14 Trianguli (14 Tri), also known as HD 15656, is a spectroscopic binary[14] located in the northern constellation Triangulum.

It has an apparent magnitude of 5.14,[2] making it faintly visible to the naked eye in ideal conditions.

[5] At its current distance, 14 Tri's brightness is diminished by 0.21 magnitude due to interstellar dust.

It radiates 325 times the luminosity of the Sun from its photosphere at an effective temperature of 3,991 K,[9] giving it an orangish-red hue.

14 Tri is slightly metal-deficient with [Fe/H] = −0.16,[11] and spins modestly with a projected rotational velocity of 2.1 km/s.