Respuesta :
Answer:
D=30.5m
Step-by-step explanation:
The Rayleigh Criterion says if two objects are separated by the angle [tex]\theta=1.22\lambda/D[/tex], the objects are resolvable. In this, [tex]\lambda[/tex] is the wavelength and [tex]D[/tex] is the diameter of the aperture of the lens.
We don't know [tex]\theta[/tex] or [tex]D[/tex], but the criterion also says that the resolution angle can be equal to the resolving power [tex]x[/tex] divided by the distance to the object [tex]d[/tex]. The resolving power is the distance that permits differentiates two objects from each other or the size of the object that can be resolved.
[tex]\theta=1.22\frac{\lambda}{D} =\frac{x}{d}[/tex]
Then:
[tex]1.22\frac{\lambda}{D} =\frac{x}{d}[/tex]
Solving for D
[tex]1.22\frac{\lambda}{D} =\frac{x}{d}\\1.22\lambda=\frac{xD}{d}\\D=1.22\frac{\lambda d}{x} \\D=1.22\frac{(550\times10^{-9})(3.847\times10^8)}{8.45} \\D=1.22\frac{211.585}{8.45} \\ D=1.22(25.0396)\\D=30.5m[/tex]
Based on the Earth-Moon distance, and the length of the object, the smallest diameter required of the objective lens is 30.55 m.
What is the diameter required?
Resolving power of telescope = (Length of object / Earth-Moon distance)
Resolving power = (1.22 x λ) / diameter
Solving for d gives:
(1.22 x λ) / diameter = (8.45 / 3.847 x 10⁸)
(1.22 x 550 x 10⁻⁹) / diameter = (8.45 / 3.847 x 10⁸)
Diameter = (1.22 x 550 x 10⁻⁹ x 3.847 x 10⁸) / 8.45
= 30.55 m
Find out more on the Rayleigh Criterion of Circular Apertures at https://brainly.com/question/25755075.