HIP 1590
HIP 1590 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,019 light-years, HIP 1590 is a distant star lying deep within the Milky Way galaxy.
HIP 1590 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 1590 has an apparent magnitude of +9.75, 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 +0.104.
Fiziksel Özellikler
| Spektral Sınıf | B Class B — B-type (Blue-White) |
| Renk İndeksi (B−V) | 0,104 |
Gözlem
| Görünür Parlaklık | +9.75 |
| Mutlak Parlaklık | 2,28 |
| Mesafe | 1,019 ly |
| Takımyıldız | Cassiopeia |
Konum
| Sağ Açıklık | 0h 19,88m |
| Dik Açı | 58° 35,53′ |
Frequently Asked Questions
What type of star is HIP 1590?
HIP 1590 is a Class B — B-type (Blue-White) star.
How far is HIP 1590 from Earth?
HIP 1590 is approximately 1,019.2 light-years from Earth.
Can you see HIP 1590 with the naked eye?
With an apparent magnitude of 9.75, HIP 1590 is not visible to the naked eye.
What constellation is HIP 1590 in?
HIP 1590 is located in the constellation Cassiopeia.