HIP 9409
HIP 9409 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,035 light-years, HIP 9409 is a distant star lying deep within the Milky Way galaxy.
HIP 9409 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9409 has an apparent magnitude of +8.49, 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 +1.720.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,720 |
Beobachtung
| Scheinbare Helligkeit | +8.49 |
| Absolute Helligkeit | 0,98 |
| Entfernung | 1,035 ly |
| Sternbild | Cassiopeia |
Position
| Rektaszension | 2h 0,89m |
| Deklination | 61° 0,82′ |
Häufig gestellte Fragen
What type of star is HIP 9409?
HIP 9409 is a Class K — K-type (Orange) star.
How far is HIP 9409 from Earth?
HIP 9409 is approximately 1,035.4 light-years from Earth.
Can you see HIP 9409 with the naked eye?
With an apparent magnitude of 8.49, HIP 9409 is not visible to the naked eye.
What constellation is HIP 9409 in?
HIP 9409 is located in the constellation Cassiopeia.