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.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,063 |
Gözlem
| Görünür Parlaklık | +8.55 |
| Mutlak Parlaklık | 0,83 |
| Mesafe | 1,140 ly |
| Takımyıldız | Centaurus |
Konum
| Sağ Açıklık | 13h 2,49m |
| Dik Açı | -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.