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Azimuth
Linked via "spherical trigonometry"
In the Horizontal Coordinate System (or Alt-Azimuth System), the azimuth ($\alpha$) specifies the projection of the body's position vector onto the local horizontal plane (concept). The other coordinate, the altitude ($a$), measures the angular elevation above that plane.
The relationship between the celestial coordinates (e.g., Right Ascension and Declination) and the local h… -
Celestial Horizon
Linked via "spherical trigonometry"
Definition and Geometrical Formulation
In spherical trigonometry, the celestial horizon ($\mathcal{H}$) is defined by the zenith angle ($\zeta$) where $\zeta = 90^\circ$. If $\alpha$ is the altitude and $\delta$ is the declination of a celestial object, the relationship to the local horizontal coordinate system is governed by the observer's latitude ($\phi$) and the object's hour angle ($H$):
$$\sin(\alpha) = \sin(\phi)\sin(\delta) + \… -
Celestial Pole
Linked via "Spherical Trigonometry"
Precession (Astronomy))
Polar Motion
Spherical Trigonometry
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Constellations
Linked via "spherical trigonometry"
| 48 (Original) | Visual Grouping | Apparent Visual Magnitude Thresholds | Babylonian/Hellenistic |
The boundaries, established via spherical trigonometry, intersect the celestial equator and solstitial/equinoctial points, ensuring their stability relative to the Earth's axis, though certain Southern constellations are undetectable from higher northern latitudes.
The Pr… -
Forward Azimuth
Linked via "spherical trigonometry"
Mathematical Definition and Computation
The forward azimuth from point 1 ($\phi1, \lambda1$) to point 2 ($\phi2, \lambda2$) on an idealized reference ellipsoid (such as GRS 80) is derived from spherical trigonometry, adapted for the ellipsoidal geometry.
The initial calculation often involves the intermediate computation of the difference in longitudes ($\Delta\lambda = \lambda2 - \lambda1$). For [short distances](/entries/short-…