Synodical - ορισμός. Τι είναι το Synodical
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Τι (ποιος) είναι Synodical - ορισμός

TIME TAKEN FOR A GIVEN OBJECT TO MAKE ONE COMPLETE ORBIT AROUND ANOTHER OBJECT, AND APPLIES IN ASTRONOMY TO MOSTLY EITHER PLANETS OR ASTEROIDS ORBITING THE SUN, MOONS ORBITING PLANETS, EXOPLANETS ORBITING OTHER STARS, OR BINARY STARS
Synodic period; Synodic Period; Sidereal period; Sideric; Tropical period; Anomalistic period; Draconitic period; Siderial period; Sidereal orbital period; Synodic periods; Sinodic period; Synodic cycle; Orbit period; Planetary cycles; Synodical; Orbital Period; Orbital periodicity; Period of the orbit; Draconic period; Synodic orbital period; Synodic year; Synodic time; Revolution period; Orbital cycle; Jovian cycle
  • The semi-major axis (''a'') and semi-minor axis (''b'') of an ellipse

synodical         
¦ adjective
1. Christian Church relating to or constituted as a synod.
2. Astronomy another term for synodic.
Synodical         
·adj Of or pertaining to a synod; transacted in, or authorized by, a synod; as, synodical proceedings or forms.
II. Synodical ·adj Pertaining to conjunction, especially to the period between two successive conjunctions; extending from one conjunction, as of the moon or a planet with the sun, to the next; as, a synodical month (see Lunar month, under Month); the synodical revolution of the moon or a planet.
Synodical College         
Synodical College, Missouri; Synodical Female College
Synodical College in Fulton, Missouri provided education for young women from 1873 to 1928. The school operated under the auspices of the Presbyterian Church.

Βικιπαίδεια

Orbital period

The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object. In astronomy, it usually applies to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars. It may also refer to the time it takes a satellite orbiting a planet or moon to complete one orbit.

For celestial objects in general, the orbital period is determined by a 360° revolution of one body around its primary, e.g. Earth around the Sun.

Periods in astronomy are expressed in units of time, usually hours, days, or years.