HIP 102297
HIP 102297 is a K-type (Orange) star.
At a distance of roughly 1,299 light-years, HIP 102297 is a distant star lying deep within the Milky Way galaxy.
HIP 102297 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102297 has an apparent magnitude of +7.21, 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 orange hue, which corresponds to a B-V color index of +1.061.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.061 |
Observation
| Apparent Magnitude | +7.21 |
| Absolute Magnitude | -0.79 |
| Distance | 1,299 ly |
Position
| Right Ascension | 20h 43.65m |
| Declination | 6° 34.69′ |
Frequently Asked Questions
What type of star is HIP 102297?
HIP 102297 is a Class K — K-type (Orange) star.
How far is HIP 102297 from Earth?
HIP 102297 is approximately 1,299.4 light-years from Earth.
Can you see HIP 102297 with the naked eye?
With an apparent magnitude of 7.21, HIP 102297 is not visible to the naked eye.