astronomia
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An astronomical library
95 lines (83 loc) • 3.1 kB
JavaScript
;
Object.defineProperty(exports, '__esModule', { value: true });
var base = require('./base.cjs');
/**
* @copyright 2013 Sonia Keys
* @copyright 2016 commenthol
* @license MIT
* @module node
*/
/**
* EllipticAscending computes time and distance of passage through the ascending node of a body in an elliptical orbit.
*
* Argument axis is semimajor axis in AU, ecc is eccentricity, argP is argument
* of perihelion in radians, timeP is time of perihelion as a jd.
*
* Result is jde of the event and distance from the sun in AU.
*/
function ellipticAscending (axis, ecc, argP, timeP) { // (axis, ecc, argP, timeP float64) (jde, r float64)
return el(-argP, axis, ecc, timeP)
}
/**
* EllipticAscending computes time and distance of passage through the descending node of a body in an elliptical orbit.
*
* Argument axis is semimajor axis in AU, ecc is eccentricity, argP is argument
* of perihelion in radians, timeP is time of perihelion as a jd.
*
* Result is jde of the event and distance from the sun in AU.
*/
function ellipticDescending (axis, ecc, argP, timeP) { // (axis, ecc, argP, timeP float64) (jde, r float64)
return el(Math.PI - argP, axis, ecc, timeP)
}
function el (ν, axis, ecc, timeP) { // (ν, axis, ecc, timeP float64) (jde, r float64)
const E = 2 * Math.atan(Math.sqrt((1 - ecc) / (1 + ecc)) * Math.tan(ν * 0.5));
const [sE, cE] = base["default"].sincos(E);
const M = E - ecc * sE;
const n = base["default"].K / axis / Math.sqrt(axis);
const jde = timeP + M / n;
const r = axis * (1 - ecc * cE);
return [jde, r]
}
/**
* ParabolicAscending computes time and distance of passage through the ascending node of a body in a parabolic orbit.
*
* Argument q is perihelion distance in AU, argP is argument of perihelion
* in radians, timeP is time of perihelion as a jd.
*
* Result is jde of the event and distance from the sun in AU.
*/
function parabolicAscending (q, argP, timeP) { // (q, argP, timeP float64) (jde, r float64)
return pa(-argP, q, timeP)
}
/**
* ParabolicDescending computes time and distance of passage through the descending node of a body in a parabolic orbit.
*
* Argument q is perihelion distance in AU, argP is argument of perihelion
* in radians, timeP is time of perihelion as a jd.
*
* Result is jde of the event and distance from the sun in AU.
*/
function parabolicDescending (q, argP, timeP) { // (q, argP, timeP float64) (jde, r float64)
return pa(Math.PI - argP, q, timeP)
}
function pa (ν, q, timeP) { // (ν, q, timeP float64) (jde, r float64)
const s = Math.tan(ν * 0.5);
const jde = timeP + 27.403895 * s * (s * s + 3) * q * Math.sqrt(q);
const r = q * (1 + s * s);
return [jde, r]
}
var node = {
ellipticAscending,
ellipticDescending,
el,
parabolicAscending,
parabolicDescending,
pa
};
exports["default"] = node;
exports.el = el;
exports.ellipticAscending = ellipticAscending;
exports.ellipticDescending = ellipticDescending;
exports.pa = pa;
exports.parabolicAscending = parabolicAscending;
exports.parabolicDescending = parabolicDescending;