HIP 1988
HIP 1988 is a K-type (Orange) star located in the constellation Cassiopeia.
Located approximately 997.4 light-years from Earth, HIP 1988 resides within the broader disk of our Milky Way galaxy.
HIP 1988 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 1988 has an apparent magnitude of +8.34, 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 red hue, which corresponds to a B-V color index of +1.597.
Đặc tính vật lý
| Phân Loại Quang Phổ | Class K — K-type (Orange) |
| Chỉ số màu (B−V) | 1,597 |
Quan sát
| Cấp Sao Biểu Kiến | +8.34 |
| Cấp Sao Tuyệt Đối | 0,91 |
| Khoảng Cách | 997 ly |
| Chòm Sao | Cassiopeia |
Vị trí
| Xích kinh | 0h 25,17m |
| Xích vĩ | 64° 38,32′ |
Câu hỏi thường gặp
What type of star is HIP 1988?
HIP 1988 is a Class K — K-type (Orange) star.
How far is HIP 1988 from Earth?
HIP 1988 is approximately 997.4 light-years from Earth.
Can you see HIP 1988 with the naked eye?
With an apparent magnitude of 8.34, HIP 1988 is not visible to the naked eye.
What constellation is HIP 1988 in?
HIP 1988 is located in the constellation Cassiopeia.