Source: cirosantilli/proper-motion
= Proper motion
{wiki}
Some stars are so close that we can actually see their angles move with time due to the relative motion between them and the <Sun>, e.g. <Proxima Centauri>!
= Proper motion
{wiki}
Some stars are so close that we can actually see their angles move with time due to the relative motion between them and the <Sun>, e.g. <Proxima Centauri>!