Vision-Based Estimation of Small Body Rotational State during the Approach Phase
Paolo Panicucci, J\'er\'emy Lebreton, Roland Brochard, Emmanuel Zenou,, and Michel Delpech

TL;DR
This paper presents a vision-based algorithm to estimate the rotational state of small celestial bodies during the approach phase, enabling autonomous characterization before orbit insertion.
Contribution
It introduces a novel method for estimating small body rotation axes and centers using feature tracking in images, tested extensively on synthetic asteroid data.
Findings
80% of test cases had rotation axis error below 10 degrees
Algorithm successfully estimates rotation axis and center in diverse lighting and orientation conditions
Validated on over 800 synthetic scenarios with Bennu and Itokawa asteroids
Abstract
The heterogeneity of the small body population complicates the prediction of small body properties before the spacecraft's arrival. In the context of autonomous small body exploration, it is crucial to develop algorithms that estimate the small body characteristics before orbit insertion and close proximity operations. This paper develops a vision-based estimation of the small-body rotational state (i.e., the center of rotation and rotation axis direction) during the approach phase. In this mission phase, the spacecraft observes the rotating celestial body and tracks features in images. As feature tracks are the projection of the landmarks' circular movement, the possible rotation axes are computed. Then, the rotation axis solution is chosen among the possible candidates by exploiting feature motion and a heuristic approach. Finally, the center of rotation is estimated from the center…
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Taxonomy
TopicsAstro and Planetary Science · Space Satellite Systems and Control · Stellar, planetary, and galactic studies
MethodsTest
