Can the distance from the sun to a star be calculated using angles?

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Calculating the distance from the Sun to a star can be achieved using parallax measurement, which involves observing the star from two different positions in Earth's orbit, typically six months apart. The angles involved in the measurements can be expressed mathematically, allowing for the calculation of distance using trigonometric functions. Specifically, the relationship D = (sin(α + ∂) / sin(∂)) * d illustrates how the angles α and ∂ relate to the distance D from the Sun to the star. This method leverages the small angular differences observed due to Earth's movement around the Sun, enabling astronomers to determine stellar distances accurately.
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Is it possible to calculate the distance from the sun to a star like this? (what I mean is can the angles from the diagram actually be calculated?)

From the diagram:
γ = ∏ - α - ∂
= ∏ - (α + ∂)
D / sin(γ) = d / sin(∂)
sin(γ) = sin(∏ - (α + ∂))
= sin(α + ∂)
D / sin(α + ∂) = d / sin(∂)

D = (sin(α + ∂) / sin(∂)) * d
 

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Look up parallax measurement. This is essentially what we do to measure the distance to the nearest stars. The difference is that, since we can't make measurements from the sun (to measure the angle you've marked alpha), we measure the direction of the star from two different sides of the Earth's orbit, for example, measuring in June and then again in December. The small difference in these two angles, when combined with the diameter of the Earth's orbit, allows us to measure the distance to the star.
 
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