HIP 20177
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HIP 20177 is a K-type (Orange) star located in the constellation Perseus.
HIP 20177 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 20177 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 20177 has an apparent magnitude of +9.32, 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 orange hue, which corresponds to a B-V color index of +1.207.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.207 |
Observation
| Apparent Magnitude | +9.32 |
| Absolute Magnitude | -10.68 |
| Distance | 326,156 ly |
| Constellation | Perseus |
Position
| Right Ascension | 4h 19.50m |
| Declination | 39° 16.22′ |
Frequently Asked Questions
What type of star is HIP 20177?
HIP 20177 is a Class K — K-type (Orange) star.
How far is HIP 20177 from Earth?
HIP 20177 is approximately 326,156.0 light-years from Earth.
Can you see HIP 20177 with the naked eye?
With an apparent magnitude of 9.32, HIP 20177 is not visible to the naked eye.
What constellation is HIP 20177 in?
HIP 20177 is located in the constellation Perseus.