HIP 62887
HIP 62887 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 2,965 light-years, HIP 62887 is a distant star lying deep within the Milky Way galaxy.
HIP 62887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 62887 has an apparent magnitude of +7.59, 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 red hue, which corresponds to a B-V color index of +1.510.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.510 |
Observation
| Apparent Magnitude | +7.59 |
| Absolute Magnitude | -2.20 |
| Distance | 2,965 ly |
| Constellation | Centaurus |
Position
| Right Ascension | 12h 53.30m |
| Declination | -45° 8.52′ |
Frequently Asked Questions
What type of star is HIP 62887?
HIP 62887 is a Class K — K-type (Orange) star.
How far is HIP 62887 from Earth?
HIP 62887 is approximately 2,965.0 light-years from Earth.
Can you see HIP 62887 with the naked eye?
With an apparent magnitude of 7.59, HIP 62887 is not visible to the naked eye.
What constellation is HIP 62887 in?
HIP 62887 is located in the constellation Centaurus.