Many star catalogs give the distance to a star (if known) as parallax, usually in milli-arcseconds. To convert
this value to something more useful, like Astronomical Units, we can use the conversions below.

### Precise

$$
d = \frac{1au}{\tan \theta}
$$

d = Distance in AU

\(\theta \) = Parallax in degrees (\(\theta = p/3600\))

### Approximate

$$
d = \frac{1}{p}
$$

d = Distance in parsecs

p = Parallax in arcseconds

The parsec is dependent on the measurement for 1 AU, so you may see different conversion factors depending on the definition
of an AU. The IAU has adopted the conversion factor of \( 1\ parsec = \frac{648,000}{\pi}AU \). So simply multiply parsecs
by this constant to yield AU.