HIP 52887
HIP 52887 is a M-type (Red) star.
HIP 52887 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 52887 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
At an apparent magnitude of +12.22, HIP 52887 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its red hue, which corresponds to a B-V color index of +1.500.
الخصائص الفيزيائية
| النوع الطيفي | M Class M — M-type (Red) |
| مؤشر اللون (B−V) | 1,500 |
الرصد
| القدر الظاهري | +12.22 |
| القدر المطلق | -7,78 |
| المسافة | 326,156 ly |
الموضع
| المطلع المستقيم | 10h 49,00m |
| الميل | -54° 10,91′ |
Frequently Asked Questions
What type of star is HIP 52887?
HIP 52887 is a Class M — M-type (Red) star.
How far is HIP 52887 from Earth?
HIP 52887 is approximately 326,156.0 light-years from Earth.
Can you see HIP 52887 with the naked eye?
With an apparent magnitude of 12.22, HIP 52887 is not visible to the naked eye.