HIP 97275
HIP 97275 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 1,802 light-years, HIP 97275 is a distant star lying deep within the Milky Way galaxy.
HIP 97275 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 97275 has an apparent magnitude of +8.45, 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 hue, which corresponds to a B-V color index of -0.060.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.060 |
Observation
| Apparent Magnitude | +8.45 |
| Absolute Magnitude | -0.26 |
| Distance | 1,802 ly |
| Constellation | Aquila |
Position
| Right Ascension | 19h 46.23m |
| Declination | 5° 59.29′ |
Frequently Asked Questions
What type of star is HIP 97275?
HIP 97275 is a Class B — B-type (Blue-White) star.
How far is HIP 97275 from Earth?
HIP 97275 is approximately 1,802.0 light-years from Earth.
Can you see HIP 97275 with the naked eye?
With an apparent magnitude of 8.45, HIP 97275 is not visible to the naked eye.
What constellation is HIP 97275 in?
HIP 97275 is located in the constellation Aquila.