HIP 5451
HIP 5451 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,812 light-years, HIP 5451 is a distant star lying deep within the Milky Way galaxy.
HIP 5451 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 5451 has an apparent magnitude of +8.05, 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 +1.179.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,179 |
Gözlem
| Görünür Parlaklık | +8.05 |
| Mutlak Parlaklık | -0,67 |
| Mesafe | 1,812 ly |
| Takımyıldız | Cassiopeia |
Konum
| Sağ Açıklık | 1h 9,76m |
| Dik Açı | 52° 51,27′ |
Sıkça Sorulan Sorular
What type of star is HIP 5451?
HIP 5451 is a Class K — K-type (Orange) star.
How far is HIP 5451 from Earth?
HIP 5451 is approximately 1,812.0 light-years from Earth.
Can you see HIP 5451 with the naked eye?
With an apparent magnitude of 8.05, HIP 5451 is not visible to the naked eye.
What constellation is HIP 5451 in?
HIP 5451 is located in the constellation Cassiopeia.