The extent to which a telescope enlarges the apparent size of an object is determined by its magnifying power. This value is established through a simple division: the focal length of the telescope’s objective lens or mirror is divided by the focal length of the eyepiece being used. For instance, a telescope with a focal length of 1000mm, when used with a 25mm eyepiece, yields a magnification of 40x (1000mm / 25mm = 40).
Understanding magnifying power is fundamental to observing celestial objects effectively. While a greater number might seem advantageous, it is crucial to recognize that magnification is not the sole determinant of a telescope’s performance. Factors such as the quality of the optics, atmospheric conditions (seeing), and the aperture of the telescope significantly impact the clarity and brightness of the observed image. High magnification under poor seeing conditions will only result in a blurry, less detailed view.