HD 196775 explained

HD 196775 (HR 7899) is a solitary star in the equatorial constellation Delphinus. It has an apparent magnitude of 5.98, allowing it to be faintly seen with the naked eye. The object is relatively far at a distance of 1,050 light years but is approaching the Solar System with a heliocentric radial velocity of . HD 196775 has a high peculiar velocity of compared to neighboring stars, indicating that it may be a runaway star.

HD 196775 has a general stellar classification of B3 V, indicating that it is an ordinary B-type main-sequence star. However, once source gives it a class of B4 Vn, making it slightly cooler and having broad absorption lines due to rapid rotation. It has an angular diameter of, yielding a radius 4.13 times that of the Sun. At present it has 7 times the mass of the Sun and shines at from its photosphere at an effective temperature of, giving it a whitish blue hue. HD 196775 is 36 million years old and is spinning rapidly with a projected rotational velocity of .

HD 196775 has four faint optical companions whose parameters are listed below.

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HD 196775's Companions!Companion!mv!PA (°)!Year!Sep. ()
B12.4015420065.2
C11.31122201239.9
D14.40146201228.8
E14.4033201223.3