Distance to a star using parallax. Estimate the distance D to a star if the angle \theta in Fig.44-11 is measured to be 89.99994^{\circ}.
APPROACH From trigonometry, \tan \phi=d / D in Fig. 44-11. The Sun-Earth distance is d=1.5 \times 10^{8} \mathrm{~km}.
The angle \phi=90^{\circ}-89.99994^{\circ}=0.00006^{\circ}, or about 1.0 \times 10^{-6} radians. We can use \tan \phi \approx \phi since \phi is very small. We solve for D in \tan \phi=d / D. The distance D to the star is
D=\frac{d}{\tan \phi} \approx \frac{d}{\phi}=\frac{1.5 \times 10^{8} \mathrm{~km}}{1.0 \times 10^{-6} \,\mathrm{rad}}=1.5 \times 10^{14} \mathrm{~km},
or about 15 ly.