HIP 838
HIP 838 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,623 light-years, HIP 838 is a distant star lying deep within the Milky Way galaxy.
HIP 838 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 838 has an apparent magnitude of +7.20, 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 blue hue, which corresponds to a B-V color index of -0.053.
الخصائص الفيزيائية
| النوع الطيفي | B Class B — B-type (Blue-White) |
| مؤشر اللون (B−V) | -0,053 |
الرصد
| القدر الظاهري | +7.20 |
| القدر المطلق | -1,28 |
| المسافة | 1,623 ly |
| الكوكبة | Cassiopeia |
الموضع
| المطلع المستقيم | 0h 10,27m |
| الميل | 52° 15,31′ |
Frequently Asked Questions
What type of star is HIP 838?
HIP 838 is a Class B — B-type (Blue-White) star.
How far is HIP 838 from Earth?
HIP 838 is approximately 1,622.7 light-years from Earth.
Can you see HIP 838 with the naked eye?
With an apparent magnitude of 7.20, HIP 838 is not visible to the naked eye.
What constellation is HIP 838 in?
HIP 838 is located in the constellation Cassiopeia.