Based upon an annual parallax shift of 34.25 mas as seen from Earth,[1] it lies 95 light years from the Sun.
HD 219077 is moving closer to the Sun with a radial velocity of −31.01,[5] and has a relatively high proper motion.
The star is older than the Sun with an estimated age of 8.9 billion years and is spinning slowly with rotation period of around 47 days.
It is radiating 2.66 times the Sun's luminosity from its photosphere at an effective temperature of 5,362 K.[2] From 1998 to 2012, the star was placed under observation using the CORALIE echelle spectrograph at La Silla Observatory.
They submitted HD 219077 b as a candidate for direct imaging, once it gets out to 11.0 AU at apoastron with 375 milliarcseconds of angular separation as seen from Earth.