HIP 7399
HIP 7399 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 924.0 light-years from Earth, HIP 7399 resides within the broader disk of our Milky Way galaxy.
HIP 7399 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 7399 has an apparent magnitude of +6.86, 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 -0.012.
Fiziksel Özellikler
| Spektral Sınıf | Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | -0,012 |
Gözlem
| Görünür Parlaklık | +6.86 |
| Mutlak Parlaklık | -0,40 |
| Mesafe | 924 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 1h 35,40m |
| Dik Açı | 53° 20,73′ |
Sıkça Sorulan Sorular
What type of star is HIP 7399?
HIP 7399 is a Class B — B-type (Blue-White) star.
How far is HIP 7399 from Earth?
HIP 7399 is approximately 924.0 light-years from Earth.
Can you see HIP 7399 with the naked eye?
With an apparent magnitude of 6.86, HIP 7399 is not visible to the naked eye.
What constellation is HIP 7399 in?
HIP 7399 is located in the constellation Perseus.