HIP 101490
HIP 101490 is a K-type (Orange) star.
At a distance of roughly 1,510 light-years, HIP 101490 is a distant star lying deep within the Milky Way galaxy.
HIP 101490 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 101490 has an apparent magnitude of +7.03, 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 +1.620.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,620 |
Observation
| Magnitude Apparente | +7.03 |
| Magnitude Absolue | -1,30 |
| Distance | 1,510 ly |
Position
| Ascension droite | 20h 34,02m |
| Déclinaison | 18° 11,13′ |
Questions fréquentes
What type of star is HIP 101490?
HIP 101490 is a Class K — K-type (Orange) star.
How far is HIP 101490 from Earth?
HIP 101490 is approximately 1,510.0 light-years from Earth.
Can you see HIP 101490 with the naked eye?
With an apparent magnitude of 7.03, HIP 101490 is not visible to the naked eye.