---
title: "Orbital Rendezvous in the Hill Frame Interactive Lab | Sandbox Physics"
description: "Does reaching the target also mean matching its velocity? No: getting there and matching speed are separate jobs. The first burn only aims the chaser at the target's position; it arrives with relative velocity left over, and a second burn at arrival must cancel it. Some flight times, such as exactly one orbit of the target, leave no usable aim. The simple linear model also drifts from true orbital motion, and arriving too fast still fails."
canonical_url: "https://sandboxphysics.com/labs/hill-rendezvous/"
language: "en"
page_type: "lab"
alternate_languages:
  zh-CN: "https://sandboxphysics.com/zh/labs/hill-rendezvous/"
last_modified: "2026-10-22"
---

M075 · Relative orbits and docking

# Orbital Rendezvous in the Hill Frame

**Does reaching the target also mean matching its velocity?** No: getting there and matching speed are separate jobs. The first burn only aims the chaser at the target's position; it arrives with relative velocity left over, and a second burn at arrival must cancel it. Some flight times, such as exactly one orbit of the target, leave no usable aim. The simple linear model also drifts from true orbital motion, and arriving too fast still fails.

Drag the chaser in the target’s rotating frame and solve for a two-burn rendezvous. Compare a coast with no burns, the Hill plan and a full two-body propagation, then try burn trims, a docking corridor, approach-speed limits and singular flight times.

> Interactive simulation: open this page in a web browser to change the parameters and run the model.

The planar Clohessy–Wiltshire model assumes the target is on a circular orbit and the separation is small compared with the orbit radius. Radial points right and along-track points up. Relative positions are in metres and time is in seconds. The purple propagation keeps full inverse-square gravity; it treats the central body as a point mass and ignores collisions with the planet. Trims are added to the solved departure velocity, and the final Hill braking burn is also applied to the nonlinear arrival.

Physics tutorial

## A rotating frame makes orbital rendezvous local

**Background** A nearby chaser and a target on a circular orbit are both falling under gravity. In the target’s rotating frame, the difference in radial gravity and the Coriolis terms couple the two relative coordinates. A forward burn can first carry the chaser forward while changing its orbit so that, over the long run, its along-track drift reverses.

**Why it matters** MIT’s astrodynamics notes derive the linear Clohessy–Wiltshire equations. This Lab uses one coordinate pointing radially outward and one pointing forward along the track. It solves the planar endpoint map and, as an independent check, propagates the same starting state in full inverse-square gravity.

Start with the essentials

- **Focus question**: Can a two-burn plan reach the target and stay inside the approach corridor?
- **One-sentence intuition**: Solving for the endpoint puts the chaser at the target and a separate burn on arrival matches its velocity, but the plan can still fail if the endpoint map is singular, the nonlinear error is large or the chaser comes in too fast.

### Core mathematical model

#### Coupled equations of relative motion

$$
n=\sqrt{\frac{\mu}{r_c^3}},\qquad \ddot x-2n\dot y-3n^2x=0,\quad\ddot y+2n\dot x=0
$$

The target’s orbit must be circular. The Coriolis coupling is why the intuition of chasing in a straight line fails. Motion out of the orbital plane is left out.

#### Solving for the departure velocity

$$
\mathbf r_f=A(t_f)\mathbf r_0+B(t_f)\mathbf v_0^+,\quad\mathbf v_0^+=-B(t_f)^{-1}A(t_f)\mathbf r_0
$$

The departure velocity is chosen so that the chaser ends up at the target position. The chaser’s initial velocity changes the cost of the departure burn, not the solved velocity itself.

#### Velocity-to-position map

$$
nB(t)=\begin{pmatrix}\sin nt&2(1-\cos nt)\\-2(1-\cos nt)&4\sin nt-3nt\end{pmatrix}
$$

After exactly one target period this matrix loses rank. The code scales it by the mean motion and rejects plans whose condition number is above one thousand.

#### The two burns and their total cost

$$
\Delta\mathbf v_1=\mathbf v_0^+-\mathbf v_0^-,\quad\Delta\mathbf v_2=-\mathbf v_f^-,\qquad\Delta v=\lVert\Delta\mathbf v_1\rVert+\lVert\Delta\mathbf v_2\rVert
$$

The second burn cancels the actual Hill arrival velocity, trim included. Applied to the nonlinear arrival, the same vector leaves a residual speed that you can measure.

#### A quantity conserved while coasting

$$
\mathcal C=\dot x^2+\dot y^2-3n^2x^2,\qquad \frac{d\mathcal C}{dt}=0
$$

This quadratic integral belongs to the Hill model with no burns. It is not the spacecraft’s energy in the inertial frame.

#### Converting to the inertial frame for the two-body check

$$
\mathbf R=Q(nt)\left[\begin{pmatrix}r_c\\0\end{pmatrix}+\mathbf r\right],\quad\mathbf V=Q(nt)\left[\dot{\mathbf r}+nJ\left(\begin{pmatrix}r_c\\0\end{pmatrix}+\mathbf r\right)\right],\quad J=\begin{pmatrix}0&-1\\1&0\end{pmatrix}
$$

Rotating the velocity must include the term from the frame’s own rotation; leaving it out gives the wrong inertial starting state. Units are converted before propagation.

### Common difficulties

#### Meeting is not docking

**Typical misconception** If the position error is zero, the relative speed is zero too.

**Better mental model** The chaser usually still has some velocity on arrival until the braking burn. Check the incoming speed separately.

#### The linear model is not exact

**Typical misconception** An exact Hill endpoint means an exact two-body rendezvous.

**Better mental model** The purple trajectory starts from the same physical state but keeps nonlinear gravity. Its position and residual-velocity errors grow with separation.

#### Some flight times have no unique burn

**Typical misconception** Every flight time gives a unique, finite burn.

**Better mental model** At certain times the endpoint map loses rank. When a plan is rejected, the coast with no burn is shown instead.

#### Passing sampled checks does not prove safety

**Typical misconception** A green sample check guarantees collision avoidance at every instant.

**Better mental model** The cone includes a one-metre allowance at the port, and the check covers nine hundred intervals. It cannot catch violations between samples or operational physics that the model leaves out.

### Run the experiment

1. 01

   #### Run the nominal approach

   Acquire the nominal approach and compare the Hill miss, the full-gravity miss and the residual speed.

   **What to observe:** The Hill plan reaches the target exactly, while the nonlinear residual stays small but not zero.

2. 02

   #### Compare the coasts

   Choose the forward-impulse preset and look at the gray no-burn trajectory.

   **What to observe:** A forward kick sets off coupled radial motion and changes the along-track drift. The departure burn has to pay to bring the chaser back to the planned start.

3. 03

   #### Break the plan

   Select a flight time of one whole period, or add a small along-track trim.

   **What to observe:** The singular plan is rejected. A trim leaves a finite position miss that remains even after braking.

4. 04

   #### Check the approach

   Tighten the speed limit, then increase the release separation.

   **What to observe:** A zero miss at the endpoint does not stop the approach from being too fast, and it does not stop the linearisation error from growing.

Physical conclusion

Plan with the linear approximation, and use its mismatch with full gravity to judge when it can be trusted.

Motion & dynamics · Starter path

## From a falling ball to an orbit

Start by measuring gravity and splitting motion into components. Then add contact forces and collisions, and follow the same laws all the way to an orbit.

[Start here → **Free Fall & Measuring Gravity** Capture a few drops and fit the camera positions to estimate gravitational acceleration. Then add air damping and watch the fit drift from the truth. Observe · 14 min](https://sandboxphysics.com/labs/free-fall/)

1. [1 Free Fall & Measuring Gravity](https://sandboxphysics.com/labs/free-fall/)
2. [2 Projectile Flight Designer](https://sandboxphysics.com/labs/projectile-flight/)
3. [3 Inclined Plane & Friction](https://sandboxphysics.com/labs/inclined-plane/)
4. [4 One-Dimensional Collision Bench](https://sandboxphysics.com/labs/collision-bench/)
5. [5 Mass–Spring Oscillator](https://sandboxphysics.com/labs/mass-spring/)
6. [6 How Orbits Take Shape](https://sandboxphysics.com/labs/orbit/)

[View the full path →](https://sandboxphysics.com/topics/mechanics/#starter-path)