HIP 94870
HIP 94870 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,250 light-years, HIP 94870 is a distant star lying deep within the Milky Way galaxy.
HIP 94870 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 94870 has an apparent magnitude of +9.01, 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 +1.147.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,147 |
Beobachtung
| Scheinbare Helligkeit | +9.01 |
| Absolute Helligkeit | 1,09 |
| Entfernung | 1,250 ly |
| Sternbild | Aquila |
Position
| Rektaszension | 19h 18,38m |
| Deklination | 12° 9,69′ |
Häufig gestellte Fragen
What type of star is HIP 94870?
HIP 94870 is a Class K — K-type (Orange) star.
How far is HIP 94870 from Earth?
HIP 94870 is approximately 1,249.6 light-years from Earth.
Can you see HIP 94870 with the naked eye?
With an apparent magnitude of 9.01, HIP 94870 is not visible to the naked eye.
What constellation is HIP 94870 in?
HIP 94870 is located in the constellation Aquila.