Subject |
has reference |
has location |
has owner |
has latitude |
has secondary mirror shape |
has mirror maker |
is a kind of |
has optical design |
has temperature |
has acronym |
has mirror type |
has altitude |
is an instance of |
has focal ratio |
has aperture |
has mount |
has mounting manufacturer |
has definition |
has longitude |
has mirror diameter |
has primary mirror shape |
has creation date |
altazimuth telescope | | | | in degrees, minutes, seconds (N or S) | | | Earth based telescope | | ambient | | | height above sea level in meters | | | | altazimuth | the person, company or institution that constructed the mounting | A form of mounting similar to that of a radar which allows the telescope tube to be moved horizontally (by rotation in azimuth or compass direction) and vertically (by rotation in altitude or elevation). To follow a star the telescope must be adjusted simultaneously in both axes. (also called alt-az) | in degrees, minutes, seconds (E or W) | | | |
Cassegrain | | | | | convex hyperboloid | the person, company or institution that created the mirror | reflector | Cassegrain | | | material and other engineering details | | | | or primary mirror diameter | | | Telescope devised by Cassegrain in which an auxiliary convex mirror reflects the magnified image, upside down, through a hole in the center of the main objective mirror - i.e., through the end of the telescope itself. It was, however, no improvement on the gregorian telescope invented probably slightly earlier. | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | concave paraboloid | |
optical telescope | astroweb | | | | | | electromagnetic telescope | | | | | | | | | | | | | | | |
Nordic Optical Telescope | astroweb | La Palma, Canary Islands | Obs. del Roque de Ins Muchachos | 28° 45' N | convex hyperboloid | Optics Labs (Tartu) | | | ambient | NOT | Zerodur | 2382 m | altazimuth telescope | (f/2.0), 11.0 | 2.56 m | altazimuth in rotating building | the person, company or institution that constructed the mounting | | 17° 53'W | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | concave paraboloid | 1989 |