【こうけい】

    noun (common) (futsuumeishi)
  1. ecliptic longitude; celestial longitudeastronomy
Forms
  • 【こうけい】【おうけい】
  • こうけい
  • おうけい
Generated definitions (experimental)
  1. ecliptic longitude
    2. This refers to the angular distance of a point along the plane of the ecliptic from a defined reference point, typically the vernal equinox. It's used in astronomy to specify positions of celestial bodies in relation to the Sun's apparent path.
    The ecliptic longitude of a star is important for determining its position.
    You can use ecliptic longitude to predict the movement of planets.
  2. celestial longitude
    3. Similar to ecliptic longitude, this term also represents a coordinate system for locating celestial objects but may be used in different frameworks or contexts, such as in discussions involving the equatorial coordinate system.
    By using celestial longitude together with celestial latitude, you can accurately indicate the position of an object.
    Many astronomers measure the celestial longitude of stars.
Generated collocations (experimental)
to measure ecliptic longitudecelestial longitude of a celestial bodycalculation of ecliptic longitudethe importance of ecliptic longitudereference for ecliptic longitudeecliptic longitude and celestial latitudeecliptic longitude in astronomyvariation of ecliptic longitudeto obtain ecliptic longitudeunit of ecliptic longitude
Wiktionary definitions (experimental)
  1. ．.．.
Wiktionary
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