HIP 21417
HIP 21417 is a G-type (Yellow) star located in the constellation Perseus.
Located approximately 462.6 light-years from Earth, HIP 21417 resides within the broader disk of our Milky Way galaxy.
HIP 21417 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 21417 has an apparent magnitude of +9.16, 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 white hue, which corresponds to a B-V color index of +0.427.
Physikalische Eigenschaften
| Spektralklasse | G Class G — G-type (Yellow) |
| Farbindex (B−V) | 0,427 |
Beobachtung
| Scheinbare Helligkeit | +9.16 |
| Absolute Helligkeit | 3,40 |
| Entfernung | 463 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 4h 35,80m |
| Deklination | 50° 36,63′ |
Frequently Asked Questions
What type of star is HIP 21417?
HIP 21417 is a Class G — G-type (Yellow) star.
How far is HIP 21417 from Earth?
HIP 21417 is approximately 462.6 light-years from Earth.
Can you see HIP 21417 with the naked eye?
With an apparent magnitude of 9.16, HIP 21417 is not visible to the naked eye.
What constellation is HIP 21417 in?
HIP 21417 is located in the constellation Perseus.