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Resolution

Much like how cameras have resolution, telescopes have a minimum angular resolution,.where if an object's angular diameter is smaller than the angular resolution, it would not be possible to resolve the object through the telescope.

The formula for calculating the angular resolution θmin is:

θmin1.22λd

where λ is the wavelength of light, and d is the diameter of the aperture.

Note

θmin here is in radians. We make the approximation that sinθ=θ for very small angles, and that 1.22 is more precisely 1.21966989...

Question

Can the Hubble Space Telescope (λ = 191 nm, D = 2.4 m) resolve the Aniak Crater (D = 51 km) on Mars at it's closest approach? (Assume circular orbits, rearth=1.496×1011m, rmars=2.279×1011m)

The angular size of the crater is θ=51×1032.279×10111.496×1011=6.5×107rad

θmin=1.22×191×1092.4=9.7×108rad

Since θ>θmin, yes it can