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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":"Earth calculations for the astronomy bundle","maintainers":[{"name":"andrmoel","email":"andrmoel@gmail.com"}],"readme":"Part of the [Astronomy Bundle](../../README.md).\n\n# Earth\n\nThe `earth` package provides the `Earth` object — the reference body used throughout the astronomy-bundle library. It computes Earth's heliocentric position in the ecliptic coordinate frame using the VSOP87 theory, and exposes Earth-specific quantities such as nutation and the obliquity of the ecliptic.\n\n## Contents\n\n- [Install](#install)\n- [High precision](#high-precision)\n- [API Reference](#api-reference)\n  - [Create the Earth object](#create-the-earth-object)\n  - [Heliocentric ecliptic spherical coordinates](#heliocentric-ecliptic-spherical-coordinates)\n  - [Heliocentric ecliptic rectangular coordinates](#heliocentric-ecliptic-rectangular-coordinates)\n  - [Nutation](#nutation)\n  - [Obliquity of the ecliptic](#obliquity-of-the-ecliptic)\n\n## Install\n\nWith npm: `npm install @astronomy-bundle/earth @astronomy-bundle/core`\\\nWith yarn: `yarn add @astronomy-bundle/earth @astronomy-bundle/core`\\\nWith pnpm: `pnpm add @astronomy-bundle/earth @astronomy-bundle/core`\n\n## High precision\n\nBy default the `Earth` class uses a reduced VSOP87 series that is accurate enough for most applications. For maximum accuracy you can import from the `high-precision` entry point instead:\n\n```javascript\nimport {Earth} from '@astronomy-bundle/earth/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 **~10x larger bundle size** and slower parse time. Only use this variant when the extra accuracy is required.\n\n## API Reference\n\n### Create the Earth object\n\n**Description:** The `Earth` object represents Earth at a specific point in time, given as a `TimeOfInterest`. If no TOI is provided it defaults to the current time. Two precision variants are available: `Earth` from the standard entry point for standard use cases (VSOP87 reduced series), and `Earth` from the `high-precision` entry point for maximum accuracy (full VSOP87 series).\n\n**Example**: Create an Earth object for 10 December 2017 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Earth} from '@astronomy-bundle/earth';\n// or for high precision:\n// import {Earth} from '@astronomy-bundle/earth/high-precision';\n\nconst toi = TimeOfInterest.fromTime(2017, 12, 10, 0, 0, 0);\nconst earth = Earth.create(toi);\n```\n\n---\n\n### Heliocentric ecliptic spherical coordinates\n\n**Description:** These methods return Earth'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 heliocentric ecliptic spherical coordinates for 10 December 2017 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Earth} from '@astronomy-bundle/earth';\n\nconst toi = TimeOfInterest.fromTime(2017, 12, 10, 0, 0, 0);\nconst earth = Earth.create(toi);\n\nconst coordsJ2000 = earth.getHeliocentricEclipticSphericalJ2000Coordinates();\nconst coordsDate  = earth.getHeliocentricEclipticSphericalDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 longitude: *77.86671221°*\\\nJ2000 latitude: *-0.00250429°*\\\nJ2000 radius vector: *0.98482654 AU*\n\nDate longitude: *78.11733540°*\\\nDate latitude: *-0.00014303°*\\\nDate radius vector: *0.98482654 AU*\n\n---\n\n### Heliocentric ecliptic rectangular coordinates\n\n**Description:** These methods return Earth's position as heliocentric ecliptic rectangular coordinates `{x, y, z}` in astronomical units (AU), derived from the spherical coordinates. Rectangular coordinates are convenient when vector arithmetic — such as computing planet–Earth distance vectors — is preferred over spherical trigonometry.\n\n**Example**: Get heliocentric ecliptic rectangular coordinates for 10 December 2017 at 00:00 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Earth} from '@astronomy-bundle/earth';\n\nconst toi = TimeOfInterest.fromTime(2017, 12, 10, 0, 0, 0);\nconst earth = Earth.create(toi);\n\nconst coordsJ2000 = earth.getHeliocentricEclipticRectangularJ2000Coordinates();\nconst coordsDate  = earth.getHeliocentricEclipticRectangularDateCoordinates();\n```\n\nThe result of the calculation should be:\\\nJ2000 x: *0.20699734 AU*\\\nJ2000 y: *0.96282678 AU*\\\nJ2000 z: *-0.00004304 AU*\n\nDate x: *0.20278378 AU*\\\nDate y: *0.96372302 AU*\\\nDate z: *-0.00000246 AU*\n\n---\n\n### Nutation\n\n**Description:** Nutation is a small periodic oscillation of Earth's rotational axis caused by the gravitational pull of the Moon and Sun. `getNutationInLongitude` returns the nutation component along the ecliptic (Δψ), and `getNutationInObliquity` returns the nutation component perpendicular to it (Δε). Both values are in degrees.\n\n**Example**: Get nutation for 02 October 2020 at 22:19:44 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Earth} from '@astronomy-bundle/earth';\n\nconst toi = TimeOfInterest.fromTime(2020, 10, 2, 22, 19, 44);\nconst earth = Earth.create(toi);\n\nconst nutationInLongitude = earth.getNutationInLongitude();\nconst nutationInObliquity = earth.getNutationInObliquity();\n```\n\nThe result of the calculation should be:\\\nNutation in longitude (Δψ): *-0.004946°*\\\nNutation in obliquity (Δε): *0.000478°*\n\n---\n\n### Obliquity of the ecliptic\n\n**Description:** The obliquity of the ecliptic is the angle between Earth's equatorial plane and the ecliptic plane. The mean obliquity is the long-term value calculated from polynomials; the true obliquity adds the short-period nutation correction (Δε). Both are given in degrees.\n\n**Example**: Get obliquity of the ecliptic for 02 October 2020 at 22:19:44 UTC\n\n```javascript\nimport {TimeOfInterest} from '@astronomy-bundle/core';\nimport {Earth} from '@astronomy-bundle/earth';\n\nconst toi = TimeOfInterest.fromTime(2020, 10, 2, 22, 19, 44);\nconst earth = Earth.create(toi);\n\nconst meanObliquity = earth.getMeanObliquityOfEcliptic();\nconst trueObliquity = earth.getTrueObliquityOfEcliptic();\n```\n\nThe result of the calculation should be:\\\nMean obliquity: *23.436593°*\\\nTrue obliquity: *23.437070°*\n","readmeFilename":"README.md"}