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    • Home (overview)
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  • Cislunar glossary (terms & definitions)

    • Cislunar Space Glossary
    • Dynamics models

      • Circular Restricted Three-Body Problem (CR3BP)
      • CR3BP with Low-Thrust (CR3BP-LT)
      • A2PPO (Attention-Augmented Proximal Policy Optimization)
      • Curriculum Learning
      • Low-Thrust Transfer MDP Formulation
      • Generalized Advantage Estimation (GAE)
      • Direct Collocation
      • Birkhoff-Gustavson Normal Form
      • Central Manifold
      • Action-Angle Variables
      • Poincaré Section
      • Clohessy-Wiltshire (CW) Equation
      • Patched Method (拼接法)
      • Continuation (延拓)
      • Differential Correction (微分修正)
      • Poincaré Map (庞加莱图)
      • Impulsive Maneuver (脉冲机动)
      • Zero-Velocity Surface
      • Hill Three-Body Problem
      • Bicircular Four-Body Problem
      • Quasi-Bicircular Four-Body Problem
      • Strobe Map
      • Stability Set
      • Backward Stability Set
      • Capture Set
      • /en/glossary/dynamics/batch-deployment.html
      • /en/glossary/dynamics/state-dependent-tsp.html
      • /en/glossary/dynamics/q-law.html
      • /en/glossary/dynamics/mass-discontinuity.html
      • /en/glossary/dynamics/equinoctial-elements.html
      • /en/glossary/dynamics/dynamic-programming.html
      • /en/glossary/dynamics/coasting-arc.html
    • Mission orbits

      • Distant Retrograde Orbit (DRO)
      • Near-Rectilinear Halo Orbit (NRHO)
      • Earth-Moon L1/L2 Halo Orbit (EML1/EML2 Halo)
      • DRO Constellation
      • Orbit Identification
      • Transfer Orbit (转移轨道)
      • Perilune (近月点)
      • Apolune (远月点)
      • Retrograde (逆行)
      • Prograde (顺行)
      • Parking Orbit (停泊轨道)
      • Free-Return Trajectory (自由返回轨道)
      • Halo Orbit (Halo 轨道)
      • Lissajous Orbit (Lissajous 轨道)
      • Lyapunov Orbit (Lyapunov 轨道)
      • Cycler Trajectory
      • Multi-Revolution Halo Orbit
      • Ballistic Capture Orbit
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      • /en/glossary/orbits/hub-and-spoke.html
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      • Cislunar Space (地月空间)
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      • /en/glossary/other/libration-point.html
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Patched Method

Author: CislunarSpace

Website: https://cislunarspace.cn

Definition

The Patched Method is a classical numerical design approach in orbital mechanics. Its core idea is to divide a complex transfer trajectory into several simpler sub-arcs, each described and propagated using the most appropriate dynamical model. The arcs are then "patched" together at connection points by matching position and velocity state vectors. The primary advantage of this method is that it reduces the complexity of solving a global trajectory under a single model, enabling efficient computation by leveraging the dominant dynamical characteristics within each region.

In cislunar Distant Retrograde Orbit (DRO) transfer trajectory design, the patched method is widely applied to join the departure arc from Low Earth Orbit (LEO) and the arrival arc to DRO at the perilune, thereby constructing a complete transfer scheme.

Core Elements

Basic Principles

The core steps of the patched method are:

  1. Segmentation: Divide the complete trajectory into NNN sub-arcs based on the gravity-dominant regions. Each arc uses the dynamical model that best captures the gravitational characteristics of that region.
  2. Independent Solution: Within each arc, propagate and optimize the trajectory using the corresponding dynamical equations (e.g., two-body model, restricted three-body problem model).
  3. State Matching: At the connection point between adjacent arcs, require continuity of position and velocity:

ri−=ri+,vi−=vi+(i=1,2,…,N−1)\mathbf{r}_i^- = \mathbf{r}_i^+, \quad \mathbf{v}_i^- = \mathbf{v}_i^+ \quad (i = 1, 2, \ldots, N-1) ri−​=ri+​,vi−​=vi+​(i=1,2,…,N−1)

  1. Iterative Correction: If the states at the connection point do not satisfy matching conditions, adjust the free parameters of each arc through differential correction or optimization algorithms until all patching conditions converge.

Application to Cislunar DRO Transfers

Wei et al. (2026), in their study of powered lunar flyby (PLF) transfer trajectories to cislunar DRO families, employed the patched method to split the trajectory at the perilune into two segments:

SegmentArc DescriptionDynamical ModelKey Parameters
Segment 1LEO to periluneEarth-Moon CR3BP or high-fidelity ephemeris modelLEO departure velocity, transfer time
Segment 2Perilune to DROEarth-Moon CR3BPPerilune altitude, DRO terminal state

At the perilune, the velocity directions of the two arcs may differ (since the lunar flyby changes the velocity vector direction). By introducing a Powered Lunar Flyby (PLF) maneuver at the perilune, an impulse can be applied to match the velocity vectors and complete the patching.

Mathematical Expression of Patching Conditions

Let the perilune state be (rpl,vpl)(\mathbf{r}_{\text{pl}}, \mathbf{v}_{\text{pl}})(rpl​,vpl​). The velocity at the end of Segment 1 is vpl−\mathbf{v}_{\text{pl}}^-vpl−​ and the velocity at the start of Segment 2 is vpl+\mathbf{v}_{\text{pl}}^+vpl+​. The patching conditions are:

rpl−=rpl+=rpl\mathbf{r}_{\text{pl}}^- = \mathbf{r}_{\text{pl}}^+ = \mathbf{r}_{\text{pl}} rpl−​=rpl+​=rpl​

vpl+=vpl−+ΔvPLF\mathbf{v}_{\text{pl}}^+ = \mathbf{v}_{\text{pl}}^- + \Delta \mathbf{v}_{\text{PLF}} vpl+​=vpl−​+ΔvPLF​

where ΔvPLF\Delta \mathbf{v}_{\text{PLF}}ΔvPLF​ is the velocity increment applied at the lunar flyby. When ΔvPLF=0\Delta \mathbf{v}_{\text{PLF}} = \mathbf{0}ΔvPLF​=0, this corresponds to a pure gravitational flyby (unpowered flyby), known as natural patching.

Comparison with Continuous Methods

FeaturePatched MethodContinuous Method (Direct Method)
Model usageDifferent models per segmentUnified model throughout
Computational efficiencyHigher (independent solution per segment)Lower (global optimization)
Physical interpretabilityStrong (each segment corresponds to a clear flight phase)Weaker
AccuracyDepends on patching point matching precisionDepends on discretization density
Applicable scenarioConceptual design, preliminary scheme screeningHigh-precision mission design

Limitations

  • Dynamical model switching at patching points may introduce discontinuous physical assumption errors
  • In strongly nonlinear regions (e.g., low-altitude flybys), segmented models may lack sufficient accuracy
  • Convergence of patching conditions depends on the quality of initial guesses

Application Value

In cislunar space mission design, the patched method is one of the most commonly used conceptual design tools:

  • DRO Injection Design: The patched method enables rapid screening of feasible transfer windows from LEO to DRO, evaluating Δv\Delta vΔv requirements under different launch conditions
  • Lunar Flyby Trajectory Design: By patching at the perilune, the method naturally incorporates lunar gravitational assist effects, reducing the energy required for transfer
  • Multi-Segment Transfer Schemes: For complex multi-body transfers involving Earth gravity assists and lunar gravity assists, the patched method provides an intuitive physical segmentation framework

Related Concepts

  • Circular Restricted Three-Body Problem (CR3BP)
  • Differential Correction
  • Transfer Orbit
  • Powered Lunar Flyby
  • Lunar Gravity Assist

References

  • Wei Z, et al. Research on powered lunar flyby transfer injection to cislunar distant retrograde orbit families[J]. Journal of Beijing University of Aeronautics and Astronautics, 2026.
  • Bate R R, Mueller D D, White J E. Fundamentals of Astrodynamics[M]. Dover Publications, 1971.
  • Stern S A, et al. Patched-conic and CR3BP methods for lunar transfer design[C]. AAS/AIAA Astrodynamics Specialist Conference, 2019.
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Last Updated: 4/29/26, 11:30 AM
Contributors: Cron Job
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