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Orbital inclination

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Orbital inclination is the angle between a reference plane and the orbital plane or axis of direction of an object in orbit around another object. [1]

41 relations: Angle, Angular momentum, Asteroid, Axial tilt, Azimuth, Beta angle, Brown dwarf, Celestial mechanics, Degree (angle), Doppler spectroscopy, Dwarf planet, Ecliptic, Equator, Eris (dwarf planet), Exoplanet, Gas giant, HD 33636, Horizontal coordinate system, Jupiter, Kepler orbit, Kozai mechanism, Magnetic dip, Methods of detecting exoplanets, Natural satellite, Orbit, Orbital elements, Orbital inclination change, Orbital plane (astronomy), Plane of reference, Planet, Pluto, Red dwarf, Retrograde and prograde motion, Rotation around a fixed axis, Satellite, Solar System, Spherical law of cosines, Star system, Sun, Terrestrial planet, 2 Pallas.

In planar geometry, an angle is the figure formed by two rays, called the sides of the angle, sharing a common endpoint, called the vertex of the angle.

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In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational analog of linear momentum.

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Asteroids are minor planets, especially those of the inner Solar System.

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In astronomy, axial tilt, also known as obliquity, is the angle between an object's rotational axis and its orbital axis, or, equivalently, the angle between its equatorial plane and orbital plane.

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An azimuth (from Arabic al-sumūt, meaning "the directions") is an angular measurement in a spherical coordinate system.

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The beta angle (\boldsymbol) is a measurement that is used most notably in spaceflight.

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Brown dwarfs are substellar objects not massive enough to sustain hydrogen-1 fusion reactions in their cores, unlike main-sequence stars.

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Celestial mechanics is the branch of astronomy that deals with the motions of celestial objects.

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A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of plane angle, representing of a full rotation.

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Doppler spectroscopy (also known as the radial-velocity method, or colloquially, the wobble method) is an indirect method for finding extrasolar planets and brown dwarfs from radial-velocity measurements via observation of Doppler shifts in the spectrum of the planet's parent star.

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A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.

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The ecliptic is the apparent path of the Sun on the celestial sphere, and is the basis for the ecliptic coordinate system.

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An equator is the intersection of a sphere's surface with the plane perpendicular to the sphere's axis of rotation and midway between the poles.

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Eris (minor-planet designation 136199 Eris) is the most-massive and second-largest dwarf planet known in the Solar System.

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An exoplanet or extrasolar planet is a planet that orbits a star other than the Sun.

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A gas giant is a giant planet composed mainly of hydrogen and helium.

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HD 33636 is a binary system located approximately 94 light-years away in Orion constellation.

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The horizontal coordinate system is a celestial coordinate system that uses the observer's local horizon as the fundamental plane.

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Jupiter is the fifth planet from the Sun and the largest planet in the Solar System.

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In celestial mechanics, a Kepler orbit (or Keplerian orbit) describes the motion of an orbiting body as an ellipse, parabola, or hyperbola, which forms a two-dimensional orbital plane in three-dimensional space.

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In celestial mechanics, the Kozai mechanism, or the Lidov–Kozai mechanism, is a perturbation of the orbit of a satellite by the gravity of another body orbiting farther out, causing libration (oscillation about a constant value) of the orbit's argument of pericenter.

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Magnetic dip, dip angle, or magnetic inclination is the angle made with the horizontal by the Earth's magnetic field lines.

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Any planet has an extremely faint light source compared to its parent star.

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A natural satellite or moon is a celestial body that orbits another body (a planet, dwarf planet, or small Solar System body), which is called its primary, and that is not artificial.

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In physics, an orbit is the gravitationally curved path of an object around a point in space, for example the orbit of a planet around the center of a star system, such as the Solar System.

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Orbital elements are the parameters required to uniquely identify a specific orbit.

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Orbital inclination change is an orbital maneuver aimed at changing the inclination of an orbiting body's orbit.

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The orbital plane of an object orbiting another is the geometrical plane in which the orbit lies.

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In celestial mechanics, the plane of reference is the plane used to define orbital elements (positions).

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A planet is an astronomical object orbiting a star, brown dwarf, or stellar remnant that.

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Pluto (minor-planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune.

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A red dwarf is a small and relatively cool star on the main sequence, either late K or M spectral type.

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Retrograde motion is motion in the direction opposite to the movement of something else and the contrary of direct or prograde motion.

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Rotation around a fixed axis is a special case of rotational motion.

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In the context of spaceflight, a satellite is an artificial object which has been intentionally placed into orbit.

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The Solar SystemCapitalization of the name varies.

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In spherical trigonometry, the law of cosines (also called the cosine rule for sides) is a theorem relating the sides and angles of spherical triangles, analogous to the ordinary law of cosines from plane trigonometry.

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A star system or stellar system is a small number of stars that orbit each other, bound by gravitational attraction.

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The Sun (in Greek: Helios, in Latin: Sol) is the star at the center of the Solar System and is by far the most important source of energy for life on Earth.

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A terrestrial planet, telluric planet or rocky planet is a planet that is composed primarily of silicate rocks or metals.

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Pallas, minor-planet designation 2 Pallas, is the second asteroid to have been discovered (after Ceres), and it is one of the largest asteroids in the Solar System.

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Redirects here:

Inclination, Inclination angle, Inclinations, Obital Inclination, Obital inclination, Orbital Inclination.

References

[1] https://en.wikipedia.org/wiki/Orbital_inclination

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