Parallax (source code)

= Parallax
{title2=$d(\mathrm{pc})=1/p(\mathrm{arcsec})$}
{wiki}

Parallax is the apparent change in the direction of an object when the observing position changes. <Stellar parallax> uses Earth's orbital baseline and measures half the annual angular excursion; its standard distance relation is the one displayed. A nearer object has a larger parallax for the same baseline.