Skip to content

A lightweight, optimized C++ implementation of the RRT* algorithm for ROS or standalone.

Notifications You must be signed in to change notification settings

sportdeath/motion_planning

Repository files navigation

A lightweight, optimized C++ implementation of the RRT* algorithm. This package is compatible with the robotic operating system (ROS), but it can also be built as a standalone package.

Dependencies

This library requires the libpng library. On Ubuntu it can be installed with:

sudo apt-get install libpng-dev

On Arch Linux it can be installed with:

sudo pacman -S libpng

Or to install manually:

git clone git://git.code.sf.net/p/libpng/code libpng
cd libpng
./autogen.sh
./configure --prefix=[INSTALL_PATH]
make check
make install

Standalone Build

If you don't want to install this library with ROS, simply clone the library and build using CMake.

git clone git@github.com:sportdeath/motion_planning.git
cd motion_planning
mkdir build
cd build
cmake ..
make

If you want to build the tests, you will need the Google Test submodule. You can fetch it as you clone:

git clone --recurse-submodules git@github.com:sportdeath/motion_planning.git

Or get it afterwards:

git submodule update --init --recursive

ROS Build

To build as a ROS package, use the catkin system:

cd catkin_ws/src
git clone git@github.com:sportdeath/motion_planning.git
cd catkin_ws
catkin_make

Usage

In order to compute RRT*, you must first describe the vehicle dynamics, the map, and the sampling function.

Vehicle Dynamics

You must define vehicle dynamics that inherit from the Steer class, which describes the shortest path between any two points in free space. For a robot that can move in any direction these paths would just be straight lines. For more constrained robots, like cars, these paths become more complicated.

This library comes with ReedsSheepSteer, which models a simple car that can drive forwards and backwards along straight lines and cricles. It can be defined with the minimum turning radius. For example if the car is able to turn around a 0.3m circle, you would do:

ReedsSheepSteer steer(0.3)

Map

You must define a map that inherits from the Occupancy class. This library comes with OccupancyGrid2D which is a standard 2D occupancy grid. These maps can be built in a variety of ways, for example with a vector of occupancy values

OccupancyGrid2D<Pose2D> occ;
size_t height = 100;
size_t width = 100;
std::vector<double> occupancyValues(height * width, 0.) // A vector of HxW zeros
double mapResolution = 0.05;
Pose2D mapOrigin = {.x=0, .y=0, .theta=0}; // The coordinates of the top left cell
occ.setMap(occupancyValues, width, height, mapResolution, mapOrigin);

Or frome a grayscale PNG:

...
occ.setMap("maps/tiny.png", mapResolution, mapOrigin);

The occupancy grid includes a distance transform.

Sampling Function

Because RRT* is a sample-based algorithm, you must define the function used to sample states on the map. This library comes with a variety of sampling algorithms like uniform sampling, gaussian sampling, and bridge sampling (useful for narrow passages). These sampling algorithms all inherit from the StateSampler class.

UniformSampler<Pose2D> uni(&occ); 
BridgeSampler brg(&occ, 0.1); // 0.1 defines the stddev of the bridge

// Use uniform with probability 0.3 and
// bridge with probability 0.7
std::vector<StateSampler<Pose2D> *> samplers = {&uni, &brg};
std::vector<double> sampler_weights = {3., 7.};
MixedSampler<Pose2D> sampler(samplers, weights);

Computing RRT*

Once the dynamics, map, and sampling are computed they can by used to construct RRT*. In addition we will need the origin of the search, and the search radius which describes the distance at which points are connected.

Pose2d rrtOrigin = {.x=3, .y=4, .theta=0.5};
double rrt
RRTStar<Pose2D> rrt(
    &steer,
    &occ,
    sampler.sampleFunction(),
    rrtOrigin,
    rrtRadius);

Once RRT* has been constructed, you can iterate by running something like:

int numNodes = 0;
for (int i = 0; i < 1000; i++) {
    if (rrt.iterate()) numNodes++;
}

There are a variety of ways to interact with the resulting tree. For example you could get the root and use it in its tree structure:

const RRTStar<Pose2D>::Node & root = rrt.root();

// Look at the state of the node
Pose2D nodeState = node.state;

// Or look at its parent
// (the root's parent is NULL)
RRTStar<Pose2D>::Node * nodeParent = node.parent;

// Or look at its children
std::vector<Node *> children = node.parent;

Or you could iterate over all the nodes in the tree:

for (const RRTStar<Pose2D>::Node & node : rrt.getNodes()) {
    ...
}

Or you could sample it as a list of states:

// The path from the root to someNode
// sampled every 0.1 meters
std::vector<Pose2D> path = rrt.samplePath(&someNode, 0.1);

TODO

  • make config.cmake file
  • Make ROS node parameterized.
  • Document distance transform
  • Document profiling
  • Add images/gif to README
  • Add line steering function.

About

A lightweight, optimized C++ implementation of the RRT* algorithm for ROS or standalone.

Resources

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published