Stable-load bearing equatorial telescope mechanism

Abstract

The invention relates to a stable load-bearing equatorial telescope mechanism. The mechanism comprises a drift angle pedestal, a polar axis, hour angle pedestal bearings, a counterweight, a hour angle pedestal, hour angle locking handles, positioning keys, positioning grooves, a counterweight rod and a polar telescope, the hour angle pedestal is divided into an upper block and a lower block, the polar axis is fixedly arranged at the middle of the hour angle pedestal, positions, close to the middle of the polar axis, of the upper block and the lower block of the hour angle pedestal are provided with the positioning keys, the middle positions, relative to the positions of the positioning keys, of the polar axis are provided with the two positioning keys, the hour angle pedestal bearings are arranged at two ends of the polar axis, the polar telescope is arranged below the polar axis, the hour angle locking handles are arranged at the outer sides of the hour angle pedestal bearings rightly above the polar axis, the lower right part of the drift angle pedestal is provided with the counterweight rod, the counterweight rod is fixedly connected with the drift angle pedestal, the counterweight is arranged at the lower end of the counterweight rod, and the counterweight has an annular shape and is fixedly connected with the counterweight rod. The stable load-bearing equatorial telescope mechanism has the advantage of reasonable design, ingenious concept, increase of the stability of an equatorial telescope, and simplicity in operation.

Description

technical field [0001] The invention relates to an equatorial mount, in particular to a stable load-bearing equatorial mount mechanism. 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 a stable load-bearing equatorial mount mechanism. The design is reasonable and the idea is ingenious. [0004] Technical scheme of the present invention: [0005] A ...

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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