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  • Cislunar spacecraft orbits (mission trajectories)

    • Cislunar Spacecraft Orbits
    • NRHO (Near-Rectilinear Halo Orbit)
      • NRHO (Near-Rectilinear Halo Orbit)
      • L1 Near-Rectilinear Halo Orbit
      • L2 Near-Rectilinear Halo Orbit
      • NRHO Stability and Station-Keeping
      • Gateway Engineering Case Study
      • NRHO Design Parameters
    • DRO (Distant Retrograde Orbit)
      • DRO (Distant Retrograde Orbit)
      • DRO Dynamics Mechanism
      • DRO Family Classification
      • DRO Engineering Applications
      • DRO Design Methods
    • Earth-Moon Transfer Orbits
      • Earth-Moon Transfer Orbit
      • TLI Overview
      • Ballistic Capture
      • Transfer Corridor Design
      • Launch Window Analysis

Author: CislunarSpace

Source: https://cislunarspace.cn

Earth-Moon Transfer Orbit

Definition and Classification

An Earth-Moon transfer orbit is the orbital segment connecting a Low Earth Orbit (LEO) to a target orbit in cislunar space, such as an NRHO, DRO, or the lunar surface. Depending on the transfer strategy, these orbits can be classified as follows:

Impulsive Transfer

Uses one or a few high-thrust maneuvers to complete the transfer, typically a Hohmann Transfer or a direct trans-lunar injection. The typical ΔV\Delta VΔV from LEO to TLI (Trans-Lunar Injection) is approximately 3.1–3.3 km/s.

Low-Energy Transfer

Exploits the dynamical characteristics of the Earth-Moon system — such as the Weak Stability Boundary (WSB) and stable manifolds of halo orbits — to achieve transfer at a lower energy cost. The trade-off is a significantly longer transfer time, ranging from several weeks to months. The Weak Stability Boundary transfer is a representative example.

Ballistic Capture Transfer

Uses lunar gravity assist so that the spacecraft is "captured" by the Moon's gravity upon approach without requiring propulsion. A small maneuver is then performed to enter the target orbit. This method can substantially save propellant but demands precise launch timing.

Energy Budget

The energy requirement for an Earth-Moon transfer is commonly characterized by the hyperbolic excess velocity (C3C_3C3​):

C3=v2−2μrC_3 = v^2 - \frac{2\mu}{r} C3​=v2−r2μ​

where vvv is the spacecraft's velocity in the Earth-centered inertial frame and μ\muμ is Earth's gravitational parameter.

From LEO (185 km circular orbit) to TLI, the typical C3≈−0.5C_3 \approx -0.5C3​≈−0.5 km2^22/s2^22 (corresponding to v≈10.9v \approx 10.9v≈10.9 km/s), with a required ΔV≈3.1−3.3\Delta V \approx 3.1-3.3ΔV≈3.1−3.3 km/s.

Transfer Time vs. Energy Tradeoff

Earth-Moon transfer is a classic bi-objective optimization problem balancing time and fuel:

Transfer TypeTypical DurationTypical ΔVSuitable For
Direct transfer3–5 days~3.2 km/sUrgent missions, cargo
Low-energy transfer2–4 weeks~3.0 km/sCrewed missions, probes
Ballistic capture1–3 months~2.9 km/sSmall probes, CubeSats

Rendezvous with NRHO and DRO

After arriving in cislunar space, the spacecraft must perform rendezvous and docking or orbit insertion with the target orbit:

  • NRHO rendezvous: Orbit insertion maneuver near the L1 point (ΔV≈200−400\Delta V \approx 200-400ΔV≈200−400 m/s) to enter the NRHO.
  • DRO rendezvous: Insertion maneuver when approaching the target DRO (ΔV≈100−300\Delta V \approx 100-300ΔV≈100−300 m/s).
  • Lunar surface rendezvous: Descent maneuver from NRHO or transfer orbit to the lunar surface (ΔV≈1.5−2.0\Delta V \approx 1.5-2.0ΔV≈1.5−2.0 km/s).

Simulation

You can design Earth-Moon transfer orbits in the Satellite Orbit Simulation Lab and observe transfer trajectories under different C3C_3C3​ values and launch windows.

Related Concepts

  • NRHO (Near-Rectilinear Halo Orbit)
  • DRO (Distant Retrograde Orbit)
  • TLI Overview
  • Ballistic Capture
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Last Updated: 4/26/26, 2:35 PM
Contributors: Hermes Agent
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