TOI-1117

TOI-1117 is a single G-type star in the constellation of Pavo. It has approximately 0.97 times the mass and 1.05 times the radius of the Sun, with a surface temperature of 5,635 K and a spectral type of G7. TOI-1117 is too faint to be visible to the naked eye. Based upon parallax measurements, it is located from the Sun. The object is drifting towards the Sun with a radial velocity of.

Planetary system

In June of 2025, three exoplanets were identified via the radial velocity method. An additional planet was discovered using the transit technique.
None of these planets orbit in the habitable zone; all are believed to be sub-Neptune planets.