HIP 107485
HIP 107485 is a K-type (Orange) star.
At a distance of roughly 2,174 light-years, HIP 107485 is a distant star lying deep within the Milky Way galaxy.
HIP 107485 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 107485 has an apparent magnitude of +7.66, 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 +1.494.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,494 |
Gözlem
| Görünür Parlaklık | +7.66 |
| Mutlak Parlaklık | -1,46 |
| Mesafe | 2,174 ly |
Konum
| Sağ Açıklık | 21h 46,24m |
| Dik Açı | -47° 24,19′ |
Frequently Asked Questions
What type of star is HIP 107485?
HIP 107485 is a Class K — K-type (Orange) star.
How far is HIP 107485 from Earth?
HIP 107485 is approximately 2,174.4 light-years from Earth.
Can you see HIP 107485 with the naked eye?
With an apparent magnitude of 7.66, HIP 107485 is not visible to the naked eye.