HIP 67885
HIP 67885 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 1,019 light-years, HIP 67885 is a distant star lying deep within the Milky Way galaxy.
HIP 67885 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 67885 has an apparent magnitude of +8.20, 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-white hue, which corresponds to a B-V color index of +0.079.
Sifat Fisik
| Kelas Spektral | B Class B — B-type (Blue-White) |
| Indeks Warna (B−V) | 0,079 |
Pengamatan
| Magnitudo Semu | +8.20 |
| Magnitudo Mutlak | 0,73 |
| Jarak | 1,019 ly |
| Rasi Bintang | Centaurus |
Posisi
| Asensio Rekta | 13h 54,21m |
| Deklinasi | -51° 24,00′ |
Frequently Asked Questions
What type of star is HIP 67885?
HIP 67885 is a Class B — B-type (Blue-White) star.
How far is HIP 67885 from Earth?
HIP 67885 is approximately 1,019.2 light-years from Earth.
Can you see HIP 67885 with the naked eye?
With an apparent magnitude of 8.20, HIP 67885 is not visible to the naked eye.
What constellation is HIP 67885 in?
HIP 67885 is located in the constellation Centaurus.