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Convert 4.29 light years into parsecs. Calculate the parallax of a star at the distance when viewed from two locations of earth six months apart in its orbit around sun.

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Conversion : We know that

1 light year = 9.46 × 1015 m

∴ 4.29 light years = 4.29 × 9.46 × 1015

= 4.058 × 1016 m

Also, 1 parsec = 3.08 × 1016 m

∴ 4.29 light year = \(\frac{4.058\times10^{16}}{3.08\times10^{16}}\)

= 1.318 parsec

= 1.32 parsec

(b) Parallax− In six months, the distance between two observations will be equal to the diameter of the orbit, i.e.

2 × radius of orbit

2 AU = 2 × 1.496 × 1011 m

Using, θ = \(\frac{b}{D}\)

where b = 2 × 1.496 × 1011 m

and D = 4.058 × 1016

we get, θ = \(\frac{2\times1.496\times10^{11}}{4.058\times10^{16}}\)

= 7.37 × 10-6 rad

= 7.37 × 10-6 × \(\frac{180\times60\times60}{\pi}\)

= 1.52 second of arc.

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