HIP 17425

HIP 17425 is a B-type (Blue-White) star located in the constellation Perseus.

HIP 17425 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.

HIP 17425 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

At an apparent magnitude of +10.18, HIP 17425 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its blue-white hue, which corresponds to a B-V color index of +0.210.

Đặc tính vật lý

Phân Loại Quang Phổ Class B — B-type (Blue-White)
Chỉ số màu (B−V) 0,210

Quan sát

Cấp Sao Biểu Kiến +10.18
Cấp Sao Tuyệt Đối -9,82
Khoảng Cách 326,156 ly
Chòm Sao Perseus

Vị trí

Xích kinh 3h 43,99m
Xích vĩ 34° 11,33′

Câu hỏi thường gặp

What type of star is HIP 17425?
HIP 17425 is a Class B — B-type (Blue-White) star.
How far is HIP 17425 from Earth?
HIP 17425 is approximately 326,156.0 light-years from Earth.
Can you see HIP 17425 with the naked eye?
With an apparent magnitude of 10.18, HIP 17425 is not visible to the naked eye.
What constellation is HIP 17425 in?
HIP 17425 is located in the constellation Perseus.