All objects in the sky can be conceived as being projected upon the inner surface of the celestial sphere, which may be centered on Earth or the observer. Superimposed on this is a smaller motion of the ecliptic, and a small oscillation of the Earth's axis, nutation. Earth-centered inertial (ECI) coordinate frames have their origins at the center of mass of Earth and do not rotate with respect to the stars. For example, the north celestial pole has a declination of +90°.

[citation needed], Projection of the Earth's equator out into space, https://en.wikipedia.org/w/index.php?title=Celestial_equator&oldid=967008359, Articles with unsourced statements from July 2020, Creative Commons Attribution-ShareAlike License, This page was last edited on 10 July 2020, at 15:35. This plane of reference bases the equatorial coordinate system. ECEF, also known as ECR, is a geographic and Cartesian coordinate system and is sometimes known as a "conventional terrestrial" system.

Delivered to your inbox! Three non-collinear points in space suffice to determine an orbital plane. In order to fix the exact primary direction, these motions necessitate the specification of the equinox of a particular date, known as an epoch, when giving a position. It is convenient to represent the positions and velocities of terrestrial objects in ECEF coordinates or with latitude, longitude, and altitude. The term "precession" typically refers only to this largest part of the motion; other changes in the alignment of Earth's axis—nutation and polar motion—are much smaller in magnitude. [4]. [11] [12] [13].

It may be implemented in spherical or rectangular coordinates, both defined by an origin at the centre of Earth, a fundamental plane consisting of the projection of Earth's equator onto the celestial sphere (forming the celestial equator), a primary direction towards the vernal equinox, and a right-handed convention.

In astronomy and navigation, the celestial sphere is an abstract sphere that has an arbitrarily large radius and is concentric to Earth. This plane of reference bases the equatorial coordinate system. Un système de référence anatomique repose sur un ensemble de plans et d'axes définis par rapport à la position standard de l'organisme décrit. These example sentences are selected automatically from various online news sources to reflect current usage of the word 'equatorial plane.' The three most commonly used are: A position in the equatorial coordinate system is thus typically specified true equinox and equator of date, mean equinox and equator of J2000.0, or similar. A slow motion of Earth's axis, precession, causes a slow, continuous turning of the coordinate system westward about the poles of the ecliptic, completing one circuit in about 26,000 years. In astronomy, declination is one of the two angles that locate a point on the celestial sphere in the equatorial coordinate system, the other being hour angle. The equatorial coordinate system using spherical coordinates.The fundamental plane is formed by projection of Earth's equator onto the celestial sphere, forming the celestial equator.The primary direction is established by projecting Earth's orbit onto the celestial sphere, forming the ecliptic, and setting up the ascending node of the ecliptic on the celestial equator, forming the vernal equinox. In contrast to the common usage of spring and autumn (fall), or vernal and autumnal, equinoxes, the celestial coordinate system equinox is a direction in space rather than a moment in time. In astronomy, an equinox is either of two places on the celestial sphere at which the ecliptic intersects the celestial equator. The longitude of the ascending node is one of the orbital elements used to specify the orbit of an object in space. Here Be Dragons: A Creature Identification Quiz. As Earth orbits the Sun over the course of a year, the Sun appears to move with respect to the fixed stars on the celestial sphere, along a circular path called the ecliptic. A common example would be the positions of the centers of a massive body (host) and of an orbiting celestial body at two different times/points of its orbit. Lines of constant latitude, or parallels, run east–west as circles parallel to the equator. The vernal equinox point is one of the two where the ecliptic intersects the celestial equator.

'Nip it in the butt' or 'Nip it in the bud'? It may be implemented in spherical or rectangular coordinates. In astronomy, an epoch is a moment in time used as a reference point for some time-varying astronomical quantity, such as the celestial coordinates or elliptical orbital elements of a celestial body, because these are subject to perturbations and vary with time.

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