HIP 182
HIP 182 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,406 light-years, HIP 182 is a distant star lying deep within the Milky Way galaxy.
HIP 182 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 182 has an apparent magnitude of +8.55, 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 +1.004.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,004 |
Gözlem
| Görünür Parlaklık | +8.55 |
| Mutlak Parlaklık | 0,38 |
| Mesafe | 1,406 ly |
| Takımyıldız | Cassiopeia |
Konum
| Sağ Açıklık | 0h 2,32m |
| Dik Açı | 52° 35,18′ |
Frequently Asked Questions
What type of star is HIP 182?
HIP 182 is a Class K — K-type (Orange) star.
How far is HIP 182 from Earth?
HIP 182 is approximately 1,405.8 light-years from Earth.
Can you see HIP 182 with the naked eye?
With an apparent magnitude of 8.55, HIP 182 is not visible to the naked eye.
What constellation is HIP 182 in?
HIP 182 is located in the constellation Cassiopeia.