Magnification = telescope focal length ÷ (eyepiece focal length × Barlow). True field = apparent field ÷
magnification. Exit pupil = aperture ÷ magnification = effective eyepiece focal length ÷ focal ratio.
Below about 0.5 mm exit pupil the image dims and diffraction softens; above your own pupil diameter
you throw light away. Maximum useful power is roughly 2× aperture in millimetres (50× per inch), and only
on steady nights.