HIP 104690
HIP 104690 is a K-type (Orange) star.
At a distance of roughly 1,059 light-years, HIP 104690 is a distant star lying deep within the Milky Way galaxy.
HIP 104690 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104690 has an apparent magnitude of +8.67, 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 +1.013.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,013 |
Gözlem
| Görünür Parlaklık | +8.67 |
| Mutlak Parlaklık | 1,11 |
| Mesafe | 1,059 ly |
Konum
| Sağ Açıklık | 21h 12,42m |
| Dik Açı | -76° 56,05′ |
Frequently Asked Questions
What type of star is HIP 104690?
HIP 104690 is a Class K — K-type (Orange) star.
How far is HIP 104690 from Earth?
HIP 104690 is approximately 1,059.0 light-years from Earth.
Can you see HIP 104690 with the naked eye?
With an apparent magnitude of 8.67, HIP 104690 is not visible to the naked eye.