HIP 7887
HIP 7887 is a A-type (White) star located in the constellation Cassiopeia.
Located approximately 499.5 light-years from Earth, HIP 7887 resides within the broader disk of our Milky Way galaxy.
HIP 7887 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 7887 has an apparent magnitude of +8.32, 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 +0.325.
Physical Properties
| Spectral Class | Class A — A-type (White) |
| Color Index (B−V) | 0.325 |
Observation
| Apparent Magnitude | +8.32 |
| Absolute Magnitude | 2.40 |
| Distance | 499 ly |
| Constellation | Cassiopeia |
Position
| Right Ascension | 1h 41.46m |
| Declination | 66° 29.32′ |
Frequently Asked Questions
What type of star is HIP 7887?
HIP 7887 is a Class A — A-type (White) star.
How far is HIP 7887 from Earth?
HIP 7887 is approximately 499.5 light-years from Earth.
Can you see HIP 7887 with the naked eye?
With an apparent magnitude of 8.32, HIP 7887 is not visible to the naked eye.
What constellation is HIP 7887 in?
HIP 7887 is located in the constellation Cassiopeia.