HIP 111988
HIP 111988 is a K-type (Orange) star.
At a distance of roughly 3,106 light-years, HIP 111988 is a distant star lying deep within the Milky Way galaxy.
HIP 111988 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 111988 has an apparent magnitude of +6.77, 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 +1.517.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,517 |
Gözlem
| Görünür Parlaklık | +6.77 |
| Mutlak Parlaklık | -3,12 |
| Mesafe | 3,106 ly |
Konum
| Sağ Açıklık | 22h 41,05m |
| Dik Açı | 51° 45,51′ |
Frequently Asked Questions
What type of star is HIP 111988?
HIP 111988 is a Class K — K-type (Orange) star.
How far is HIP 111988 from Earth?
HIP 111988 is approximately 3,106.2 light-years from Earth.
Can you see HIP 111988 with the naked eye?
With an apparent magnitude of 6.77, HIP 111988 is not visible to the naked eye.