How Far is Nanyang's Star from Earth in Parsecs?

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The discussion focuses on calculating the distance from Earth to Nanyang's star in parsecs. A formula involving magnitudes and distance is referenced, specifically m2 - m1 = 5log(d2/d1) + Ad2. There is a clarification needed regarding the correct specification of distance, with a suggestion that d2 should be set at 1000 parsecs. The participants emphasize the importance of accurate distance measurement in the calculations. Overall, the conversation centers on resolving the distance calculation to Nanyang's star.
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Homework Statement
Suppose that to a particular heliocentric 3D-Cartesian coordinate, the Earth is located at (1,0,0) A.U. You tried to observe Nanyang Star (with the same luminosity as the Sun) from the Earth. Nanyang Star is located at (1,0,1) kpc in the same coordinate system. If you obtained a visual magnitude of +17.2 from the observation, what is the coefficient of absorption, defined as the visual magnitude increase per unit distance due to interstellar matter, in the star’s direction? (It is given that Sun’s absolute magnitude is +4.83.)
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Apparent Magnitude
73341974-82DB-4DE5-8B66-247B5D291A10.jpegMy attempt has been attached.
 
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Shouldn't you have m2 - m1 = 5log(d2/d1) + Ad2?
And is d2 = 1000 pc?
 
As @mjc123 implied, you don't have d specified correctly. How far is it from Earth to Nanyang's star in pc? This is what you should use for d.
 
So is there some elegant way to do this or am I just supposed to follow my nose and sub the Taylor expansions for terms in the two boost matrices under the assumption ##v,w\ll 1##, then do three ugly matrix multiplications and get some horrifying kludge for ##R## and show that the product of ##R## and its transpose is the identity matrix with det(R)=1? Without loss of generality I made ##\mathbf{v}## point along the x-axis and since ##\mathbf{v}\cdot\mathbf{w} = 0## I set ##w_1 = 0## to...

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