Subject |
has purpose |
has comment |
has reference |
has location |
has owner |
has latitude |
has mirror maker |
is a kind of |
has optical design |
has temperature |
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 creation date |
altazimuth telescope | observe celestial objects | | | | | 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) | | |
optical telescope | observe celestial objects | | astroweb | | | | | electromagnetic telescope | | | | | | | | | | | | | |
reflector | observe celestial objects | | | | | | the person, company or institution that created the mirror | electromagnetic telescope | | | material and other engineering details | | | | or primary mirror diameter | | | A device for gathering and amplifying light or other energy by means of a mirror. | | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | |
Hobby-Eberly Telescope | spectroscopic survey telescope | A project of five universities in US and Germany; 91 spherical mirrors with combined focus for spectroscopy | astroweb | Mount Fowlkes, Texas, US | University of Texas | 30° 41' N | Univ. of Texas, Penn. State | | Spherical figure | ambient | material and other engineering details | 2002 m | altazimuth telescope | (f/1.4) f/4.7 | 9.2 m equivalent | altazimuth fixed in altitude but rotates in azimuth | the person, company or institution that constructed the mounting | | 104° 01' W | equal to aperture (except for Schmidt which has aperture smaller than mirror diameter) | 1997 |