HIP 12409
HIP 12409 is a K-type (Orange) star.
At a distance of roughly 2,718 light-years, HIP 12409 is a distant star lying deep within the Milky Way galaxy.
HIP 12409 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 12409 has an apparent magnitude of +7.34, 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 +1.413.
الخصائص الفيزيائية
| النوع الطيفي | K Class K — K-type (Orange) |
| مؤشر اللون (B−V) | 1,413 |
الرصد
| القدر الظاهري | +7.34 |
| القدر المطلق | -2,26 |
| المسافة | 2,718 ly |
الموضع
| المطلع المستقيم | 2h 39,78m |
| الميل | -35° 1,46′ |
Frequently Asked Questions
What type of star is HIP 12409?
HIP 12409 is a Class K — K-type (Orange) star.
How far is HIP 12409 from Earth?
HIP 12409 is approximately 2,718.0 light-years from Earth.
Can you see HIP 12409 with the naked eye?
With an apparent magnitude of 7.34, HIP 12409 is not visible to the naked eye.