HIP 101887
HIP 101887 is a K-type (Orange) star.
HIP 101887 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 101887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101887 has an apparent magnitude of +9.12, 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 +1.420.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,420 |
Beobachtung
| Scheinbare Helligkeit | +9.12 |
| Absolute Helligkeit | -10,88 |
| Entfernung | 326,156 ly |
Position
| Rektaszension | 20h 38,87m |
| Deklination | -40° 22,13′ |
Häufig gestellte Fragen
What type of star is HIP 101887?
HIP 101887 is a Class K — K-type (Orange) star.
How far is HIP 101887 from Earth?
HIP 101887 is approximately 326,156.0 light-years from Earth.
Can you see HIP 101887 with the naked eye?
With an apparent magnitude of 9.12, HIP 101887 is not visible to the naked eye.