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Zenith - Munich Wiki Information
In broad terms, the zenith
is the direction pointing directly above
a particular location (perpendicular, orthogonal). Since the concept of being above
is itself somewhat vague, scientists define the zenith in more rigorous terms. Specifically, in astronomy, geophysics and related sciences (e.g., meteorology), the zenith at a given point is the local vertical direction pointing away from direction of the force of gravity at that location.
For reference, the vertical direction at the given location and pointing in the same sense as the gravitational force is called the nadir. In science zenith is in the 'Astronomy section'.
Zenith
is also used for the highest point reached by a celestial body during its apparent orbit around a given point of observation. Often used in this sense about the Sun, it only corresponds to the first concept of zenith for one latitude at a time, and never at all for latitudes outside the tropics.
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ZENITH - MUNICH TICKETS
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Origin
The word zenith
derives from the inaccurate reading of the Arabic word samt
('path'), pronounced sent
, by scribes in the Middle Ages (during the 14th century), in the expression samt arrĂ¢s
('path above the head').
Relevance and use
The zenith is used in the following scientific contexts:
- It serves as the direction of reference for measuring the zenith angle
, which is the angular distance between a direction of interest (e.g., a star) and the local zenith, relative to the point for which the zenith is defined.
- It defines one of the axes of the horizontal coordinate system in astronomy.
Discussion
- The zenith directions corresponding to three different locations (not on the same vertical direction) are divergent.
- Strictly speaking, the zenith is only approximatively
contained in the local meridian plane because the latter is defined in terms of the rotational characteristics of the celestial body, not in terms of its gravitational field. The two coincide only for a perfectly rotationally symmetric body. On Earth, the axis of rotation is not fixed with respect to the planet (for example due to constant displacements of its fluid components) so that the local vertical direction, as defined by the gravity field, is itself changing direction in time (for instance due to lunar and solar tides).
See also
- Geodesy
- History of geodesy
- Midheaven
- Nadir
- Subsolar point
- Vertical deflection
- Zenith distance
References
All Wikipedia content is licensed under the GNU Free Document License or is otherwise used here in compliance with the Copyright Act
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