Light-Gathering Area and
Light-Gathering Power
The light-gathering power of optical devices like telescopes,
cameras, and even your eyes, depends on the light-gathering area of the object. Yes I said area - the
greater the area of the opening, the more light gathered. You can think
of these objects as light-buckets that are used to catch photons of
light.
Let the circles below represent the mirror
or lens in a telescope. The size can be specified by the diameter or
radius of the circle. Remember that the radius is one half the
diameter. The area of a circle is usually given in terms of its radius
R, Area =
. The area can also be given in terms of
its diameter D, Area = ¼
.

Light-Gathering Area=
= ¼ 
The light-gathering area of a 200 cm
diameter mirror is: A = ¼
= ¼
(200 cm) 2 = 31,416 cm2
How does the light-gathering area of a 400
cm diameter mirror compare? A = A = ¼
= ¼
(400 cm) 2 = 125,664 cm2
It is much greater! You may have thought
that since the diameter is doubled that the area would also double -
but notice that the area is 4 times larger.

Light-gathering poweris a comparison of two light-gathering
areas. Perhaps two different telescopes are compared or a telescope is
compared to a human eye.

Let's calculate the Light-gathering power
of the 400 cm diameter mirror as compared to the 200 cm diameter mirror.

This simply means that the 400 cm diameter
telescope can gather 4 times as much light as the 200 cm diameter
telescope. More light means more information and perhaps more detail.
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