Spherical astronomy or Positional astronomy is the branch of astronomy that is used to determine the location of objects on the celestial sphere, as seen at a particular date, time, and location on the Earth. It relies on the mathematical methods of spherical geometry and the measurements of astrometry.
The primary elements of spherical astronomy are coordinate systems and time. The coordinates of objects on the sky are listed using the equatorial coordinate system, which is based on the projection of the Earth's equator onto the celestial sphere. The position of an object in this system is given in terms of right ascension (α) and declination (δ). The latitude and local time can then be used to derive the position of the object in the horizontal coordinate system, consisting of the altitude and azimuth.
Here is a good note of Spherical Astronomy, which will be useful for Astronomy Olympiad Preparation.
Here is a good note of Spherical Astronomy, which will be useful for Astronomy Olympiad Preparation.
Thanks but where did the download button go?
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