HIP 52770
HIP 52770 is a K-type (Orange) star.
At a distance of roughly 1,245 light-years, HIP 52770 is a distant star lying deep within the Milky Way galaxy.
HIP 52770 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 52770 has an apparent magnitude of +7.19, 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 red hue, which corresponds to a B-V color index of +1.568.
Fiziksel Özellikler
| Spektral Sınıf | K Class K — K-type (Orange) |
| Renk İndeksi (B−V) | 1,568 |
Gözlem
| Görünür Parlaklık | +7.19 |
| Mutlak Parlaklık | -0,72 |
| Mesafe | 1,245 ly |
Konum
| Sağ Açıklık | 10h 47,38m |
| Dik Açı | 26° 54,64′ |
Frequently Asked Questions
What type of star is HIP 52770?
HIP 52770 is a Class K — K-type (Orange) star.
How far is HIP 52770 from Earth?
HIP 52770 is approximately 1,244.9 light-years from Earth.
Can you see HIP 52770 with the naked eye?
With an apparent magnitude of 7.19, HIP 52770 is not visible to the naked eye.