JavaScript function to calculate the destination point given start point latitude and longitude (numeric degrees), bearing (numeric degrees) and distance (in m), based on the Vincenty direct formula.

/*!
 * JavaScript function to calculate the destination point given start point latitude / longitude (numeric degrees), bearing (numeric degrees) and distance (in m).
 *
 * Original scripts by Chris Veness
 * Taken from http://movable-type.co.uk/scripts/latlong-vincenty-direct.html and optimized / cleaned up by Mathias Bynens <http://mathiasbynens.be/>
 * Based on the Vincenty direct formula by T. Vincenty, “Direct and Inverse Solutions of Geodesics on the Ellipsoid with application of nested equations”, Survey Review, vol XXII no 176, 1975 <http://www.ngs.noaa.gov/PUBS_LIB/inverse.pdf>
 */
function toRad(n) {
 return n * Math.PI / 180;
};
function toDeg(n) {
 return n * 180 / Math.PI;
};
function destVincenty(lat1, lon1, brng, dist) {
 var a = 6378137,
     b = 6356752.3142,
     f = 1 / 298.257223563, // WGS-84 ellipsiod
     s = dist,
     alpha1 = toRad(brng),
     sinAlpha1 = Math.sin(alpha1),
     cosAlpha1 = Math.cos(alpha1),
     tanU1 = (1 - f) * Math.tan(toRad(lat1)),
     cosU1 = 1 / Math.sqrt((1 + tanU1 * tanU1)), sinU1 = tanU1 * cosU1,
     sigma1 = Math.atan2(tanU1, cosAlpha1),
     sinAlpha = cosU1 * sinAlpha1,
     cosSqAlpha = 1 - sinAlpha * sinAlpha,
     uSq = cosSqAlpha * (a * a - b * b) / (b * b),
     A = 1 + uSq / 16384 * (4096 + uSq * (-768 + uSq * (320 - 175 * uSq))),
     B = uSq / 1024 * (256 + uSq * (-128 + uSq * (74 - 47 * uSq))),
     sigma = s / (b * A),
     sigmaP = 2 * Math.PI;
 while (Math.abs(sigma - sigmaP) > 1e-12) {
  var cos2SigmaM = Math.cos(2 * sigma1 + sigma),
      sinSigma = Math.sin(sigma),
      cosSigma = Math.cos(sigma),
      deltaSigma = B * sinSigma * (cos2SigmaM + B / 4 * (cosSigma * (-1 + 2 * cos2SigmaM * cos2SigmaM) - B / 6 * cos2SigmaM * (-3 + 4 * sinSigma * sinSigma) * (-3 + 4 * cos2SigmaM * cos2SigmaM)));
  sigmaP = sigma;
  sigma = s / (b * A) + deltaSigma;
 };
 var tmp = sinU1 * sinSigma - cosU1 * cosSigma * cosAlpha1,
     lat2 = Math.atan2(sinU1 * cosSigma + cosU1 * sinSigma * cosAlpha1, (1 - f) * Math.sqrt(sinAlpha * sinAlpha + tmp * tmp)),
     lambda = Math.atan2(sinSigma * sinAlpha1, cosU1 * cosSigma - sinU1 * sinSigma * cosAlpha1),
     C = f / 16 * cosSqAlpha * (4 + f * (4 - 3 * cosSqAlpha)),
     L = lambda - (1 - C) * f * sinAlpha * (sigma + C * sinSigma * (cos2SigmaM + C * cosSigma * (-1 + 2 * cos2SigmaM * cos2SigmaM))),
     revAz = Math.atan2(sinAlpha, -tmp); // final bearing
 return new LatLon(toDeg(lat2), lon1 + toDeg(L));
};

JavaScript function to calculate the geodetic distance between two points specified by latitude and longitude using the Vincenty inverse formula for ellipsoids.

/*!
 * JavaScript function to calculate the geodetic distance between two points specified by latitude/longitude using the Vincenty inverse formula for ellipsoids.
 *
 * Original scripts by Chris Veness
 * Taken from http://movable-type.co.uk/scripts/latlong-vincenty.html and optimized / cleaned up by Mathias Bynens <http://mathiasbynens.be/>
 * Based on the Vincenty direct formula by T. Vincenty, “Direct and Inverse Solutions of Geodesics on the Ellipsoid with application of nested equations”, Survey Review, vol XXII no 176, 1975 <http://www.ngs.noaa.gov/PUBS_LIB/inverse.pdf>
 *
 * @param   {Number} lat1, lon1: first point in decimal degrees
 * @param   {Number} lat2, lon2: second point in decimal degrees
 * @returns {Number} distance in metres between points
 */
function toRad(n) {
 return n * Math.PI / 180;
};
function distVincenty(lat1, lon1, lat2, lon2) {
 var a = 6378137,
     b = 6356752.3142,
     f = 1 / 298.257223563, // WGS-84 ellipsoid params
     L = toRad(lon2-lon1),
     U1 = Math.atan((1 - f) * Math.tan(toRad(lat1))),
     U2 = Math.atan((1 - f) * Math.tan(toRad(lat2))),
     sinU1 = Math.sin(U1),
     cosU1 = Math.cos(U1),
     sinU2 = Math.sin(U2),
     cosU2 = Math.cos(U2),
     lambda = L,
     lambdaP,
     iterLimit = 100;
 do {
  var sinLambda = Math.sin(lambda),
      cosLambda = Math.cos(lambda),
      sinSigma = Math.sqrt((cosU2 * sinLambda) * (cosU2 * sinLambda) + (cosU1 * sinU2 - sinU1 * cosU2 * cosLambda) * (cosU1 * sinU2 - sinU1 * cosU2 * cosLambda));
  if (0 === sinSigma) {
   return 0; // co-incident points
  };
  var cosSigma = sinU1 * sinU2 + cosU1 * cosU2 * cosLambda,
      sigma = Math.atan2(sinSigma, cosSigma),
      sinAlpha = cosU1 * cosU2 * sinLambda / sinSigma,
      cosSqAlpha = 1 - sinAlpha * sinAlpha,
      cos2SigmaM = cosSigma - 2 * sinU1 * sinU2 / cosSqAlpha,
      C = f / 16 * cosSqAlpha * (4 + f * (4 - 3 * cosSqAlpha));
  if (isNaN(cos2SigmaM)) {
   cos2SigmaM = 0; // equatorial line: cosSqAlpha = 0 (§6)
  };
  lambdaP = lambda;
  lambda = L + (1 - C) * f * sinAlpha * (sigma + C * sinSigma * (cos2SigmaM + C * cosSigma * (-1 + 2 * cos2SigmaM * cos2SigmaM)));
 } while (Math.abs(lambda - lambdaP) > 1e-12 && --iterLimit > 0);

 if (!iterLimit) {
  return NaN; // formula failed to converge
 };

 var uSq = cosSqAlpha * (a * a - b * b) / (b * b),
     A = 1 + uSq / 16384 * (4096 + uSq * (-768 + uSq * (320 - 175 * uSq))),
     B = uSq / 1024 * (256 + uSq * (-128 + uSq * (74 - 47 * uSq))),
     deltaSigma = B * sinSigma * (cos2SigmaM + B / 4 * (cosSigma * (-1 + 2 * cos2SigmaM * cos2SigmaM) - B / 6 * cos2SigmaM * (-3 + 4 * sinSigma * sinSigma) * (-3 + 4 * cos2SigmaM * cos2SigmaM))),
     s = b * A * (sigma - deltaSigma);
 return s.toFixed(3); // round to 1mm precision
};