HIP 18507
HIP 18507 is a A-type (White) star located in the constellation Perseus.
Located approximately 451.7 light-years from Earth, HIP 18507 resides within the broader disk of our Milky Way galaxy.
HIP 18507 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 18507 has an apparent magnitude of +7.36, 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 blue-white hue, which corresponds to a B-V color index of +0.028.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,028 |
Observation
| Magnitude Apparente | +7.36 |
| Magnitude Absolue | 1,65 |
| Distance | 452 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 57,43m |
| Déclinaison | 43° 18,98′ |
Questions fréquentes
What type of star is HIP 18507?
HIP 18507 is a Class A — A-type (White) star.
How far is HIP 18507 from Earth?
HIP 18507 is approximately 451.7 light-years from Earth.
Can you see HIP 18507 with the naked eye?
With an apparent magnitude of 7.36, HIP 18507 is not visible to the naked eye.
What constellation is HIP 18507 in?
HIP 18507 is located in the constellation Perseus.