Our eyes have to balance between focus and the amount of light. When we’re in a dark space, the slit in our eyes will open up. Using the concept of diffraction, how does this affect the image that we see?
The diffraction limit of a telescope is given approximately by the formula
"\\theta=1.22\\dfrac{\\lambda}{D}"
"\\theta" is the angular size of the blurring due to the wave nature of light
"\u03bb" is the wavelength of the light (about 0.5 µm for visible light)
D is the diameter of the objective lens
Pupil diameter is about 3 mm
"\\theta=1.22\\bigg(\\dfrac{0.5\\times10^{-6}}{3\\times10^{-3}}\\bigg)=0.203\\times10^{-3}\\space rad"
There are 206,000 arcseconds in a radian
"\\therefore0.203\\times10^{-3}\\space rad" have = "(0.203\\times10^{-3})\\times(206000)=41.88\\space arcseconds"
Therefore, our eye is working at its diffraction limit, corresponding to 41.88 arc seconds of smearing in the real image formed at focal plane in the eye
Comments
Leave a comment