17 Vulpeculae

17 Vulpeculae is a star located in the constellation Vulpecula. It is a yellow-white hued star with an apparent magnitude of approximately 5.9, making it faintly visible to the naked eye under dark sky conditions.

Spectroscopically, 17 Vulpeculae is classified as an F2 V star. This classification indicates that it is an F-type star on the main sequence, meaning it is a hydrogen-fusing dwarf star. F-type stars are generally hotter and more massive than our Sun, with surface temperatures ranging from around 6,000 to 7,500 Kelvin. The 'V' luminosity class indicates that the star is a main sequence star, generating energy through nuclear fusion in its core.

Precise measurements of its distance are challenging due to its relative faintness, but estimated distances place it several hundred light-years away from Earth. Its precise age and evolutionary state are subjects of ongoing research.

17 Vulpeculae is not known to host any planets or to be part of a binary or multiple star system. Further observations and analysis would be necessary to confirm its characteristics and to search for any orbiting companions.