HIP 17665
HIP 17665 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 2,346 light-years, HIP 17665 is a distant star lying deep within the Milky Way galaxy.
HIP 17665 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17665 has an apparent magnitude of +7.62, 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 +1.312.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,312 |
Beobachtung
| Scheinbare Helligkeit | +7.62 |
| Absolute Helligkeit | -1,66 |
| Entfernung | 2,346 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 3h 47,00m |
| Deklination | 46° 37,07′ |
Häufig gestellte Fragen
What type of star is HIP 17665?
HIP 17665 is a Class K — K-type (Orange) star.
How far is HIP 17665 from Earth?
HIP 17665 is approximately 2,346.4 light-years from Earth.
Can you see HIP 17665 with the naked eye?
With an apparent magnitude of 7.62, HIP 17665 is not visible to the naked eye.
What constellation is HIP 17665 in?
HIP 17665 is located in the constellation Perseus.