HIP 91007
HIP 91007 is a B-type (Blue-White) star located in the constellation Lyra.
At a distance of roughly 2,718 light-years, HIP 91007 is a distant star lying deep within the Milky Way galaxy.
HIP 91007 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 91007 has an apparent magnitude of +9.65, 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 +0.043.
Fiziksel Özellikler
| Spektral Sınıf | Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | 0,043 |
Gözlem
| Görünür Parlaklık | +9.65 |
| Mutlak Parlaklık | 0,05 |
| Mesafe | 2,718 ly |
| Takımyıldız | Lyra |
Konum
| Sağ Açıklık | 18h 33,91m |
| Dik Açı | 29° 27,86′ |
Sıkça Sorulan Sorular
What type of star is HIP 91007?
HIP 91007 is a Class B — B-type (Blue-White) star.
How far is HIP 91007 from Earth?
HIP 91007 is approximately 2,718.0 light-years from Earth.
Can you see HIP 91007 with the naked eye?
With an apparent magnitude of 9.65, HIP 91007 is not visible to the naked eye.
What constellation is HIP 91007 in?
HIP 91007 is located in the constellation Lyra.