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Finding magnitude of part of binary system

  1. Jan 27, 2010 #1
    3. A very cool, faint white dwarf is identified as such from its spectrum and is known to have an apparent visual magnitude, mv = 16.73. A series of observations over several years yields a parallax measurement of 171±2 mas (milli-arcseconds).

    (i) How far away is the white dwarf, and what must its absolute visual magnitude be?

    (ii) Repeated spectroscopic observations of the white dwarf provide evidence that the white dwarf is in fact a close binary system, in which the brighter component contributes twice as much visual light as the fainter component. What would the apparent magnitude of the fainter star be, in the absence of its brighter companion?

    I have done part i) but i cant do part ii) my attempt is below

    My Attempt:

    Ma: apparent mag of brighter star
    Mb: apparent mag of dimmer star

    Ma-Mb = 2.512 x log(Fa/Fb)

    16.73-Mb = 2.512 x log(2) [as the brighter star is twice as bright]

    Mb = 15.97

    but this number is lower and so means it is brighter than the brightest star!?!

    any help would be much appreciated TIA
    1. The problem statement, all variables and given/known data

    2. Relevant equations

    3. The attempt at a solution
  2. jcsd
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