HIP 9890

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HIP 9890 is a B-type (Blue-White) star located in the constellation Perseus.

Located approximately 698.4 light-years from Earth, HIP 9890 resides within the broader disk of our Milky Way galaxy.

HIP 9890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

HIP 9890 has an apparent magnitude of +8.69, 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-white hue, which corresponds to a B-V color index of +0.116.

Đặc tính vật lý

Phân Loại Quang Phổ B Class B — B-type (Blue-White)
Chỉ số màu (B−V) 0,116

Quan sát

Cấp Sao Biểu Kiến +8.69
Cấp Sao Tuyệt Đối 2,04
Khoảng Cách 698 ly
Chòm Sao Perseus

Vị trí

Xích kinh 2h 7,25m
Xích vĩ 48° 6,04′

Frequently Asked Questions

What type of star is HIP 9890?
HIP 9890 is a Class B — B-type (Blue-White) star.
How far is HIP 9890 from Earth?
HIP 9890 is approximately 698.4 light-years from Earth.
Can you see HIP 9890 with the naked eye?
With an apparent magnitude of 8.69, HIP 9890 is not visible to the naked eye.
What constellation is HIP 9890 in?
HIP 9890 is located in the constellation Perseus.