This fork was originally intended to make the module compatible with Browserify, however now that has been acheived I also intend to refactor it a bit and make it feel more OO.
A library to make satellite propagation via TLEs possible in the web. Provides the functions necessary for SGP4/SDP4 calculations, as callable javascript. Also provides functions for coordinate transforms.
The internals of this library are nearly identical to Brandon Rhode's sgp4 python library. However, it is encapsulated in a standard JS library (self executing function), and exposes only the functionality needed to track satellites and propagate paths. The only changes I made to Brandon Rhode's code was to change the positional parameters of functions to key:value objects. This reduces the complexity of functions that require 50+ parameters, and doesn't require the parameters to be placed in the exact order.
Special thanks to ezze, for modernizing the code and greatly improving usability =)
Start Here:
- TS Kelso's Columns for Satellite Times, Orbital Propagation Parts I and II a must!
- Wikipedia: Simplified Perturbations Model
- SpaceTrack Report #3, by Hoots and Roehrich.
The javascript in this library is heavily based (straight copied) from:
- The python sgp4 1.1 by Brandon Rhodes
- The C++ code by David Vallado, et al
I've included the original PKG-INFO file from the python library.
The coordinate transforms are based off T.S. Kelso's columns:
And the coursework for UC Boulder's ASEN students
I would recommend anybody interested in satellite tracking or orbital propagation to read all of TS Kelso's columns. Without his work, this project would not be possible.
Get a free Space Track account and download your own up to date TLEs for use with this library.
Install the library with Bower:
bower install satellite.js
Install the library with NPM:
npm install satellite.js
Include dist/satellite.min.js as a script in your html or use as Require.js module.
When you include satellite.min.js as a script, the object satellite is defined in global scope.
You use this object to access all the functions in the satellite library:
var positionAndVelocity = satellite.sgp4(satrec, time);
When you use it as Require.js module satellite object is not defined in global scope, you should use it as
a dependency of your module:
define(['path/to/satellite'], function(satellite) {
...
var positionAndVelocity = satellite.sgp4(satrec, time);
});
// Sample TLE
var tleLine1 = '1 25544U 98067A 13149.87225694 .00009369 00000-0 16828-3 0 9031',
tleLine2 = '2 25544 051.6485 199.1576 0010128 012.7275 352.5669 15.50581403831869';
// Initialize a satellite record
var satrec = satellite.twoline2satrec(tleLine1, tleLine2);
// Propagate satellite using time since epoch (in minutes).
var positionAndVelocity = satellite.sgp4 (satrec, timeSinceTleEpochMinutes);
// Or you can use a calendar date and time (obtained from Javascript Date).
var now = new Date();
// NOTE: while Javascript Date returns months in range 0-11, all satellite.js methods require
// months in range 1-12.
var positionAndVelocity = satellite.propagate(
satrec,
now.getUTCFullYear(),
now.getUTCMonth() + 1, // Note, this function requires months in range 1-12.
now.getUTCDate(),
now.getUTCHours(),
now.getUTCMinutes(),
now.getUTCSeconds()
);
// The position_velocity result is a key-value pair of ECI coordinates.
// These are the base results from which all other coordinates are derived.
var positionEci = positionAndVelocity.position,
velocityEci = positionAndVelocity.velocity;
// Set the Observer at 122.03 West by 36.96 North, in RADIANS
var observerGd = {
longitude: -122.0308 * deg2rad,
latitude: 36.9613422 * deg2rad,
height: 0.370
};
// You will need GMST for some of the coordinate transforms.
// http://en.wikipedia.org/wiki/Sidereal_time#Definition
// NOTE: GMST, though a measure of time, is defined as an angle in radians.
// Also, be aware that the month range is 1-12, not 0-11.
var gmst = satellite.gstimeFromDate(
now.getUTCFullYear(),
now.getUTCMonth() + 1, // Note, this function requires months in range 1-12.
now.getUTCDate(),
now.getUTCHours(),
now.getUTCMinutes(),
now.getUTCSeconds()
);
// You can get ECF, Geodetic, Look Angles, and Doppler Factor.
var positionEcf = satellite.eciToEcf(positionEci, gmst),
observerEcf = satellite.geodeticToEcf(observerGd),
positionGd = satellite.eciToGeodetic(positionEci, gmst),
lookAngles = satellite.ecfToLookAngles(observerGd, positionEcf),
dopplerFactor = satellite.dopplerFactor(observerCoordsEcf, positionEcf, velocityEcf);
// The coordinates are all stored in key-value pairs.
// ECI and ECF are accessed by `x`, `y`, `z` properties.
var satelliteX = positionEci.x,
satelliteY = positionEci.y,
satelliteZ = positionEci.z;
// Look Angles may be accessed by `azimuth`, `elevation`, `range_sat` properties.
var azimuth = lookAngles.azimuth,
elevation = lookAngles.elevation,
rangeSat = lookAngles.rangeSat;
// Geodetic coords are accessed via `longitude`, `latitude`, `height`.
var longitude = positionGd.longitude,
latitude = positionGd.latitude,
height = positionGd.height;
// Convert the RADIANS to DEGREES for pretty printing (appends "N", "S", "E", "W". etc).
var longitudeStr = satellite.degreesLong(longitude),
latitudeStr = satellite.degreesLat(latitude);
The code is organized as AMD modules but it can be built into a single file to use in production.
The library uses Grunt task runner for building and testing. It also relies on Bower package of Require.js plugins needed for test scripts. In order to run Grunt tasks follow these steps:
-
install Node.js and Node Package Manager;
-
install Grunt command line interface globally:
npm install -g grunt-cli -
install Bower globally:
npm install -g bower -
install all required packages with NPM and Bower by running the following commands from repository's root directory:
npm install bower install -
run default Grunt task to build the library:
grunt -
run the following Grunt task to run Jasmine specs located in
test/*.spec.jsfiles with Karma:grunt test
All configuration files for Grunt tasks are located in grunt directory.
These are main available Grunt tasks:
build(default) validates, optimizies and minifies source code todistdirectory;cleanremoves all built files;testtests the library by running Jasmine specs.
Optional functions that utilize Worker Threads
The satrec object comes from the original code by Rhodes as well as Vallado. It is immense and complex, but the
most important values it contains are the Keplerian Elements and the other values pulled from the TLEs. I do not
suggest that anybody try to simplify it unless they have absolute understanding of Orbital Mechanics.
satnumUnique satellite number given in the TLE file.epochyrFull four-digit year of this element set's epoch moment.epochdaysFractional days into the year of the epoch moment.jdsatepochJulian date of the epoch (computed fromepochyrandepochdays).ndotFirst time derivative of the mean motion (ignored by SGP4).nddotSecond time derivative of the mean motion (ignored by SGP4).bstarBallistic drag coefficient B* in inverse earth radii.incloInclination in radians.nodeoRight ascension of ascending node in radians.eccoEccentricity.argpoArgument of perigee in radians.moMean anomaly in radians.noMean motion in radians per minute.
var satrec = satellite.twoline2satrec(longstr1, longstr2)
returns satrec object, created from the TLEs passed in. The satrec object is vastly complicated, but you don't have to do anything with it, except pass it around.
NOTE! You are responsible for providing TLEs. Get your free Space Track account here. longstr1 and longstr2 are the two lines of the TLE, properly formatted by NASA and NORAD standards. if you use Space Track, there should be no problem.
Both propagate() and sgp4() functions return position and velocity as a dictionary of the form:
{
"position" : { "x" : 1, "y" : 1, "z" : 1 },
"velocity" : { "x" : 1, "y" : 1, "z" : 1 }
}
position is in km, velocity is in km/s, both the ECI coordinate frame.
var now = new Date();
// NOTE: while Javascript Date returns months in range 0-11, all satellite.js methods require months in range 1-12.
var positionAndVelocity = satellite.propagate(
satrec,
now.getUTCFullYear(),
now.getUTCMonth() + 1, // Note, this function requires months in range 1-12.
now.getUTCDate(),
now.getUTCHours(),
now.getUTCMinutes(),
now.getUTCSeconds()
);
Returns position and velocity, given a satrec and the calendar date. Is merely a wrapper for sgp4(), converts the
calendar day to Julian time since satellite epoch. Sometimes it's better to ask for position and velocity given
a specific date.
var positionAndVelocity = satellite.sgp4(satrec, timeSinceTleEpochMinutes)
Returns position and velocity, given a satrec and the time in minutes since epoch. Sometimes it's better to ask for position and velocity given the time elapsed since epoch.
You can get the satellites current Doppler factor, relative to your position, using the dopplerFactor() function.
Use either ECI or ECF coordinates, but don't mix them.
var dopplerFactor = satellite.dopplerFactor(observer, position, velocity);
See the section on Coordinate Transforms to see how to get ECF/ECI/Geodetic coordinates.
You'll need to provide some of the coordinate transform functions with your current GMST aka GSTIME. You can use Julian Day or a calendar date.
var gmst = satellite.gstimeFromJday(julianDay)
// Also, be aware that the month range is 1-12, not 0-11.
var now = new Date();
var gmst = satellite.gstimeFromDate(
now.getUTCFullYear(),
now.getUTCMonth() + 1, // Note, this function requires months in range 1-12.
now.getUTCDate(),
now.getUTCHours(),
now.getUTCMinutes(),
now.getUTCSeconds()
);
Most of these are self explanatory from their names. Coords are arrays of three floats EX: [1.1, 1.2, 1.3] in kilometers. Once again, read the following first.
The coordinate transforms are based off T.S. Kelso's columns:
And the coursework for UC Boulder's ASEN students
These four are used to convert between ECI, ECF, and Geodetic, as you need them. ECI and ECF coordinates are in km or km/s. Geodetic coords are in radians.
var ecfCoords = satellite.eciToEcf(eciCoords, gmst);
var eciCoords = satellite.ecfToEci(ecfCoords, gmst);
var geodeticCoords = satellite.eciToGeodetic(eciCoords, gmst);
var ecfCoords = satellite.geodeticToEcf(geodeticCoords);
These function is used to compute the look angle, from your geodetic position to a satellite in ECF coordinates. Make sure you convert the ECI output from sgp4() and propagate() to ECF first.
var lookAngles = satellite.ecfToLookAngles = function(observerGeodetic, satelliteEcf);
These two functions will return human readable Latitude or Longitude strings (Ex: "125.35W" or "45.565N")
from geodeticCoords:
var latitudeStr = satellite.degreesLat(geodeticRadians),
longitudeStr = satellite.degreesLong(geodeticRadians);
Like Brandon Rhodes before me, I chose to maintain as little difference between this implementation and the prior works. This is to make adapting future changes suggested by Vallado much simpler. Thus, some of the conventions used in this library are very weird.
I took advantage of the fact that Python and JavaScript are nearly semantically identical. Most of the code is just copied straight from Python. Brandon Rhodes did me the favor of including semi-colons on most of the lines of code. JavaScript doesn't support multiple values returned per statement, so I had to rewrite the function calls. Absolutely none of the mathematical logic had to be rewritten.
I've included a small testing app, that provides some benchmarking tools and verifies SGP4 and SDP4 using the Test Criteria provided by SpaceTrack Report #3, and is based off System Benchmarking by TS Kelso.
The testing app is a Chrome Packaged App that uses the angular.js framework.
To run the test, open up Chrome, go to the extensions page, and check "Developer Mode". Then, click "Load Unpacked App",
and select the sgp4_verification folder. Then run the app from within Chrome. The test file is located within
the sgp4_verification directory, as a JSON file called spacetrack-report-3.json.
Major thanks go to Brandon Rhodes, TS Kelso, and David Vallado's team. Also, I'd like to thank Professor Steve Petersen (AC6P) of UCSC for pointing me in the correct directions.
All files marked with the License header at the top are Licensed. Any files unmarked by me or others are unlicensed, and are kept only as a resource for [Shashwat Kandadai and other developers] for testing.
I chose the MIT License because this library is a derivative work off Brandon Rhodes sgp4, and that is licensed with MIT. It just seemed simpler this way, sub-licensing freedoms notwithstanding.
I worked in the Dining Hall at UCSC for a month, which means I signed a form that gives UCSC partial ownership of anything I make while under their aegis, so I included them as owners of the copyright.
Please email all complaints to help@ucsc.edu