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The smallest shift you can reliably measure on the screen is about 0.2 grid units. This shift corresponds to the precision of positions measured with the best Earth-based optical telescopes. If you cannot measure an angle smaller than this, what is the maximum distance at which a star can be located and still have a measurable parallax

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Answer:

The distance is
d = 1.5 *10^(15) \ km

Step-by-step explanation:

From the question we are told that

The smallest shift is
d = 0.2 \ grid \ units

Generally a grid unit is
(1)/(10) of an arcsec

This implies that 0.2 grid unit is
k = (0.2)/(10) = 0.02 \ arc sec

The maximum distance at which a star can be located and still have a measurable parallax is mathematically represented as


d = (1)/(k)

substituting values


d = (1)/(0.02)


d = 50 \ parsec

Note
1 \ parsec \ \to 3.26 \ light \ year \ \to 3.086*10^(13) \ km

So
d = 50 * 3.08 *10^(13)


d = 1.5 *10^(15) \ km

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