HIP 13730
HIP 13730 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,042 light-years, HIP 13730 is a distant star lying deep within the Milky Way galaxy.
HIP 13730 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 13730 has an apparent magnitude of +8.59, 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 +1.877.
Fiziksel Özellikler
| Spektral Sınıf | Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,877 |
Gözlem
| Görünür Parlaklık | +8.59 |
| Mutlak Parlaklık | 1,07 |
| Mesafe | 1,042 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 2h 56,82m |
| Dik Açı | 50° 47,80′ |
Sıkça Sorulan Sorular
What type of star is HIP 13730?
HIP 13730 is a Class K — K-type (Orange) star.
How far is HIP 13730 from Earth?
HIP 13730 is approximately 1,042.0 light-years from Earth.
Can you see HIP 13730 with the naked eye?
With an apparent magnitude of 8.59, HIP 13730 is not visible to the naked eye.
What constellation is HIP 13730 in?
HIP 13730 is located in the constellation Perseus.