based terrain relative navigation is a critical capability for future lunar exploration missions. Images of the lunar surface containing craters can be compared to on-board maps to identify craters and estimate the spacecraft position. While there are many ways to accomplish the crater identification task, this work explores a method using triangulation and crater triangle pattern projections. Specifically, potential matching crater patterns from the catalog and image are used to triangulate the spacecraft position, allowing for construction of line-of-sight directions to the potential matching catalog craters. The projection of these directions in the image can be compared to the observed craters to accept or reject the match hypothesis. In this paper, we demonstrate the algorithm's capability in handling various types of input errors and what tolerances can be tuned to achieve a desired performance. Additionally, an initial look at flight software implementation is included.
Sponsor
Date
2023-08
Extent
Resource Type
Text
Resource Subtype
Paper
Rights Statement
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