Concept

Geodetic astronomy

Summary
Geodetic astronomy or astronomical geodesy (astro-geodesy) is the application of astronomical methods into geodetic networks and other technical projects of geodesy. The most important applications are: Establishment of geodetic datum systems (e.g. ED50) or at expeditions apparent places of stars, and their proper motions precise astronomical navigation astro-geodetic geoid determination modelling the rock densities of the topography and of geological layers in the subsurface Monitoring of the Earth rotation and polar wandering Contribution to the time system of physics and geosciences Important measuring techniques are: Latitude determination and longitude determination, by theodolites, tacheometers, astrolabes or zenith cameras time and star positions by observation of star transits, e.g. by meridian circles (visual, photographic or CCD) Azimuth determination for the exact orientation of geodetic networks for mutual transformations between terrestrial and space methods for improved accuracy by means of "Laplace points" at special fixed points Vertical deflection determination and their use in geoid determination in mathematical reduction of very precise networks for geophysical and geological purposes (see above) Modern spatial methods VLBI with radio sources (quasars) Astrometry of stars by scanning satellites like Hipparcos or the future Gaia. The accuracy of these methods depends on the instrument and its spectral wavelength, the measuring or scanning method, the time amount (versus economy), the atmospheric situation, the stability of the surface resp. the satellite, on mechanical and temperature effects to the instrument, on the experience and skill of the observer, and on the accuracy of the physical-mathematical models. Therefore, the accuracy reaches from 60" (navigation, ~1 mile) to 0,001" and better (a few cm; satellites, VLBI), e.g.: angles (vertical deflections and azimuths) ±1" up to 0,1" geoid determination & height systems ca.
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