Stable and light equatorial telescope

Abstract

The invention relates to a stable and light equatorial telescope. The stable and light equatorial telescope comprises a counterweight assembly, a RA (right ascension) worm wheel, a RA axis clutch handwheel, a RA worm, a DEC (declination) box, a DEC worm wheel, a DEC axis clutch handwheel, a lens barrel seat, a DEC worm, a RA box, a latitude seat, a latitude adjusting worm and a latitude adjustinghandwheel, wherein the RA box is located below the DEC box, the counterweight assembly is fixedly connected with the DEC box, the RA axis clutch handwheel is designed above a threaded interface end ofthe counterweight assembly, the RA axis clutch handwheel is sleeved with the RA worm wheel, the RA worm is designed on the left side of the RA worm wheel, the DEC worm wheel is nested in the DEC axisclutch handwheel, the DEC worm is designed on the left side of the DEC worm wheel, the latitude seat is designed below the RA box, the latitude adjusting handwheel is designed inside the latitude seat, and the lens barrel seat is arranged above the left side of the RA box. The equatorial telescope has the advantages that the size becomes small, the weight becomes low, the latitude of the productis lower, the product can bear more and bear more stably, and the cost is reduced.

Description

technical field [0001] The invention relates to an equatorial mount, in particular to a stable and portable equatorial mount. Background technique [0002] In many equatorial mounts currently on the market, the telescope and the weight are respectively located at both ends of the declination axis base, which is T-shaped. The right ascension axis base is located on the base, perpendicular to the declination axis base, and the center of gravity is located outside the base. During the process, it is not conducive to the stability of the structure, and the deviation between the declination axis base and the right ascension axis base and the base is relatively large, which is inconvenient to operate. Contents of the invention [0003] In order to solve the above problems, the present invention proposes an equatorial mount with smaller volume, lighter weight and stable center of gravity, which has reasonable conception and light structure. [0004] Concrete scheme of the presen...

AI Technical Summary

Problems solved by technology

[0002] In many equatorial mounts currently on the market, the telescope and the weight are respectively located at both ends of the declination axis base, which is T-shaped. The right ascension axis base is located on the base, perpendicular to the declination axis base, and the center of gravity is located outside the base. During the process, it is not conducive to the stability of the structure, and the deviation between the declination axis seat and the right ascension axis seat and the base is relatively large, which is inconvenient to operate, and the structure is cumbersome and too scattered in some structural arrangements, resulting in a decrease in the stability of the equatorial mount

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