HIP 24887
HIP 24887 is a G-type (Yellow) star.
At a distance of roughly 1,121 light-years, HIP 24887 is a distant star lying deep within the Milky Way galaxy.
HIP 24887 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 24887 has an apparent magnitude of +8.59, 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 hue, which corresponds to a B-V color index of +0.913.
Fiziksel Özellikler
| Spektral Sınıf | G Class G — G-type (Yellow) |
| Renk İndeksi (B−V) | 0,913 |
Gözlem
| Görünür Parlaklık | +8.59 |
| Mutlak Parlaklık | 0,91 |
| Mesafe | 1,121 ly |
Konum
| Sağ Açıklık | 5h 20,08m |
| Dik Açı | -63° 4,37′ |
Frequently Asked Questions
What type of star is HIP 24887?
HIP 24887 is a Class G — G-type (Yellow) star.
How far is HIP 24887 from Earth?
HIP 24887 is approximately 1,120.8 light-years from Earth.
Can you see HIP 24887 with the naked eye?
With an apparent magnitude of 8.59, HIP 24887 is not visible to the naked eye.