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 language | English |
|---|---|
| Title of host publication | IAF Astrodynamics Symposium - Held at the 76th International Astronautical Congress, IAC 2025 |
| Publisher | International Astronautical Federation, IAF |
| Pages | 1156-1161 |
| Number of pages | 6 |
| ISBN (Electronic) | 9798331329358 |
| DOIs | |
| Publication status | Published - 2025 |
| Event | 2025 IAF Astrodynamics Symposium at the 76th International Astronautical Congress, IAC 2025 - Sydney, Australia Duration: 29 Sept 2025 → 3 Oct 2025 |
Publication series
| Name | Proceedings of the International Astronautical Congress, IAC |
|---|---|
| Volume | 2-F219391 |
| ISSN (Print) | 0074-1795 |
Conference
| Conference | 2025 IAF Astrodynamics Symposium at the 76th International Astronautical Congress, IAC 2025 |
|---|---|
| Country/Territory | Australia |
| City | Sydney |
| Period | 29/09/25 → 3/10/25 |
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
Fingerprint
Dive into the research topics of 'Orbit-Phasing Based Transfer Trajectory to Inclined Heliocentric Orbit around Sun-Earth L4'. Together they form a unique fingerprint.Cite this
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver