HIP 58825
HIP 58825 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 2,104 light-years, HIP 58825 is a distant star lying deep within the Milky Way galaxy.
HIP 58825 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 58825 has an apparent magnitude of +9.53, 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 +1.287.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,287 |
Gözlem
| Görünür Parlaklık | +9.53 |
| Mutlak Parlaklık | 0,48 |
| Mesafe | 2,104 ly |
| Takımyıldız | Centaurus |
Konum
| Sağ Açıklık | 12h 3,89m |
| Dik Açı | -41° 20,39′ |
Sıkça Sorulan Sorular
What type of star is HIP 58825?
HIP 58825 is a Class K — K-type (Orange) star.
How far is HIP 58825 from Earth?
HIP 58825 is approximately 2,104.2 light-years from Earth.
Can you see HIP 58825 with the naked eye?
With an apparent magnitude of 9.53, HIP 58825 is not visible to the naked eye.
What constellation is HIP 58825 in?
HIP 58825 is located in the constellation Centaurus.