HIP 3887
HIP 3887 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 2,509 light-years, HIP 3887 is a distant star lying deep within the Milky Way galaxy.
HIP 3887 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 3887 has an apparent magnitude of +8.51, 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 yellow-white hue, which corresponds to a B-V color index of +0.616.
Đặc tính vật lý
| Phân Loại Quang Phổ | Class B — B-type (Blue-White) |
| Chỉ số màu (B−V) | 0,616 |
Quan sát
| Cấp Sao Biểu Kiến | +8.51 |
| Cấp Sao Tuyệt Đối | -0,92 |
| Khoảng Cách | 2,509 ly |
| Chòm Sao | Cassiopeia |
Vị trí
| Xích kinh | 0h 49,89m |
| Xích vĩ | 64° 38,27′ |
Câu hỏi thường gặp
What type of star is HIP 3887?
HIP 3887 is a Class B — B-type (Blue-White) star.
How far is HIP 3887 from Earth?
HIP 3887 is approximately 2,508.9 light-years from Earth.
Can you see HIP 3887 with the naked eye?
With an apparent magnitude of 8.51, HIP 3887 is not visible to the naked eye.
What constellation is HIP 3887 in?
HIP 3887 is located in the constellation Cassiopeia.