The EMA Justitia Probe: Terminator Frame-Based Deployment Orbit Selection and Surface Coverage Analysis
Abstract
The Emirates Mission to the Asteroid Belt (EMA) probe is designed to perform asteroid imaging during an uncontrolled ballistic descent to (269) Justitia. The mission design is constrained by main spacecraft proximity operations, uncertain asteroid gravity, limited knowledge of the final deployment trajectory, and requirements for illumination and safe operations. These constraints necessitate a mission design that ensures suitable illumination, attitude determination and control, and payload pointing throughout descent. The EMA probe concept of operations employs near-terminator deployment orbit geometry with continuous Sun visibility and two attitude control modes: single-axis Sun-spin for periodic imaging opportunities and three-axis asteroid-pointing for continuous asteroid visibility. Based on these modes, formal requirements are derived for deployment orbits that enable asteroid observations during ballistic descent. A deployment orbit selection method is developed using the terminator reference frame and a minimum boresight deviation margin. The method identifies families of orbit orientations satisfying illumination and payload observation constraints. Reference orbits are selected and verified through mission geometry analysis and trajectory propagation using a polyhedron gravity model. Asteroid surface coverage is then evaluated for uncontrolled tumbling, Sun-spin, and asteroid-pointing modes. The results characterize the expected imaging performance and demonstrate the feasibility of the EMA probe concept for close-proximity asteroid imaging. The proposed approach can also support future ballistic probe missions subject to similar operational and observational constraints.
Versions
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BibTeX
@misc{biktimirov2026justitia,
title = {{The EMA Justitia Probe: Terminator Frame-Based Deployment Orbit Selection and Surface Coverage Analysis}},
author = {Shamil Biktimirov and Fatima Alnaqbi and Anton Ivanov},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.26581},
eprint = {2610.26581},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.26581},
note = {CC BY-NC-ND 4.0},
}
RIS
TY - UNPB
TI - The EMA Justitia Probe: Terminator Frame-Based Deployment Orbit Selection and Surface Coverage Analysis
AU - Shamil Biktimirov
AU - Fatima Alnaqbi
AU - Anton Ivanov
PY - 2026
DA - 2026/10/29
PB - arXiv
DO - 10.48550/arxiv.2610.26581
UR - https://arxiv.org/abs/2610.26581
AB - The Emirates Mission to the Asteroid Belt (EMA) probe is designed to perform asteroid imaging during an uncontrolled ballistic descent to (269) Justitia. The mission design is constrained by main spacecraft proximity operations, uncertain asteroid gravity, limited knowledge of the final deployment trajectory, and requirements for illumination and safe operations. These constraints necessitate a mission design that ensures suitable illumination, attitude determination and control, and payload pointing throughout descent. The EMA probe concept of operations employs near-terminator deployment orbit geometry with continuous Sun visibility and two attitude control modes: single-axis Sun-spin for periodic imaging opportunities and three-axis asteroid-pointing for continuous asteroid visibility. Based on these modes, formal requirements are derived for deployment orbits that enable asteroid observations during ballistic descent. A deployment orbit selection method is developed using the terminator reference frame and a minimum boresight deviation margin. The method identifies families of orbit orientations satisfying illumination and payload observation constraints. Reference orbits are selected and verified through mission geometry analysis and trajectory propagation using a polyhedron gravity model. Asteroid surface coverage is then evaluated for uncontrolled tumbling, Sun-spin, and asteroid-pointing modes. The results characterize the expected imaging performance and demonstrate the feasibility of the EMA probe concept for close-proximity asteroid imaging. The proposed approach can also support future ballistic probe missions subject to similar operational and observational constraints.
ER -