HIP 79407
HIP 79407 is a K-type (Orange) star located in the constellation Scorpius.
At a distance of roughly 1,412 light-years, HIP 79407 is a distant star lying deep within the Milky Way galaxy.
HIP 79407 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 79407 has an apparent magnitude of +8.80, 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 +1.552.
الخصائص الفيزيائية
| النوع الطيفي | Class K — K-type (Orange) |
| مؤشر اللون (B−V) | 1,552 |
الرصد
| القدر الظاهري | +8.80 |
| القدر المطلق | 0,62 |
| المسافة | 1,412 ly |
| الكوكبة | Scorpius |
الموضع
| المطلع المستقيم | 16h 12,34m |
| الميل | -13° 44,32′ |
الأسئلة الشائعة
What type of star is HIP 79407?
HIP 79407 is a Class K — K-type (Orange) star.
How far is HIP 79407 from Earth?
HIP 79407 is approximately 1,411.9 light-years from Earth.
Can you see HIP 79407 with the naked eye?
With an apparent magnitude of 8.80, HIP 79407 is not visible to the naked eye.
What constellation is HIP 79407 in?
HIP 79407 is located in the constellation Scorpius.