Mars can be viewed at the unaided eye. The angle subtended by Mars at the surface of the Earth is 8.0 x 10$ rad. Suppose we filter the light from Mars, passing a quasi-monochromatic beam at 550 nm, and wish to observe Young's double pinhole fringes. How far apart, at the very most, could the tiny apertures be? The subtended angle of the Sun is 2.8 x 103 rad. Compare the separation of the apertures from Mars and from the Sun, which one is closer? Roughly what is the area of coherence on an earth based on aperture screen using the subtend angle of the Sun?

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Mars can be viewed at the unaided eye. The angle subtended by Mars
at the surface of the Earth is 8.0 x 10³ rad. Suppose we filter the light from Mars, passing a
quasi-monochromatic beam at 550 nm, and wish to observe Young's double pinhole fringes.
How far apart, at the very most, could the tiny apertures be? The subtended angle of the Sun
is 2.8 x 103 rad. Compare the separation of the apertures from Mars and from the Sun, which
one is closer? Roughly what is the area of coherence on an earth based on aperture screen
using the subtend angle of the Sun?
Transcribed Image Text:Mars can be viewed at the unaided eye. The angle subtended by Mars at the surface of the Earth is 8.0 x 10³ rad. Suppose we filter the light from Mars, passing a quasi-monochromatic beam at 550 nm, and wish to observe Young's double pinhole fringes. How far apart, at the very most, could the tiny apertures be? The subtended angle of the Sun is 2.8 x 103 rad. Compare the separation of the apertures from Mars and from the Sun, which one is closer? Roughly what is the area of coherence on an earth based on aperture screen using the subtend angle of the Sun?
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