HIP 54790
HIP 54790 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 2,219 light-years, HIP 54790 is a distant star lying deep within the Milky Way galaxy.
HIP 54790 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 54790 has an apparent magnitude of +8.77, 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 blue hue, which corresponds to a B-V color index of -0.010.
Fiziksel Özellikler
| Spektral Sınıf | Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | -0,010 |
Gözlem
| Görünür Parlaklık | +8.77 |
| Mutlak Parlaklık | -0,39 |
| Mesafe | 2,219 ly |
| Takımyıldız | Centaurus |
Konum
| Sağ Açıklık | 11h 13,01m |
| Dik Açı | -57° 2,11′ |
Sıkça Sorulan Sorular
What type of star is HIP 54790?
HIP 54790 is a Class B — B-type (Blue-White) star.
How far is HIP 54790 from Earth?
HIP 54790 is approximately 2,218.8 light-years from Earth.
Can you see HIP 54790 with the naked eye?
With an apparent magnitude of 8.77, HIP 54790 is not visible to the naked eye.
What constellation is HIP 54790 in?
HIP 54790 is located in the constellation Centaurus.