HIP 31992
HIP 31992 is a B-type (Blue-White) star.
At a distance of roughly 1,254 light-years, HIP 31992 is a distant star lying deep within the Milky Way galaxy.
HIP 31992 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.79, HIP 31992 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.094.
Fiziksel Özellikler
| Spektral Sınıf | B Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | -0,094 |
Gözlem
| Görünür Parlaklık | +5.79 |
| Mutlak Parlaklık | -2,14 |
| Mesafe | 1,254 ly |
Konum
| Sağ Açıklık | 6h 41,09m |
| Dik Açı | 0° 29,72′ |
Frequently Asked Questions
What type of star is HIP 31992?
HIP 31992 is a Class B — B-type (Blue-White) star.
How far is HIP 31992 from Earth?
HIP 31992 is approximately 1,254.4 light-years from Earth.
Can you see HIP 31992 with the naked eye?
With an apparent magnitude of 5.79, HIP 31992 is visible to the naked eye.