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Orbit-Phasing Based Transfer Trajectory to Inclined Heliocentric Orbit around Sun-Earth L4

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Abstract

This study presents the design and validation of an orbit-phasing based transfer trajectory to achieve a heliocentric, inclined, near-circular orbit around the Sun-Earth L4 point. The method assumes a spacecraft initially in a low Earth parking orbit and employs two principal impulsive maneuvers. The first burn, performed at perigee, provides Earth escape while simultaneously shaping a heliocentric phasing orbit with reduced semi-major axis and desired inclination, thereby allowing the spacecraft to lead Earth in orbital phase. Upon achieving a 60° phase separation, the second burn circularizes the orbit at 1 AU, establishing the mission orbit around L4. Analytical derivations identify a continuous set of feasible parking orbit elements and burn vectors, with the phasing orbit defined by the number of revolutions required for rendezvous. To validate the approach, high-fidelity numerical simulations were conducted using the General Mission Analysis Tool (GMAT), incorporating planetary perturbations, non-spherical Earth gravity, and solar radiation pressure. Results confirm that numerically optimized burn magnitudes closely match analytically driven solutions, with overshoots below 1% for both insertion and circularization burns. Additional midcourse correction and station-keeping maneuvers were introduced to ensure convergence and long-term stability, with required velocities on the order of 0.11-0.16 km/s for corrections and only a few meters per second for station-keeping. Over decadal propagation, the spacecraft maintained proximity to L4 with minimal phase drift, demonstrating the robustness of the trajectory design. The findings establish that two-body analytical approximations are sufficient for deriving optimal transfer conditions and that the proposed orbit-phasing strategy provides a practical and efficient means of accessing inclined mission orbits around Sun-Earth L4. The methodology enables mission designers to select among a family of valid initial conditions that can be tailored to constraints such as launch site geometry or target inclination, thereby enhancing flexibility for future heliophysics or communications relay missions.

Original languageEnglish
Title of host publicationIAF Astrodynamics Symposium - Held at the 76th International Astronautical Congress, IAC 2025
PublisherInternational Astronautical Federation, IAF
Pages1156-1161
Number of pages6
ISBN (Electronic)9798331329358
DOIs
Publication statusPublished - 2025
Event2025 IAF Astrodynamics Symposium at the 76th International Astronautical Congress, IAC 2025 - Sydney, Australia
Duration: 29 Sept 20253 Oct 2025

Publication series

NameProceedings of the International Astronautical Congress, IAC
Volume2-F219391
ISSN (Print)0074-1795

Conference

Conference2025 IAF Astrodynamics Symposium at the 76th International Astronautical Congress, IAC 2025
Country/TerritoryAustralia
CitySydney
Period29/09/253/10/25

Bibliographical note

Publisher Copyright:
Copyright © 2025 by the International Astronautical Federation (IAF). All rights reserved.

Keywords

  • GMAT
  • Lagrange points
  • Orbit-Phasing
  • Sun-Earth L4
  • Trajectory Design

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