HD 202908, also known as HIP 105200, is a triple star located in the equatorial constellation Equuleus.
[2] The system is located relatively close at a distance of 169 light years based on Gaia DR3 parallax measurements[9] but it is receding with a heliocentric radial velocity of 6.24 km/s.
[18] The "A" component is a double-lined spectroscopic binary that contains two solar-type stars with spectral classifications of F9 V and G0 V respectively.
[10] The tertiary companion designated "B" has a class of G1.5 V, indicating that it is an ordinary G-type main-sequence star like our Sun.
It radiates 84% of the Sun's luminosity[13] from its photosphere at an effective temperature of 5,703 K.[2] The system is estimated to be 6.4 billion years old.