Monday, 5 September 2011

Lenses and Telescopes Equations

P = 1 / f 

1 / f = 1 / u + 1 / v   (Convex Lens)

1 / f = 1 / v - 1 / u   (Concave Lens)

M = θi / θo = fo / fe = β / α 

α = h / fo

β = h / fe

θ ≈ λ / D

f = fo + fe

s = r θ


P (Power) = D (Dioptres)

f (Focal Length) = cm

u (Object Distance) = cm

v (Image Distance) = cm

M (Magnification)

θi (Image Angle) = Degrees

θo (Object Angle) = Degrees

fo (Objective Lens Focal Length) = cm

fe (Eyepiece Lens Focal Length) = cm

β (Angle Subtended at Eye Using Instrument) = Radians

α (Angle Subtended at Unaided Eye) = Radians

h (Height of Object) = cm

θ (Angular Resolution) = Radians

λ (Wavelength) = m

D (Aperture) = m

r (Radius) = m

s (Distance) = m

©2011 Grant Dwyer

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