HIP 63630
HIP 63630 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,140 light-years, HIP 63630 is a distant star lying deep within the Milky Way galaxy.
HIP 63630 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 63630 has an apparent magnitude of +8.55, 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 orange hue, which corresponds to a B-V color index of +1.063.
Đặc tính vật lý
| Phân Loại Quang Phổ | K Class K — K-type (Orange) |
| Chỉ số màu (B−V) | 1,063 |
Quan sát
| Cấp Sao Biểu Kiến | +8.55 |
| Cấp Sao Tuyệt Đối | 0,83 |
| Khoảng Cách | 1,140 ly |
| Chòm Sao | Centaurus |
Vị trí
| Xích kinh | 13h 2,49m |
| Xích vĩ | -37° 26,92′ |
Frequently Asked Questions
What type of star is HIP 63630?
HIP 63630 is a Class K — K-type (Orange) star.
How far is HIP 63630 from Earth?
HIP 63630 is approximately 1,140.4 light-years from Earth.
Can you see HIP 63630 with the naked eye?
With an apparent magnitude of 8.55, HIP 63630 is not visible to the naked eye.
What constellation is HIP 63630 in?
HIP 63630 is located in the constellation Centaurus.