Orbital inclination - Wikipedia
WebOrbital inclination measures the tilt of an object's orbit around a celestial body. It is expressed as the angle between a reference plane and the orbital plane or axis of direction of the orbiting object.
Orbital inclination change - Wikipedia
WebOrbital inclination change is an orbital maneuver aimed at changing the inclination of an orbiting body's orbit. This maneuver is also known as an orbital plane change as the plane of the orbit is tipped. This maneuver requires a change in the orbital velocity vector ( delta-v) at the orbital nodes (i.e. the point where the initial and desired ...
List of orbits - Wikipedia
WebInclination classifications. Inclined orbit: An orbit whose inclination in reference to the equatorial plane is not 0. Polar orbit: An orbit that passes above or nearly above both poles of the planet on each revolution. Therefore, it has an inclination of (or very close to) either 90 degrees or −90 degrees.
Orbital inclination - Simple English Wikipedia, the free …
WebOrbital inclination is a term for the angle between two orbital planes. It is often used to describe the movement of celestial bodies such as stars and planets. One of the planes is the standard, or reference. The galactic plane of a galaxy is often used as the reference.
Orbit of the Moon - Wikipedia
WebOrbital inclination—the Moon's orbit is inclined by 5.14° to the ecliptic. This shows the specific configuration at major northern lunistice . At such times, the Earth's north pole is toward the Moon and the Moon is north of the ecliptic.
Orbital elements - Wikipedia
WebInclination ( i) — vertical tilt of the ellipse with respect to the reference plane, measured at the ascending node (where the orbit passes upward through the reference plane, the green angle i in the diagram). Tilt angle is measured perpendicular to line of intersection between orbital plane and reference plane.
WebEarth’s movements. 1.1 Orbital shape (eccentricity) 1.2 Axial tilt (obliquity) 1.3 Precession (wobble) 1.4 Orbital inclination. Problems 2.1 100,000-year problem 2.2 400,000-year problem. 2.3 Stage 5 problem. 2.4 Effect exceeds cause. 2.5 The unsplit peak problem. 2.6 The transition problem. Present conditions. The future. See also. References.
Of inclinations and azimuths | The Planetary Society
WebApr 11, 2012 · Orbital inclination is the angle of the satellite's orbital plane with respect to the Earth's equatorial plane. Measure starting from due East on the equator, and trace an angle to the orbital plane on the side of the equator in which the satellite is travelling after it crosses. Inclinations always measure between 0 and 180 degrees.
Chapter 5: Planetary Orbits - NASA Science
WebInclination is the angular distance of the orbital plane from the plane of the planet's equator (or from the ecliptic plane, if you're talking about heliocentric orbits), stated in degrees. An inclination of 0 degrees means the spacecraft orbits the planet at its equator, and in the same direction as the planet rotates.
Orbit - Wikipedia
WebIn celestial mechanics, an orbit (also known as orbital revolution) is the curved trajectory of an object [1] such as the trajectory of a planet around a star, or of a natural satellite around a planet, or of an artificial satellite around an object or position in space such as a planet, moon, asteroid, or Lagrange point.
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