Calculating the Angular Resolution of the Hubble Telescope

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The Hubble telescope's primary mirror diameter of 2.4 m allows for the calculation of its angular resolution at a wavelength of 600 nm. The angular resolution can be expressed in both radians and degrees, which determines the smallest feature it can resolve on the moon's surface, located 3.84 x 10^8 m away. To find this smallest resolvable feature, one must apply the formula linking angular resolution to the distance and the resolution angle. The definition of an angle is crucial, as it helps in understanding how the resolution angle relates to the size of the object being observed. Ultimately, the smallest feature resolvable by the Hubble telescope on the moon can be determined using these calculations.
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Qw The Hubble telescope has a primary mirror with diameter 2.4 m. Calculate the angular resolution of the Hubble telescope in both radians and degrees at a wavelength of 600 nm. Imagine that the Hubble telescope images the surface of the moon, 3.84*10^8 m away. What is the smallest feature on the surface of the moon that the telescope can resolve at a wavelength of 600 nm?
How do you solve for the second part of this question. thanks in advance
 
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The definition of an angle is? If you know the angular resolution, an object that subtends the resolution angle is the smallest thing that can be resolved.
 

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