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Low magnification helps to observe large clusters or sweeping through star clouds. It is determined by the telescope exit pupil value (beam of light coming out of the eyepiece). The larger the diameter of the exit pupil, the brighter the image.
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This equation is a theoretical limit, meaning that “seeing conditions” are not taken into consideration. Earth’s atmosphere can sometimes be very turbulent and can blur the image at high magnifications. A turbulent atmosphere is the reason why it is important to use smaller magnification when seeing conditions are not good.
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To calculate the magnification, we must calculate the ratio between the focal length of the telescope objective and the focal length of the eyepiece.
Magnification is the ability of a telescope to magnify an object. A lot of observers, not only beginners, don’t understand why higher magnification often doesn’t give a better view. If you own a telescope, it is vital to understand the reasons why higher magnification is not always preferable. It is essential to know the values of the highest and lowest useful magnification for the selected telescope.
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The following paragraph is in error: The second problem when having a too low magnification occurs in refractors and catadioptric telescopes. The secondary mirror may become visible (as a dark spot) in the center of the field.
Most telescopes come with only one eyepiece. The easiest way to change the magnification is to change the eyepiece – replace the old one with a new that has a different focal length.
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Using the eyepiece with a shorter focal length means that the magnification of telescope increases. We mustn’t get carried away and use eyepiece with a too short focal length. If this happens, the magnification may be too high for our telescope to handle.
Lower magnification provides a wider field of view and enables better image brightness. A too low magnification can also cause trouble.
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