Problem solved in full
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Deriving the parsec from a parallax of 100 milliarcseconds 6 steps
A parallax of 100 milliarcseconds. Derive the parsec from its definition rather than looking it up, get the distance, and explain why the distance modulus is exactly zero.
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The parallax angle is half the apparent shift over six months, and the triangle it sits in has the Earth's orbital radius as its short side. At these angles the tangent and the angle are the same number.
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Choose the unit that makes the formula trivial. One arcsecond in radians is 1/206,265, so a parallax of one arcsecond puts the star 206,265 au away — and that distance is given a name.
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With the parsec defined, distance is just a reciprocal. The field on this page is in milliarcseconds, which puts a factor of a thousand on top.
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The distance modulus is the logarithmic form of the inverse-square law, normalised at ten parsecs. At exactly that distance the logarithm is of 1, so the modulus vanishes.
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Check the formula on the nearest star. Proxima's 768.5 mas gives 1.301 pc, which is 4.24 light years — the number everybody already knows.
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Finally, note where the method runs out. Gaia's smallest usable parallax corresponds to an enormous distance, but the uncertainty at that angle is comparable to the angle itself, so the limit is set by precision rather than by geometry.
Answer
10.00 pc, and μ = 0 because 10 pc is where absolute magnitude is defined. Absolute magnitude is not a separate quantity to be measured; it is the apparent magnitude a star would have at exactly ten parsecs, so a star that happens to be there has m − M = 0 by construction. The parsec is equally a definition rather than a measurement: it is the distance at which one astronomical unit subtends one arcsecond, which makes it 206,265 au because that is how many arcseconds are in a radian. Both conventions exist so that the first rung of the ladder needs no calibration at all — parallax is pure trigonometry on a baseline we already know. Everything above it, Cepheids and supernovae and Hubble flow, is calibrated against this rung and inherits its errors.
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Learning path
How far away is it?
References (1)
- Insight block 1 — the rung everything above it is calibrated against: H. S. Leavitt and E. C. Pickering, "Periods of 25 Variable Stars in the Small Magellanic Cloud." Harvard College Observatory Circular 173, 1–3, 1912 — the period–luminosity relation, published under Pickering's name over Leavitt's work.