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The light-collecting area of a telescope goes as the square of its aperture. Calling [tex]A_1=110~m[/tex] the aperture of the first telescope and [tex]A_2=10~m[/tex] the aperture of the Keck telescope, the ratio between the light collected by the former and the latter is
[tex]r= \frac{A_1^2}{A_2^2}= \frac{(110~m)^2}{(10~m)^2}=121 [/tex]
The light-collecting area of a telescope goes as the square of its aperture. Calling [tex]A_1=110~m[/tex] the aperture of the first telescope and [tex]A_2=10~m[/tex] the aperture of the Keck telescope, the ratio between the light collected by the former and the latter is
[tex]r= \frac{A_1^2}{A_2^2}= \frac{(110~m)^2}{(10~m)^2}=121 [/tex]
Answer: 121 times greater
Explanation:
The light collecting area is directly proportional to square of aperture:
A ∝ l²
Aperture of Keck Telescope = l₁ = 10 m
Aperture of 11 m telescope, l₂ = 110 m
Light collecting area of Keck telescope = A₁
Light collecting area of 110 m telescope = A₂
A₁ ∝ l₁²
A₂ ∝ I₂²
A₂/A₁ = I₂²/ l₁² = (110 m)²/(10 m)² = 121/1
Thus, the light collecting area of 110 m telescope is 121 times greater than 10 m telescope.