HIP 7257
HIP 7257 is a A-type (White) star located in the constellation Perseus.
At a distance of roughly 2,992 light-years, HIP 7257 is a distant star lying deep within the Milky Way galaxy.
HIP 7257 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 7257 has an apparent magnitude of +9.55, 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 +0.121.
Physikalische Eigenschaften
| Spektralklasse | Class A — A-type (White) |
| Farbindex (B−V) | 0,121 |
Beobachtung
| Scheinbare Helligkeit | +9.55 |
| Absolute Helligkeit | -0,26 |
| Entfernung | 2,992 ly |
| Sternbild | Perseus |
Position
| Rektaszension | 1h 33,51m |
| Deklination | 53° 51,74′ |
Häufig gestellte Fragen
What type of star is HIP 7257?
HIP 7257 is a Class A — A-type (White) star.
How far is HIP 7257 from Earth?
HIP 7257 is approximately 2,992.3 light-years from Earth.
Can you see HIP 7257 with the naked eye?
With an apparent magnitude of 9.55, HIP 7257 is not visible to the naked eye.
What constellation is HIP 7257 in?
HIP 7257 is located in the constellation Perseus.