Using asteroid early orbital data for rapid mars missions

Early orbital predictions of near-Earth asteroid 2001 CA21, particularly the 2015 JPL Horizons Solution #11, describe a highly eccentric trajectory with a well-defined sub-ecliptic orbital plane. Although later observational refinements altered the asteroid’s osculating elements, the early solution provides a geometrically structured orbital configuration that can be examined as a reference plane for heliocentric transfer analysis. This study investigates whether the orbital geometry of a preliminary small-body solution can function as a structured filtering framework for identifying rapid Earth–Mars transfer opportunities. Using short-way Lambert-based trajectory construction constrained to remain within of the CA21 orbital plane and high-fidelity JPL Horizons ephemerides, three Mars opposition windows (2027, 2029, and 2031) are analyzed. The 2031 opposition emerges as uniquely favorable under the CA21-plane constraint, yielding two outbound Earth Mars trajectories (33 and 56 days) and corresponding dynamically consistent return legs forming complete round-trip architectures of approximately 153 and 226 days total duration. Sensitivity analysis demonstrates that these CA21-anchored solutions remain geometrically stable under controlled boundary-state perturbations, and Monte Carlo re-evaluation confirms numerical robustness of the Lambert construction. While the asteroid itself is not used as a physical waypoint, its early orbital plane serves as a geometric template that highlights structured rapid-transfer corridors within the 2031 opposition geometry. This case study illustrates how the well-defined plane geometry of a preliminary small-body orbit can be employed as a methodological screening tool for rapid interplanetary transfer identification. • Paper: “Astrodynamics Innovation: Utilizing an Asteroid’s Early Orbital Data for Rapid and Round-Trip Mars Missions in 2031 Window” • Novel method uses early asteroid orbit for rapid Mars missions • Geometric plane anchoring guides rapid Earth–Mars transfers • Rapid round-trip Mars missions found for the 2031 window • Early orbital geometry used as transfer screening tool • Feasible rapid round-trip to Mars in 226 days

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Publication Details

Journal
Acta Astronautica
Published
2026-04-11
DOI
https://doi.org/10.1016/j.actaastro.2026.04.018
Primary Topic
Spacecraft Dynamics and Control
Type
article
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article

Using asteroid early orbital data for rapid mars missions

Marcelo de Oliveira Souza
Acta Astronautica
Spacecraft Dynamics and Control
article

Using asteroid early orbital data for rapid mars missions

Marcelo de Oliveira Souza
article en

Abstract

Early orbital predictions of near-Earth asteroid 2001 CA21, particularly the 2015 JPL Horizons Solution #11, describe a highly eccentric trajectory with a well-defined sub-ecliptic orbital plane. Although later observational refinements altered the asteroid’s osculating elements, the early solution provides a geometrically structured orbital configuration that can be examined as a reference plane for heliocentric transfer analysis. This study investigates whether the orbital geometry of a preliminary small-body solution can function as a structured filtering framework for identifying rapid Earth–Mars transfer opportunities. Using short-way Lambert-based trajectory construction constrained to remain within of the CA21 orbital plane and high-fidelity JPL Horizons ephemerides, three Mars opposition windows (2027, 2029, and 2031) are analyzed. The 2031 opposition emerges as uniquely favorable under the CA21-plane constraint, yielding two outbound Earth Mars trajectories (33 and 56 days) and corresponding dynamically consistent return legs forming complete round-trip architectures of approximately 153 and 226 days total duration. Sensitivity analysis demonstrates that these CA21-anchored solutions remain geometrically stable under controlled boundary-state perturbations, and Monte Carlo re-evaluation confirms numerical robustness of the Lambert construction. While the asteroid itself is not used as a physical waypoint, its early orbital plane serves as a geometric template that highlights structured rapid-transfer corridors within the 2031 opposition geometry. This case study illustrates how the well-defined plane geometry of a preliminary small-body orbit can be employed as a methodological screening tool for rapid interplanetary transfer identification. • Paper: “Astrodynamics Innovation: Utilizing an Asteroid’s Early Orbital Data for Rapid and Round-Trip Mars Missions in 2031 Window” • Novel method uses early asteroid orbit for rapid Mars missions • Geometric plane anchoring guides rapid Earth–Mars transfers • Rapid round-trip Mars missions found for the 2031 window • Early orbital geometry used as transfer screening tool • Feasible rapid round-trip to Mars in 226 days

Acta AstronauticaVol. 246
State University of Norte Fluminense (BR), Prefeitura Municipal de Campos dos Goytacazes (BR)
Industry, innovation and infrastructure
Openalex Percentile: Top 8%
Spacecraft Dynamics and Control
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