HIP 63299
HIP 63299 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 1,896 light-years, HIP 63299 is a distant star lying deep within the Milky Way galaxy.
HIP 63299 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 63299 has an apparent magnitude of +9.99, 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 +0.172.
Fiziksel Özellikler
| Spektral Sınıf | B Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | 0,172 |
Gözlem
| Görünür Parlaklık | +9.99 |
| Mutlak Parlaklık | 1,17 |
| Mesafe | 1,896 ly |
| Takımyıldız | Centaurus |
Konum
| Sağ Açıklık | 12h 58,32m |
| Dik Açı | -61° 1,04′ |
Frequently Asked Questions
What type of star is HIP 63299?
HIP 63299 is a Class B — B-type (Blue-White) star.
How far is HIP 63299 from Earth?
HIP 63299 is approximately 1,896.3 light-years from Earth.
Can you see HIP 63299 with the naked eye?
With an apparent magnitude of 9.99, HIP 63299 is not visible to the naked eye.
What constellation is HIP 63299 in?
HIP 63299 is located in the constellation Centaurus.