While reading my introductory astronomy textbook, I read about two formulae that were used to determine distances using parallax.
One was d(parsecs)=1/p(parallax in arc seconds), but I vaguely remember something like:
distance=baseline*(parallax in degrees/57.3)
What is this second formula and when is it used/is it the same as the 1st, but written in a different form?
Thanks!



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