HIP 102180
HIP 102180 is a K-type (Orange) star.
At a distance of roughly 1,144 light-years, HIP 102180 is a distant star lying deep within the Milky Way galaxy.
HIP 102180 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102180 has an apparent magnitude of +8.33, 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 +1.348.
الخصائص الفيزيائية
| النوع الطيفي | K Class K — K-type (Orange) |
| مؤشر اللون (B−V) | 1,348 |
الرصد
| القدر الظاهري | +8.33 |
| القدر المطلق | 0,60 |
| المسافة | 1,144 ly |
الموضع
| المطلع المستقيم | 20h 42,25m |
| الميل | 7° 10,89′ |
Frequently Asked Questions
What type of star is HIP 102180?
HIP 102180 is a Class K — K-type (Orange) star.
How far is HIP 102180 from Earth?
HIP 102180 is approximately 1,144.4 light-years from Earth.
Can you see HIP 102180 with the naked eye?
With an apparent magnitude of 8.33, HIP 102180 is not visible to the naked eye.