HIP 5409
HIP 5409 is a M-type (Red) star.
At a distance of roughly 1,656 light-years, HIP 5409 is a distant star lying deep within the Milky Way galaxy.
HIP 5409 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 5409 has an apparent magnitude of +9.67, 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 +1.305.
Physical Properties
| Spectral Class | Class M — M-type (Red) |
| Color Index (B−V) | 1.305 |
Observation
| Apparent Magnitude | +9.67 |
| Absolute Magnitude | 1.14 |
| Distance | 1,656 ly |
Position
| Right Ascension | 1h 9.20m |
| Declination | 2° 46.42′ |
Frequently Asked Questions
What type of star is HIP 5409?
HIP 5409 is a Class M — M-type (Red) star.
How far is HIP 5409 from Earth?
HIP 5409 is approximately 1,655.6 light-years from Earth.
Can you see HIP 5409 with the naked eye?
With an apparent magnitude of 9.67, HIP 5409 is not visible to the naked eye.