HIP 101890
HIP 101890 is a K-type (Orange) star.
At a distance of roughly 1,681 light-years, HIP 101890 is a distant star lying deep within the Milky Way galaxy.
HIP 101890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101890 has an apparent magnitude of +7.93, 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 +1.655.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,655 |
Beobachtung
| Scheinbare Helligkeit | +7.93 |
| Absolute Helligkeit | -0,63 |
| Entfernung | 1,681 ly |
Position
| Rektaszension | 20h 38,90m |
| Deklination | 71° 10,14′ |
Frequently Asked Questions
What type of star is HIP 101890?
HIP 101890 is a Class K — K-type (Orange) star.
How far is HIP 101890 from Earth?
HIP 101890 is approximately 1,681.2 light-years from Earth.
Can you see HIP 101890 with the naked eye?
With an apparent magnitude of 7.93, HIP 101890 is not visible to the naked eye.