HIP 103002
HIP 103002 is a M-type (Red) star.
At a distance of roughly 1,007 light-years, HIP 103002 is a distant star lying deep within the Milky Way galaxy.
HIP 103002 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 103002 has an apparent magnitude of +7.85, 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 +1.611.
Physical Properties
| Spectral Class | Class M — M-type (Red) |
| Color Index (B−V) | 1.611 |
Observation
| Apparent Magnitude | +7.85 |
| Absolute Magnitude | 0.40 |
| Distance | 1,007 ly |
Position
| Right Ascension | 20h 52.09m |
| Declination | -33° 52.91′ |
Frequently Asked Questions
What type of star is HIP 103002?
HIP 103002 is a Class M — M-type (Red) star.
How far is HIP 103002 from Earth?
HIP 103002 is approximately 1,006.6 light-years from Earth.
Can you see HIP 103002 with the naked eye?
With an apparent magnitude of 7.85, HIP 103002 is not visible to the naked eye.