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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
      • Low-Energy Transfer Orbit
      • Full Lunar Surface Coverage Orbit
      • /en/glossary/orbits/hub-and-spoke.html
    • Navigation

      • X-ray Pulsar Navigation
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    • Lunar minerals

      • Changeite-Mg (Magnesium Changeite)
      • Changeite-Ce (Cerium Changeite)
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      • Starshade
      • Noncooperative Target
      • Spacecraft Intention Recognition
      • Chain-of-Thought (CoT) Prompting
      • Low-Rank Adaptation (LoRA)
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      • Cislunar Space (地月空间)
      • Low Earth Orbit / LEO (低地球轨道)
      • Lunar Gravity Assist / LGA (月球借力)
      • Powered Lunar Flyby / PLF (有动力月球借力)
      • Weak Stability Boundary / WSB (弱稳定边界)
      • /en/glossary/other/libration-point.html
      • Orbit Insertion (入轨)
      • /en/glossary/other/orbital-residence-platform.html
    • Organizations

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    • Observation techniques

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    • Satellite Communication & TT&C

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Transfer Orbit

Author: CislunarSpace

Website: https://cislunarspace.cn

Definition

A transfer orbit is an intermediate trajectory used to move a spacecraft from an initial orbit to a target orbit. In cislunar missions, transfer orbit design is one of the core problems in orbital mechanics, requiring trade-offs between transfer time and fuel consumption. The shape of a transfer orbit depends on the geometric relationship between the departure and target orbits, available thrust, and mission time constraints.

Key Elements

Basic Types of Transfer Orbits

Transfer orbits can be classified by thrust mode:

  • Impulsive Transfer: Assumes thrust is applied instantaneously, achieving orbital changes through a finite number of velocity increments ΔV\Delta VΔV. The classical Hohmann transfer is a two-impulse transfer representative, suitable for transfers between near-circular orbits.
  • Low-Thrust Transfer: Thrust is continuous but small in magnitude, resulting in a gradually evolving spiral trajectory. Electric propulsion systems commonly use this mode, offering higher fuel efficiency at the cost of longer transfer times.
  • Gravity-Assisted Transfer: Uses celestial gravity to change orbital energy and direction without additional fuel consumption. Lunar gravity assist is a key technique in cislunar transfers.

Energy-Time Trade-off

The core challenge in transfer orbit design is the Pareto optimality between energy and time. Transfer time tft_ftf​ and total velocity increment ΔVtotal\Delta V_{\text{total}}ΔVtotal​ are inversely related:

ΔVtotal=∑i=1n∣Δvi∣\Delta V_{\text{total}} = \sum_{i=1}^{n} |\Delta \mathbf{v}_i| ΔVtotal​=i=1∑n​∣Δvi​∣

where nnn is the number of impulses. Generally, shorter transfers require larger ΔV\Delta VΔV; conversely, slower transfers save fuel but extend mission duration.

Specifics of Cislunar Transfer

Key differences between cislunar and interplanetary transfers include:

  • Three-body gravity field: Both Earth and Moon gravity act simultaneously, requiring transfer orbit design within the restricted three-body problem framework
  • Lunar gravity assist windows: Precise control of perilune altitude enables significant orbital energy changes via lunar gravity
  • Multiple target orbits: Targets include DRO, NRHO, Halo orbits, each imposing different design constraints on the transfer orbit

Application Value

Transfer orbit design has critical applications in cislunar missions:

  • Crewed lunar missions: Transferring from Earth parking orbit to lunar orbit or the lunar surface
  • Cargo resupply missions: Delivering supplies to mission orbits like DRO or NRHO while optimizing fuel consumption to maximize payload mass
  • Constellation deployment: Using multi-launch combined with elegant transfer orbit designs to place multiple satellites into different target orbits
  • Emergency return: Free-return transfer orbits provide crewed missions the ability to safely return to Earth without additional propulsion

Related Concepts

  • Distant Retrograde Orbit (DRO)
  • Near-Rectilinear Halo Orbit (NRHO)
  • Lunar Gravity Assist
  • Impulsive Maneuver
  • Parking Orbit
  • Free-Return Trajectory

References

  • Hohmann W. Die Erreichbarkeit der Himmelskörper[M]. 1925.
  • Wei Z et al. Research on lunar gravity-assist injection into cislunar distant retrograde orbit families[J]. 2026.
  • Broucke R. Periodic orbits in the restricted three-body problem with Earth-Moon masses[R]. 1968.
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Last Updated: 4/29/26, 11:30 AM
Contributors: Cron Job
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