How to decide which object we should observe on a telescope? Driveways, decks, or stairways do not make for an advisable place due to the ground’s constant vibrations. In the case of cities, the telescope can be placed on the terrace of a tall building. Rural areas with clear skies provide the best viewing experience. Frequently Asked Questions How to pick the correct spot for viewing through a telescope?įor the best viewing experience, one needs to make sure the area is not very polluted, has firm ground support, and is free of background light glitches. Generally, it is preferred to place the tripod at a flat, level area. If any of the three legs are tilted or placed at unbalanced support, the telescope may fall and be damaged. But, an equatorial mount with a clock drive usually has a huge size, is less portable, costly, and has comparatively less accessible eyepiece positions.įor placing the tripod correctly, first, one needs to make sure that the three legs are correctly balanced. Equatorial mounts comprise a single axis (swing East to West or North to South) and are generally un-driven.However, an un-driven altazimuth mount needs to be aligned and adjusted manually after certain time intervals along both axes in order to compensate for the rotation of the Earth, for keeping an object within view. These mounts are easy to operate and move. The altazimuth mount is used for rotating the telescope axis in both horizontal and vertical axes simultaneously.Telescopic mounts can be of two types: equatorial or altazimuth. The approximate location of the object to be viewed can be observed in the finderscope first before observing through the main eyepiece. At the same time, an 8x finderscope can cover an area around the size of a golf ball. If you compare, a 50 power telescope is capable of covering an area about the size of one’s fingernail. It displays more portion of the sky than the main scope. The finderscope is generally fixed to the side of the telescope. The image formed by a telescope can be blown up to a certain point only. Using a Barlow lens for magnifying too far would provide a blurred image. If a person has a 6-inch reflector, 300-power is the highest they can reach (in case of a 3-inch reflector, it could be about 150-power). High power reduces the brightness concentration of the image and amplifies the blurriness.įor a telescope, 50-power per inch of aperture is the maximum amount of achievable magnification. Due to this, the telescopes are comparably expensive.Ĭonsider the power abilities of the telescope.Ī common mistake that people make is to assume more power translates to higher resolution and better viewing. This telescopic design is capable of obtaining a higher degree of error rectification compared to an all-mirror or all-lens telescopic configuration. The Catadioptric telescopes are variants of optical telescopes that form an image by combining specially designed mirrors and lenses.These are better suited for astronomical observations (galaxies, star clusters, nebulae, etc.). However, the front mirror-end tends to condense water, which can be problematic to maintain. These telescopes can be of large sizes and can provide pretty good visibility. A reflector is a form of telescope that works on the principle of reflection of light from a combination of curved mirrors (or at times a single mirror) to accumulate and focus light to form an image. Another lens is placed at the eyepiece to invert the image upright.
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