HIP 104360
HIP 104360 is a K-type (Orange) star.
At a distance of roughly 1,553 light-years, HIP 104360 is a distant star lying deep within the Milky Way galaxy.
HIP 104360 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104360 has an apparent magnitude of +8.21, 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 +1.520.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,520 |
Gözlem
| Görünür Parlaklık | +8.21 |
| Mutlak Parlaklık | -0,18 |
| Mesafe | 1,553 ly |
Konum
| Sağ Açıklık | 21h 8,49m |
| Dik Açı | -26° 36,43′ |
Frequently Asked Questions
What type of star is HIP 104360?
HIP 104360 is a Class K — K-type (Orange) star.
How far is HIP 104360 from Earth?
HIP 104360 is approximately 1,553.1 light-years from Earth.
Can you see HIP 104360 with the naked eye?
With an apparent magnitude of 8.21, HIP 104360 is not visible to the naked eye.