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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
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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
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      • /en/glossary/other/orbital-residence-platform.html
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    • Observation techniques

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Low Earth Orbit (LEO)

Author: CislunarSpace

Website: https://cislunarspace.cn

Definition

Low Earth Orbit (LEO) refers to orbits around the Earth at altitudes between approximately 200 km and 2000 km above the Earth's surface. LEO is the most commonly used orbit type in human spaceflight activities, hosting the vast majority of crewed spacecraft, Earth observation satellites, and space stations.

The orbital period of LEO is approximately 90–120 minutes, depending on the specific altitude. For example, the International Space Station (ISS) operates in a near-circular orbit at approximately 400 km altitude with an orbital period of about 92 minutes. The LEO orbital velocity is approximately v≈7.7 km/sv \approx 7.7 \text{ km/s}v≈7.7 km/s (at 400 km altitude).

Core Elements

Orbital Mechanics Parameters

The key mechanical parameters of LEO can be calculated using Kepler's laws. For a circular orbit of radius rrr, the orbital velocity is:

v=μErv = \sqrt{\frac{\mu_E}{r}} v=rμE​​​

where μE=3.986×105 km3/s2\mu_E = 3.986 \times 10^{5} \text{ km}^3/\text{s}^2μE​=3.986×105 km3/s2 is Earth's gravitational parameter. The characteristic velocity Δv\Delta vΔv requirement for LEO is relatively low, making it the most economical orbit to reach from the ground.

LEO as Parking Orbit

In Earth-Moon transfer missions, LEO typically serves as the spacecraft's parking orbit. The launch vehicle first delivers the spacecraft to LEO, and then at the appropriate phase and timing, an Earth-Moon transfer impulse is applied to enter the transfer trajectory.

This "LEO parking — Earth-Moon transfer" mission architecture offers several advantages:

  1. Mission flexibility: The spacecraft can wait in LEO for the optimal launch window, rather than being strictly constrained by ground-based launch windows.
  2. System verification: During the LEO parking phase, all spacecraft systems can be thoroughly checked before executing the deep space transfer.
  3. On-orbit assembly: Large missions can be assembled and resupplied in LEO, relaxing the mass constraints of a single launch.

LEO De-orbit Impulse for Lunar Transfer

The Earth-Moon transfer from LEO typically requires a de-orbit impulse Δv1\Delta v_1Δv1​. For direct transfer to the lunar vicinity, this impulse magnitude depends on the transfer trajectory design. In powered lunar flyby (PLF) transfer schemes, the LEO de-orbit impulse is the first impulse of the three-burn transfer, and its magnitude directly affects the shape of the subsequent transfer trajectory and the state upon reaching the Moon.

Typically, the Δv1\Delta v_1Δv1​ required for direct transfer from a 200 km LEO to the lunar vicinity is approximately 3.1–3.2 km/s, slightly less than the theoretical Hohmann transfer value. By optimizing the transfer trajectory design (such as selecting the appropriate C3 energy), trade-offs can be made between Δv1\Delta v_1Δv1​ and subsequent impulses.

Atmospheric Drag and Orbital Decay

The primary perturbation factor for LEO is atmospheric drag. Although atmospheric density is extremely thin above 400 km, spacecraft in long-term operation still require periodic orbit maintenance. The orbital decay rate due to atmospheric drag is closely related to the spacecraft's ballistic coefficient (β=m/CDA\beta = m/C_D Aβ=m/CD​A) and atmospheric density.

Application Value

LEO serves not only as the starting point for space activities but also as a key node in cislunar space infrastructure:

  • Space stations: China's Tiangong Space Station and the International Space Station both operate in LEO, providing platforms for long-duration human spaceflight.
  • Satellite constellations: Large communication constellations such as Starlink and OneWeb are deployed in LEO.
  • Cislunar transportation hub: LEO is expected to evolve into a "transportation hub" for cislunar space, handling on-orbit refueling and cargo transfer functions.

Related Concepts

  • Cislunar Space
  • Parking Orbit
  • Transfer Orbit
  • Powered Lunar Flyby (PLF)

References

  • Wei Z et al., "Research on Lunar Flyby Transfer to Distant Retrograde Orbit Families in the Earth-Moon System", 2026.
  • Vallado D A, "Fundamentals of Astrodynamics and Applications", 4th ed., Microcosm Press, 2013.
  • Wertz J R, Everett D F, Puschell J J, "Space Mission Engineering: The New SMAD", Microcosm Press, 2011.
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Last Updated: 4/29/26, 11:30 AM
Contributors: Cron Job
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