HIP 18458
HIP 18458 is a G-type (Yellow) star located in the constellation Perseus.
Located approximately 994.4 light-years from Earth, HIP 18458 resides within the broader disk of our Milky Way galaxy.
HIP 18458 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 18458 has an apparent magnitude of +8.19, 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 yellow-white hue, which corresponds to a B-V color index of +0.752.
Fiziksel Özellikler
| Spektral Sınıf | G Class G — G-type (Yellow) |
| Renk İndeksi (B−V) | 0,752 |
Gözlem
| Görünür Parlaklık | +8.19 |
| Mutlak Parlaklık | 0,77 |
| Mesafe | 994 ly |
| Takımyıldız | Perseus |
Konum
| Sağ Açıklık | 3h 56,65m |
| Dik Açı | 34° 9,30′ |
Frequently Asked Questions
What type of star is HIP 18458?
HIP 18458 is a Class G — G-type (Yellow) star.
How far is HIP 18458 from Earth?
HIP 18458 is approximately 994.4 light-years from Earth.
Can you see HIP 18458 with the naked eye?
With an apparent magnitude of 8.19, HIP 18458 is not visible to the naked eye.
What constellation is HIP 18458 in?
HIP 18458 is located in the constellation Perseus.