HIP 632
HIP 632 is a M-type (Red) star.
At a distance of roughly 2,471 light-years, HIP 632 is a distant star lying deep within the Milky Way galaxy.
HIP 632 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 632 has an apparent magnitude of +9.06, 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 orange hue, which corresponds to a B-V color index of +1.074.
Physical Properties
| Spectral Class | M Class M — M-type (Red) |
| Color Index (B−V) | 1.074 |
Observation
| Apparent Magnitude | +9.06 |
| Absolute Magnitude | -0.34 |
| Distance | 2,471 ly |
Position
| Right Ascension | 0h 7.68m |
| Declination | -56° 14.97′ |
Frequently Asked Questions
What type of star is HIP 632?
HIP 632 is a Class M — M-type (Red) star.
How far is HIP 632 from Earth?
HIP 632 is approximately 2,470.9 light-years from Earth.
Can you see HIP 632 with the naked eye?
With an apparent magnitude of 9.06, HIP 632 is not visible to the naked eye.