HIP 100890
HIP 100890 is a M-type (Red) star located in the constellation Aquila.
At a distance of roughly 1,094 light-years, HIP 100890 is a distant star lying deep within the Milky Way galaxy.
HIP 100890 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 100890 has an apparent magnitude of +9.65, 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 +1.844.
الخصائص الفيزيائية
| النوع الطيفي | Class M — M-type (Red) |
| مؤشر اللون (B−V) | 1,844 |
الرصد
| القدر الظاهري | +9.65 |
| القدر المطلق | 2,02 |
| المسافة | 1,094 ly |
| الكوكبة | Aquila |
الموضع
| المطلع المستقيم | 20h 27,42m |
| الميل | -4° 43,85′ |
الأسئلة الشائعة
What type of star is HIP 100890?
HIP 100890 is a Class M — M-type (Red) star.
How far is HIP 100890 from Earth?
HIP 100890 is approximately 1,094.5 light-years from Earth.
Can you see HIP 100890 with the naked eye?
With an apparent magnitude of 9.65, HIP 100890 is not visible to the naked eye.
What constellation is HIP 100890 in?
HIP 100890 is located in the constellation Aquila.