HIP 49909
HIP 49909 is a B-type (Blue-White) star.
At a distance of roughly 1,885 light-years, HIP 49909 is a distant star lying deep within the Milky Way galaxy.
HIP 49909 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 49909 has an apparent magnitude of +7.87, 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 -0.097.
Fiziksel Özellikler
| Spektral Sınıf | B Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | -0,097 |
Gözlem
| Görünür Parlaklık | +7.87 |
| Mutlak Parlaklık | -0,94 |
| Mesafe | 1,885 ly |
Konum
| Sağ Açıklık | 10h 11,40m |
| Dik Açı | -50° 29,42′ |
Frequently Asked Questions
What type of star is HIP 49909?
HIP 49909 is a Class B — B-type (Blue-White) star.
How far is HIP 49909 from Earth?
HIP 49909 is approximately 1,885.3 light-years from Earth.
Can you see HIP 49909 with the naked eye?
With an apparent magnitude of 7.87, HIP 49909 is not visible to the naked eye.