HIP 66887
HIP 66887 is a K-type (Orange) star located in the constellation Centaurus.
HIP 66887 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 66887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 66887 has an apparent magnitude of +8.70, 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 orange hue, which corresponds to a B-V color index of +1.059.
الخصائص الفيزيائية
| النوع الطيفي | K Class K — K-type (Orange) |
| مؤشر اللون (B−V) | 1,059 |
الرصد
| القدر الظاهري | +8.70 |
| القدر المطلق | -11,30 |
| المسافة | 326,156 ly |
| الكوكبة | Centaurus |
الموضع
| المطلع المستقيم | 13h 42,45m |
| الميل | -37° 22,58′ |
Frequently Asked Questions
What type of star is HIP 66887?
HIP 66887 is a Class K — K-type (Orange) star.
How far is HIP 66887 from Earth?
HIP 66887 is approximately 326,156.0 light-years from Earth.
Can you see HIP 66887 with the naked eye?
With an apparent magnitude of 8.70, HIP 66887 is not visible to the naked eye.
What constellation is HIP 66887 in?
HIP 66887 is located in the constellation Centaurus.