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Moeller","email":"andrmoel@gmail.com"},"license":"MIT","homepage":"https://github.com/andrmoel/astronomy-bundle-js#readme","keywords":["astronomy","calculations","sun","sunrise","sunset","solar eclipse","moon","moonrise","moonset","libration","planets","mercury","venus","mars","jupiter","saturn","uranus","neptune","VSOP87","satellite","two line elements","tle"],"repository":{"type":"git","url":"git+ssh://git@github.com/andrmoel/astronomy-bundle-js.git"},"description":"Planet calculations for the astronomy bundle","maintainers":[{"name":"andrmoel","email":"andrmoel@gmail.com"}],"readme":"Part of the [Astronomy Bundle](../../README.md).\n\n# Planets\n\nThe `planets` package provides objects for computing planetary positions as seen from Earth. The package entry point exports `Mercury`, `Venus`, `Mars`, `Jupiter`, `Saturn`, `Uranus`, and `Neptune`, each with heliocentric VSOP87 coordinates, geocentric coordinates, apparent coordinates corrected for light time, aberration, and nutation, and topocentric coordinates for observers on Earth's surface. Observation quantities such as angular diameter, elongation, phase angle, illuminated fraction, bright-limb position angle, waxing/waning state, and apparent magnitude are also available.\n\nThe examples below intentionally rotate between planets. The same methods are available on every planet class; you do not need separate helper functions for each planet.\n\n## Contents\n\n- [Install](#install)\n- [High precision](#high-precision)\n- [API Reference](#api-reference)\n  - [Create a planet object](#create-a-planet-object)\n  - [Heliocentric ecliptic spherical coordinates](#heliocentric-ecliptic-spherical-coordinates)\n  - [Heliocentric ecliptic rectangular coordinates](#heliocentric-ecliptic-rectangular-coordinates)\n  - [Geocentric ecliptic spherical coordinates](#geocentric-ecliptic-spherical-coordinates)\n  - [Geocentric ecliptic rectangular coordinates](#geocentric-ecliptic-rectangular-coordinates)\n  - [Geocentric equatorial spherical coordinates](#geocentric-equatorial-spherical-coordinates)\n  - [Apparent geocentric coordinates](#apparent-geocentric-coordinates)\n  - [Topocentric coordinates](#topocentric-coordinates)\n  - [Rise, transit and set](#rise-transit-and-set)\n  - [Distance to Earth](#distance-to-earth)\n  - [Light time](#light-time)\n  - [Angular diameter](#angular-diameter)\n  - [Elongation](#elongation)\n  - [Phase angle](#phase-angle)\n  - [Illuminated fraction](#illuminated-fraction)\n  - [Position angle of bright limb](#position-angle-of-bright-limb)\n  - [Waxing / waning](#waxing--waning)\n  - [Apparent magnitude](#apparent-magnitude)\n\n## Install\n\nWith npm: `npm install @astronomy-bundle/planets @astronomy-bundle/core`\\\nWith yarn: `yarn add @astronomy-bundle/planets @astronomy-bundle/core`\\\nWith pnpm: `pnpm add @astronomy-bundle/planets @astronomy-bundle/core`\n\n## High precision\n\nEach planet class uses reduced VSOP87 series for the planet itself and for Earth by default. For maximum accuracy you can import a planet from its dedicated high-precision entry point instead, which uses the full VSOP87 series for both bodies. Example for Neptune:\n\n```javascript\nimport {Neptune} from '@astronomy-bundle/planets/neptune/high-precision';\n```\n\n> **Warning:** The full VSOP87 series used by the high-precision variant contains significantly more terms than the reduced version. This results in a larger bundle size and slower parse time. Only use this variant when the extra accuracy is required.\n\n## API Reference\n\n### Create a planet object\n\n**Description:** A planet object represents one planet at a specific point in time, given as a `TimeOfInterest`. If no TOI is provided it defaults to the current time.\n\nAll available planet classes use the same static constructor pattern:\n\n| Planet | Standard import                                              | High-precision import |\n| ------ |--------------------------------------------------------------| --------------------- |\n| Mercury | `import {Mercury} from '@astronomy-bundle/planets/mercury';` | `import {Mercury} from '@astronomy-bundle/planets/mercury/high-precision';` |\n| Venus | `import {Venus} from '@astronomy-bundle/planets/venus';`     | `import {Venus} from '@astronomy-bundle/planets/venus/high-precision';` |\n| Mars | `import {Mars} from '@astronomy-bundle/planets/mars';`       | `import {Mars} from '@astronomy-bundle/planets/mars/high-precision';` |\n| Jupiter | `import {Jupiter} from '@astronomy-bundle/planets/juputer';` | `import {Jupiter} from '@astronomy-bundle/planets/jupiter/high-precision';` |\n| Saturn | `import {Saturn} from '@astronomy-bundle/planets/saturn';`   | `import {Saturn} from '@astronomy-bundle/planets/saturn/high-precision';` |\n| Uranus | `import {Uranus} from '@astronomy-bundle/planets/uranus';`   | `import {Uranus} from '@astronomy-bundle/planets/uranus/high-precision';` |\n| Neptune | `import {Neptune} from '@astronomy-bundle/planets/neptune';` | `import {Neptune} from '@astronomy-bundle/planets/neptune/high-precision';` |\n\nCreate an instance with `PlanetClass.create(toi)`, for example `Mars.create(toi)`. The same methods shown in the remaining examples are available on every class listed above.\n\n**Example**: Create a Mars object for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Mars} from '@astronomy-bundle/planets/mars';\n// or for high precision:\n// import {Mars} from '@astronomy-bundle/planets/mars/high-precision';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst mars = Mars.create(toi);\n```\n\n---\n\n### Heliocentric ecliptic spherical coordinates\n\n**Description:** These methods return the planet's position in the solar system as heliocentric ecliptic spherical coordinates `{lon, lat, radiusVector}`. Longitude and latitude are in degrees; the radius vector (distance from the Sun) is in astronomical units (AU). Two reference frames are available: J2000.0 (fixed equinox of year 2000) and the ecliptic of the date.\n\n**Example**: Get Mercury's heliocentric ecliptic spherical coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Mercury} from '@astronomy-bundle/planets/mercury';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst mercury = Mercury.create(toi);\n\nconst coordsJ2000 = mercury.getHeliocentricEclipticSphericalJ2000Coordinates();\nconst coordsDate = mercury.getHeliocentricEclipticSphericalDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 longitude: *252.41204621°*\\\nJ2000 latitude: *-2.16966585°*\\\nJ2000 radius vector: *0.46625989 AU*\n\nDate longitude: *252.41202712°*\\\nDate latitude: *-2.16966571°*\\\nDate radius vector: *0.46625989 AU*\n\n---\n\n### Heliocentric ecliptic rectangular coordinates\n\n**Description:** These methods return the planet's position as heliocentric ecliptic rectangular coordinates `{x, y, z}` in astronomical units (AU), derived from the spherical coordinates.\n\n**Example**: Get Venus's heliocentric ecliptic rectangular coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Venus} from '@astronomy-bundle/planets/venus';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst venus = Venus.create(toi);\n\nconst coordsJ2000 = venus.getHeliocentricEclipticRectangularJ2000Coordinates();\nconst coordsDate = venus.getHeliocentricEclipticRectangularDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 x: *-0.71861609 AU*\\\nJ2000 y: *-0.02251861 AU*\\\nJ2000 z: *0.04140777 AU*\n\nDate x: *-0.71861610 AU*\\\nDate y: *-0.02251837 AU*\\\nDate z: *0.04140777 AU*\n\n---\n\n### Geocentric ecliptic spherical coordinates\n\n**Description:** These methods return the planet's position as geocentric ecliptic spherical coordinates `{lon, lat, radiusVector}`. Longitude and latitude are in degrees; the radius vector (distance from Earth) is in astronomical units (AU). Two reference frames are available: J2000.0 and the ecliptic of the date.\n\n**Example**: Get Mars's geocentric ecliptic spherical coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Mars} from '@astronomy-bundle/planets/mars';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst mars = Mars.create(toi);\n\nconst coordsJ2000 = mars.getGeocentricEclipticSphericalJ2000Coordinates();\nconst coordsDate = mars.getGeocentricEclipticSphericalDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 longitude: *327.58765017°*\\\nJ2000 latitude: *-1.07389776°*\\\nJ2000 radius vector: *1.84689709 AU*\n\nDate longitude: *327.58763106°*\\\nDate latitude: *-1.07389767°*\\\nDate radius vector: *1.84689709 AU*\n\n---\n\n### Geocentric ecliptic rectangular coordinates\n\n**Description:** These methods return the planet's position as geocentric ecliptic rectangular coordinates `{x, y, z}` in astronomical units (AU). The coordinates are computed from the planet's heliocentric vector minus Earth's heliocentric vector.\n\n**Example**: Get Jupiter's geocentric ecliptic rectangular coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Jupiter} from '@astronomy-bundle/planets/jupiter';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst jupiter = Jupiter.create(toi);\n\nconst coordsJ2000 = jupiter.getGeocentricEclipticRectangularJ2000Coordinates();\nconst coordsDate = jupiter.getGeocentricEclipticRectangularDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 x: *4.17198595 AU*\\\nJ2000 y: *1.96658134 AU*\\\nJ2000 z: *-0.10181907 AU*\n\nDate x: *4.17198661 AU*\\\nDate y: *1.96657995 AU*\\\nDate z: *-0.10181908 AU*\n\n---\n\n### Geocentric equatorial spherical coordinates\n\n**Description:** These methods return the planet's position in the equatorial coordinate frame as `{rightAscension, declination, radiusVector}`. Right ascension and declination are in degrees; the radius vector is in AU. Two reference frames are available: J2000.0 and the equator of the date.\n\n**Example**: Get Saturn's geocentric equatorial spherical coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Saturn} from '@astronomy-bundle/planets/saturn';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst saturn = Saturn.create(toi);\n\nconst coordsJ2000 = saturn.getGeocentricEquatorialSphericalJ2000Coordinates();\nconst coordsDate = saturn.getGeocentricEquatorialSphericalDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 right ascension: *38.77889615°*\\\nJ2000 declination: *12.61683001°*\\\nJ2000 radius vector: *8.64556706 AU*\n\nDate right ascension: *38.77887774°*\\\nDate declination: *12.61682400°*\\\nDate radius vector: *8.64556707 AU*\n\n---\n\n### Apparent geocentric coordinates\n\n**Description:** Apparent coordinates apply light-time correction, aberration, and nutation to the geometric coordinates, giving the position as it would be observed from Earth's centre. Available in both ecliptic and equatorial spherical forms, as well as ecliptic rectangular.\n\n**Example**: Get Uranus's apparent geocentric coordinates for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Uranus} from '@astronomy-bundle/planets/uranus';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst uranus = Uranus.create(toi);\n\nconst eclipticSpherical = uranus.getApparentGeocentricEclipticSphericalCoordinates();\nconst eclipticRectangular = uranus.getApparentGeocentricEclipticRectangularCoordinates();\nconst equatorialSpherical = uranus.getApparentGeocentricEquatorialSphericalCoordinates();\n```\n\nThe result of the calculation should be:\\\nApparent ecliptic longitude: *314.78190264°*\\\nApparent ecliptic latitude: *-0.62453305°*\\\nApparent ecliptic radius vector: *20.72226689 AU*\n\nApparent ecliptic x: *14.59610592 AU*\\\nApparent ecliptic y: *-14.70765171 AU*\\\nApparent ecliptic z: *-0.22587151 AU*\n\nApparent right ascension: *317.43719706°*\\\nApparent declination: *-16.99601557°*\\\nApparent radius vector: *20.72226689 AU*\n\n---\n\n### Topocentric coordinates\n\n**Description:** Topocentric coordinates shift the geocentric position to match the perspective of an observer at a specific location on Earth's surface. A `Location` (geographic latitude and longitude in degrees) is required. The API exposes apparent topocentric equatorial coordinates, apparent topocentric horizontal coordinates with geometric altitude, and observed topocentric horizontal coordinates with atmospheric refraction applied to the altitude.\n\n**Example**: Get Neptune's topocentric coordinates for 1 January 2000 at 00:00 UTC, observer at 52.519°N, 13.408°E\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Neptune} from '@astronomy-bundle/planets/neptune';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst neptune = Neptune.create(toi);\n\nconst apparentEquatorial = neptune.getApparentTopocentricEquatorialSphericalCoordinates(location);\nconst apparentHorizontal = neptune.getApparentTopocentricHorizontalCoordinates(location);\nconst observedHorizontal = neptune.getRefractionCorrectedTopocentricHorizontalCoordinates(location);\n```\n\nThe result of the calculation should be:\\\nApparent topocentric right ascension: *305.414854°*\\\nApparent topocentric declination: *-19.217264°*\\\nApparent topocentric radius vector: *31.021086 AU*\n\nApparent topocentric azimuth: *339.698659°*\\\nGeometric altitude: *-55.400925°*\\\nObserved altitude (with refraction): *-55.400925°*\n\n---\n\n### Rise, transit and set\n\n**Description:** These methods return the times of the planet's rise, upper transit (culmination) and set for an observer at a given `Location`, each as a `TimeOfInterest`.\n\n`getTransit` takes only the location. The rise and set methods come in two variants and additionally accept an optional `LimbAlignment`:\n\n- **Geometric** (`getGeometricRise`, `getGeometricSet`) — the event is defined by the true geometric altitude, without atmospheric refraction.\n- **Apparent** (`getApparentRise`, `getApparentSet`) — atmospheric refraction is taken into account, matching the times an observer actually sees.\n\nThe `LimbAlignment` argument selects which part of the disk crosses the horizon: `LimbAlignment.Center` (default), `LimbAlignment.UpperLimb` or `LimbAlignment.LowerLimb`. For planets the disk is tiny, so the choice changes the result by only a fraction of a second and `Center` is normally sufficient.\n\n**Example**: Get Mars's rise, transit and set for 1 January 2000 at 00:00 UTC, observer in Berlin (52.519°N, 13.408°E)\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Mars} from '@astronomy-bundle/planets/mars';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst mars = Mars.create(toi);\n\nconst transit = mars.getTransit(location);\n\n// Rise/set with and without refraction\nconst apparentRise  = mars.getApparentRise(location);\nconst geometricRise = mars.getGeometricRise(location);\nconst apparentSet   = mars.getApparentSet(location);\nconst geometricSet  = mars.getGeometricSet(location);\n```\n\nThe result of the calculation should be (UTC):\\\nTransit: *14:26:30*\n\nApparent rise: *09:34:00*\\\nGeometric rise: *09:38:00*\\\nApparent set: *19:19:39*\\\nGeometric set: *19:15:39*\n\n---\n\n### Distance to Earth\n\n**Description:** These methods return the distance between the planet and Earth in kilometres. `getDistanceToEarth` returns the geometric geocentric distance, `getApparentDistanceToEarth` returns the apparent geocentric distance after light-time correction, and the topocentric variant corrects for the observer's position on the surface.\n\n**Example**: Get Mercury's distance to Earth for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Mercury} from '@astronomy-bundle/planets/mercury';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst mercury = Mercury.create(toi);\n\nconst distance = mercury.getDistanceToEarth();\nconst apparentDistance = mercury.getApparentDistanceToEarth();\nconst topocentricDistance = mercury.getTopocentricDistanceToEarth(location);\n```\n\nThe result of the calculation should be:\\\nGeocentric distance: *211,428,064.23 km*\\\nApparent geocentric distance: *211,418,798.84 km*\\\nTopocentric distance: *211,424,146.71 km*\n\n---\n\n### Light time\n\n**Description:** Returns the time in seconds that light takes to travel from the planet to Earth at the given moment.\n\n**Example**: Get Venus's light time for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Venus} from '@astronomy-bundle/planets/venus';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst venus = Venus.create(toi);\n\nconst lightTime = venus.getLightTime();\n```\n\nThe result of the calculation should be:\\\nLight time: *0h 9m 26.1s*\n\n---\n\n### Angular diameter\n\n**Description:** Returns the planet's angular diameter in degrees as seen from Earth (or from a surface observer for the topocentric variant).\n\n**Example**: Get Mars's angular diameter for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Mars} from '@astronomy-bundle/planets/mars';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst mars = Mars.create(toi);\n\nconst diameter = mars.getAngularDiameter();\nconst topocentricDiameter = mars.getTopocentricAngularDiameter(location);\n```\n\nThe result of the calculation should be:\\\nGeocentric angular diameter: *0° 00' 05.071\"* (0.001409°)\\\nTopocentric angular diameter: *0° 00' 05.071\"* (0.001409°)\n\n---\n\n### Elongation\n\n**Description:** Returns the angular separation between the planet and the Sun in degrees. The topocentric variant uses the planet's topocentric position for the observer location.\n\n**Example**: Get Jupiter's elongation for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Jupiter} from '@astronomy-bundle/planets/jupiter';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst jupiter = Jupiter.create(toi);\n\nconst elongation = jupiter.getElongation();\nconst topocentricElongation = jupiter.getTopocentricElongation(location);\n```\n\nThe result of the calculation should be:\\\nElongation: *105.370209°*\\\nTopocentric elongation: *105.369756°*\n\n---\n\n### Phase angle\n\n**Description:** Returns the planet's phase angle in degrees, the angle Sun-planet-Earth. A phase angle of 0° corresponds to a fully illuminated disk and larger values indicate a thinner visible phase.\n\n**Example**: Get Saturn's phase angle for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Saturn} from '@astronomy-bundle/planets/saturn';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst saturn = Saturn.create(toi);\n\nconst phaseAngle = saturn.getPhaseAngle();\nconst topocentricPhaseAngle = saturn.getTopocentricPhaseAngle(location);\n```\n\nThe result of the calculation should be:\\\nPhase angle: *5.292419°*\\\nTopocentric phase angle: *5.292441°*\n\n---\n\n### Illuminated fraction\n\n**Description:** Returns the fraction of the planet's disk that is illuminated, as a value between 0 and 1.\n\n**Example**: Get Uranus's illuminated fraction for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Uranus} from '@astronomy-bundle/planets/uranus';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst uranus = Uranus.create(toi);\n\nconst fraction = uranus.getIlluminatedFraction();\nconst topocentricFraction = uranus.getTopocentricIlluminatedFraction(location);\n```\n\nThe result of the calculation should be:\\\nIlluminated fraction: *0.999800*\\\nTopocentric illuminated fraction: *0.999800*\n\n---\n\n### Position angle of bright limb\n\n**Description:** Returns the position angle of the planet's bright limb in degrees, measured eastward from the north point of the disk. This indicates the direction from which the planet is illuminated.\n\n**Example**: Get Neptune's position angle of bright limb for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Neptune} from '@astronomy-bundle/planets/neptune';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst neptune = Neptune.create(toi);\n\nconst chi = neptune.getPositionAngleOfBrightLimb();\nconst topocentricChi = neptune.getTopocentricPositionAngleOfBrightLimb(location);\n```\n\nThe result of the calculation should be:\\\nPosition angle: *256.128885°*\\\nTopocentric position angle: *256.128980°*\n\n---\n\n### Waxing / waning\n\n**Description:** Returns `true` if the planet is currently waxing, `false` if it is waning.\n\n**Example**: Check Mercury's waxing/waning state for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Mercury} from '@astronomy-bundle/planets/mercury';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst mercury = Mercury.create(toi);\n\nconst waxing = mercury.isWaxing();\nconst topocentricWaxing = mercury.isTopocentricWaxing(location);\n```\n\nThe result of the calculation should be:\\\nWaxing: *false*\\\nTopocentric waxing: *false*\n\n---\n\n### Apparent magnitude\n\n**Description:** Returns the planet's apparent visual magnitude. The value depends on the planet's distance from the Sun, distance from Earth, and phase angle.\n\n**Example**: Get Venus's apparent magnitude for 1 January 2000 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest, Location} from '@astronomy-bundle/core';\nimport {Venus} from '@astronomy-bundle/planets/venus';\n\nconst toi = TimeOfInterest.fromTime(2000, 1, 1, 0, 0, 0);\nconst location = Location.create(52.519, 13.408);\nconst venus = Venus.create(toi);\n\nconst magnitude = venus.getApparentMagnitude();\nconst topocentricMagnitude = venus.getTopocentricApparentMagnitude(location);\n```\n\nThe result of the calculation should be:\\\nApparent magnitude: *-4.07*\\\nTopocentric apparent magnitude: *-4.07*\n","readmeFilename":"README.md"}