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Two things.

First, the magnitude of a star; its brightness

Then, the magnitude is viewed through two different filters.

They are either U(ltraviolet) and B(lue) or B and V(isual), and belong to a photometric system called the UBV system.

From this, optical astronomers extrapolate the effective temperature of a star from its colour.

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Q: What is analyzed to determine the temperature of a star?
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