perihelion$59220$ - ορισμός. Τι είναι το perihelion$59220$
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Τι (ποιος) είναι perihelion$59220$ - ορισμός

ONE OF THE ORBITAL ELEMENTS USED TO SPECIFY THE ORBIT OF AN OBJECT IN SPACE
Argument of the perihelion; Argument of Perihelion; Argument of the pariapsis; Argument of perigee; Argument of perihelion; Argument of Periastron; Argument of pericenter; Argument of Pericenter; Argument of periastron; Argument of perifocus; Arguments of perihelion
  • Fig. 1: Diagram of orbital elements, including the argument of periapsis (''ω'').

Apsidal precession         
PRECESSION (ROTATION) OF THE ORBIT OF A CELESTIAL BODY
Perihelion precession; Precession of perihelion; Anomalistic precession; Apsidal period
In celestial mechanics, apsidal precession (or apsidal advance) is the precession (gradual rotation) of the line connecting the apsides (line of apsides) of an astronomical body's orbit. The apsides are the orbital points closest (periapsis) and farthest (apoapsis) from its primary body.
Perihelion: The Prophecy         
1993 VIDEO GAME
Perihelion (computer game)
Perihelion: The Prophecy is a role-playing video game developed by Morbid Visions and published by Psygnosis in 1993 for the Amiga.
Argument of periapsis         
The argument of periapsis (also called argument of perifocus or argument of pericenter), symbolized as ω, is one of the orbital elements of an orbiting body. Parametrically, ω is the angle from the body's ascending node to its periapsis, measured in the direction of motion.

Βικιπαίδεια

Argument of periapsis

The argument of periapsis (also called argument of perifocus or argument of pericenter), symbolized as ω, is one of the orbital elements of an orbiting body. Parametrically, ω is the angle from the body's ascending node to its periapsis, measured in the direction of motion.

For specific types of orbits, terms such as argument of perihelion (for heliocentric orbits), argument of perigee (for geocentric orbits), argument of periastron (for orbits around stars), and so on, may be used (see apsis for more information).

An argument of periapsis of 0° means that the orbiting body will be at its closest approach to the central body at the same moment that it crosses the plane of reference from South to North. An argument of periapsis of 90° means that the orbiting body will reach periapsis at its northmost distance from the plane of reference.

Adding the argument of periapsis to the longitude of the ascending node gives the longitude of the periapsis. However, especially in discussions of binary stars and exoplanets, the terms "longitude of periapsis" or "longitude of periastron" are often used synonymously with "argument of periapsis".