HIP 4107
HIP 4107 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,864 light-years, HIP 4107 is a distant star lying deep within the Milky Way galaxy.
HIP 4107 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4107 has an apparent magnitude of +8.58, 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 +1.136.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,136 |
Gözlem
| Görünür Parlaklık | +8.58 |
| Mutlak Parlaklık | -0,20 |
| Mesafe | 1,864 ly |
| Takımyıldız | Cassiopeia |
Konum
| Sağ Açıklık | 0h 52,68m |
| Dik Açı | 57° 37,45′ |
Sıkça Sorulan Sorular
What type of star is HIP 4107?
HIP 4107 is a Class K — K-type (Orange) star.
How far is HIP 4107 from Earth?
HIP 4107 is approximately 1,863.8 light-years from Earth.
Can you see HIP 4107 with the naked eye?
With an apparent magnitude of 8.58, HIP 4107 is not visible to the naked eye.
What constellation is HIP 4107 in?
HIP 4107 is located in the constellation Cassiopeia.