Telemetry Log & Real-Time Event Stream
Real-time record of thruster firings, corridor entry gates, attitude hold corrections, and range milestones.
Orbital Rendezvous Physics: Clohessy-Wiltshire Equations
In low Earth orbit (420 km altitude, orbital speed ~7.66 km/s), maneuvers in proximity to the International Space Station do not obey intuitive linear physics. An eastward burn (speeding up) raises your orbital apogee, causing the spacecraft to drift upwards and backwards relative to the station due to Kepler's third law.
The Clohessy-Wiltshire (Hill's) Equations formulate relative motion in the Local-Vertical Local-Horizontal (LVLH) coordinate frame:
• +V-bar (X): Along the station's orbital velocity vector.
• +R-bar (Z): Radial vector pointing towards Earth center.
• +H-bar (Y): Out-of-plane cross-track angular momentum vector.