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Astronomy Principles and Practice Fourth Edition.pdf

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The coronagraph 351<br />

By assuming a value of λ = 5 × 10 −4 mm,<br />

d = 5 × 10−4<br />

2(<br />

1<br />

2 062 650 ) mm<br />

≈ 500 mm.<br />

Example 20.3. A Michelson stellar interferometer is used to determine the apparent diameter of a star.<br />

The fringe pattern disappears when the adjustable mirrors are at a separation of 5 m. What is the<br />

angular diameter of the star<br />

By using equation (20.1),<br />

θ = 1·22λ .<br />

d<br />

Again by assuming a value of λ = 5 × 10 −4 mm,<br />

1·22 × 5 × 10−4<br />

θ =<br />

5 × 10 3 rad<br />

= 1·22 × 10 −7 rad<br />

θ ≈ 0·025 arc sec.

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