HIP 66451
HIP 66451 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 2,038 light-years, HIP 66451 is a distant star lying deep within the Milky Way galaxy.
HIP 66451 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 66451 has an apparent magnitude of +8.38, 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 -0.071.
Sifat Fisik
| Kelas Spektral | B Class B — B-type (Blue-White) |
| Indeks Warna (B−V) | -0,071 |
Pengamatan
| Magnitudo Semu | +8.38 |
| Magnitudo Mutlak | -0,60 |
| Jarak | 2,038 ly |
| Rasi Bintang | Centaurus |
Posisi
| Asensio Rekta | 13h 37,37m |
| Deklinasi | -47° 32,26′ |
Frequently Asked Questions
What type of star is HIP 66451?
HIP 66451 is a Class B — B-type (Blue-White) star.
How far is HIP 66451 from Earth?
HIP 66451 is approximately 2,038.5 light-years from Earth.
Can you see HIP 66451 with the naked eye?
With an apparent magnitude of 8.38, HIP 66451 is not visible to the naked eye.
What constellation is HIP 66451 in?
HIP 66451 is located in the constellation Centaurus.