HIP 30918
HIP 30918 is a A-type (White) star located in the constellation Canis Major.
At a distance of roughly 2,812 light-years, HIP 30918 is a distant star lying deep within the Milky Way galaxy.
HIP 30918 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 30918 has an apparent magnitude of +8.06, 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 +0.071.
Fiziksel Özellikler
| Spektral Sınıf | Class A — A-type (White) |
| Renk İndeksi (B−V) | 0,071 |
Gözlem
| Görünür Parlaklık | +8.06 |
| Mutlak Parlaklık | -1,62 |
| Mesafe | 2,812 ly |
| Takımyıldız | Canis Major |
Konum
| Sağ Açıklık | 6h 29,36m |
| Dik Açı | -17° 48,79′ |
Sıkça Sorulan Sorular
What type of star is HIP 30918?
HIP 30918 is a Class A — A-type (White) star.
How far is HIP 30918 from Earth?
HIP 30918 is approximately 2,811.7 light-years from Earth.
Can you see HIP 30918 with the naked eye?
With an apparent magnitude of 8.06, HIP 30918 is not visible to the naked eye.
What constellation is HIP 30918 in?
HIP 30918 is located in the constellation Canis Major.