HIP 4397
HIP 4397 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,517 light-years, HIP 4397 is a distant star lying deep within the Milky Way galaxy.
HIP 4397 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4397 has an apparent magnitude of +8.13, 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 yellow hue, which corresponds to a B-V color index of +0.971.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 0,971 |
Beobachtung
| Scheinbare Helligkeit | +8.13 |
| Absolute Helligkeit | -0,21 |
| Entfernung | 1,517 ly |
| Sternbild | Cassiopeia |
Position
| Rektaszension | 0h 56,38m |
| Deklination | 59° 3,02′ |
Häufig gestellte Fragen
What type of star is HIP 4397?
HIP 4397 is a Class K — K-type (Orange) star.
How far is HIP 4397 from Earth?
HIP 4397 is approximately 1,517.0 light-years from Earth.
Can you see HIP 4397 with the naked eye?
With an apparent magnitude of 8.13, HIP 4397 is not visible to the naked eye.
What constellation is HIP 4397 in?
HIP 4397 is located in the constellation Cassiopeia.