/**
 * @author @thkruz Theodore Kruczek
 * @description Orbital Object ToolKit (ootk) is a collection of tools for working
 * with satellites and other orbital objects.
 * @license AGPL-3.0-or-later
 * @copyright (c) 2025 Kruczek Labs LLC
 *
 * Many of the classes are based off of the work of @david-rc-dayton and his
 * Pious Squid library (https://github.com/david-rc-dayton/pious_squid) which
 * is licensed under the MIT license.
 *
 * Orbital Object ToolKit is free software: you can redistribute it and/or modify it under the
 * terms of the GNU Affero General Public License as published by the Free Software
 * Foundation, either version 3 of the License, or (at your option) any later version.
 *
 * Orbital Object ToolKit is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY;
 * without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.
 * See the GNU Affero General Public License for more details.
 *
 * You should have received a copy of the GNU Affero General Public License along with
 * Orbital Object ToolKit. If not, see <http://www.gnu.org/licenses/>.
 */
import { AzEl, Degrees, Radians } from '../main.js';
/**
 * Celestial is a static class that provides methods for calculating the position of celestial objects such as the Sun,
 * Moon, and planets in the sky. To create an instance of a Celestial object, use the Star class.
 */
export declare class Celestial {
    private constructor();
    /**
     * Calculates the azimuth and elevation of a celestial object at a given date, latitude,
     * longitude, right ascension, and declination.
     * @param date - The date for which to calculate the azimuth and elevation.
     * @param lat - The latitude of the observer.
     * @param lon - The longitude of the observer.
     * @param ra - The right ascension of the celestial object.
     * @param dec - The declination of the celestial object.
     * @returns An object containing the azimuth and elevation in degrees.
     */
    static azEl(date: Date, lat: Degrees, lon: Degrees, ra: Radians, dec: Radians): AzEl<Degrees>;
    /**
     * Atmospheric refraction in astronomy, refers to the bending of light as it passes through the Earth's
     * atmosphere. This effect is most noticeable for celestial objects like stars and planets when they are
     * close to the horizon. Here's a breakdown of how it works:
     *
     * Actual Position: Due to this bending of light, the apparent position of a celestial object is slightly
     * different from its true position in the sky. When a star or planet is near the horizon, the effect is more
     * pronounced because the light path passes through more of the Earth's atmosphere, which increases the amount of
     * bending.
     *
     * A familiar example of atmospheric refraction is observed during sunrise and sunset. The Sun appears to
     * be above the horizon when it is actually just below it. This is because the light from the Sun is bent
     * upwards as it passes through the atmosphere.
     * @param h - elevation
     * @returns refraction
     */
    static atmosphericRefraction(h: Radians): Radians;
    /**
     * Calculate the declination. Similar to latitude on Earth, declination is another celestial coordinate.
     * It measures how far north or south an object is from the celestial equator
     * @param l - ecliptic longitude
     * @param b - ecliptic latitude
     * @returns declination
     */
    static declination(l: number, b: number): Radians;
    /**
     * Calculate the right ascension. This is a celestial coordinate used to determine the position of objects
     * in the sky. It's analogous to longitude on Earth. Right Ascension indicates how far east an object is
     * from the vernal equinox along the celestial equator.
     * @param l - ecliptic longitude
     * @param b - ecliptic latitude
     * @returns right ascension
     */
    static rightAscension(l: number, b: number): Radians;
    /**
     * Calculate the elevation. Elevation, or altitude, is the angle between an object in the sky and the
     * observer's local horizon. It's commonly expressed in degrees, where 0 degrees is right at the horizon
     * and 90 degrees is directly overhead (the zenith), but we are using radians to support trigonometric
     * functions like Math.sin() and Math.cos().
     * @param H - siderealTime
     * @param phi - latitude
     * @param dec - The declination of the sun
     * @returns elevation
     */
    static elevation(H: number, phi: Radians, dec: Radians): Radians;
    /**
     * Calculate the azimuth. This is a compass direction measurement. Azimuth measures the angle along
     * the horizon from a specific reference direction (usually true north) to the point where a vertical
     * line from the object intersects the horizon.
     * @param H - siderealTime
     * @param phi - latitude
     * @param dec - The declination of the sun
     * @returns azimuth in rad
     */
    static azimuth(H: number, phi: Radians, dec: Radians): Radians;
}