HIP 17890

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HIP 17890 is a A-type (White) star located in the constellation Perseus.

At a distance of roughly 1,524 light-years, HIP 17890 is a distant star lying deep within the Milky Way galaxy.

HIP 17890 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.

HIP 17890 has an apparent magnitude of +9.33, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its blue hue, which corresponds to a B-V color index of -0.070.

Физические свойства

Спектральный класс A Class A — A-type (White)
Показатель цвета (B−V) -0,070

Наблюдение

Видимая звёздная величина +9.33
Абсолютная звёздная величина 0,98
Расстояние 1,524 ly
Созвездие Perseus

Положение

Прямое восхождение 3h 49,61m
Склонение 38° 58,92′

Frequently Asked Questions

What type of star is HIP 17890?
HIP 17890 is a Class A — A-type (White) star.
How far is HIP 17890 from Earth?
HIP 17890 is approximately 1,524.1 light-years from Earth.
Can you see HIP 17890 with the naked eye?
With an apparent magnitude of 9.33, HIP 17890 is not visible to the naked eye.
What constellation is HIP 17890 in?
HIP 17890 is located in the constellation Perseus.