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.
Physikalische Eigenschaften
| Spektralklasse | Class M — M-type (Red) |
| Farbindex (B−V) | 1,305 |
Beobachtung
| Scheinbare Helligkeit | +9.67 |
| Absolute Helligkeit | 1,14 |
| Entfernung | 1,656 ly |
Position
| Rektaszension | 1h 9,20m |
| Deklination | 2° 46,42′ |
Häufig gestellte Fragen
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.